{"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"B_iram"}} {"id": "B/iram", "title_cds": "IRAM Observation Logs", "title_create": "IRAM 1991-2020", "year": "2020", "author": "Dan M., Neri R., Sievers A.", "title_pub": "IRAM Observation Logs (Plateau de Bure Interferometer and 30-m telescope)", "first_author": "Dan M.", "ref_biblio": [""], "see_also": ["http://www.iram-institute.org/ : the IRAM Home Page"], "keyword_cds": "Observatory log ; Interferometry ; Radio sources", "description": ["The Institut de Radio Astronomie Millimetrique (IRAM) was founded in", "1979 and is operated as a French-German-Spanish collaboration. Its", "partner institutes are the CNRS (Centre National de la Recherche", "Scientifique, France), the MPG (Max Planck Gesellschaft, Germany), and", "the IGN (Instituto Geografico Nacional, Spain). The principal activity", "of IRAM is the study of cold matter (molecular gas and dust) in the", "solar system, in our Galaxy, and out to cosmological distances in", "order to determine its composition, density, mass, temperature, and", "kinematics.", "IRAM operates two observatories at millimeter wavelengths which are", "open to the international astronomical community: The 30-m single-dish", "telescope on Pico Veleta (2850m), Spain, and the six-antenna", "interferometer on the Plateau de Bure (2550m) in France. Both sites", "are at high altitude to reduce the absorption by water vapor. The", "observatories are supported by the IRAM offices and laboratories in", "Granada and Grenoble.", "The observation log included here concerns the Plateau de Bure site,", "and summarizes the observations made there from December 1990.", "The observations log of the 30-m single-dish telescope covers a", "period starting in January 2009. This log was produced using a header", "archive, a collaborative effort between IRAM and IAA/CSIC.", "NOEMA (NOrthern Extended Millimeter Array) is the successor to the", "Plateau du Bure observatory. During its history, the observatory at", "the Plateau de Bure underwent several track extensions, received", "additional antennas (all of 15m diameter and similar construction as", "the first ones) and technical upgrades. From a three antenna", "interferometer with a maximum baseline of 288 meters in 1988, it has", "evolved to a eight-antenna array with baselines up to 760 meters in", "2016. With the inauguration of the seventh antenna in September 2014,", "the observatory has started its transformation into NOEMA."], "alias": ["logIRAM", "IRAM", "PdBI"], "type": ["OC"], "records": ["653695 obs."], "data": "f-v", "date_creation": "29-Jun-2004", "xmatch": "B/iram/pdbi", "last_update": "26-Apr-2021", "catid": "102016", "date_update": "26-Apr-2021", "tables": [{"name": "pdbi.dat", "desc": "The Plateau de Bure Interferometer Observation Log since 1991-12-01", "columns": [{"name": "Nw", "desc": "[11,18] Internal indicator "}, {"name": "Prog", "desc": "Identification code of the program "}, {"name": "Name", "desc": "Source name, as mentioned in the observing program"}, {"name": "Obs.Y", "desc": "Starting date of the Observation (year) (5) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.M", "desc": "Starting date of the Observation (month) (5) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.D", "desc": "Starting date of the Observation (day) (5) "}, {"name": "t1.h", "desc": "LST Time of the first scan on source "}, {"name": "---", "desc": "[:] "}, {"name": "t1.m", "desc": "LST Time of the first scan on source "}, {"name": "t2.h", "desc": "LST Time of the last scan on source "}, {"name": "---", "desc": "[:] "}, {"name": "t2.m", "desc": "LST Time of the last scan on source "}, {"name": "tos", "desc": "Total on-source correlation time "}, {"name": "Type", "desc": "Program type (1) "}, {"name": "oEq", "desc": "? Original equinox of position (2) "}, {"name": "RAh", "desc": "? Right Ascension J2000 (hours) "}, {"name": "---", "desc": "[:] "}, {"name": "RAm", "desc": "? Right Ascension J2000 (minutes) "}, {"name": "---", "desc": "[:] "}, {"name": "RAs", "desc": "? Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? Declination J2000 (degrees) "}, {"name": "---", "desc": "[:] "}, {"name": "DEm", "desc": "? Declination J2000 (minutes) "}, {"name": "---", "desc": "[:] "}, {"name": "DEs", "desc": "? Declination J2000 (seconds) "}, {"name": "Vel", "desc": "Velocity of the source (3) "}, {"name": "n_Vel", "desc": "[LH] LSR or Heliocentric velocity "}, {"name": "Flow", "desc": "?=0 Sky Frequency of the 3mm receiver (6) "}, {"name": "n_Flow", "desc": "[UL] Signal Upper/Lower band of the 3mm receiver "}, {"name": "Fhigh", "desc": "?=0 Sky Frequency of the 1mm receiver (6) "}, {"name": "n_Fhigh", "desc": "[UL] Signal Upper/Lower band of the 1mm receiver "}, {"name": "pol", "desc": "[HV ] Horizontal/Vertical polarisations (6) "}, {"name": "p4", "desc": "[HV ] Polarisation of 4GHz continuum (6) "}, {"name": "Conf", "desc": "Configuration code of the interferometer "}, {"name": "Config", "desc": "Detailed configuration (4) "}]}, {"name": "pdbi_pi.dat", "desc": "List of PI investigators of PdBI instrument ", "columns": [{"name": "Prog", "desc": "Identification code of the program "}, {"name": "PI", "desc": "Principal Investigator's name "}]}, {"name": "noema.dat", "desc": "The Plateau de Bure Interferometer (Noema) Observation Log since 2016", "columns": [{"name": "Nw", "desc": "[11,19] Internal indicator "}, {"name": "Prog", "desc": "Identification code of the program "}, {"name": "Name", "desc": "Source name, as mentioned in the observing program"}, {"name": "Obs.Y", "desc": "Starting date of the Observation (year) (5) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.M", "desc": "Starting date of the Observation (month) (5) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.D", "desc": "Starting date of the Observation (day) (5) "}, {"name": "t1.h", "desc": "LST Time of the first scan on source "}, {"name": "---", "desc": "[:] "}, {"name": "t1.m", "desc": "LST Time of the first scan on source "}, {"name": "t2.h", "desc": "LST Time of the last scan on source "}, {"name": "---", "desc": "[:] "}, {"name": "t2.m", "desc": "LST Time of the last scan on source "}, {"name": "tos", "desc": "Total on-source correlation time "}, {"name": "Type", "desc": "Program type (1) "}, {"name": "oEq", "desc": "? Original equinox of position (2) "}, {"name": "RAh", "desc": "? Right Ascension J2000 (hours) "}, {"name": "---", "desc": "[:] "}, {"name": "RAm", "desc": "? Right Ascension J2000 (minutes) "}, {"name": "---", "desc": "[:] "}, {"name": "RAs", "desc": "? Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? Declination J2000 (degrees) "}, {"name": "---", "desc": "[:] "}, {"name": "DEm", "desc": "? Declination J2000 (minutes) "}, {"name": "---", "desc": "[:] "}, {"name": "DEs", "desc": "? Declination J2000 (seconds) "}, {"name": "Vel", "desc": "Velocity of the source (3) "}, {"name": "n_Vel", "desc": "[LH] LSR or Heliocentric velocity "}, {"name": "Flow", "desc": "?=0 Sky Frequency of the 3mm receiver (6) "}, {"name": "n_Flow", "desc": "[UL] Signal Upper/Lower band of the 3mm receiver "}, {"name": "Fhigh", "desc": "?=0 Sky Frequency of the 1mm receiver (6) "}, {"name": "n_Fhigh", "desc": "[UL] Signal Upper/Lower band of the 1mm receiver "}, {"name": "pol", "desc": "[HV ] Horizontal/Vertical polarisations (6) "}, {"name": "p4", "desc": "[HV ] Polarisation of 4GHz continuum (6) "}, {"name": "Conf", "desc": "Configuration code of the interferometer "}, {"name": "Config", "desc": "Detailed configuration (4) "}]}, {"name": "noema_pi.dat", "desc": "List of PI investigators of Noema instrument ", "columns": [{"name": "Prog", "desc": "Identification code of the program "}, {"name": "PI", "desc": "Principal Investigator's name "}]}, {"name": "30m.dat", "desc": "List of observations at 30m instrument since 2009-09-30", "columns": [{"name": "Name", "desc": "Target source name "}, {"name": "sys", "desc": "[BJG] equinox system "}, {"name": "Eq", "desc": "? equinox year "}, {"name": "RAh", "desc": "[]? Right ascension (hours) J2000 "}, {"name": "---", "desc": "[:] "}, {"name": "RAm", "desc": "? Right ascension (minutes) J2000 "}, {"name": "---", "desc": "[:] "}, {"name": "RAs", "desc": "? Right ascension (seconds) J2000 "}, {"name": "DE-", "desc": "Declination (sign) J2000 "}, {"name": "DEd", "desc": "? Declination (degrees) J2000 "}, {"name": "---", "desc": "[:] "}, {"name": "DEm", "desc": "? Declination (minutes) J2000 "}, {"name": "---", "desc": "[:] "}, {"name": "DEs", "desc": "? Declination (seconds) J2000 "}, {"name": "Obs.Y", "desc": "Starting date of the Observation (year) (from ncsID)"}, {"name": "---", "desc": "[-] "}, {"name": "Obs.M", "desc": "Starting date of the Observation (month) "}, {"name": "---", "desc": "[-] "}, {"name": "Obs.D", "desc": "Starting date of the Observation (day) "}, {"name": "---", "desc": "[.] "}, {"name": "scan", "desc": "Scan No. (Date.scan = ncsID) "}, {"name": "t1.h", "desc": "? Starting time in UTC (hour) "}, {"name": "---", "desc": "? [:] "}, {"name": "t1.m", "desc": "? Starting time (min) "}, {"name": "---", "desc": "? [:] "}, {"name": "t1.s", "desc": "? Starting time (sec) "}, {"name": "t2.h", "desc": "? End time (hour) "}, {"name": "---", "desc": "? [:] "}, {"name": "t2.m", "desc": "? End time (min) "}, {"name": "---", "desc": "? [:] "}, {"name": "t2.s", "desc": "? End time (sec) "}, {"name": "obsMode", "desc": "Observation mode (1) "}, {"name": "Prog", "desc": "Identification code of the program "}, {"name": "tau", "desc": "? Zenith {tau} at 225 GHz from tipping taumeter "}, {"name": "receiv", "desc": "Short name of the receiver(band) used "}, {"name": "line", "desc": "Name of line observed "}, {"name": "Freq", "desc": "Frequency used for the observation "}]}, {"name": "30m_pi.dat", "desc": "List of PI investigators of 30m instrument ", "columns": [{"name": "Prog", "desc": "Identification code of the program "}, {"name": "PI", "desc": "Principal Investigator's name "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"B_pn"}} {"id": "B/pn", "title_cds": "Atlas of Galactic Planetary Nebulae", "title_create": "Miszalski+ 2011", "year": "2011", "author": "Miszalski B., Acker A., Ochsenbein F., Parker Q.", "title_pub": "A digital Atlas of Galactic Planetary Nebulae", "first_author": "Miszalski B.", "ref_biblio": ["< (in preparation) >"], "bibcode": ["2010yCat.0....0M"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "records": ["records"], "data": "", "date_update": "16-Nov-2010"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"B_simbad"}} {"id": "B/simbad", "title_cds": "Simbad objects catalogue", "title_create": "M.Wenger 2000", "year": "2000", "author": "M.Wenger; Ochsenbein, F.; Egret, D.; Dubois, P.; Bonnarel, F.; Borde, S.; Genova, F.; Jasniewicz, G.; Laloe, S.; Lesteven, S.; Monier, R", "title_pub": "Simbad objects catalogue", "first_author": "M.Wenger; Ochsenbein", "ref_biblio": ["<2000A&AS..143....9W>"], "bibcode": ["2000A&AS..143....9W"], "keyword_cds": "Bibliography; Photometry; Positional data; Proper motions", "description": ["Simbad is the reference database for identification and bibliography of", "astronomical objects. It contains identifications, ``basic data'',", "bibliography, and selected observational measurements for several million", "astronomical objects. Simbad is developed and maintained by CDS, Strasbourg.", "Building the database contents is achieved with the help of several", "contributing institutes. Scanning the bibliography is the result of the", "collaboration of CDS with bibliographers in Observatoire de Paris (DASGAL),", "Institut d'Astrophysique de Paris, and Observatoire de Bordeaux. When", "selecting catalogues and tables for inclusion, priority is given to optimal", "multi-wavelength coverage of the database, and to support of research", "developments linked to large projects. In parallel, the systematic scanning", "of the bibliography reflects the diversity and general trends of", "astronomical research. A WWW interface to Simbad is available at:", "{http://simbad.u-strasbg.fr/Simbad}."], "alias": ["simbad"], "type": ["GCC"], "records": ["7000000 sources"], "doi_pub": ["10.1051/aas:2000332"], "data": "f", "islargetable": true, "date_creation": "12-Feb-2013", "date_update": "08-Aug-2018", "tables": [{"name": "simbad.out", "desc": "Simbad sample ", "columns": [{"name": "Id", "desc": "Main Simbad Identifier "}, {"name": "RAdeg", "desc": "Right ascention (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "errMaj", "desc": "?Half Major axis of the positional error "}, {"name": "errMin", "desc": "?Half Minor axis of the positional error "}, {"name": "errPA", "desc": "?Position angle of the positional error "}, {"name": "Bmag", "desc": "?Magnitude in B "}, {"name": "Vmag", "desc": "?Magnitude in V "}, {"name": "Rmag", "desc": "?Magnitude in R "}, {"name": "Jmag", "desc": "?Magnitude in J "}, {"name": "Hmag", "desc": "?Magnitude in H "}, {"name": "Kmag", "desc": "?Magnitude in K "}, {"name": "oType", "desc": "Object type "}, {"name": "pmRa", "desc": "?Proper motion in rigth ascention "}, {"name": "pmDe", "desc": "?Proper motion in declination "}, {"name": "sp", "desc": "Spectral type "}, {"name": "nBibCode", "desc": "Number of bibcode associated "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"I_253"}} {"id": "I/253", "title_cds": "STARNET", "title_create": "Roeser 1996", "year": "1996", "author": "Roeser S.", "title_pub": "STARNET, an updated GSC for minor planet observations", "first_author": "Roeser S.", "ref_biblio": [""], "see_also": ["http://ad.usno.navy.mil/wds/ : the WDS Home page", "V/111 : Fifth Catalog of Orbits of Visual Double Stars"], "keyword_cds": "Stars, double and multiple ; Positional data", "description": ["The Washington Double Star Catalog (WDS), maintained by the United", "States Naval Observatory, is the world's principal database of", "astrometric double and multiple star information. The WDS Catalog", "contains positions (J2000), discoverer designations, epochs, position", "angles, separations, magnitudes, spectral types, proper motions and", "when available, Durchmusterung numbers and notes for the components of", "84,486 systems based on 563,326 means. The current version (updated", "nightly) is available online. A brief summary and statistical analysis", "of the contents of the catalog are presented."], "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["WDS", "WDS\\_20001"], "type": ["GCC"], "records": ["84486 binaries"], "data": "", "date_update": "12-Aug-2012"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"I_286"}} {"id": "I/286", "title_cds": "The Astrometric Catalogue ARIHIP", "title_create": "Wielen+ 2001", "year": "2001", "author": "Wielen R., Schwan H., Dettbarn C., Lenhardt H., Jahreiss H., Jaehrling R., Khalisi E.", "title_pub": "Astrometric Catalogue ARIHIP containing stellar data selected from the Combination Catalogues FK6, GC+HIP, TYC2+HIP and from the HIPPARCOS Catalogue.", "first_author": "Wielen R.", "ref_biblio": [""], "bibcode": ["2001VeARI..40....1W"], "see_also": ["http://www.ari.uni-heidelberg.de/arihip/ : ARIHIP home page", "I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)", "I/264 : Sixth Catalogue of Fundamental Stars (FK6) (Wielen+ 2000)", "I/113 : General Catalogue of 33342 stars (GC) (Boss 1937)"], "keyword_cds": "Fundamental catalog ; Positional data ; Proper motions", "alias": ["ARIHIP"], "records": ["90842 stars"], "data": "", "date_update": "29-Oct-2014", "tables": [{"name": "arihcx01.dat", "desc": "The big astrometric Catalogue ARIHIP (lastr update: 2003-04-11)", "columns": [{"name": "HIP", "desc": "[1/120404] Hipparcos Catalog Number (I/239) (#1) "}, {"name": "FK6", "desc": "[4/6125]? FK6 number of the star (Wielen et al. I/264) (#2) "}, {"name": "n_FK6", "desc": "FK6 subsample (#3) (1) "}, {"name": "GC", "desc": "[1/33343]? General Catalogue number (I/113) (#4) "}, {"name": "TYC1", "desc": "[1/9537] Explain column (#5) "}, {"name": "TYC2", "desc": "[1/12111] Explain column (#5) "}, {"name": "TYC3", "desc": "[1] Tycho "}, {"name": "Sel", "desc": "Selected catalogue (#6) (2) "}, {"name": "---", "desc": "Reference flag for double systems (empty) (#7) "}, {"name": "RAh", "desc": "Right Ascension ICRS, Sp=J2000 (hours) (#8) "}, {"name": "RAm", "desc": "Right Ascension ICRS, Sp=J2000 (minutes) (#8) "}, {"name": "RAs", "desc": "Right Ascension ICRS, Sp=J2000 (seconds) (#8) "}, {"name": "DE-", "desc": "Declination ICRS, Sp=J2000 (sign) (#9) "}, {"name": "DEd", "desc": "Declination ICRS, Sp=J2000 (degrees) (#9) "}, {"name": "DEm", "desc": "Declination ICRS, Sp=J2000 (minutes) (#9) "}, {"name": "DEs", "desc": "Declination ICRS, Sp=J2000 (seconds) (#9) "}, {"name": "pmRA", "desc": "[-3257.91/6766.91] proper-motion component {mu}_{alpha}*_ (#10) "}, {"name": "pmDE", "desc": "[-5815.07/10328] proper motionn component {mu}_{delta}_ (#11) "}, {"name": "EpRA", "desc": "[89.87/92.33] Central RA epoch -1900 (#12) "}, {"name": "e_RA", "desc": "[0.28/17.44] Mean error on {alpha}* at EpRA (#13) "}, {"name": "e_pmRA", "desc": "[0.2/33.74] Mean error on pmRA (#14) "}, {"name": "EpDE", "desc": "[90.35/92.41] Central Declination epoch -1900 (#15) "}, {"name": "e_DE", "desc": "[0.3/10.88] Mean error on Declination (#16) "}, {"name": "e_pmDE", "desc": "[0.18/26.46] Mean error on pmDE (#17) "}, {"name": "plx", "desc": "[-29.58/549.01] Parallax of the star (#18) "}, {"name": "e_plx", "desc": "[0.04/20.8] Mean error on plx (#19) "}, {"name": "r_plx", "desc": "[HP] Origin of plx: H=Hippacros, P=photometric (#20) "}, {"name": "RV", "desc": "[-409/471]? Radial velocity of star (#21) "}, {"name": "Vmag", "desc": "[-0.62/14.08] Apparent visual magnitude of star (#22) "}, {"name": "f_Vmag", "desc": "[1/3]? variability of star (#23) (3) "}, {"name": "bin", "desc": "[11/99] Flag for the object binarity (#24) (4) "}, {"name": "Kp", "desc": "[1/2]? double-star nature of the object (#25) (5) "}, {"name": "Q", "desc": "[1/3]? astrometrically excellent star (#26) (6) "}, {"name": "dRA1", "desc": "[-206.34/334.92] LTP {Delta}{alpha}* (#27) (7) "}, {"name": "dRA2", "desc": "[-99.55/127.47] STP {Delta}{alpha}* (#28) (7) "}, {"name": "dRA3", "desc": "[-153.77/190.35] HIP {Delta}{alpha}* (#29) (7) "}, {"name": "dRA4", "desc": "[-15861/12259.9]? CAT1 {Delta}{alpha}* (#30) (7) "}, {"name": "dDE1", "desc": "[-251.7/232.99] LTP {Delta}{delta} (#31) (7) "}, {"name": "dDE2", "desc": "[-154.41/96.01] STP {Delta}{delta} (#32) (7) "}, {"name": "dDE3", "desc": "[-350.04/140.66] HIP {Delta}{delta} (#33) (7) "}, {"name": "dDE4", "desc": "[-7277.05/5483.3]? CAT1 {Delta}{delta}(#34) (7) "}, {"name": "dpmRA1", "desc": "[-24.87/40.64] LTP {Delta}{mu}_{alpha}*_ (#35) (7) "}, {"name": "dpmRA2", "desc": "[-11.03/14.59] STP {Delta}{mu}_{alpha}*_ (#36) (7) "}, {"name": "dpmRA3", "desc": "[-17.24/20.76] HIP {Delta}{mu}_{alpha}*_ (#37) (7) "}, {"name": "dpmRA4", "desc": "[-129.35/146.72]? CAT1 {Delta}{mu}_{alpha}*_ (#38) (7) "}, {"name": "dpmRA5", "desc": "[-28.93/62.39]? mu0 {Delta}{mu}_{alpha}*_ (#39) (7) "}, {"name": "dpmDE1", "desc": "[-29.99/25.87] LTP {Delta}{mu}_{delta}_ (#40) (7) "}, {"name": "dpmDE2", "desc": "[-17.69/11.04] STP {Delta}{mu}_{delta}_ (#41) (7) "}, {"name": "dpmDE3", "desc": "[-42.38/16.27] HIP {Delta}{mu}_{delta}_ (#42) (7) "}, {"name": "dpmDE4", "desc": "[-79.24/80.87]? CAT1 {Delta}{mu}_{delta}_ (#43) (7) "}, {"name": "dpmDE5", "desc": "[-39.43/28.18]? mu0 {Delta}{mu}_{delta}_ (#44) (7) "}, {"name": "EpRA1", "desc": "[1957.05/1992.27] LTP RA epoch (#45) "}, {"name": "EpRA2", "desc": "[1989.87/1992.33] STP RA epoch (#46) "}, {"name": "EpRA3", "desc": "[1989.87/1992.38] HIP RA epoch (#47) "}, {"name": "EpRA4", "desc": "[1877.5/1992.47]? CAT1 RA epoch (#48) "}, {"name": "eRA1", "desc": "[0.33/18.57] LTP {epsilon}_{alpha}*_ (#49) "}, {"name": "eRA2", "desc": "[0.28/17.44] STP {epsilon}_{alpha}*_ (#50) "}, {"name": "eRA3", "desc": "[0.28/17.44] HIP {epsilon}_{alpha}*_ (#51) "}, {"name": "eRA4", "desc": "[3/326.77]? CAT1 {epsilon}_{alpha}*_ (#52) "}, {"name": "pmRA1", "desc": "[0.24/33.74] LTP {epsilon}_{mu}{alpha}*_ (#53) "}, {"name": "pmRA2", "desc": "[0.3/33.74] STP {epsilon}_{mu}{alpha}*_ (#54) "}, {"name": "pmRA3", "desc": "[0.31/33.74] HIP {epsilon}_{mu}{alpha}*_ (#55) "}, {"name": "pmRA4", "desc": "[0.3/40.03]? CAT1 {epsilon}_{mu}{alpha}*_ (#56) "}, {"name": "pmRA5", "desc": "[0.24/8.58]? mu0 {epsilon}_{mu}{alpha}*_ (#57) "}, {"name": "EpDE1", "desc": "[1954.47/1992.41] LTP {delta} epoch (#58) "}, {"name": "EpDE2", "desc": "[1990.35/1992.41] STP {delta} epoch (#59) "}, {"name": "EpDE3", "desc": "[1990.32/1992.5] HIP {delta} epoch (#60) "}, {"name": "EpDE4", "desc": "[1876.8/1991.96]? CAT1 {delta} epoch (#61) "}, {"name": "eDE1", "desc": "[0.36/18.44] LTP {epsilon}_{delta} (#62) "}, {"name": "eDE2", "desc": "[0.3/10.88] STP {epsilon}_{delta} (#63) "}, {"name": "eDE3", "desc": "[0.3/10.88] HIP {epsilon}_{delta} (#64) "}, {"name": "eDE4", "desc": "[3/282.26]? CAT1 {epsilon}_{delta} (#65) "}, {"name": "pmDE1", "desc": "[0.21/26.52] LTP {epsilon}_{mu}{delta}_ (#66) "}, {"name": "pmDE2", "desc": "[0.31/26.46] STP {epsilon}_{mu}{delta}_ (#67) "}, {"name": "pmDE3", "desc": "[0.32/26.46] HIP {epsilon}_{mu}{delta}_ (#68) "}, {"name": "pmDE4", "desc": "[0.3/43]? CAT1 {epsilon}_{mu}{delta}_ (#69) "}, {"name": "pmDE5", "desc": "[0.23/14.65]? mu0 {epsilon}_{mu}{delta}_ (#70) "}, {"name": "plx0", "desc": "[-29.58/548.37] SI parallax (#71) "}, {"name": "plx1", "desc": "[-29.58/548.82] LTP parallax (#72) "}, {"name": "plx3", "desc": "[-29.58/549.01] HIP parallax (#73) "}, {"name": "eplx0", "desc": "[0.42/20.8] SI error on parallax (#74) "}, {"name": "eplx1", "desc": "[0.42/20.8] LTP error on parallax (#75) "}, {"name": "eplx3", "desc": "[0.42/20.8] HIP error on parallax (#76) "}, {"name": "da", "desc": "[-325.11/401.93]? {Delta}{alpha}*_sys_ (#77) "}, {"name": "dd", "desc": "[-283.52/228.76]? {Delta}{delta}_sys_ (#78) "}, {"name": "dpa", "desc": "[-11.9/12.21]? {Delta}{mu}_{alpha}*sys_ (#79) "}, {"name": "dpd", "desc": "[-13.57/14.33]? {Delta}{mu}_{delta}sys_ (#80) "}, {"name": "ea", "desc": "[5.63/41.88]? {epsilon}{alpha}*_sys_ (#81) "}, {"name": "ed", "desc": "[5.38/38.07]? {epsilon}{delta}_sys_ (#82) "}, {"name": "epa", "desc": "[0.21/1.82]? {epsilon}{mu}{alpha}*_sys_ (#83) "}, {"name": "epd", "desc": "[0.13/1.9]? {epsilon}{mu}{delta}_sys_ (#84) "}, {"name": "Kpos", "desc": "[1/1]? Flag indicating that the star was used in the comparison of positions in CAT1 and HIP (#85) "}, {"name": "Kpm", "desc": "[1/1]? Flag indicating that the star was used in the comparison of proper motions in CAT1 and HIP (#86) "}, {"name": "F(FH)", "desc": "[0.03/28.32]? F parameter based on the difference Delta_mu_{FH} = mu_F - mu_H between "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"I_288"}} {"id": "I/288", "title_cds": "Low-luminosity members of the Hyades cluster", "title_create": "van Altena, 1966", "year": "1966", "author": "Van Altena W.F.", "title_pub": "Low-luminosity members of the Hyades cluster", "first_author": "Van Altena W.F.", "ref_biblio": [""], "bibcode": ["1966AJ.....71..482V", "1966AJ.....71..482V", "2013yCat.1288....0V"], "keyword_cds": "Clusters, open ; Positional data ;", "keyword_pub": "", "curator": "Francois Ochsenbein [CDS]", "alias": ["VA"], "type": ["OC"], "records": ["778 stars"], "doi_pub": ["10.1086/109952"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"I_301"}} {"id": "I/301", "title_cds": "WDS 2005", "title_create": "Mason+ 2005", "year": "2005", "author": "Brian D. Mason, Gary L. Wycoff, William I. Hartkopf, Geoffrey G. Douglass, Charles E. Worley", "title_pub": "The Washington Visual Double Star Catalog, Version 2005-05-09", "first_author": "Brian D. Mason", "ref_biblio": ["< Astrometry Department, U.S. Naval Observatory >"], "see_also": ["http://ad.usno.navy.mil/wds/ : the WDS home page"], "keyword_cds": "Stars, double and multiple ; Positional data", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["WDS", "WDS\\_2005"], "type": ["GCC"], "records": ["102234 binaries"], "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"I_314"}} {"id": "I/314", "title_cds": "Second Hispano-Argentinian Meridian Catalogue (HAMC2)", "title_create": "HAMC, 2008", "year": "2008", "author": "HAMC", "title_pub": "Second Hispano-Argentinian Meridian Catalogue. Observations from December 1999 to May 2007.", "first_author": "HAMC", "ref_biblio": [""], "keyword_cds": "Meridian observations ; Surveys ; Positional data ; Photometry, CCD", "keyword_pub": "astrometry -- catalogs -- methods: data analysis", "abstract": ["The Brorfelde Schmidt CCD Catalog (BSCC) contains about 13.7 million", "stars, north of +49{deg} Declination with precise positions and V, R", "photometry. The catalog has been constructed from the reductions of", "18,667 CCD frames observed with the Brorfelde Schmidt Telescope", "between 2000 and 2007. The Tycho-2 catalog was used for astrometric", "and photometric reference stars. Errors of individual positions are", "about 20 to 200 mas for stars in the R = 10 to 18 mag range. External", "comparisons with 2MASS and SDSS reveal possible small systematic", "errors in the BSCC of up to about 30 mas. The catalog is supplemented", "with J, H, and Ks magnitudes from the 2MASS catalog."], "description": ["All data are on a single file, formatted (ASCII), sorted by", "declination. Positions are mean, observed positions on the", "International Celestial Reference System (ICRS, as represented by the", "Tycho-2 catalog) at mean epoch of observation. There are no proper", "motions provided in the BSCC. There are 13,771,775 data rows (stars).", "Stars are identified by the IAU registered acronym \"BSCC\", followed by", "a fixed-length, 8-digit running record number without a space, thus", "star names are BSCC00000001 to BSCC13771775."], "curator": "Francois Ochsenbein [CDS]", "alias": ["BSCC"], "type": ["OC"], "records": ["13771775 stars"], "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"I_336"}} {"id": "I/336", "title_cds": "Gaia rehearsal test data", "title_create": "Gaia consortium, 2016", "year": "2016", "author": "Gaia consortium", "title_pub": "Gaia rehearsal test data", "first_author": "Gaia consortium", "ref_biblio": [""], "bibcode": ["2016yCat.1336....0G"], "keyword_cds": "Positional data", "keyword_pub": "catalogs - surveys - astrometry", "mission": "Gaia", "abstract": ["Gaia CU9 rehearsal data. This catalogue provides simulated Gaia data and is", "for testing purposes only."], "alias": ["Gaia test data"], "type": ["OC"], "records": ["1079921303 records"], "data": "", "islargetable": true, "date_update": "01-Sep-2016", "tables": [{"name": "gaia.sam", "desc": "Sample of GaiaSource test data ", "columns": [{"name": "srcId", "desc": "(source_id) "}, {"name": "RAJ2000", "desc": "Right ascension in ICRS at epoch \"ref_epoch\" (ra)"}, {"name": "DEJ2000", "desc": "Declination in ICRS at epoch \"ref_epoch\" (dec)"}, {"name": "solution_id", "desc": "(solution_id) "}, {"name": "random_index", "desc": "? (random_index) "}, {"name": "ref_epoch", "desc": "(ref_epoch) "}, {"name": "e_RAJ2000", "desc": "(ra_error) "}, {"name": "e_DEJ2000", "desc": "(dec_error) "}, {"name": "Plx", "desc": "? (parallax) "}, {"name": "e_Plx", "desc": "? (parallax_error) "}, {"name": "pmRA", "desc": "? Proper motion in right ascension (pmra)"}, {"name": "e_pmRA", "desc": "? Standard error of proper motion in right ascension (pmra_error)"}, {"name": "pmDE", "desc": "? Proper motion in declination (pmdec)"}, {"name": "e_pmDE", "desc": "? Standard error of proper motion in declination (pmdec_error)"}, {"name": "ra_dec_corr", "desc": "? (ra_dec_corr) "}, {"name": "ra_parallax_corr", "desc": "? (ra_parallax_corr) "}, {"name": "ra_pmra_corr", "desc": "? (ra_pmra_corr) "}, {"name": "ra_pmdec_corr", "desc": "? (ra_pmdec_corr) "}, {"name": "dec_parallax_corr", "desc": "? (dec_parallax_corr) "}, {"name": "dec_pmra_corr", "desc": "? (dec_pmra_corr) "}, {"name": "dec_pmdec_corr", "desc": "? (dec_pmdec_corr) "}, {"name": "parallax_pmra_corr", "desc": "? (parallax_pmra_corr) "}, {"name": "parallax_pmdec_corr", "desc": "? (parallax_pmdec_corr) "}, {"name": "pmra_pmdec_corr", "desc": "? (pmra_pmdec_corr) "}, {"name": "astro_n_obs_al", "desc": "? (astrometric_n_obs_ac) "}, {"name": "astro_n_obs_ac", "desc": "? (astrometric_n_obs_al) "}, {"name": "astro_n_outliers_al", "desc": "? (astrometric_n_outliers_al) "}, {"name": "astro_n_outliers_ac", "desc": "? (astrometric_n_outliers_ac) "}, {"name": "astro_chi2_al", "desc": "? (astrometric_chi2_al) "}, {"name": "astro_chi2_ac", "desc": "? (astrometric_chi2_ac) "}, {"name": "astro_xs_noise", "desc": "? (astrometric_excess_noise) "}, {"name": "astro_xs_noise_sig", "desc": "(astrometric_excess_noise_sig) "}, {"name": "astro_params_solved", "desc": "(astrometric_params_solved) "}, {"name": "astro_primary_flag", "desc": "(astrometric_primary_flag) "}, {"name": "astro_rel_factor", "desc": "(astrometric_relegation_factor) "}, {"name": "astro_weight_al", "desc": "? (astrometric_weight_al) "}, {"name": "astro_weight_ac", "desc": "? (astrometric_weight_ac) "}, {"name": "astro_priors_used", "desc": "(astrometric_priors_used) "}, {"name": "matched_obs", "desc": "(matched_observations) "}, {"name": "scan_dir_strength_k1", "desc": "? Mean position angle of scan directions across the source"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"I_41"}} {"id": "I/41", "title_cds": "Catalogue of 964 Stars, Zones +5 to +15", "title_create": "Fayet, 1963", "year": "1963", "author": "Fayet G.", "title_pub": "Etoiles intermediaires (zone +5 a +15deg): catalogue deduit des positions observees a l'aide du cercle meridien de l' Observatoire de Nice de 1912 a 1914", "first_author": "Fayet G.", "ref_biblio": [""], "keyword_cds": "Positional data", "description": ["This catalog contains meridian circle positions for 4 to 6 stars in", "each hour of right ascension, between the eighth and ninth magnitude,", "and in the declination range +5 deg. to +15 deg. The equinox of the", "positions is 1910.0. Mean errors in right ascension range from 0.025s", "to 0.30s. Those in declination range from 0.47\" to 0.58\". The catalog", "also contains a running number, the magnitude, from the \"Henry Draper", "Catalog\" when available, annual precession and secular variation, and", "the number of observations and their mean date. Proper motions have", "not been included in the reduction of the positions."], "records": ["964 stars"], "data": "", "date_update": "21-Jan-2019", "tables": [{"name": "data_01.dat", "desc": "Data ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"II_254"}} {"id": "II/254", "title_cds": "Minnesota Automated Plate Scanner catalog", "title_create": "Cabanela+ 2003", "year": "2003", "author": "Cabanela J.E., Humphreys R.M., Aldering G., Larsen J.A., Odewahn S.C., Thurmes P.M., Cornuelle C.S.", "title_pub": "The Minnesota Automated Plate Scanner catalog of the POSS I (MAPS)", "first_author": "Cabanela J.E.", "ref_biblio": [""], "bibcode": ["2003PASP..115..837C"], "see_also": ["http://iparrizar.stcloudstate.edu/~juan/MAPS_Database/catalog/"], "keyword_cds": "Surveys ; Photometry, photographic ; Photometry, surface", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["MAPS"], "records": ["records"], "doi_pub": ["10.1086/375625"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"II_268"}} {"id": "II/268", "title_cds": "The 2dF QSO Redshift Survey Input Catalogue", "title_create": "Smith+ 2005", "year": "2005", "author": "Smith R.J., Croom S.M., Boyle B.J., Shanks T., Miller L., Loaring N.S.", "title_pub": "The 2dF QSO Redshift Survey - III. The Input Catalogue", "first_author": "Smith R.J.", "ref_biblio": [""], "see_also": ["http://www.2dfquasar.org/Phot_Cat/ubrcatalogue.html"], "keyword_cds": "Photometry, photographic ; Survey", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["2dF"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "04-Jun-2006"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"II_279"}} {"id": "II/279", "title_cds": "EROS-II in the Magellanic Clouds", "title_create": "Marquette+ 2007", "year": "2007", "author": "Marquette J.B., Lesquoy E., (EROS collaboration)", "title_pub": "Final photometric catalog of EROS-II in the Magellanic Clouds", "first_author": "Marquette J.B.", "ref_biblio": ["< Astron. Astrophys. (in press) >"], "keyword_cds": "Magellanic Clouds ; Surveys ; Photometry, CCD ; Stars, variable", "keyword_pub": "(A&A )", "alias": ["EROS2"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "08-Jun-2007", "tables": [{"name": "fields.dat", "desc": "Limits in the EROS-II fields ", "columns": [{"name": "Field", "desc": "Name of field, starting by \"lm\" or \"sm\" for Large and Small Magellanic cloud respectively."}, {"name": "RAmin", "desc": "Lower limit of RA (J2000) in Field "}, {"name": "RAmax", "desc": "Upper limit of RA (J2000) in Field "}, {"name": "DEmin", "desc": "Lower limit of Dec (J2000) in Field "}, {"name": "DEmax", "desc": "Upper limit of Dec (J2000) in Field "}]}, {"name": "CAT/*/*.dat", "desc": "Field files with a total of 32,687,748 stars ", "columns": [{"name": "EROSid", "desc": "EROS identification (1) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Rmag", "desc": "Red magnitude (filter?) "}, {"name": "e_Rmag", "desc": "Mean error on Rmag "}, {"name": "Rx", "desc": "X position in red observation "}, {"name": "Ry", "desc": "Y position in red observation "}, {"name": "Bmag", "desc": "Blue magnitude (filter?) "}, {"name": "e_Bmag", "desc": "Mean error on Bmag "}, {"name": "Bx", "desc": "X position in blue observation "}, {"name": "By", "desc": "Y position in blue observation "}, {"name": "Var", "desc": "[0,511] Variability flags (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"II_291"}} {"id": "II/291", "title_cds": "Third Photometric Magnitude Difference Catalog", "title_create": "Mason, 2008", "year": "2008", "author": "Worley C.E., Mason B.D., Wycoff G.L.", "title_pub": "Third Photometric Magnitude Difference Catalog", "first_author": "Worley C.E.", "ref_biblio": [""], "see_also": ["http://ad.usno.navy.mil/wds/dm3.html : the Magnitude Difference Catalog", "B/wds : Washington Double Star Catalog (WDS)"], "keyword_cds": "Stars, double and multiple ; Photometry", "keyword_pub": "Binaries: General, Stars: Binaries: Visual, Catalogs", "description": ["The Photometric Magnitude Difference Catalog is a collection of all", "double star photometric data which does not contain astrometric", "information and is therefore inappropriate for the Washington Double", "Star Catalog. Magnitude difference information can be useful in", "estimating mass ratios, determining photocentric positions which are", "color dependent, or into investigations of variability in close binary", "systems. Due to uncertainties in bandpass characteristics or", "variability, no summary line is presented, rather a complete listing", "of all data.", "This version supersedes the"], "type": ["BCC"], "records": ["45445 binaries"], "data": "", "date_update": "12-Aug-2012", "tables": [{"name": "deltam.dat", "desc": "Delta-M Catalog ", "columns": [{"name": "RAh", "desc": "*Right Ascension 2000 (hours) "}, {"name": "RAdm", "desc": "*Right Ascension 2000 (minutes) "}, {"name": "DE-", "desc": "*Declination 2000 (sign) "}, {"name": "DEd", "desc": "*Declination 2000 (degrees) "}, {"name": "DEm", "desc": "*Declination 2000 (minutes) "}, {"name": "DiscName", "desc": "*Discoverer Code & Number "}, {"name": "Comp", "desc": "*Component Identification "}, {"name": "dm", "desc": "Magnitude Difference "}, {"name": "o_dm", "desc": "?Number of observations used to compute dm"}, {"name": "r_dm", "desc": "*Reference Code "}, {"name": "Meth", "desc": "*Observational Method "}, {"name": "Notes", "desc": "*?Notes "}]}, {"name": "dm.txt", "desc": "Delta-M Catalog Documentation ", "columns": []}, {"name": "table1.txt", "desc": "ascii version of Table 1 ", "columns": []}, {"name": "method.txt", "desc": "method key for deltam.dat ", "columns": []}, {"name": "refs.dat", "desc": "Reference file ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"II_302"}} {"id": "II/302", "title_cds": "The SWIRE Data Release 2", "title_create": "Surace+ 2005", "year": "2005", "author": "Surace et al.", "title_pub": "The Spitzer Wide-area InfraRed Extragalactic survey (SWIRE) Data Release 2", "first_author": "Surace et al.", "ref_biblio": ["< Caltech, 2005 >"], "bibcode": ["2012yCat.2302....0S"], "see_also": ["http://irsa.ipac.caltech.edu/data/SPITZER/SWIRE/ : SWIRE Home page", "II/290 : SWIRE Photometric Redshift Catalogue (Rowan-Robinson+, 2008)"], "keyword_cds": "Surveys ; Galaxies, IR ; Galaxies, photometry", "mission": "Spitzer", "description": ["The Spitzer Wide-area InfraRed Extragalactic Survey (SWIRE) is a", "wide-area, high galactic latitude, imaging survey to trace the", "evolution of dusty, star-forming galaxies, evolved stellar", "populations, and active galactic nuclei. SWIRE has surveyed roughly 50", "square degrees with the MIPS far-infrared camera and the with the IRAC", "mid-infrared camera. The regions included are ELAIS-N1, ELAIS-N2,", "XMM-LSS, the Lockman Hole (LH), ELAIS-S1 and Chandra Deep Field South", "(CDFS)."], "curator": "Francois Ochsenbein [CDS]", "alias": ["SWIRE-2", "SWIRE"], "records": ["records"], "data": "", "date_update": "12-Dec-2012"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"II_304"}} {"id": "II/304", "title_cds": "UKIDSS-DR5", "title_create": "Lawrence+ 2011", "year": "2011", "author": "UKIDSS Consortium", "title_pub": "UKIRT Infrred Deep Sky Survey (UKIDSS) Release 5", "first_author": "UKIDSS Consortium", "ref_biblio": [""], "bibcode": ["2007MNRAS.379.1599L", "2011yCat.2304....0U"], "see_also": ["http://www.ukidss.org/ : UKIDSS Home page"], "keyword_cds": "Surveys ; Infrared sources ; Photometry, infrared", "keyword_pub": "surveys - infrared: general", "description": ["The UKIRT Infrared Deep Sky Survey (UKIDSS) can be considered the", "near-infrared (near-IR) counterpart of the Sloan Digital Sky Survey", "(SDSS; see Cat. II/294). It does not cover the whole sky, but is many", "times deeper than the Two-Micron All-Sky Survey (2MASS, see Cat.", "II/246; Skrutskie et al. 2006AJ....131.1163S). It is in fact not a", "single survey but a survey programme combining a set of five survey", "components of complementary combinations of depth and area, covering", "several thousand square degrees to K~18, 35deg^2^ to K~21, and", "0.77deg^2^ to K~23. The survey uses the Wide Field Camera (WFCAM) on", "the 3.8m United Kingdom Infra-Red Telescope (UKIRT). WFCAM has an", "instantaneous field of view of 0.21 deg^2^, considerably larger than", "any previous IR camera on a 4-m class telescope, along with a pixel", "size of 0.4arcsec. The tip-tilt system on UKIRT delivers close to", "natural seeing (median size 0.6 arcsec) across the whole field of", "view. The combination of large telescope, large field of view, and", "good image quality, makes possible a survey of considerably greater", "scope than that of 2MASS. The various surveys employ up to five", "filters ZYJHK covering the wavelength range 0.83\u00ad2.37{mu}m and extend", "over both high and low Galactic latitudes. The survey began on 2005", "May 13, and is expected to take 7yr to complete. The survey is being", "carried out by a private consortium but is fully public with no", "proprietary rights for the consortium. Data products are being being", "released in stages, with the intention of having these roughly twice", "a year."], "curator": "Francois Ochsenbein [CDS]", "alias": ["UKIDSS-DR5", "UKIDSS"], "type": ["OC"], "records": ["47230108 sources"], "doi_pub": ["10.1111/j.1365-2966.2007.12040.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"II_352"}} {"id": "II/352", "title_cds": "The VISTA Hemisphere Survey (VHS) catalog", "title_create": "McMahon+, 2013", "year": "2013", "author": "McMahon, R. G., Banerji, M., Gonzalez, E., Koposov, S. E., Bejar, V. J., Lodieu, N., Rebolo, R., The VHS Collaboration", "title_pub": "VISTA Hemisphere Survey band-merged multi-waveband catalogues (VHS)", "first_author": "McMahon", "ref_biblio": [""], "bibcode": ["2013Msngr.154...35M", "2017yCat.2352....0M"], "see_also": ["http://www.vista-vhs.org/ : VHS home page", "http://horus.roe.ac.uk/vsa/ : VISTA Science Archive home page"], "keyword_cds": "Photometry, infrared ; Surveys", "mission": "ESO", "abstract": ["The first Galactic and extragalactic results from the VISTA Hemisphere", "Survey (VHS) are presented. The aim of the VHS is to carry out a", "near-infrared survey which, when combined with other VISTA public", "surveys, will result in coverage of the whole southern celestial", "hemisphere (~20000deg^2^) to a depth 30 times fainter than the Two", "Micron All Sky Survey in at least two wavebands (J and Ks). The VHS", "vision includes a deep optical survey over the same area and this is", "now being realised with the VST surveys and the Dark Energy Survey,", "which has recently started. A summary of the survey progress is", "presented, with some follow-up results on low-mass stars and", "high-redshift quasars."], "description": ["Observations were made with the VIRCAM instrument on the ESO-VISTA", "telescope between 2009 November and 2013 October in Y, J, H and Ks", "filters."], "ack": ["Please include the following acknowledgment in any published material", "that makes use of the VHS products: Based on observations made with", "ESO Telescopes at the La Silla or Paranal Observatories under", "programme ID 179.A-2010"], "alias": ["VHS"], "type": ["OC"], "records": ["590835393 records"], "orcid_pub": ["0000-0001-8447-8869", "0000-0001-8447-8869"], "data": "", "islargetable": true, "date_creation": "21-Nov-2017", "date_update": "25-Feb-2021", "tables": [{"name": "vhs_dr3.sam", "desc": "VISTA Hemisphere Survey band-merged multi-waveband catalogues (VHS) DR3; sample output (on a total of 590,835,393 sources)", "columns": [{"name": "SrcID", "desc": "[472446402561/473037940311] Unique ID of this merged detection as assigned by merge algorithm (SOURCEID)"}, {"name": "RAdeg", "desc": "Celestial Right Ascension; J2000 (RA2000) "}, {"name": "DEdeg", "desc": "Celestial Declination; J2000 (DEC2000) "}, {"name": "Name", "desc": "Source name in IAU convention (SOURCENAME) "}, {"name": "CuID", "desc": "[451771] Unique ID of curation event giving rise to this record (always \"451771\") (CUEVENTID)"}, {"name": "FrID", "desc": "Unique ID of the set of frames that this merged source comes from (FRAMESETID)"}, {"name": "GLON", "desc": "Galactic longitude (L) "}, {"name": "GLAT", "desc": "Galactic latitude (B) "}, {"name": "priOrSec", "desc": "Seam code for a unique (=0) or duplicated (!=0) source (PRIORSEC)"}, {"name": "Y-Jpnt", "desc": "[-13/9]? Point source colour Y-J (using aperMag3) (YMJPNT)"}, {"name": "e_Y-Jpnt", "desc": "[/5999]? Error on Y-Jpnt (YMJPNTERR) "}, {"name": "J-Hpnt", "desc": "[-12/10]? Point source colour J-H (using aperMag3) (JMHPNT)"}, {"name": "e_J-Hpnt", "desc": "[/744]? Error on J-Hpnt (JMHPNTERR) "}, {"name": "H-Kspnt", "desc": "[-11/12]? Point source colour H-Ks (using aperMag3) (HMKSPNT)"}, {"name": "e_H-Kspnt", "desc": "[/627]? Error on H-Kspnt (HMKSPNTERR) "}, {"name": "J-Kspnt", "desc": "[-12/22]? Point source colour J-Ks (using aperMag3) (JMKSPNT)"}, {"name": "e_J-Kspnt", "desc": "[/13621]? Error on J-Kspnt (JMKSPNTERR) "}, {"name": "Y-Jext", "desc": "[-12/9]? Extended source colour Y-J (using aperMagNoAperCorr3) (YMJEXT)"}, {"name": "e_Y-Jext", "desc": "[/5999]? Error on Y-Jext (YMJEXTERR) "}, {"name": "J-Hext", "desc": "[-12/10]? Extended source colour J-H (using aperMagNoAperCorr3) (JMHEXT)"}, {"name": "e_J-Hext", "desc": "[/744]? Error on J-Hext (JMHEXTERR) "}, {"name": "H-Ksext", "desc": "[-11/12]? Extended source colour H-Ks (using aperMagNoAperCorr3) (HMKSEXT)"}, {"name": "e_H-Ksext", "desc": "[/627]? Error on H-Ksext (HMKSEXTERR) "}, {"name": "J-Ksext", "desc": "[-12/23]? Extended source colour J-Ks (using aperMagNoAperCorr3) (JMKSEXT)"}, {"name": "e_J-Ksext", "desc": "[/13621]? Error on J-Ksext (JMKSEXTERR) "}, {"name": "Clst", "desc": "Merged N(0,1) stellarness-of-profile statistic (MERGEDCLASSSTAT)"}, {"name": "Cl", "desc": "[-3/1] Class flag (MERGEDCLASS) (1) "}, {"name": "pStar", "desc": "Probability that the source is a star (PSTAR) "}, {"name": "pGal", "desc": "Probability that the source is a galaxy (PGALAXY) "}, {"name": "pNoise", "desc": "Probability that the source is noise (PNOISE) "}, {"name": "E(B-V)", "desc": "[0.001/8] The galactic dust extinction value measured from the Schlegel maps (EBV)"}, {"name": "AY", "desc": "[0.001/11] The galactic extinction correction in the Y band (AY)"}, {"name": "AJ", "desc": "[0.001/8] The galactic extinction correction in the J band (AJ)"}, {"name": "AH", "desc": "[/5] The galactic extinction correction in the H band (AH)"}, {"name": "AKs", "desc": "[/4] The galactic extinction correction in the Ks band (AKS)"}, {"name": "Ypmag", "desc": "[4/35]? Extended source VISTA Y mag (Petrosian) (YPETROMAG)"}, {"name": "e_Ypmag", "desc": "[0/255661]? Error in Ypmag (YPETROMAGERR) "}, {"name": "Yap3", "desc": "[4/34]? Default point source Y aperture corrected mag (2.0 arcsec diam) (YAPERMAG3)"}, {"name": "e_Yap3", "desc": "[/63914]? Error in default point/extended source Y mag (YAPERMAG3ERR)"}, {"name": "Yap4", "desc": "[4/34]? Point source Y aperture corrected mag (2.8 arcsec aperture diam) (YAPERMAG4)"}, {"name": "e_Yap4", "desc": "[/63442]? Error in point/extended source Y mag (2.8 arcsec aperture diam) (YAPERMAG4ERR)"}, {"name": "Yap6", "desc": "[3/38]? Point source Y aperture corrected mag (5.7 arcsec aperture diam) (YAPERMAG6)"}, {"name": "e_Yap6", "desc": "[/2719583]? Error in point/extended source Y mag (5.7 arcsec aperture diam) (YAPERMAG6ERR)"}, {"name": "Yapc3", "desc": "[4/35]? Default extended source Y aperture mag (2.0 arcsec diam) (YAPERMAGNOAPERCORR3)"}, {"name": "Yapc4", "desc": "[4/35]? Extended source Y aperture mag (2.8\" aperture diameter) (YAPERMAGNOAPERCORR4)"}, {"name": "Yapc6", "desc": "[3/38]? Extended source Y aperture mag (5.7\" aperture diameter) (YAPERMAGNOAPERCORR6)"}, {"name": "Yamaj", "desc": "[0/19]? Seeing corrected half-light, semi-major axis in Y band (YHLCORSMJRADAS)"}, {"name": "Yrms", "desc": "[0.7/303]? RMS of axes of ellipse fit in Y (YGAUSIG)"}, {"name": "Yell", "desc": "? 1-b/a, where a/b=semi-major/minor axes in Y (YELL)"}, {"name": "YPA", "desc": "? Ellipse fit celestial orientation in Y (YPA) "}, {"name": "Yerrb", "desc": "[/28] Processing warning/error bitwise flags in Y (YERRBITS)"}, {"name": "Yavg", "desc": "[0/112]? Average confidence in 2 arcsec diam default aperture 3 Y-band (YAVERAGECONF)"}, {"name": "YCl", "desc": "[/1] Discrete image classification flag in Y (YCLASS) (1)"}, {"name": "YClst", "desc": "[-109/444]? N(0,1) stellarness-of-profile statistic in Y (YCLASSSTAT)"}, {"name": "Yperrb", "desc": "[0/12587216] Additional Wide Field Astronomy Unit (WFAU) post-processing error bits in Y (<256: minor issues) (YPPERRBITS) (2)"}, {"name": "Yseq", "desc": "[/110314] The running number of the Y detection (YSEQNUM)"}, {"name": "Jpmag", "desc": "[-24/]? Extended source VISTA J mag (Petrosian) (JPETROMAG)"}, {"name": "e_Jpmag", "desc": "[0/]? Error in Jpmag (JPETROMAGERR) "}, {"name": "Jap3", "desc": "[-22/35]? Default point source J aperture corrected mag (2.0 arcsec diam) (JAPERMAG3)"}, {"name": "e_Jap3", "desc": "[0/76220]? Error in Jap3 (JAPERMAG3ERR) "}, {"name": "Jap4", "desc": "[-22/36]? Point source J aperture corrected mag (2.8 arcsec aperture diam) (JAPERMAG4)"}, {"name": "e_Jap4", "desc": "[0/1565601]? Error in Jap4 (JAPERMAG4ERR) "}, {"name": "Jap6", "desc": "[-22/38]? Point source J aperture corrected mag (5.7 arcsec aperture diam) (JAPERMAG6)"}, {"name": "e_Jap6", "desc": "[0/8556921]? Error in Jap6 (JAPERMAG6ERR) "}, {"name": "Japc3", "desc": "[-21/35]? Default extended source J aperture mag (2.0 arcsec diam) (JAPERMAGNOAPERCORR3)"}, {"name": "Japc4", "desc": "[-22/37]? Extended source J aperture mag (2.8\" aperture diameter) (JAPERMAGNOAPERCORR4)"}, {"name": "Japc6", "desc": "[-22/38]? Extended source J aperture mag (5.7\" aperture diameter) (JAPERMAGNOAPERCORR6)"}, {"name": "Jamaj", "desc": "[0/19]? Seeing corrected half-light, semi-major axis in J band (JHLCORSMJRADAS)"}, {"name": "Jrms", "desc": "[0.7/584]? RMS of axes of ellipse fit in J (JGAUSIG)"}, {"name": "Jell", "desc": "? 1-b/a, where a/b=semi-major/minor axes in J (JELL)"}, {"name": "JPA", "desc": "? Ellipse fit celestial orientation in J "}, {"name": "Jerrb", "desc": "[/28] Processing warning/error bitwise flags in J (JERRBITS)"}, {"name": "Javg", "desc": "[0/112]? Average confidence in 2 arcsec diam default aperture 3 J-band (JAVERAGECONF)"}, {"name": "JCl", "desc": "[/1] Discrete image classification flag in J (JCLASS) (1)"}, {"name": "JClst", "desc": "[-310/445]? N(0,1) stellarness-of-profile statistic in J (JCLASSSTAT)"}, {"name": "Jperrb", "desc": "[0/12587216] Additional WFAU post-processing error bits in J (<256: minor issues) (JPPERRBITS) (2)"}, {"name": "Jseq", "desc": "[/1661208] The running number of the J detection (JSEQNUM)"}, {"name": "Jxi", "desc": "? Offset of J detection from Y master position (+east/-west) (JXI)"}, {"name": "Jeta", "desc": "? Offset of J detection from Y master position (+north/-south) (JETA)"}, {"name": "Hpmag", "desc": "[-24/36]? Extended source VISTA H mag (Petrosian) (HPETROMAG)"}, {"name": "e_Hpmag", "desc": "[0/2056313]? Error in Hpmag (HPETROMAGERR) "}, {"name": "Hap3", "desc": "[-22/29]? Default point source H aperture corrected mag (2.0 arcsec diam) (HAPERMAG3)"}, {"name": "e_Hap3", "desc": "[0/2609]? Error in Hap3 (HAPERMAG3ERR) "}, {"name": "Hap4", "desc": "[-22/31]? Point source H aperture corrected mag (2.8 arcsec aperture diam) (HAPERMAG4)"}, {"name": "e_Hap4", "desc": "[0/15921]? Error in Hap4 (HAPERMAG4ERR) "}, {"name": "Hap6", "desc": "[-23/35]? Point source H aperture corrected mag (5.7 arcsec aperture diam) (HAPERMAG6)"}, {"name": "e_Hap6", "desc": "[0/737931]? Error in Hap6 (HAPERMAG6ERR) "}, {"name": "Hapc3", "desc": "[-21/30]? Default extended source H aperture mag (2.0 arcsec diam) (HAPERMAGNOAPERCORR3)"}, {"name": "Hapc4", "desc": "[-22/31]? Extended source H aperture mag (2.8\" aperture diameter) (HAPERMAGNOAPERCORR4)"}, {"name": "Hapc6", "desc": "[-23/35]? Extended source H aperture mag (5.7\" aperture diameter) (HAPERMAGNOAPERCORR6)"}, {"name": "Hamaj", "desc": "[0/19]? Seeing corrected half-light, semi-major axis in H band (HHLCORSMJRADAS)"}, {"name": "Hrms", "desc": "[0.7/584]? RMS of axes of ellipse fit in H (HGAUSIG)"}, {"name": "Hell", "desc": "? 1-b/a, where a/b=semi-major/minor axes in H (HELL)"}, {"name": "HPA", "desc": "? Ellipse fit celestial orientation in H (HPA) "}, {"name": "Herrb", "desc": "[/28] Processing warning/error bitwise flags in H (HERRBITS)"}, {"name": "Havg", "desc": "[0/112]? Average confidence in 2 arcsec diam default aperture 3 H (HAVERAGECONF)"}, {"name": "HCl", "desc": "[/1] Discrete image classification flag in H (HCLASS) (1)"}, {"name": "HClst", "desc": "[-96/383]? N(0,1) stellarness-of-profile statistic in H (HCLASSSTAT)"}, {"name": "Hperrb", "desc": "[0/12587216] Additional WFAU post-processing error bits in H (<256: minor issues) (HPPERRBITS) (2)"}, {"name": "Hseq", "desc": "[/125514] The running number of the H detection (HSEQNUM)"}, {"name": "Hxi", "desc": "? Offset of H detection from Y master position (+east/-west) (HXI)"}, {"name": "Heta", "desc": "? Offset of H detection from Y master position (+north/-south) (HETA)"}, {"name": "Kspmag", "desc": "[-20/]? Extended source VISTA Ks mag (Petrosian) (KSPETROMAG)"}, {"name": "e_Kspmag", "desc": "[0/]? Error in Kspmag (KSPETROMAGERR) "}, {"name": "Ksap3", "desc": "[-34/28]? Default point source Ks aperture corrected mag (2.0 arcsec diam) (KSAPERMAG3)"}, {"name": "e_Ksap3", "desc": "[0/2186]? Error Ksap3 (KSAPERMAG3ERR) "}, {"name": "Ksap4", "desc": "[-34/36]? Point source Ks aperture corrected mag (2.8 arcsec aperture diam) (KSAPERMAG4)"}, {"name": "e_Ksap4", "desc": "[0/3715233]? Error in Ksap4 (KSAPERMAG4ERR) "}, {"name": "Ksap6", "desc": "[-34/37]? Point source Ks aperture corrected mag (5.7 arcsec aperture diam) (KSAPERMAG6)"}, {"name": "e_Ksap6", "desc": "[0/]? Error in Ksap6 (KSAPERMAG6ERR) "}, {"name": "Ksapc3", "desc": "[-34/28]? Default extended source Ks aperture mag (2.0 arcsec diam) (KSAPERMAGNOAPERCORR3)"}, {"name": "Ksapc4", "desc": "[-34/36]? Extended source Ks aperture mag (2.8\" aperture diameter) (KSAPERMAGNOAPERCORR4)"}, {"name": "Ksapc6", "desc": "[-34/37]? Extended source Ks aperture mag (5.7\" aperture diameter) (KSAPERMAGNOAPERCORR6)"}, {"name": "Kamaj", "desc": "[0/19]? Seeing corrected half-light, semi-major axis in Ks band (KSHLCORSMJRADAS)"}, {"name": "Ksrms", "desc": "[0.7/549]? RMS of axes of ellipse fit in Ks (KSGAUSIG)"}, {"name": "Ksell", "desc": "? 1-b/a, where a/b=semi-major/minor axes in Ks (KSELL)"}, {"name": "KsPA", "desc": "? Ellipse fit celestial orientation in Ks (KSPA) "}, {"name": "Kserrb", "desc": "[/24] Processing warning/error bitwise flags in Ks (KSERRBITS)"}, {"name": "Ksavg", "desc": "[0/112]? Average confidence in 2 arcsec diam default aperture 3 Ks-band (KSAVERAGECONF)"}, {"name": "KsCl", "desc": "[/1] Discrete image classification flag in Ks (KSCLASS) (1)"}, {"name": "KsClst", "desc": "[-108/385]? N(0,1) stellarness-of-profile statistic in Ks (KSCLASSSTAT)"}, {"name": "Ksperrb", "desc": "[0/12587216] Additional WFAU post-processing error bits in Ks (<256: minor issues) (KSPPERRBITS) (2)"}, {"name": "Ksseq", "desc": "[/1455550] The running number of the Ks detection (KSSEQNUM)"}, {"name": "Ksxi", "desc": "? Offset of Ks detection from Y master position (+east/-west) (KSXI)"}, {"name": "Kseta", "desc": "? Offset of Ks detection from Y master position (+north/-south) (KSETA)"}, {"name": "Prim", "desc": "[0/1] Flag indicates primary sources (=1), otherwise (=0) (PRIMARY_SOURCE)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"II_71"}} {"id": "II/71", "title_cds": "Merged Infrared Catalog, first Edition", "title_create": "Schmitz+ 1978", "year": "1978", "author": "Schmitz M., Brown L.W., Mead J.M., Nagy T.A.", "title_pub": "Merged Infrared Catalog, First Edition", "first_author": "Schmitz M.", "ref_biblio": [""], "see_also": ["II/184 : Catalog of Infrared observations, 3rd Edition (Gezari+ 1993)"], "description": ["A compilation of equatorlal coordinates, spectral types, magnitudes,", "and fluxes from five catalogues of infrared [IR] observations is", "presented. This first edition of the Merged InFrared Catalogue [MIRC]", "contains 11,201 observations from a) the Two-Micron Sky Survey (TMSS)", "b) Observations of Infrared Radiation from Cool Stars (GMS), c) the", "Air Force Geophysics Laboratory Four Color Infrared Sky Survey (AFGL),", "and d) Supplemental Catalog (AFGL S), and e) A Catalog of 10um", "Celestial Objects (HALL). This compilation is a by-product of a", "computerized infrared data base under development at Goddard Space", "Flight Center; the objective is to maintain a complete and current", "record of all infrared observations from 1um to 10um of non-solar", "system objects. These observations are being placed into a", "standardized system. Periodically, updated editions of MIRC will be", "produced as additional catalogues are m erged into the IR data base."], "curator": "Francois Ochsenbein [CDS]", "records": ["11201 records"], "data": "", "date_update": "06-May-2004"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"II_76A"}} {"id": "II/76A", "title_cds": "O star catalogue, 4th Ed.", "title_create": "Goy 1980", "year": "1980", "author": "GOY G.", "title_pub": "Catalogue general d'etoiles de type O (O Star Catalogue, 4th Edition)", "first_author": "GOY G.", "ref_biblio": [""], "bibcode": ["1980A&AS...42...91G"], "curator": "Francois Ochsenbein [CDS]", "records": ["971 stars"], "data": "", "date_update": "04-Jul-1995"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_220"}} {"id": "III/220", "title_cds": "30 Dor spectral types and UBV magnitudes", "title_create": "Schild+, 1998", "year": "1998", "author": "Schild H., Testor G.", "title_pub": "Spectral types and UBV magnitudes of stars in the 30 Doradus complex", "first_author": "Schild H.", "ref_biblio": ["< 92, 729 (1992); 130, 527 (1998) >"], "keyword_cds": "Magellanic Clouds ; MK spectral classification; Photometry, UBV", "keyword_pub": "", "abstract": ["Photometric and spectroscopic observations are described for stars in", "four selected areas in the periphery of the 30 Doradus region. The", "areas are located at distances ranging from 7 to 20 arcmin from the", "central cluster. UBV magnitudes and spectral types for more than 250", "stars are presented. A total of 70 new O stars is reported, most of", "which are located in the two inner regions. Photometric and", "spectroscopic data are given of the Wolf-Rayet stars in the surveyed", "fields. For WR stars in tight clusters, spatially resolved photometry", "is given. A carbon star is also identified."], "curator": "Francois Ochsenbein [CDS]", "alias": ["[ST92]"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "04-Jul-2017"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_241"}} {"id": "III/241", "title_cds": "Spectroscopy of SDSS Data Release 3 (SDSS-DR3)", "title_create": "ARC, 2005", "year": "2005", "author": "Astrophysical Research Consortium (ARC)", "title_pub": "The Sloan Digital Sky Survey Data Release 3 (SDSS-DR3): Spectroscopy", "first_author": "Astrophysical Research Consortium (ARC)", "ref_biblio": [""], "keyword_cds": "Spectroscopy ; Redshifts; Surveys ; Velocity dispersion", "keyword_pub": "", "description": ["The Sloan Digital Sky Survey", "The descrition of the Second Data Release has been published by Abazajian", "et al. (2004AJ....128..502A)", "The Data Release 3 (DR3) spectroscopic data result from 826 plates", "of 640 spectra each, and cover 4188 square degrees", "The technical aspects are described by York D.G., Adelman J.,", "Anderson J.E., et al. (2000AJ....120.1579Y)", "Details at http://www.astro.psu.edu/users/dps/sdsstechrefs.html"], "ack": ["Refer to the SDSS pages at", "http://www.sdss.org/collaboration/credits.html", "Data from the SDSS public archive may not be used for any commercial", "publication or other commercial purpose except with explicit approval", "by the Astrophysical Research Consortium (ARC).", "Non-commercial scientific and technical publications using SDSS data", "should include the acknowledgment detailed at", "http://www.sdss.org/collaboration/credits.html"], "curator": "Francois Ochsenbein [CDS]", "alias": ["SDSS-DR3", "SDSS"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "26-May-2005"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_234"}} {"id": "III/234", "title_cds": "Distribution of stars in Carrington zone", "title_create": "Petersson, 1927", "year": "1927", "author": "Petersson J.H.", "title_pub": "Coordinates and identifications for north polar stars observed spectrophotometrically by Petersson", "first_author": "Petersson J.H.", "ref_biblio": [""], "bibcode": ["1927MeUpp..29....1P"], "see_also": ["III/233 : Catalogue of Stellar Spectral Classifications (Skiff, 2005)"], "keyword_cds": "Spectral types", "keyword_pub": "", "records": ["2007 stars"], "data": "", "date_update": "16-Mar-2006", "tables": [{"name": "catalog.dat", "desc": "Spectral Types by Petersson ", "columns": [{"name": "n_Name", "desc": "[*] Individual notes (1) "}, {"name": "Name", "desc": "Star name (BD or AC) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "rPos", "desc": "[TM] Source of prosition "}, {"name": "Vmag", "desc": "Visual magnitude "}, {"name": "SpType", "desc": "MK spectral type "}, {"name": "Note", "desc": "Remark (by Brian Skiff) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_247"}} {"id": "III/247", "title_cds": "Proven and probable members in the SMC", "title_create": "Sanduleak, 1968-1975", "year": "1975", "author": "Sanduleak N.", "title_pub": "Proven and probable members in the Small Magellanic Cloud", "first_author": "Sanduleak N.", "ref_biblio": ["< Astron. J. 73, 246 (1968); 74, 877 (1969); Astron. Astrophys. 39, 461 (1975) >"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["Sk"], "records": ["records"], "data": "", "date_update": "12-Jan-2007"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_236"}} {"id": "III/236", "title_cds": "Faint stars in two regions of the Milky Way", "title_create": "Apriamashivili, 1964", "year": "1964", "author": "Apriamashivili S.P.", "title_pub": "The catalogue of photographic magnitudes, color-indices, spectra, and", "first_author": "Apriamashivili S.P.", "ref_biblio": [""], "bibcode": ["1964AbaOB..31...27A"], "keyword_cds": "Magnitudes, photographic ; Colors ; Spectral types ; Milky Way", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "type": ["OC"], "records": ["records"], "data": "", "date_update": "12-Aug-2003"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_11"}} {"id": "III/11A", "title_cds": "F2 and earlier stars in SA28, 54, 106, 107", "title_create": "Upgren, Staron 1969", "year": "1969", "author": "Upgren Jr. A.R., Staron R.T.", "title_pub": "F2 and Earlier Stars in S.A. 28, 54, 106, 107", "first_author": "Upgren Jr. A.R.", "ref_biblio": [""], "bibcode": ["1969ApJ...157..327U"], "keyword_cds": "Selected areas", "description": ["The catalog contains the results of an objective-prism survey for", "498 stars of spectral classes F2 and earlier, brighter than", "magnitude 11.5, in four regions of intermediate galactic latitude.", "This objective-prism survey is part of a study of stellar densities", "aiming at the determination of the inclination to the galactic plane", "of surfaces of equal stellar density. Each region is centered on one", "of the Selected Areas 28, 54, 106, and 107. The fields, 4 x 4", "degrees in size, were each photographed on two IIa-O emulsion", "plates, one with an exposure time of three minutes on which bright", "stars could be classified and one with an exposure time of 40", "minutes extending to faint stars. The plates were taken with the", "24-inch Baker-Schmidt telescope of the Dyer Observatory. The", "dispersion of the objective prism is about 330 A/mm at H-gamma. The", "stars were classified according to the criteria established by", "Nassau and Seyfert (1946) and Nassau and van Albada (1947).", "Photographic magnitudes were found from direct IIa-O plates taken", "with the eight-inch Ross camera of the Yale Observatory. The", "catalog includes BD numbers, magnitudes, and spectral classes for BD", "stars. For non BD stars, the BD number listed in column (1)", "indicates a nearby BD star from which the star listed is offset, as", "indicated by the data of columns (2) and (3)."], "date_update": "26-Feb-2016", "tables": [{"name": "bdstars.dat", "desc": "BD stars catalog data ", "columns": [{"name": "Sarea", "desc": "Selected Area number "}, {"name": "BD", "desc": "BD number "}, {"name": "Photomag", "desc": "Photographic magnitude "}, {"name": "Sp", "desc": "Spectral type "}, {"name": "u_Sp", "desc": "uncertainty in Sp "}]}, {"name": "nonbd.dat", "desc": "Non-BD stars ", "columns": [{"name": "Sarea", "desc": "Selected Area number "}, {"name": "BD", "desc": "BD number of nearby star "}, {"name": "RAoffset", "desc": "Right ascension offset from BD star given in bytes 5-12, minutes of arc"}, {"name": "DEoffset", "desc": "Declination offset from BD star given in bytes 5-12, minutes of arc"}, {"name": "Photomag", "desc": "Photographic magnitude "}, {"name": "Sp", "desc": "Spectral type "}, {"name": "u_Sp", "desc": "uncertainty in Sp "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_12"}} {"id": "III/12A", "title_cds": "F5 and Later Stars in SA28, 54, 106, 107", "title_create": "Upgren, Staron 1970", "year": "1970", "author": "Upgren Jr. A.R., Staron R.T.", "title_pub": "F5 and Later Stars in Selected Areas 28, 54, 106, 107", "first_author": "Upgren Jr. A.R.", "ref_biblio": [""], "bibcode": ["1970ApJS...19..367U"], "keyword_cds": "Selected areas", "description": ["The catalog is an objective-prism survey of 2181 stars later than", "spectral class F2; the earlier stars are in catalog ADC# 3011A. The", "limiting magnitude is about 11.5. Four regions of intermediate", "galactic latitude are included in this survey. Each region is", "centered on one of the Selected Areas 28, 54, 106, and 107 and", "consists of a square 7 degrees on a side or about 50 square degrees", "in area. The fields, 4 x 4 degrees in size, were each photographed", "on two IIa-O emulsion plates, one with an exposure time of three", "minutes on which bright stars could be classified and one with an", "exposure time of 40 minutes extending to faint stars. The plates", "were taken with the 24-inch Baker-Schmidt telescope of the Dyer", "Observatory. The dispersion of the objective prism is about 330", "A/mm at H-gamma. The stars were classified according to the", "criteria established by Nassau and Seyfert (1946) and Nassau and van", "Albada (1947). Photographic magnitudes were found from direct IIa-O", "plates taken with the 8-inch Ross camera of the Yale University", "Observatory. The catalog includes BD numbers, magnitudes, and", "spectral classes for BD stars. For non BD stars, the BD number", "listed in bytes 1-3 indicates a nearby BD star from which the star", "listed is offset by the values in bytes 5-12 and 15-17 given in", "minutes of arc."], "date_update": "15-Dec-2015", "tables": [{"name": "bdstars.dat", "desc": "catalog data for BD stars ", "columns": [{"name": "AreaNum", "desc": "Selected Area number "}, {"name": "BD", "desc": "BD number "}, {"name": "PhotoMag", "desc": "Photographic magnitude "}, {"name": "u_PhotoMag", "desc": "Colon for uncertainty in photographic magnitude"}, {"name": "SpTemp", "desc": "Spectral type, temperature class and subclass "}, {"name": "u_SpTemp", "desc": "Colon for uncertainty in temperature class/subclass"}, {"name": "LumCl", "desc": "luminosity class "}, {"name": "u_LumCl", "desc": "Colon for uncertainty in luminosity class "}]}, {"name": "nonbd.dat", "desc": "data for non-BD stars ", "columns": [{"name": "AreaNum", "desc": "Selected Area number "}, {"name": "BD", "desc": "BD number of nearby star "}, {"name": "RAoffset", "desc": "Right ascension offset from BD star given in bytes 5-12, minutes of arc"}, {"name": "DEoffset", "desc": "Declination offset from BD star given in bytes 5-12, minutes of arc"}, {"name": "PhotoMag", "desc": "Photographic magnitude "}, {"name": "u_PhotoMag", "desc": "Colon for uncertainty in photographic magnitude"}, {"name": "SpTemp", "desc": "Spectral type, temperature class and subclass "}, {"name": "u_SpTemp", "desc": "Colon for uncertainty in temperature class/subclass"}, {"name": "LumCl", "desc": "luminosity class "}, {"name": "u_LumCl", "desc": "Colon for uncertainty in luminosity class "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_160A"}} {"id": "III/160A", "title_cds": "Bibliographic Catalogue of Radial Velocities", "title_create": "Barbier+ 1990", "year": "1990", "author": "Barbier-Brossat M., Petit M.", "title_pub": "Catalogue Bibliographique de Vitesses Radiales Stellaires", "first_author": "Barbier-Brossat M.", "ref_biblio": [""], "bibcode": ["1990A&AS...85..885B"], "keyword_cds": "Radial velocities", "description": ["This compilation of stellar radial velocities is a continuation of Abt", "& Biggs (III/4), and supersedes the previous catalog (III/118). It", "includes about 24200 references for Galactic, Large and Small", "Magellanic stars published between 1970 and 1985."], "type": ["BCC"], "data": "", "status": "obsolete", "date_creation": "01-Dec-1994", "date_update": "22-Sep-2015", "tables": [{"name": "main.dat", "desc": "The Bibliography of Stellar Radial Velocities ", "columns": [{"name": "HD", "desc": "Identification in HD (III/135) "}, {"name": "RAh", "desc": "? Right Ascension 1950 (hours) "}, {"name": "RAm", "desc": "? Right Ascension 1950 (minutes) "}, {"name": "u_pos", "desc": "[*] '*' indicates an approximative position "}, {"name": "DE-", "desc": "Declination 1950 (sign) "}, {"name": "DEd", "desc": "[-90/90]? Declination 1950 (degrees) "}, {"name": "DEm", "desc": "[0/60[? Declination 1950 (minutes) "}, {"name": "n_mag", "desc": "[*V] '*' for Photographic magnitude, 'V' for variable"}, {"name": "mag", "desc": "? Visual magnitude, or photographic when byte 22 contains a * . Values as found in"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_187"}} {"id": "III/187", "title_cds": "Classification of stars in BCD", "title_create": "Barbier/Chalonge/Divan", "title_pub": "CLASSIFICATION OF STARS IN THE BCD SYSTEM", "first_author": "BARBIER D.", "author": "BARBIER D., CHALONGE D., DIVAN L.: 1941--1969", "ref_biblio": ["< >"], "bibcode": ["1941AnAp....4...30B", "1951CR....232.2079B", "1952CoIAB..83.....C", "1952CoIAP.124.....F", "1956AnAp....6..287D", "1956AZh....33.....C", "1955JO.....38..345D", "1955CoIAB.129.....B", "1955JO.....38...93D", "1965POHP....7..(39B", "1966CoIAB.286..311D", "1963AnAp....4..289V", "1957CoIAP.227.....D", "1958CoIAB.181.....B", "1958JO.....41...(6A", "1964CoIAP.308.....C", "1969CoIAP.383.....D", "1956AnAp....6..294B"], "curator": "Francois Ochsenbein [CDS]", "alias": ["BCD"], "data": "", "date_update": "12-Oct-2000"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_212"}} {"id": "III/212", "title_cds": "Spectra of V568 Cyg in Period 1982-1988", "title_create": "Coluzzi, 1990", "year": "1990", "author": "Coluzzi R.", "title_pub": "Digitized Photographic Prism Spectrogram Archive of the long-monitored peculiar star V568 Cyg", "first_author": "Coluzzi R.", "ref_biblio": [""], "bibcode": ["1990A&A...230..307B"], "keyword_cds": "Spectroscopy; Stars, variable", "object": [], "curator": "Francois Ochsenbein [CDS]", "records": ["74 spectra"], "data": "", "date_update": "05-Oct-2012"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_240"}} {"id": "III/240", "title_cds": "Near-infrared spectra of MK standards", "title_create": "Wallace+ 1997-2002", "year": "2002", "author": "Wallace L., Meyer M.R., Hinkle K., Edwards S., Strom S.E.", "title_pub": "Near-infrared classification spectroscopy", "first_author": "Wallace L.", "ref_biblio": [""], "keyword_cds": "Spectroscopy ; Redshifts; Surveys ; Velocity dispersion", "keyword_pub": "", "object": [], "ack": ["Refer to the SDSS pages at", "http://www.sdss.org/collaboration/credits.html", "Data from the SDSS public archive may not be used for any commercial", "publication or other commercial purpose except with explicit approval", "by the Astrophysical Research Consortium (ARC).", "Non-commercial scientific and technical publications using SDSS data", "should include the acknowledgment detailed at", "http://www.sdss.org/collaboration/credits.html"], "curator": "Francois Ochsenbein [CDS]", "alias": ["SDSS-DR6", "SDSS"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "30-May-2009"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_259"}} {"id": "III/259", "title_cds": "Stephenson's dwarf K and M stars (StKM)", "title_create": "Stephenson, 1986", "year": "1986", "author": "Stephenson C.B.", "title_pub": "Dwarf K And M stars of small proper motion found in a Large Spectroscopic Survey", "first_author": "Stephenson C.B.", "ref_biblio": ["", ""], "bibcode": ["1986AJ.....91..144S", "1986AJ.....92..139S"], "keyword_cds": "Stars, dwarfs ; Stars, late-type ; Spectral types", "abstract": ["More than 2000 candidates for K and M dwarf status, generally having", "proper motions that are either unknown or less than 0.2\" per annum,", "have been identified in an objective-prism survey covering the entire", "sky north of declination -25deg and more than 10deg from the galactic", "plane. More than 95% have no previous indication that they are dwarfs.", "Several dozen appear to be visual double stars."], "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["StKM"], "type": ["OC"], "records": ["4102 stars"], "doi_pub": ["10.1086/113994"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_269"}} {"id": "III/269", "title_cds": "VIMOS VLT Deep Survey (VVDS)", "title_create": "Le Fevre+, 2013", "year": "2013", "author": "Le Fevre O., Cassata P., O. Cucciati O., Garilli B., Ilbert O., Le Brun V., Maccagni D., Moreau C., Scodeggio M., Tresse L., Zamorani G., Adami C., Arnouts S., Bardelli S., Bolzonella M., Bondi M., Bongiorno A., Bottini D., Cappi A., Charlot S., Ciliegi P., Contini T., de la Torre S., Foucaud S., Franzetti P., Gavignaud I., Guzzo L., Iovino A., Lemaux B., McCracken H.J., Marano B., Marinoni C., Mazure A., Mellier Y., Merighi R., Merluzzi P., Paltani S., Pello R., Pollo A., Pozzetti L., Scaramella R., Vergani D., Vettolani G., Zanichelli A., Zucca} E.", "title_pub": "The VIMOS VLT Deep Survey final data release: a spectroscopic sample of 35016 galaxies and AGN out to z~6.7 selected with 17.5<=i_AB_<=24.75", "first_author": "Le Fevre O.", "ref_biblio": [""], "bibcode": ["2013A&A...559A..14L"], "keyword_cds": "Photometry, UBVRI ; Photometry, infrared; Galaxies, spectra ; Atlases", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: high redshift - cosmology: observations - cosmology: large-scale structure of Universe - astronomical databases: surveys", "abstract": ["Context. Deep representative surveys of galaxies at different epochs", "are needed to make progress in understanding galaxy evolution.", "Aims. We describe the completed VIMOS VLT Deep Survey, and the final", "data release of 35016 galaxies and type-I AGN with measured", "spectroscopic redshifts covering all epochs up to redshift z~6.7, in", "areas from 0.142 to 8.7 square degrees, and volumes from 0.5x10^6^ to", "2x10^7^h^-3^Mpc^3^.", "Methods. We have selected samples of galaxies based solely on their", "i-band magnitude reaching i_AB_=24.75. Spectra have been obtained with", "VIMOS on the ESO-VLT integrating 0.75h, 4.5h and 18h for the Wide,", "Deep, and Ultra-Deep nested surveys, respectively. We demonstrate that", "any 'redshift desert' can be crossed successfully using spectra", "covering 3650<={lambda}<=9350{AA}. A total of 1263 galaxies have been", "re-observed independently within the VVDS, and from the VIPERS and", "MASSIV surveys. They are used to establish the redshift measurements", "reliability, to assess completeness in the VVDS samples, and to", "provide a weighting scheme taking into account the survey selection", "function"], "curator": "Francois Ochsenbein [CDS]", "alias": ["VVDS"], "type": ["OC"], "records": ["records"], "doi_pub": ["10.1051/0004-6361/201322179"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_o26"}} {"id": "III/26", "title_cds": "Abundances of Na, Mg, and Ca in K giants, Table II", "title_create": "Peat+ 1968", "year": "1968", "author": "Peat D.W., Pemberton A.C.", "title_pub": "Abundances of Sodium, Magnesium and Calcium in K-Type Giant Stars. Table II", "first_author": "Peat D.W.", "ref_biblio": [""], "bibcode": ["1968MNRAS.140...21P"], "keyword_cds": "Abundances; Stars, K-type; Stars, giant", "abstract": ["Narrow band photometric measures of the strengths of the Mg b, Ca triplet,", "and Na D lines in 312 G and K type giant stars have been analyzed with a", "model atmosphere technique to determine abundances of magnesium, calcium", "and sodium."], "date_update": "06-May-2020", "tables": [{"name": "table2.dat", "desc": "Abundance ratios, surface gravity = 500 and 200 ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"III_283"}} {"id": "III/283", "title_cds": "RAVE 6th data release", "title_create": "Steinmetz+, 2020", "year": "2020", "author": "Steinmetz M., Matijevic G., Enke H., Zwitter T., Guiglion G., McMillan P.J., Kordopatis G., Valentini M., Chiappini C., Casagrande L., Wojno J., Anguiano B., Bienayme O., Bijaoui A., Binney J., Burton D., Cass P., de Laverny P., Fiegert K., Freeman K., Fulbright J.P., Gibson B.K., Gilmore G., Grebel E.K., Helmi A., Kunder A., Munari U., Navarro J.F., Parker Q., Ruchti G.R., Recio-Blanco A., Reid W., Seabroke G.M., Siviero A., Siebert A., Stupar M., Watson F., Williams M.E.K., Wyse R.F.G., Anders F., Antoja T., Birko D., Bland-Hawthorn J., Bossini D., Garcia R.A., Carrillo I., Chaplin W.J., Elsworth Y., Famaey B., Gerhard O., Jofre P., Just A., Mathur S., Miglio A., Minchev I., Monari G., Mosser B., Ritter A., Rodrigues T.S., Scholz R.-D., Sharma S., Sysoliatina K. (The Rave collaboration)", "title_pub": "The sixth data release of the Radial Velocity Experiment (RAVE). I. Survey description, spectra, and radial velocities. II. Stellar atmospheric parameters, chemical abundances, and distances.", "first_author": "Steinmetz M.", "ref_biblio": [""], "bibcode": ["2020yCat.3283....0s", "2020AJ....160...82S"], "keyword_cds": "Surveys ; Radial velocities; Milky Way; Stars, fundamental ; Photometry", "keyword_pub": "Stellar populations - Galaxy stellar content - Milky Way Galaxy - Milky Way dynamics - Surveys - Sky surveys - Catalogs", "abstract": ["The Radial Velocity Experiment (RAVE) is a magnitude-limited (9", "", ""], "bibcode": ["1968ArA.....4..587L", "1986AJ.....91..326C"], "keyword_cds": "Clusters, open ; Photometry, UBV ; Cross identifications", "keyword_pub": "", "curator": "Francois Ochsenbein [CDS]", "alias": ["NGC2567"], "type": ["OC"], "records": ["181 stars"], "data": "", "date_update": "15-Aug-2008"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"IV_37"}} {"id": "IV/37", "title_cds": "The ATLAS all-sky stellar reference catalog", "title_create": "Tonry+, 2018", "year": "2018", "author": "Tonry J.L., Denneau L., Flewelling H., Heinze A.N., Onken C.A., Smartt S.J., Stalder B., Weiland H.J., Wolf C.", "title_pub": "The ATLAS all-sky stellar reference catalog.", "first_author": "Tonry J.L.", "ref_biblio": [""], "bibcode": ["2018ApJ...867..105T", "2019yCat.4037....0"], "keyword_cds": "; Parallaxes, trigonometric ; Proper motions ; Effective temperatures ; Extinction ; Photometry, ugriz ; Photometry, infrared", "keyword_pub": "atmospheric effects - instrumentation: photometers - surveys - techniques: photometric", "abstract": ["The Asteroid Terrestrial-impact Last Alert System (ATLAS) observes", "most of the sky every night in search of dangerous asteroids. Its data", "are also used to search for photometric variability, where sensitivity", "to variability is limited by photometric accuracy. Since each exposure", "spans 7.6{deg} corner to corner, variations in atmospheric transparency", "in excess of 0.01 mag are common, and 0.01 mag photometry cannot be", "achieved by using a constant flat-field calibration image. We therefore", "have assembled an all-sky reference catalog of approximately one billion", "stars to m~19 from a variety of sources to calibrate each exposure's", "astrometry and photometry. Gaia DR2 (Cat. I/345) is the source of", "astrometry for this ATLAS Refcat2. The sources of g, r, i, and z photometry", "include Pan-STARRS DR1 (Cat. II/349), the ATLAS Pathfinder photometry", "project, ATLAS reflattened APASS data, SkyMapper DR1 (Cat. II/358),", "APASS DR9 (Cat. II/336), the Tycho-2 catalog (Cat. I/259), and the Yale", "Bright Star Catalog (BSC; Hoffleit 1964cbs..book.....H). We have attempted", "to make this catalog at least 99% complete to m<19, including the brightest", "stars in the sky. We believe that the systematic errors are no larger", "than 5 mmag rms, although errors are as large as 20 mmag in small patches", "near the Galactic plane."], "curator": "Thomas Boch, Tiphaine Pouvreau [CDS]", "alias": [""], "records": ["records"], "doi_pub": ["10.3847/1538-4357/aae386"], "orcid_pub": ["0000-0003-2858-9657"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"IX_26"}} {"id": "IX/26", "title_cds": "Einstein Observatory, Revision 1B. Processings", "title_create": "Giacconi+, 1979", "year": "1979", "author": "Giacconi et al.", "title_pub": "Einstein Observatory, the 1B data revision tables and results.", "first_author": "Giacconi et al.", "ref_biblio": ["< >"], "bibcode": [""], "keyword_cds": "X-ray sources ; Surveys", "mission": "Einstein", "description": ["Various parameters for the IPC observations of the Einstein Observatory", "in the Rev1B Processing."], "records": ["18780 sources"], "data": "", "date_update": "29-Apr-1999", "tables": [{"name": "r1b_det.dat", "desc": "Source Detection Parameters for Rev1B Processing ", "columns": [{"name": "Seqno", "desc": "IPC Sequence Number (G1) "}, {"name": "rev1b", "desc": "IPC Rev1b source number (G2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "LHypos", "desc": "Y position: Ldetect in hard band (1) "}, {"name": "LHzpos", "desc": "Z position: Ldetect in hard band (1) "}, {"name": "e_LHypos", "desc": "Radius of error circle (1) "}, {"name": "LHccnts", "desc": "Cell counts: Ldetect in hard band (2) "}, {"name": "e_LHccnts", "desc": "Error on LH cell counts (2) "}, {"name": "LHbcnts", "desc": "Background cell counts: Ldetect hard band (3) "}, {"name": "e_LHbcnts", "desc": "Error on LH background cell counts (3) "}, {"name": "LHncnts", "desc": "Net cell counts: Ldetect in hard band (4) "}, {"name": "e_LHncnts", "desc": "Error on LH net cell counts (4) "}, {"name": "LHthrc", "desc": "Threshold cell counts: Ldetect hard band (5) "}, {"name": "LH_SNR", "desc": "Signal-to-noise ratio: Ldetect hard band (5) "}, {"name": "LBypos", "desc": "Y position: Ldetect in broad band (1) "}, {"name": "LBzpos", "desc": "Z position: Ldetect in broad band (1) "}, {"name": "e_LBypos", "desc": "Radius of error circle (1) "}, {"name": "LBccnts", "desc": "Cell counts: Ldetect in broad band (2) "}, {"name": "e_LBccnts", "desc": "Error on LB cell counts (2) "}, {"name": "LBbcnts", "desc": "Backgrnd cell counts: Ldetect broad band (3) "}, {"name": "e_LBbcnts", "desc": "Error on LB background cell counts (3) "}, {"name": "LBncnts", "desc": "Net cell counts: Ldetect in broad band (4) "}, {"name": "e_LBncnts", "desc": "Error on LB net cell counts (4) "}, {"name": "LBthrc", "desc": "Threshold cell counts: Ldetect broad band (5) "}, {"name": "LB_SNR", "desc": "Signal-to-noise ratio: Ldetect broad band (5) "}, {"name": "LSypos", "desc": "Y position: Ldetect in soft band (1) "}, {"name": "LSzpos", "desc": "Z position: Ldetect in soft band (1) "}, {"name": "e_LSypos", "desc": "Radius of error circle (1) "}, {"name": "LSccnts", "desc": "Cell counts: Ldetect in soft band (2) "}, {"name": "e_LSccnts", "desc": "Error on LS cell counts (2) "}, {"name": "LSbcnts", "desc": "Background cell counts: Ldetect soft band (3) "}, {"name": "e_LSbcnts", "desc": "Error on LS background cell counts (3) "}, {"name": "LSncnts", "desc": "Net cell counts: Ldetect in soft band (4) "}, {"name": "e_LSncnts", "desc": "Error on LS net cell counts (4) "}, {"name": "LSthrc", "desc": "Threshold cell counts: Ldetect soft band (5) "}, {"name": "LS_SNR", "desc": "Signal-to-noise ratio: Ldetect soft band (5) "}, {"name": "MHypos", "desc": "Y position: Mdetect in hard band (1) "}, {"name": "MHzpos", "desc": "Z position: Mdetect in hard band (1) "}, {"name": "e_MHypos", "desc": "Radius of error circle (1) "}, {"name": "MHccnts", "desc": "Cell counts: Mdetect in hard band (2) "}, {"name": "e_MHccnts", "desc": "Error on MH cell counts (2) "}, {"name": "MHbcnts", "desc": "Background cell counts: Mdetect hard band (3) "}, {"name": "e_MHbcnts", "desc": "Error on MH background cell counts (3) "}, {"name": "MHncnts", "desc": "Net cell counts: Mdetect in hard band (4) "}, {"name": "e_MHncnts", "desc": "Error on MH net cell counts (4) "}, {"name": "MHthrc", "desc": "Threshold cell counts: Mdetect hard band (5) "}, {"name": "MH_SNR", "desc": "Signal-to-noise ratio: Mdetect hard band (5) "}, {"name": "MBypos", "desc": "Y position: Mdetect in broad band (1) "}, {"name": "MBzpos", "desc": "Z position: Mdetect in broad band (1) "}, {"name": "e_MBypos", "desc": "Radius of error circle (1) "}, {"name": "MBccnts", "desc": "Cell counts: Mdetect in broad band (2) "}, {"name": "e_MBccnts", "desc": "Error on MB cell counts (2) "}, {"name": "MBbcnts", "desc": "Backgrnd cell counts: Mdetect broad band (3) "}, {"name": "e_MBbcnts", "desc": "Error on MB background cell counts (3) "}, {"name": "MBncnts", "desc": "Net cell counts: Mdetect in broad band (4) "}, {"name": "e_MBncnts", "desc": "Error on MB net cell counts (4) "}, {"name": "MBthrc", "desc": "Threshold cell counts: Mdetect broad band (5) "}, {"name": "MB_SNR", "desc": "Signal-to-noise ratio: Mdetect broad band (5) "}, {"name": "MSypos", "desc": "Y position: Mdetect in soft band (1) "}, {"name": "MSzpos", "desc": "Z position: Mdetect in soft band (1) "}, {"name": "e_MSypos", "desc": "Radius of error circle (1) "}, {"name": "MSccnts", "desc": "Cell counts: Mdetect in soft band (2) "}, {"name": "e_MSccnts", "desc": "Error on MS cell counts (2) "}, {"name": "MSbcnts", "desc": "Background cell counts: Mdetect soft band (3) "}, {"name": "e_MSbcnts", "desc": "Error on MS background cell counts (3) "}, {"name": "MSncnts", "desc": "Net cell counts: Mdetect in soft band (4) "}, {"name": "e_MSncnts", "desc": "Error on MS net cell counts (4) "}, {"name": "MSthrc", "desc": "Threshold cell counts: Mdetect soft band (5) "}, {"name": "MS_SNR", "desc": "Signal-to-noise ratio: Mdetect soft band (5) "}, {"name": "MS_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "MH_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "MB_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "LS_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "LH_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}, {"name": "LB_cmpf", "desc": "[01] '1' if src has component in this method/band (6)"}]}, {"name": "r1b_rad.dat", "desc": "Count distributions for Rev 1B IPC sources ", "columns": [{"name": "Seqno", "desc": "Sequence Number (G1) "}, {"name": "rev1b", "desc": "Rev1b Source Number (G2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "hpe", "desc": "High ph band extent (2) "}, {"name": "e_hpe", "desc": "High ph band extent error (2) "}, {"name": "sabkg", "desc": "Source annulus area background (3) "}, {"name": "sarea", "desc": "Source circle area (3) "}]}, {"name": "r1b_spc.dat", "desc": "IPC Spectral Information from Rev1B Processing ", "columns": [{"name": "Seqno", "desc": "IPC Sequence Number (G1) "}, {"name": "rev1b", "desc": "IPC Rev1b source number (G2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}]}, {"name": "r1b_sum.dat", "desc": "Summary of Observation Parameters for Rev1B Sources ", "columns": [{"name": "Seqno", "desc": "IPC Sequence Number (G1) "}, {"name": "rev1b", "desc": "IPC Rev1b source number (G2) "}, {"name": "pcod", "desc": "[LMSHB] Pcod flag - origin of position (1) "}, {"name": "ypos", "desc": "Pcod Y pixel position (2) "}, {"name": "zpos", "desc": "Pcod Z pixel position (2) "}, {"name": "yzp_err", "desc": "Pixel radius of error circle (2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "ra_err", "desc": "Right ascension error (3) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "dec_err", "desc": "Declination error (3) "}, {"name": "GLONr", "desc": "Pcod galactic longitude (4) "}, {"name": "e_GLONr", "desc": "Galactic longitude error (4) "}, {"name": "GLATr", "desc": "Pcod galactic latitude (4) "}, {"name": "e_GLATr", "desc": "Galactic latitude error (4) "}, {"name": "vigncorr", "desc": "Vignetting correction (5) "}, {"name": "SBcts", "desc": "Pcod position cell counts in soft band (6) "}, {"name": "e_SBcts", "desc": "Error on cell counts in soft band (6) "}, {"name": "HBcts", "desc": "Pcod position cell counts in hard band (6) "}, {"name": "e_HBcts", "desc": "Error on cell counts in hard band (6) "}, {"name": "BBcts", "desc": "Pcod position cell counts in broad band (6) "}, {"name": "e_BBcts", "desc": "Error on cell counts in broad band (6) "}, {"name": "SBbgcts", "desc": "Pcod cell background counts in soft band (7) "}, {"name": "e_SBbgcts", "desc": "Error on cell background counts in soft band (7) "}, {"name": "HBbgcts", "desc": "Pcod cell background counts in hard band (7) "}, {"name": "e_HBbgcts", "desc": "Error on cell background counts in hard band (7) "}, {"name": "BBbgcts", "desc": "Pcod cell background counts in broad band (7) "}, {"name": "e_BBbgcts", "desc": "Error on cell background counts, broad band (7) "}, {"name": "SBccrate", "desc": "Pcod corrected count rate in soft band (8) "}, {"name": "e_SBccrate", "desc": "Error on corrected count rate in soft band (8) "}, {"name": "HBccrate", "desc": "Pcod corrected count rate in hard band (8) "}, {"name": "e_HBccrate", "desc": "Error on corrected count rate in hard band (8) "}, {"name": "BBccrate", "desc": "Pcod corrected count rate in broad band (8) "}, {"name": "e_BBccrate", "desc": "Error on corrected count rate in broad band (8) "}, {"name": "SBflux", "desc": "Pcod source flux in soft band (9) "}, {"name": "e_SBflux", "desc": "Error on source flux in soft band (9) "}, {"name": "HBflux", "desc": "Pcod source flux in hard band (9) "}, {"name": "e_HBflux", "desc": "Error on source flux in hard band (9) "}, {"name": "BBflux", "desc": "Pcod source flux in broad band (9) "}, {"name": "e_BBflux", "desc": "Error on source flux in broad band (9) "}, {"name": "EBflux", "desc": "Pcod source flux in Einstein band (9) "}, {"name": "e_EBflux", "desc": "Error on source flux in Einstein band (9) "}, {"name": "prffit", "desc": "PRF fit\t(10) "}, {"name": "reco", "desc": "Combined ribs and edges code (11) "}, {"name": "sel_flag", "desc": "Flagged 0.0 if source included in EOSCAT (12) "}]}, {"name": "r1b_var.dat", "desc": "Variability Parameters for Rev1B Processing ", "columns": [{"name": "Seqno", "desc": "IPC Sequence Number (G1) "}, {"name": "rev1b", "desc": "IPC Rev1b source number (G2) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) (1) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) (1) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "chicode", "desc": "Variability code chisq analysis (2) "}, {"name": "Chi2", "desc": "Reduced chisq (2) "}, {"name": "nChi2", "desc": "Degrees of freedom (2) "}, {"name": "Cprob", "desc": "Probability that source is constant (3) "}, {"name": "eqsigma", "desc": "Equivalent number of sigma (3) "}, {"name": "nbins", "desc": "Number of bins (4) "}, {"name": "bintime", "desc": "Bintime (4) "}, {"name": "counts", "desc": "Source circle counts (5) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"IX_27"}} {"id": "IX/27", "title_cds": "Einstein Observatory Catalog (OCAT) (Yellow Book)", "title_create": "Seward+, 1986", "year": "1986", "author": "Seward F.D., Martenis P.", "title_pub": "Einstein Observations: OCAT alias ``Yellow Book\"", "first_author": "Seward F.D.", "ref_biblio": ["< Einstein Observatory Catalog of Observations (5th ed.; Cambridge: Harvard-Smithsonian Center for Astrophysics). >"], "see_also": ["IX/22 : The CfA Einstein observatory extended deep X-ray survey", "IX/23 : Einstein Observatory Source Catalog", "IX/24 : The Einstein Observatory High Resolution Imager Source List", "IX/25 : Einstein Observatory Imaging Proportional Counter (IPC) Parameters", "IX/26 : Einstein Observatory, Revision 1B. Processings"], "keyword_cds": "X-ray sources ; Surveys", "mission": "Einstein", "description": ["This catalog contains details on the Einstein Observatory Catalog of", "Observations (OCA), observations, databank requests, observers and the", "observations themselves are provided. This is also known as the", "Einstein Observatory's \"Yellow Book\"."], "alias": ["OCAT"], "records": ["5656 sources"], "data": "", "date_update": "29-Apr-1999", "tables": [{"name": "categs.dat", "desc": "Categories of Einstein Observations ", "columns": [{"name": "categ", "desc": "Eight letter category code (1) "}, {"name": "descr", "desc": "Category title as used in the original Yellow Book "}]}, {"name": "db_reqs.dat", "desc": "Einstein Observatory Databank Requests ", "columns": [{"name": "req_num", "desc": "Request's identifying number (1) "}, {"name": "req_date", "desc": "Date of the request (1) "}, {"name": "name", "desc": "Name and institution of the person requesting the data"}, {"name": "title", "desc": "Title describing the topic of the request "}]}, {"name": "obsnames.dat", "desc": "Einstein Observers ", "columns": [{"name": "obs_num", "desc": "The observer's identifying number (1) "}, {"name": "obs_name", "desc": "The observer's name and institution "}]}, {"name": "pointing.dat", "desc": "Einstein Observations (OCAT alias \"Yellow Book\") ", "columns": [{"name": "Seqno", "desc": "The sequence number of the observation (1) "}, {"name": "RAh", "desc": "Right Ascension (B1950) (hour) "}, {"name": "RAm", "desc": "Right Ascension (B1950) (min) "}, {"name": "RAs", "desc": "Right Ascension (B1950) (sec) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) (deg) "}, {"name": "DEm", "desc": "Declination (B1950) (arcmin) "}, {"name": "DEs", "desc": "Declination (B1950) (arcsec) "}, {"name": "instr", "desc": "The instrument at the focus (2) "}, {"name": "obs_num", "desc": "The observer identification number (3) "}, {"name": "TIPI", "desc": "Time In Processed Image (3) "}, {"name": "obs_date", "desc": "The date the observation was started (3) "}, {"name": "categ", "desc": "Category code based upon the observation's target (4)"}, {"name": "title", "desc": "The name of target and/or name of observing program (4)"}, {"name": "req_num", "desc": "Identifying numbers of databank requests (5) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"IX_38"}} {"id": "IX/38", "title_cds": "ROSAT Sources for the PSPC with filter (2RXF)", "title_create": "ROSAT Team, 2001", "year": "2001", "author": "ROSAT Scientific Team", "title_pub": "ROSAT Results Archive Sources for the PSPC with filter", "first_author": "ROSAT Scientific Team", "ref_biblio": [""], "keyword_cds": "X-ray sources ; Surveys", "mission": "ROSAT", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["2RXF"], "records": ["records"], "data": "", "date_update": "04-Mar-2004"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_151_372"}} {"id": "J/A+A/151/372", "title_cds": "Effective temperatures of F stars", "title_create": "Saxner+, 1985", "year": "1985", "author": "Saxner M., Hammarback G.", "title_pub": "An empirical temperature calibration for F dwarfs.", "first_author": "Saxner M.", "ref_biblio": [""], "bibcode": ["1985A&A...151..372S"], "keyword_cds": "Effective temperatures", "keyword_pub": "stellar atmospheres - effective temperature calibration - photometric systems - F dwarfs - solar colours", "curator": "Eric Mamajek [CfA] Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_17_326"}} {"id": "J/A+A/17/326", "title_cds": "Positions of GV stars", "title_create": "Sanduleak+, 1972", "year": "1972", "author": "Sanduleak N.", "title_pub": "Comparison of the Large Magellanic Cloud catalogue of Sanduleak and Fehrenbach-Duflot.", "first_author": "Sanduleak N.", "ref_biblio": [""], "bibcode": ["1972A&A....17..326S"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_177_217"}} {"id": "J/A+A/177/217", "title_cds": "Teff and Luminosity from MK spectral class", "title_create": "De Jager+ 1987", "year": "1987", "author": "De Jager C., Nieuwenhuijzen H.", "title_pub": "A new determination of the statistical relations between stellar spectral and luminosity classes and stellar effective temperature and lumonosity.", "first_author": "De Jager C.", "ref_biblio": [""], "bibcode": ["1987A&A...177..217D"], "keyword_cds": "", "keyword_pub": "stars: classificaition ; stars: Hertzsprung-Russel diagrapn ; stars: luminosity ; stars: temperatures", "abstract": ["From a set of 199 determinations of bolometric stellar luminosity L", "and 268 of stellar effective temperature T_eff_ we derived the", "statical dependences of log(T_eff_) and log(L/L{sun}) respectively on", "spectral type and luminosity class. For computer use we introduced", "continuous variables s (for spectral type) and b (for luminosity", "class). The relations T_eff_(s,b) and logL(s,b) are given in terms of", "Chebychev polynomials and their cross-products. A comparison is made", "with existing systems; there are small differences that we ascribe to", "the addition of new data to temperature and luminosity, not used in", "previous determinations. The 1-{sigma} values for determinations of", "unit weight of logT_eff_ and logL respectively appear to be 0.021 and", "0.164, which shows that there is a factor 8 in their relative", "accuracies."], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "10-Sep-2014"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_18_271"}} {"id": "J/A+A/18/271", "title_cds": "Photometry of bright stars in LMC", "title_create": "Dachs+, 1972", "year": "1972", "author": "Dachs J.", "title_pub": "Photometry of bright stars in the Large Magellanic Cloud.", "first_author": "Dachs J.", "ref_biblio": [""], "bibcode": ["1972A&A....18..271D"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_379_436"}} {"id": "J/A+A/379/436", "title_cds": "EIS survey: selected stellar fields", "title_create": "Momany+, 2001", "year": "2001", "author": "Momany Y., Vandame B., Zaggia S., Mignani R.P., Da Costa L., Arnouts S., Groenewegen M.A.T., Hatziminaoglou E., Madejsky R., Rite C., Schirmer M., Slijkhuis R.", "title_pub": "ESO imaging survey. Pre-FLAMES survey: Observations of selected stellar fields.", "first_author": "Momany Y.", "ref_biblio": [""], "bibcode": ["2001A&A...379..436M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1051/0004-6361:20011325"], "orcid_pub": ["0000-0001-8946-8723"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_398_89"}} {"id": "J/A+A/398/89", "title_cds": "Evolutionary synthesis models. II.", "title_create": "Schulz+, 2003", "year": "2003", "author": "Schulz J., Fritze-v. Alvensleben U., Fricke K.J.", "title_pub": "Wavelength and redshift dependence of bulge/total light ratios in galaxies.", "first_author": "Schulz J.", "ref_biblio": [""], "bibcode": ["2003A&A...398...89S"], "see_also": ["http://www.uni-sw.gwdg.de/~galev : The Goettingen Galaxy Evolution Group", "J/A+A/392/1 : Spectrophotometry of simulated SSPs (Schulz+, 2002)", "J/A+A/401/1063 : Evolutionary synthesis models. III. (Anders+, 2003)"], "keyword_cds": "Models, evolutionary ; Galaxies, photometry", "keyword_pub": "galaxies: general - galaxies, evolution - galaxies, formation - galaxies: fundamental parameters - galaxies: stellar content", "abstract": ["HST has opened the possibility to decompose the surface brightness", "profiles of galaxies up to significant redshifts and look-back times", "into r^1/4^-bulge and exponential disk components. This should allow", "to study the redshift evolution of bulge and disk luminosity", "contributions and discriminate between the different formation", "scenarios for these galaxy components currently discussed, i.e. decide", "if star formation in bulges and disks started at the same time or was", "delayed in either of the two components. An indispensable prerequisite", "for the comparison of bulge-to-disk ratios of galaxies at different", "redshifts is to properly account for cosmological band shift and", "evolutionary effects.", "We present evolutionary synthesis models for both components and add", "their spectra in various proportions to obtain the full range of local", "galaxies' B-band bulge-to-total light ratios. Bulge star formation is", "assumed to occur on a short timescale of 10^9^yr, disk star", "formation proceeds at a constant rate. We study the evolution of the", "relative light contributions of both components backward in time and,", "for a given cosmological model, as a function of redshift. This allows", "us to see how far back into the past the locally well-established", "correlation between galaxy morphologies and spectral properties can", "hold. To cope with the present uncertainty about the formation epochs", "of bulge and disk components we present models for three scenarios:", "bulges and disks of equal age, old bulges and delayed disk star", "formation, and old disks with subsequent bulge star formation.", "We quantitatively show the wavelength dependence of bulge-to-total", "(=B/T) light ratios for local galaxies. The different star formation", "timescales for bulge and disk components lead to B/T ratios that", "significantly increase from U through I-bands (by factors 4-6 for", "weak bulge systems ~Sc) with the rate of increase slightly depending", "on the relative ages of the two components.", "The redshift evolution of B/T-ratios in various bands U,B,V,I,H is", "calculated accounting both for cosmological and evolutionary", "corrections assuming a standard cosmology (H_0_=65, Omega_0_)=0.1,", "Lambda_0_=0). In particular, for the two scenarios with old bulges and", "old or younger disks, the redshift evolution of B/T-ratios is dramatic", "in every band and both for galaxies ending up at z~0 with low and high", "B-band B/T light ratios. Our results clearly show that it does not", "make any sense to compare B/T ratios measured in one and the same band", "for galaxies at different redshifts without fully accounting for", "evolutionary and cosmological effects. These, unfortunately,", "significantly depend on the relative ages of the two components and,", "hence, on the galaxy formation scenario adopted.", "We also show that simultaneous decomposition of galaxy profiles in", "several bands can give direct information about these relative ages", "and constrain formation scenarios for the different galaxy components."], "description": ["Spectra, colors, luminosities and B/T ratios in various filter-systems", "as well as cosmological and evolutionary corrections in the cosmology", "(H_0_=65, Omega_0_=0.1, Lambda_0_=0.0) for the 4 components and their", "related B/T scenarios. The timestep is 4*10^6^years. the UBV filters", "are from Buser & Kurucz (1978A&A....70..555B), the RI filter from", "Bessell (1990PASP..102.1181B) and JHK from Bessel & Brett", "(1988PASP..100.1134B). Files are sorted in directorys with following", "naming-convention:", "84-84 = scenario with equally old bulge and disk", "84-50 = scenario with old bulge and young disk", "50-84 = scenario with old disk and young bulge", "the e- & k-corrections can be found in ec*.dat, kc*.dat and ka*.dat", "corresponding to the cosmology with H_0_=65 as seen above. Both", "k-corrections with and without attenuation are included."], "doi_pub": ["10.1051/0004-6361:20021631"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "johesd.dat", "desc": "Luminosities and colors from the spectra in Johnson filter-system, Scalo IMF, Only Elliptical or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "Umag", "desc": "Johnson U magnitude "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "Rmag", "desc": "Johnson R magnitude "}, {"name": "Imag", "desc": "Johnson I magnitude "}, {"name": "Jmag", "desc": "Johnson J magnitude "}, {"name": "Hmag", "desc": "Johnson H magnitude "}, {"name": "Kmag", "desc": "Johnson K magnitude "}, {"name": "Lmag", "desc": "Johnson L magnitude "}, {"name": "U-B", "desc": "Johnson U-B colour index "}, {"name": "B-V", "desc": "Johnson B-V colour index "}, {"name": "U-V", "desc": "Johnson U-V colour index "}, {"name": "V-R", "desc": "Johnson V-R colour index "}, {"name": "R-I", "desc": "Johnson R-I colour index "}, {"name": "V-K", "desc": "Johnson V-K colour index "}, {"name": "I-K", "desc": "Johnson I-K colour index "}, {"name": "B-R", "desc": "Johnson B-R colour index "}, {"name": "B-H", "desc": "Johnson B-H colour index "}, {"name": "J-H", "desc": "Johnson J-H colour index "}, {"name": "H-K", "desc": "Johnson H-K colour index "}]}, {"name": "magesd.dat", "desc": "Luminosities from the spectra in Koo, Thuan & Gunn, Washinton and Stroemgren filter-systems, Scalo IMF, Only Elliptical or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "age", "desc": "Age of system "}, {"name": "kumag", "desc": "Koo u magnitude "}, {"name": "kjmag", "desc": "Koo j magnitude "}, {"name": "kfmag", "desc": "Koo f magnitude "}, {"name": "knmag", "desc": "Koo n magnitude "}, {"name": "gmag", "desc": "Thuan & Gunn g magnitude "}, {"name": "rmag", "desc": "Thuan & Gunn r magnitude "}, {"name": "Cmag", "desc": "Washington C magnitude "}, {"name": "Mmag", "desc": "Washington M magnitude "}, {"name": "T1mag", "desc": "Washington T1 magnitude "}, {"name": "T2mag", "desc": "Washington T2 magnitude "}, {"name": "sumag", "desc": "Stroemgren u magnitude "}, {"name": "svmag", "desc": "Stroemgren v magnitude "}, {"name": "sbmag", "desc": "Stroemgren b magnitude "}, {"name": "symag", "desc": "Stroemgren y magnitude "}]}, {"name": "hstesd.dat", "desc": "Luminosities from the spectra in HST filter-system, Scalo IMF, Only E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "F160BW", "desc": "HST F160BW magnitude "}, {"name": "F170W", "desc": "HST F170W magnitude "}, {"name": "F185W", "desc": "HST F185W magnitude "}, {"name": "F218W", "desc": "HST F218W magnitude "}, {"name": "F255W", "desc": "HST F255W magnitude "}, {"name": "F300W", "desc": "HST F300W = U(HDF) magnitude "}, {"name": "F336W", "desc": "HST F336W magnitude "}, {"name": "F380W", "desc": "HST F380W magnitude "}, {"name": "F439W", "desc": "HST F439W magnitude "}, {"name": "F450W", "desc": "HST F450W = B(HDF) magnitude "}, {"name": "F555W", "desc": "HST F555W = V(YSC) magnitude "}, {"name": "F569W", "desc": "HST F569W magnitude "}, {"name": "F606W", "desc": "HST F606W = V(HDF) magnitude "}, {"name": "F622W", "desc": "HST F622W magnitude "}, {"name": "F675W", "desc": "HST F675W magnitude "}, {"name": "F702W", "desc": "HST F702W magnitude "}, {"name": "F791W", "desc": "HST F791W magnitude "}, {"name": "F814W", "desc": "HST F814W = I(HDF) magnitude "}]}, {"name": "ecesd.dat", "desc": "Coefficients of e-correction in luminosity, H0=65 Scalo IMF, E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Model redshift "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies "}, {"name": "z", "desc": "? Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "kcesd.dat", "desc": "Coefficients of k-correction in luminosity, H0=65 Scalo IMF, E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Model redshift "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies "}, {"name": "z", "desc": "? Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "kaesd.dat", "desc": "Coefficients of k-correction with attenuation in Scalo IMF, E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Model redshift "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies "}, {"name": "z", "desc": "? Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "gspesd.dat", "desc": "Spectra, with Scalo IMF, E or SD galaxies ", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial metallicity (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "lambda", "desc": "Wavelength "}, {"name": "Flux1", "desc": "? Flux at a system age of 1.4000E+08yrs "}, {"name": "Flux2", "desc": "? Flux at a system age of 2.8000E+08yrs "}, {"name": "Flux3", "desc": "? Flux at a system age of 4.2000E+08yrs "}, {"name": "Flux4", "desc": "? Flux at a system age of 5.6000E+08yrs "}, {"name": "Flux5", "desc": "? Flux at a system age of 7.0000E+08yrs "}, {"name": "Flux6", "desc": "? Flux at a system age of 8.4000E+08yrs "}, {"name": "Flux7", "desc": "? Flux at a system age of 9.8000E+08yrs "}, {"name": "Flux8", "desc": "? Flux at a system age of 1.1200E+09yrs "}, {"name": "Flux9", "desc": "? Flux at a system age of 1.2600E+09yrs "}, {"name": "Flux10", "desc": "? Flux at a system age of 1.4000E+09yrs "}, {"name": "Flux11", "desc": "? Flux at a system age of 1.5400E+09yrs "}, {"name": "Flux12", "desc": "? Flux at a system age of 1.6800E+09yrs "}, {"name": "Flux13", "desc": "? Flux at a system age of 1.8200E+09yrs "}, {"name": "Flux14", "desc": "? Flux at a system age of 1.9600E+09yrs "}, {"name": "Flux15", "desc": "? Flux at a system age of 2.1000E+09yrs "}, {"name": "Flux16", "desc": "? Flux at a system age of 2.2400E+09yrs "}, {"name": "Flux17", "desc": "? Flux at a system age of 2.3800E+09yrs "}, {"name": "Flux18", "desc": "? Flux at a system age of 2.5200E+09yrs "}, {"name": "Flux19", "desc": "? Flux at a system age of 2.6600E+09yrs "}, {"name": "Flux20", "desc": "? Flux at a system age of 2.8000E+09yrs "}, {"name": "Flux21", "desc": "? Flux at a system age of 2.9400E+09yrs "}, {"name": "Flux22", "desc": "? Flux at a system age of 3.0800E+09yrs "}, {"name": "Flux23", "desc": "? Flux at a system age of 3.2200E+09yrs "}, {"name": "Flux24", "desc": "? Flux at a system age of 3.3600E+09yrs "}, {"name": "Flux25", "desc": "? Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? Flux at a system age of 4.7600E+09yrs "}, {"name": "Flux35", "desc": "Flux at a system age of 4.9000E+09yrs "}, {"name": "Flux36", "desc": "Flux at a system age of 5.0400E+09yrs "}, {"name": "Flux37", "desc": "Flux at a system age of 5.1800E+09yrs "}, {"name": "Flux38", "desc": "Flux at a system age of 5.3200E+09yrs "}, {"name": "Flux39", "desc": "Flux at a system age of 5.4600E+09yrs "}, {"name": "Flux40", "desc": "Flux at a system age of 5.6000E+09yrs "}, {"name": "Flux41", "desc": "Flux at a system age of 5.7400E+09yrs "}, {"name": "Flux42", "desc": "Flux at a system age of 5.8800E+09yrs "}, {"name": "Flux43", "desc": "Flux at a system age of 6.0200E+09yrs "}, {"name": "Flux44", "desc": "Flux at a system age of 6.1600E+09yrs "}, {"name": "Flux45", "desc": "Flux at a system age of 6.3000E+09yrs "}, {"name": "Flux46", "desc": "Flux at a system age of 6.4400E+09yrs "}, {"name": "Flux47", "desc": "Flux at a system age of 6.5800E+09yrs "}, {"name": "Flux48", "desc": "Flux at a system age of 6.7200E+09yrs "}, {"name": "Flux49", "desc": "Flux at a system age of 6.8600E+09yrs "}, {"name": "Flux51", "desc": "Flux at a system age of 7.0000E+09yrs "}, {"name": "Flux52", "desc": "Flux at a system age of 7.1400E+09yrs "}, {"name": "Flux53", "desc": "Flux at a system age of 7.2800E+09yrs "}, {"name": "Flux54", "desc": "Flux at a system age of 7.4200E+09yrs "}, {"name": "Flux55", "desc": "Flux at a system age of 7.5600E+09yrs "}, {"name": "Flux56", "desc": "Flux at a system age of 7.7000E+09yrs "}, {"name": "Flux57", "desc": "Flux at a system age of 7.8400E+09yrs "}, {"name": "Flux58", "desc": "Flux at a system age of 7.9800E+09yrs "}, {"name": "Flux59", "desc": "Flux at a system age of 8.1200E+09yrs "}, {"name": "Flux60", "desc": "Flux at a system age of 8.2600E+09yrs "}, {"name": "Flux61", "desc": "Flux at a system age of 8.4000E+09yrs "}, {"name": "Flux62", "desc": "Flux at a system age of 8.5400E+09yrs "}, {"name": "Flux63", "desc": "Flux at a system age of 8.6800E+09yrs "}, {"name": "Flux64", "desc": "Flux at a system age of 8.8200E+09yrs "}, {"name": "Flux65", "desc": "Flux at a system age of 8.9600E+09yrs "}, {"name": "Flux66", "desc": "Flux at a system age of 9.1000E+09yrs "}, {"name": "Flux67", "desc": "Flux at a system age of 9.2400E+09yrs "}, {"name": "Flux68", "desc": "Flux at a system age of 9.3800E+09yrs "}, {"name": "Flux69", "desc": "Flux at a system age of 9.5200E+09yrs "}, {"name": "Flux70", "desc": "Flux at a system age of 9.6600E+09yrs "}, {"name": "Flux71", "desc": "Flux at a system age of 9.8000E+09yrs "}, {"name": "Flux72", "desc": "Flux at a system age of 9.9400E+09yrs "}, {"name": "Flux73", "desc": "Flux at a system age of 1.0080E+10yrs "}, {"name": "Flux74", "desc": "Flux at a system age of 1.0220E+10yrs "}, {"name": "Flux75", "desc": "Flux at a system age of 1.0360E+10yrs "}, {"name": "Flux76", "desc": "Flux at a system age of 1.0500E+10yrs "}, {"name": "Flux77", "desc": "Flux at a system age of 1.0640E+10yrs "}, {"name": "Flux78", "desc": "Flux at a system age of 1.0780E+10yrs "}, {"name": "Flux79", "desc": "Flux at a system age of 1.0920E+10yrs "}, {"name": "Flux80", "desc": "Flux at a system age of 1.1060E+10yrs "}, {"name": "Flux81", "desc": "Flux at a system age of 1.1200E+10yrs "}, {"name": "Flux82", "desc": "Flux at a system age of 1.1340E+10yrs "}, {"name": "Flux83", "desc": "Flux at a system age of 1.1480E+10yrs "}, {"name": "Flux84", "desc": "Flux at a system age of 1.1620E+10yrs "}, {"name": "Flux85", "desc": "Flux at a system age of 1.1760E+10yrs "}, {"name": "Flux86", "desc": "Flux at a system age of 1.1900E+10yrs "}, {"name": "Flux87", "desc": "Flux at a system age of 1.2040E+10yrs "}, {"name": "Flux88", "desc": "Flux at a system age of 1.2180E+10yrs "}, {"name": "Flux89", "desc": "Flux at a system age of 1.2320E+10yrs "}, {"name": "Flux90", "desc": "Flux at a system age of 1.2460E+10yrs "}, {"name": "Flux91", "desc": "Flux at a system age of 1.2600E+10yrs "}, {"name": "Flux92", "desc": "Flux at a system age of 1.2740E+10yrs "}, {"name": "Flux93", "desc": "Flux at a system age of 1.2880E+10yrs "}, {"name": "Flux94", "desc": "Flux at a system age of 1.3020E+10yrs "}, {"name": "Flux95", "desc": "Flux at a system age of 1.3160E+10yrs "}, {"name": "Flux96", "desc": "Flux at a system age of 1.3300E+10yrs "}, {"name": "Flux97", "desc": "Flux at a system age of 1.3440E+10yrs "}, {"name": "Flux98", "desc": "Flux at a system age of 1.3580E+10yrs "}, {"name": "Flux99", "desc": "Flux at a system age of 1.3720E+10yrs "}, {"name": "Flux100", "desc": "Flux at a system age of 1.3860E+10yrs "}, {"name": "Flux101", "desc": "Flux at a system age of 1.4000E+10yrs "}]}, {"name": "pl1esd.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 1 E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) (1) "}, {"name": "z0", "desc": "? Initial redshift (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "Age", "desc": "Actual age "}, {"name": "MassSys", "desc": "Total mass of system "}, {"name": "MassStar", "desc": "Total mass of stars in system "}, {"name": "MassGas", "desc": "Total mass of gas in system "}, {"name": "Y", "desc": "Helium abundance, Y "}, {"name": "Z0", "desc": "[0.00000] Metallicity Z (0 for SSPs) "}, {"name": "SFR", "desc": "Star formation rate "}, {"name": "---", "desc": "[0.00000] ? "}, {"name": "ezj", "desc": "[0.00000] Ejection rate (0 for SSPs) "}]}, {"name": "pl2esd.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 2 E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "Age", "desc": "Actual age "}, {"name": "mbol", "desc": "Bolometric magnitude "}, {"name": "Umag", "desc": "Johnson U magnitude "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "Rmag", "desc": "Johnson R magnitude "}, {"name": "Imag", "desc": "Johnson I magnitude "}, {"name": "Jmag", "desc": "Johnson J magnitude "}, {"name": "Hmag", "desc": "Johnson H magnitude "}, {"name": "Kmag", "desc": "Johnson K magnitude "}, {"name": "Lmag", "desc": "[0.0000] Johnson L magnitude (not included in the isochrones)"}]}, {"name": "pl3esd.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 3 E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "Age", "desc": "Actual age "}, {"name": "U-B", "desc": "Color U-B "}, {"name": "B-V", "desc": "Color B-V "}, {"name": "V-R", "desc": "Color V-R "}, {"name": "R-I", "desc": "Color R-I "}, {"name": "I-J", "desc": "Color I-J "}, {"name": "J-H", "desc": "Color J-H "}, {"name": "H-K", "desc": "Color H-K "}, {"name": "L-J", "desc": "[0.0000] Color L-J (not included) "}, {"name": "U-V", "desc": "Color U-V "}, {"name": "V-K", "desc": "Color V-K "}]}, {"name": "pl4esd.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 4 E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "Age", "desc": "Actual age "}, {"name": "lbol", "desc": "Bolometric luminosity "}, {"name": "lUmag", "desc": "Luminosity in U band "}, {"name": "lBmag", "desc": "Luminosity in B band "}, {"name": "lVmag", "desc": "Luminosity in V band "}, {"name": "lRmag", "desc": "Luminosity in R band "}, {"name": "lImag", "desc": "Luminosity in I band "}, {"name": "lJmag", "desc": "Luminosity in J band "}, {"name": "lHmag", "desc": "Luminosity in H band "}, {"name": "lKmag", "desc": "Luminosity in k band "}, {"name": "lLmag", "desc": "[0.0000] Luminosity in L band (not included) "}, {"name": "lLya", "desc": "[0.0000] Lyman-continuum-photons (not calculated)"}]}, {"name": "johshift.dat", "desc": "Luminosities and colors from the spectra in Johnson filter-system, Scalo IMF, Shift Only Elliptical or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "Umag", "desc": "Johnson U magnitude "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "Rmag", "desc": "Johnson R magnitude "}, {"name": "Imag", "desc": "Johnson I magnitude "}, {"name": "Jmag", "desc": "Johnson J magnitude "}, {"name": "Hmag", "desc": "Johnson H magnitude "}, {"name": "Kmag", "desc": "Johnson K magnitude "}, {"name": "Lmag", "desc": "Johnson L magnitude "}, {"name": "U-B", "desc": "Johnson U-B colour index "}, {"name": "B-V", "desc": "Johnson B-V colour index "}, {"name": "U-V", "desc": "Johnson U-V colour index "}, {"name": "V-R", "desc": "Johnson V-R colour index "}, {"name": "R-I", "desc": "Johnson R-I colour index "}, {"name": "V-K", "desc": "Johnson V-K colour index "}, {"name": "I-K", "desc": "Johnson I-K colour index "}, {"name": "B-R", "desc": "Johnson B-R colour index "}, {"name": "B-H", "desc": "Johnson B-H colour index "}, {"name": "J-H", "desc": "Johnson J-H colour index "}, {"name": "H-K", "desc": "Johnson H-K colour index "}]}, {"name": "magshift.dat", "desc": "Luminosities from the spectra in Koo, Thuan & Gunn, Washinton and Stroemgren filter-systems, Scalo IMF, Shift, Only E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? 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Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "kcshift.dat", "desc": "Coefficients of k-correction in luminosity, H0=65 Scalo IMF, Shift, E or SD galaxies", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? 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Redshift "}, {"name": "cu", "desc": "? e or k-correction for Johnson U "}, {"name": "cb", "desc": "? e or k-correction for Johnson B "}, {"name": "cv", "desc": "? e or k-correction for Johnson V "}, {"name": "cr", "desc": "? e or k-correction for Johnson R "}, {"name": "ci", "desc": "? e or k-correction for Johnson I "}, {"name": "cj", "desc": "? e or k-correction for Johnson J "}, {"name": "ch", "desc": "? e or k-correction for Johnson H "}, {"name": "ck", "desc": "? e or k-correction for Johnson K "}, {"name": "cku", "desc": "e or k-correction for Koo u "}, {"name": "ckb", "desc": "e or k-correction for Koo j "}, {"name": "ckv", "desc": "e or k-correction for Koo f "}, {"name": "ckr", "desc": "e or k-correction for Koo n "}, {"name": "cgi", "desc": "e or k-correction for Thuan & gunn g "}, {"name": "cgj", "desc": "e or k-correction for Thuan & gunn r "}, {"name": "cF160BW", "desc": "e or k-correction HST F160BW "}, {"name": "cF170W", "desc": "e or k-correction HST F170W "}, {"name": "cF185W", "desc": "e or k-correction HST F185W "}, {"name": "cF218W", "desc": "e or k-correction HST F218W "}, {"name": "cF255W", "desc": "e or k-correction HST F255W "}, {"name": "cF300W", "desc": "e or k-correction HST F300W <==> U(HDF) "}, {"name": "cF336W", "desc": "e or k-correction HST F336W "}, {"name": "cF380W", "desc": "e or k-correction HST F380W "}, {"name": "cF439W", "desc": "e or k-correction HST F439W "}, {"name": "cF450W", "desc": "e or k-correction HST F450W <==> B(HDF) "}, {"name": "cF555W", "desc": "e or k-correction HST F555W <==> V(YSC) "}, {"name": "cF569W", "desc": "e or k-correction HST F569W "}, {"name": "cF606W", "desc": "e or k-correction HST F606W <==> V(HDF) "}, {"name": "cF622W", "desc": "e or k-correction HST F622W "}, {"name": "cF675W", "desc": "e or k-correction HST F675W "}, {"name": "cF702W", "desc": "e or k-correction HST F702W "}, {"name": "eF791W", "desc": "e or k-correction HST F791W "}, {"name": "eF814W", "desc": "e or k-correction HST F814W <==> I(HDF) "}]}, {"name": "gspshift.dat", "desc": "Spectra, with Scalo IMF, Shift, E or SD galaxies ", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial metallicity (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "lambda", "desc": "Wavelength "}, {"name": "Flux1", "desc": "? Flux at a system age of 1.4000E+08yrs "}, {"name": "Flux2", "desc": "? Flux at a system age of 2.8000E+08yrs "}, {"name": "Flux3", "desc": "? Flux at a system age of 4.2000E+08yrs "}, {"name": "Flux4", "desc": "? Flux at a system age of 5.6000E+08yrs "}, {"name": "Flux5", "desc": "? Flux at a system age of 7.0000E+08yrs "}, {"name": "Flux6", "desc": "? Flux at a system age of 8.4000E+08yrs "}, {"name": "Flux7", "desc": "? Flux at a system age of 9.8000E+08yrs "}, {"name": "Flux8", "desc": "? Flux at a system age of 1.1200E+09yrs "}, {"name": "Flux9", "desc": "? Flux at a system age of 1.2600E+09yrs "}, {"name": "Flux10", "desc": "? Flux at a system age of 1.4000E+09yrs "}, {"name": "Flux11", "desc": "? Flux at a system age of 1.5400E+09yrs "}, {"name": "Flux12", "desc": "? Flux at a system age of 1.6800E+09yrs "}, {"name": "Flux13", "desc": "? Flux at a system age of 1.8200E+09yrs "}, {"name": "Flux14", "desc": "? Flux at a system age of 1.9600E+09yrs "}, {"name": "Flux15", "desc": "? Flux at a system age of 2.1000E+09yrs "}, {"name": "Flux16", "desc": "? Flux at a system age of 2.2400E+09yrs "}, {"name": "Flux17", "desc": "? Flux at a system age of 2.3800E+09yrs "}, {"name": "Flux18", "desc": "? Flux at a system age of 2.5200E+09yrs "}, {"name": "Flux19", "desc": "? Flux at a system age of 2.6600E+09yrs "}, {"name": "Flux20", "desc": "? Flux at a system age of 2.8000E+09yrs "}, {"name": "Flux21", "desc": "? Flux at a system age of 2.9400E+09yrs "}, {"name": "Flux22", "desc": "? Flux at a system age of 3.0800E+09yrs "}, {"name": "Flux23", "desc": "? Flux at a system age of 3.2200E+09yrs "}, {"name": "Flux24", "desc": "? Flux at a system age of 3.3600E+09yrs "}, {"name": "Flux25", "desc": "? Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? Flux at a system age of 4.7600E+09yrs "}, {"name": "Flux35", "desc": "Flux at a system age of 4.9000E+09yrs "}, {"name": "Flux36", "desc": "Flux at a system age of 5.0400E+09yrs "}, {"name": "Flux37", "desc": "Flux at a system age of 5.1800E+09yrs "}, {"name": "Flux38", "desc": "Flux at a system age of 5.3200E+09yrs "}, {"name": "Flux39", "desc": "Flux at a system age of 5.4600E+09yrs "}, {"name": "Flux40", "desc": "Flux at a system age of 5.6000E+09yrs "}, {"name": "Flux41", "desc": "Flux at a system age of 5.7400E+09yrs "}, {"name": "Flux42", "desc": "Flux at a system age of 5.8800E+09yrs "}, {"name": "Flux43", "desc": "Flux at a system age of 6.0200E+09yrs "}, {"name": "Flux44", "desc": "Flux at a system age of 6.1600E+09yrs "}, {"name": "Flux45", "desc": "Flux at a system age of 6.3000E+09yrs "}, {"name": "Flux46", "desc": "Flux at a system age of 6.4400E+09yrs "}, {"name": "Flux47", "desc": "Flux at a system age of 6.5800E+09yrs "}, {"name": "Flux48", "desc": "Flux at a system age of 6.7200E+09yrs "}, {"name": "Flux49", "desc": "Flux at a system age of 6.8600E+09yrs "}, {"name": "Flux51", "desc": "Flux at a system age of 7.0000E+09yrs "}, {"name": "Flux52", "desc": "Flux at a system age of 7.1400E+09yrs "}, {"name": "Flux53", "desc": "Flux at a system age of 7.2800E+09yrs "}, {"name": "Flux54", "desc": "Flux at a system age of 7.4200E+09yrs "}, {"name": "Flux55", "desc": "Flux at a system age of 7.5600E+09yrs "}, {"name": "Flux56", "desc": "Flux at a system age of 7.7000E+09yrs "}, {"name": "Flux57", "desc": "Flux at a system age of 7.8400E+09yrs "}, {"name": "Flux58", "desc": "Flux at a system age of 7.9800E+09yrs "}, {"name": "Flux59", "desc": "Flux at a system age of 8.1200E+09yrs "}, {"name": "Flux60", "desc": "Flux at a system age of 8.2600E+09yrs "}, {"name": "Flux61", "desc": "Flux at a system age of 8.4000E+09yrs "}, {"name": "Flux62", "desc": "Flux at a system age of 8.5400E+09yrs "}, {"name": "Flux63", "desc": "Flux at a system age of 8.6800E+09yrs "}, {"name": "Flux64", "desc": "Flux at a system age of 8.8200E+09yrs "}, {"name": "Flux65", "desc": "Flux at a system age of 8.9600E+09yrs "}, {"name": "Flux66", "desc": "Flux at a system age of 9.1000E+09yrs "}, {"name": "Flux67", "desc": "Flux at a system age of 9.2400E+09yrs "}, {"name": "Flux68", "desc": "Flux at a system age of 9.3800E+09yrs "}, {"name": "Flux69", "desc": "Flux at a system age of 9.5200E+09yrs "}, {"name": "Flux70", "desc": "Flux at a system age of 9.6600E+09yrs "}, {"name": "Flux71", "desc": "Flux at a system age of 9.8000E+09yrs "}, {"name": "Flux72", "desc": "Flux at a system age of 9.9400E+09yrs "}, {"name": "Flux73", "desc": "Flux at a system age of 1.0080E+10yrs "}, {"name": "Flux74", "desc": "Flux at a system age of 1.0220E+10yrs "}, {"name": "Flux75", "desc": "Flux at a system age of 1.0360E+10yrs "}, {"name": "Flux76", "desc": "Flux at a system age of 1.0500E+10yrs "}, {"name": "Flux77", "desc": "Flux at a system age of 1.0640E+10yrs "}, {"name": "Flux78", "desc": "Flux at a system age of 1.0780E+10yrs "}, {"name": "Flux79", "desc": "Flux at a system age of 1.0920E+10yrs "}, {"name": "Flux80", "desc": "Flux at a system age of 1.1060E+10yrs "}, {"name": "Flux81", "desc": "Flux at a system age of 1.1200E+10yrs "}, {"name": "Flux82", "desc": "Flux at a system age of 1.1340E+10yrs "}, {"name": "Flux83", "desc": "Flux at a system age of 1.1480E+10yrs "}, {"name": "Flux84", "desc": "Flux at a system age of 1.1620E+10yrs "}, {"name": "Flux85", "desc": "Flux at a system age of 1.1760E+10yrs "}, {"name": "Flux86", "desc": "Flux at a system age of 1.1900E+10yrs "}, {"name": "Flux87", "desc": "Flux at a system age of 1.2040E+10yrs "}, {"name": "Flux88", "desc": "Flux at a system age of 1.2180E+10yrs "}, {"name": "Flux89", "desc": "Flux at a system age of 1.2320E+10yrs "}, {"name": "Flux90", "desc": "Flux at a system age of 1.2460E+10yrs "}, {"name": "Flux91", "desc": "Flux at a system age of 1.2600E+10yrs "}, {"name": "Flux92", "desc": "Flux at a system age of 1.2740E+10yrs "}, {"name": "Flux93", "desc": "Flux at a system age of 1.2880E+10yrs "}, {"name": "Flux94", "desc": "Flux at a system age of 1.3020E+10yrs "}, {"name": "Flux95", "desc": "Flux at a system age of 1.3160E+10yrs "}, {"name": "Flux96", "desc": "Flux at a system age of 1.3300E+10yrs "}, {"name": "Flux97", "desc": "Flux at a system age of 1.3440E+10yrs "}, {"name": "Flux98", "desc": "Flux at a system age of 1.3580E+10yrs "}, {"name": "Flux99", "desc": "Flux at a system age of 1.3720E+10yrs "}, {"name": "Flux100", "desc": "Flux at a system age of 1.3860E+10yrs "}, {"name": "Flux101", "desc": "Flux at a system age of 1.4000E+10yrs "}]}, {"name": "joh50-84.dat", "desc": "Luminosities and colors from the spectra in Johnson filter-system, Scalo IMF, scenario with old disk and young bulge", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "Umag", "desc": "Johnson U magnitude "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "Rmag", "desc": "Johnson R magnitude "}, {"name": "Imag", "desc": "Johnson I magnitude "}, {"name": "Jmag", "desc": "Johnson J magnitude "}, {"name": "Hmag", "desc": "Johnson H magnitude "}, {"name": "Kmag", "desc": "Johnson K magnitude "}, {"name": "Lmag", "desc": "Johnson L magnitude "}, {"name": "U-B", "desc": "Johnson U-B colour index "}, {"name": "B-V", "desc": "Johnson B-V colour index "}, {"name": "U-V", "desc": "Johnson U-V colour index "}, {"name": "V-R", "desc": "Johnson V-R colour index "}, {"name": "R-I", "desc": "Johnson R-I colour index "}, {"name": "V-K", "desc": "Johnson V-K colour index "}, {"name": "I-K", "desc": "Johnson I-K colour index "}, {"name": "B-R", "desc": "Johnson B-R colour index "}, {"name": "B-H", "desc": "Johnson B-H colour index "}, {"name": "J-H", "desc": "Johnson J-H colour index "}, {"name": "H-K", "desc": "Johnson H-K colour index "}]}, {"name": "mag50-84.dat", "desc": "Luminosities from the spectra in Koo, Thuan & Gunn, Washinton and Stroemgren filter-systems, Scalo IMF, old disk and young bulge", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "age", "desc": "Age of system "}, {"name": "kumag", "desc": "Koo u magnitude "}, {"name": "kjmag", "desc": "Koo j magnitude "}, {"name": "kfmag", "desc": "Koo f magnitude "}, {"name": "knmag", "desc": "Koo n magnitude "}, {"name": "gmag", "desc": "Thuan & Gunn g magnitude "}, {"name": "rmag", "desc": "Thuan & Gunn r magnitude "}, {"name": "Cmag", "desc": "Washington C magnitude "}, {"name": "Mmag", "desc": "Washington M magnitude "}, {"name": "T1mag", "desc": "Washington T1 magnitude "}, {"name": "T2mag", "desc": "Washington T2 magnitude "}, {"name": "sumag", "desc": "Stroemgren u magnitude "}, {"name": "svmag", "desc": "Stroemgren v magnitude "}, {"name": "sbmag", "desc": "Stroemgren b magnitude "}, {"name": "symag", "desc": "Stroemgren y magnitude "}]}, {"name": "hst50-84.dat", "desc": "Luminosities from the spectra in HST filter-system, Scalo IMF, old disk and young bulge", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial redshift (not for e and sd models) (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "Age", "desc": "Age of system "}, {"name": "F160BW", "desc": "HST F160BW magnitude "}, {"name": "F170W", "desc": "HST F170W magnitude "}, {"name": "F185W", "desc": "HST F185W magnitude "}, {"name": "F218W", "desc": "HST F218W magnitude "}, {"name": "F255W", "desc": "HST F255W magnitude "}, {"name": "F300W", "desc": "HST F300W = U(HDF) magnitude "}, {"name": "F336W", "desc": "HST F336W magnitude "}, {"name": "F380W", "desc": "HST F380W magnitude "}, {"name": "F439W", "desc": "HST F439W magnitude "}, {"name": "F450W", "desc": "HST F450W = B(HDF) magnitude "}, {"name": "F555W", "desc": "HST F555W = V(YSC) magnitude "}, {"name": "F569W", "desc": "HST F569W magnitude "}, {"name": "F606W", "desc": "HST F606W = V(HDF) magnitude "}, {"name": "F622W", "desc": "HST F622W magnitude "}, {"name": "F675W", "desc": "HST F675W magnitude "}, {"name": "F702W", "desc": "HST F702W magnitude "}, {"name": "F791W", "desc": "HST F791W magnitude "}, {"name": "F814W", "desc": "HST F814W = I(HDF) magnitude "}]}, {"name": "gsp50-84.dat", "desc": "Spectra, with Scalo IMF, old disk and young bulge ", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) "}, {"name": "z0", "desc": "? Initial metallicity (G1) "}, {"name": "Mod", "desc": "[es] e: elliptical, s: sd galaxies (G1) "}, {"name": "J", "desc": "Index "}, {"name": "lambda", "desc": "Wavelength "}, {"name": "Flux1", "desc": "? Flux at a system age of 1.4000E+08yrs "}, {"name": "Flux2", "desc": "? Flux at a system age of 2.8000E+08yrs "}, {"name": "Flux3", "desc": "? Flux at a system age of 4.2000E+08yrs "}, {"name": "Flux4", "desc": "? Flux at a system age of 5.6000E+08yrs "}, {"name": "Flux5", "desc": "? Flux at a system age of 7.0000E+08yrs "}, {"name": "Flux6", "desc": "? Flux at a system age of 8.4000E+08yrs "}, {"name": "Flux7", "desc": "? Flux at a system age of 9.8000E+08yrs "}, {"name": "Flux8", "desc": "? Flux at a system age of 1.1200E+09yrs "}, {"name": "Flux9", "desc": "? Flux at a system age of 1.2600E+09yrs "}, {"name": "Flux10", "desc": "? Flux at a system age of 1.4000E+09yrs "}, {"name": "Flux11", "desc": "? Flux at a system age of 1.5400E+09yrs "}, {"name": "Flux12", "desc": "? Flux at a system age of 1.6800E+09yrs "}, {"name": "Flux13", "desc": "? Flux at a system age of 1.8200E+09yrs "}, {"name": "Flux14", "desc": "? Flux at a system age of 1.9600E+09yrs "}, {"name": "Flux15", "desc": "? Flux at a system age of 2.1000E+09yrs "}, {"name": "Flux16", "desc": "? Flux at a system age of 2.2400E+09yrs "}, {"name": "Flux17", "desc": "? Flux at a system age of 2.3800E+09yrs "}, {"name": "Flux18", "desc": "? Flux at a system age of 2.5200E+09yrs "}, {"name": "Flux19", "desc": "? Flux at a system age of 2.6600E+09yrs "}, {"name": "Flux20", "desc": "? Flux at a system age of 2.8000E+09yrs "}, {"name": "Flux21", "desc": "? Flux at a system age of 2.9400E+09yrs "}, {"name": "Flux22", "desc": "? Flux at a system age of 3.0800E+09yrs "}, {"name": "Flux23", "desc": "? Flux at a system age of 3.2200E+09yrs "}, {"name": "Flux24", "desc": "? Flux at a system age of 3.3600E+09yrs "}, {"name": "Flux25", "desc": "? Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? Flux at a system age of 4.7600E+09yrs "}, {"name": "Flux35", "desc": "Flux at a system age of 4.9000E+09yrs "}, {"name": "Flux36", "desc": "Flux at a system age of 5.0400E+09yrs "}, {"name": "Flux37", "desc": "Flux at a system age of 5.1800E+09yrs "}, {"name": "Flux38", "desc": "Flux at a system age of 5.3200E+09yrs "}, {"name": "Flux39", "desc": "Flux at a system age of 5.4600E+09yrs "}, {"name": "Flux40", "desc": "Flux at a system age of 5.6000E+09yrs "}, {"name": "Flux41", "desc": "Flux at a system age of 5.7400E+09yrs "}, {"name": "Flux42", "desc": "Flux at a system age of 5.8800E+09yrs "}, {"name": "Flux43", "desc": "Flux at a system age of 6.0200E+09yrs "}, {"name": "Flux44", "desc": "Flux at a system age of 6.1600E+09yrs "}, {"name": "Flux45", "desc": "Flux at a system age of 6.3000E+09yrs "}, {"name": "Flux46", "desc": "Flux at a system age of 6.4400E+09yrs "}, {"name": "Flux47", "desc": "Flux at a system age of 6.5800E+09yrs "}, {"name": "Flux48", "desc": "Flux at a system age of 6.7200E+09yrs "}, {"name": "Flux49", "desc": "Flux at a system age of 6.8600E+09yrs "}, {"name": "Flux51", "desc": "Flux at a system age of 7.0000E+09yrs "}, {"name": "Flux52", "desc": "Flux at a system age of 7.1400E+09yrs "}, {"name": "Flux53", "desc": "Flux at a system age of 7.2800E+09yrs "}, {"name": "Flux54", "desc": "Flux at a system age of 7.4200E+09yrs "}, {"name": "Flux55", "desc": "Flux at a system age of 7.5600E+09yrs "}, {"name": "Flux56", "desc": "Flux at a system age of 7.7000E+09yrs "}, {"name": "Flux57", "desc": "Flux at a system age of 7.8400E+09yrs "}, {"name": "Flux58", "desc": "Flux at a system age of 7.9800E+09yrs "}, {"name": "Flux59", "desc": "Flux at a system age of 8.1200E+09yrs "}, {"name": "Flux60", "desc": "Flux at a system age of 8.2600E+09yrs "}, {"name": "Flux61", "desc": "Flux at a system age of 8.4000E+09yrs "}, {"name": "Flux62", "desc": "Flux at a system age of 8.5400E+09yrs "}, {"name": "Flux63", "desc": "Flux at a system age of 8.6800E+09yrs "}, {"name": "Flux64", "desc": "Flux at a system age of 8.8200E+09yrs "}, {"name": "Flux65", "desc": "Flux at a system age of 8.9600E+09yrs "}, {"name": "Flux66", "desc": "Flux at a system age of 9.1000E+09yrs "}, {"name": "Flux67", "desc": "Flux at a system age of 9.2400E+09yrs "}, {"name": "Flux68", "desc": "Flux at a system age of 9.3800E+09yrs "}, {"name": "Flux69", "desc": "Flux at a system age of 9.5200E+09yrs "}, {"name": "Flux70", "desc": "Flux at a system age of 9.6600E+09yrs "}, {"name": "Flux71", "desc": "Flux at a system age of 9.8000E+09yrs "}, {"name": "Flux72", "desc": "Flux at a system age of 9.9400E+09yrs "}, {"name": "Flux73", "desc": "Flux at a system age of 1.0080E+10yrs "}, {"name": "Flux74", "desc": "Flux at a system age of 1.0220E+10yrs "}, {"name": "Flux75", "desc": "Flux at a system age of 1.0360E+10yrs "}, {"name": "Flux76", "desc": "Flux at a system age of 1.0500E+10yrs "}, {"name": "Flux77", "desc": "Flux at a system age of 1.0640E+10yrs "}, {"name": "Flux78", "desc": "Flux at a system age of 1.0780E+10yrs "}, {"name": "Flux79", "desc": "Flux at a system age of 1.0920E+10yrs "}, {"name": "Flux80", "desc": "Flux at a system age of 1.1060E+10yrs "}, {"name": "Flux81", "desc": "Flux at a system age of 1.1200E+10yrs "}, {"name": "Flux82", "desc": "Flux at a system age of 1.1340E+10yrs "}, {"name": "Flux83", "desc": "Flux at a system age of 1.1480E+10yrs "}, {"name": "Flux84", "desc": "Flux at a system age of 1.1620E+10yrs "}, {"name": "Flux85", "desc": "Flux at a system age of 1.1760E+10yrs "}, {"name": "Flux86", "desc": "Flux at a system age of 1.1900E+10yrs "}, {"name": "Flux87", "desc": "Flux at a system age of 1.2040E+10yrs "}, {"name": "Flux88", "desc": "Flux at a system age of 1.2180E+10yrs "}, {"name": "Flux89", "desc": "Flux at a system age of 1.2320E+10yrs "}, {"name": "Flux90", "desc": "Flux at a system age of 1.2460E+10yrs "}, {"name": "Flux91", "desc": "Flux at a system age of 1.2600E+10yrs "}, {"name": "Flux92", "desc": "Flux at a system age of 1.2740E+10yrs "}, {"name": "Flux93", "desc": "Flux at a system age of 1.2880E+10yrs "}, {"name": "Flux94", "desc": "Flux at a system age of 1.3020E+10yrs "}, {"name": "Flux95", "desc": "Flux at a system age of 1.3160E+10yrs "}, {"name": "Flux96", "desc": "Flux at a system age of 1.3300E+10yrs "}, {"name": "Flux97", "desc": "Flux at a system age of 1.3440E+10yrs "}, {"name": "Flux98", "desc": "Flux at a system age of 1.3580E+10yrs "}, {"name": "Flux99", "desc": "Flux at a system age of 1.3720E+10yrs "}, {"name": "Flux100", "desc": "Flux at a system age of 1.3860E+10yrs "}, {"name": "Flux101", "desc": "Flux at a system age of 1.4000E+10yrs "}]}, {"name": "pl150-84.dat", "desc": "Scalo IMF isochrone intrinsic colors, part 1 old disk and young bulge", "columns": [{"name": "Z", "desc": "Metallicity (Z=0.02) (1) "}, {"name": "z0", "desc": "? 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Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? 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Flux at a system age of 1.6800E+09yrs "}, {"name": "Flux13", "desc": "? Flux at a system age of 1.8200E+09yrs "}, {"name": "Flux14", "desc": "? Flux at a system age of 1.9600E+09yrs "}, {"name": "Flux15", "desc": "? Flux at a system age of 2.1000E+09yrs "}, {"name": "Flux16", "desc": "? Flux at a system age of 2.2400E+09yrs "}, {"name": "Flux17", "desc": "? Flux at a system age of 2.3800E+09yrs "}, {"name": "Flux18", "desc": "? Flux at a system age of 2.5200E+09yrs "}, {"name": "Flux19", "desc": "? Flux at a system age of 2.6600E+09yrs "}, {"name": "Flux20", "desc": "? Flux at a system age of 2.8000E+09yrs "}, {"name": "Flux21", "desc": "? Flux at a system age of 2.9400E+09yrs "}, {"name": "Flux22", "desc": "? Flux at a system age of 3.0800E+09yrs "}, {"name": "Flux23", "desc": "? Flux at a system age of 3.2200E+09yrs "}, {"name": "Flux24", "desc": "? Flux at a system age of 3.3600E+09yrs "}, {"name": "Flux25", "desc": "? Flux at a system age of 3.5000E+09yrs "}, {"name": "Flux26", "desc": "? Flux at a system age of 3.6400E+09yrs "}, {"name": "Flux27", "desc": "? Flux at a system age of 3.7800E+09yrs "}, {"name": "Flux28", "desc": "? Flux at a system age of 3.9200E+09yrs "}, {"name": "Flux29", "desc": "? Flux at a system age of 4.0600E+09yrs "}, {"name": "Flux30", "desc": "? Flux at a system age of 4.2000E+09yrs "}, {"name": "Flux31", "desc": "? Flux at a system age of 4.3400E+09yrs "}, {"name": "Flux32", "desc": "? Flux at a system age of 4.4800E+09yrs "}, {"name": "Flux33", "desc": "? Flux at a system age of 4.6200E+09yrs "}, {"name": "Flux34", "desc": "? Flux at a system age of 4.7600E+09yrs "}, {"name": "Flux35", "desc": "Flux at a system age of 4.9000E+09yrs "}, {"name": "Flux36", "desc": "Flux at a system age of 5.0400E+09yrs "}, {"name": "Flux37", "desc": "Flux at a system age of 5.1800E+09yrs "}, {"name": "Flux38", "desc": "Flux at a system age of 5.3200E+09yrs "}, {"name": "Flux39", "desc": "Flux at a system age of 5.4600E+09yrs "}, {"name": "Flux40", "desc": "Flux at a system age of 5.6000E+09yrs "}, {"name": "Flux41", "desc": "Flux at a system age of 5.7400E+09yrs "}, {"name": "Flux42", "desc": "Flux at a system age of 5.8800E+09yrs "}, {"name": "Flux43", "desc": "Flux at a system age of 6.0200E+09yrs "}, {"name": "Flux44", "desc": "Flux at a system age of 6.1600E+09yrs "}, {"name": "Flux45", "desc": "Flux at a system age of 6.3000E+09yrs "}, {"name": "Flux46", "desc": "Flux at a system age of 6.4400E+09yrs "}, {"name": "Flux47", "desc": "Flux at a system age of 6.5800E+09yrs "}, {"name": "Flux48", "desc": "Flux at a system age of 6.7200E+09yrs "}, {"name": "Flux49", "desc": "Flux at a system age of 6.8600E+09yrs "}, {"name": "Flux51", "desc": "Flux at a system age of 7.0000E+09yrs "}, {"name": "Flux52", "desc": "Flux at a system age of 7.1400E+09yrs "}, {"name": "Flux53", "desc": "Flux at a system age of 7.2800E+09yrs "}, {"name": "Flux54", "desc": "Flux at a system age of 7.4200E+09yrs "}, {"name": "Flux55", "desc": "Flux at a system age of 7.5600E+09yrs "}, {"name": "Flux56", "desc": "Flux at a system age of 7.7000E+09yrs "}, {"name": "Flux57", "desc": "Flux at a system age of 7.8400E+09yrs "}, {"name": "Flux58", "desc": "Flux at a system age of 7.9800E+09yrs "}, {"name": "Flux59", "desc": "Flux at a system age of 8.1200E+09yrs "}, {"name": "Flux60", "desc": "Flux at a system age of 8.2600E+09yrs "}, {"name": "Flux61", "desc": "Flux at a system age of 8.4000E+09yrs "}, {"name": "Flux62", "desc": "Flux at a system age of 8.5400E+09yrs "}, {"name": "Flux63", "desc": "Flux at a system age of 8.6800E+09yrs "}, 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III.", "title_create": "Anders+, 2003", "year": "2003", "author": "Anders P., Fritze-v.Alvensleben U.", "title_pub": "Spectral and photometric evolution of young stellar populations: The impact of gaseous emission at various metallicities.", "first_author": "Anders P.", "ref_biblio": [""], "bibcode": ["2003A&A...401.1063A"], "see_also": ["http://www.uni-sw.gwdg.de/~galev : The Goettingen Galaxy Evolution Group", "J/A+A/392/1 : Spectrophotometry of simulated SSPs (Schulz+, 2002)", "J/A+A/398/89 : Evolutionary synthesis models. II. (Schulz+, 2003)"], "keyword_cds": "Clusters, globular ; Clusters, open ; Spectrophotometry ; Colors", "keyword_pub": "globular clusters: general - open clusters and associations: general - galaxies: star clusters - galaxies: evolution", "abstract": ["We include gaseous continuum and line emission into our GALEV models", "for the spectral and photometric evolution of Simple Stellar", "Populations (SSPs) for various metallicities in the range", "0.02<=Z/Z_{Sun}_<=2.5. This allows to extend them to significantly", "younger ages than before. They now cover the age range from 4 Myr all", "through 14 Gyr. We point out the very important contributions of", "gaseous emission to broad band fluxes and their strong metallicity", "dependence during very early evolutionary stages of star clusters,", "galaxies or subgalactic fragments with vigorous ongoing star", "formation. Emission-line contributions are commonly seen in these", "actively star-forming regions. Models without gaseous emission cannot", "explain their observed colors at all, or lead to wrong age estimates.", "We use up-to-date Lyman continuum (=Lyc) emission rates and decided to", "use recent empirical determinations of emission line ratios relative", "to H{beta} for subsolar metallicities. We justify this approach for", "all situations where no or not enough spectral information is", "available to determine all the parameters required by photoionization", "models. The effects of gaseous line and continuum emission on broad", "band fluxes are shown for different metallicities and as a function of", "age. In addition to the many filter systems already included in our", "earlier models, we here also include the HST NICMOS and Advanced", "Camera for Surveys (=ACS) filter systems."], "description": ["The models are calculated for 5 metallicities, Z=0.0004, Z=0.004,", "Z=0.008, Z=0.02, and Z=0.05, with an assumed IMF Phi(m) = m^{alpha}^,", "salpeter <-> {alpha}=-2.35 for all masses;", "scalo <-> {alpha}=-1.25 for m<=1M_{sun}_,", "{alpha}=-2.35 for 1M_{sun}_"], "bibcode": ["1975A&A....41..413M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_413_37"}} {"id": "J/A+A/413/37", "title_cds": "Synthetic spectra of galaxies", "title_create": "Bicker+, 2004", "year": "2004", "author": "Bicker J., Fritze-V.Alvensleben U., Moeller C.S., Fricke K.J.", "title_pub": "Chemically consistent evolution of galaxies. II. Spectrophotometric evolution from zero to high redshift.", "first_author": "Bicker J.", "ref_biblio": [""], "bibcode": ["2004A&A...413...37B"], "keyword_cds": "", "keyword_pub": "", "mission": "", "description": ["All data are available for following galaxy types: E, Sa, Sb,", "Sc, and Sd.", "The e and k- corrections and the apparent magnitudes (VEGAMAG system)", "are given for the Johnson-Cousins-Bessell&Brett U, B, V, Rc, Ic, J, H,", "K passbands and for the HST/WFPC2 wide-band passbands up to a redshift", "of z=5.", "The spectra are given as a function of redshift and as a", "function of evolution time in the restframe.", "In case of the redshift evolution the k-correction and the", "spectra are given with and without the effect of attenuation.", "For the cosmology we assume H0=65, Omega0=0.1 and a formation", "of galaxies at z=5.", "The fluxes of the spectra are given in [erg/cm^2^/s/{AA}"], "object": [], "curator": "James Marcout, Patricia Bauer [CDS]", "doi_pub": ["10.1051/0004-6361:20031483"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_445_93"}} {"id": "J/A+A/445/93", "title_cds": "Abundances of DLAs", "title_create": "Dessauges-Zavadsky+, 2006", "year": "2006", "author": "Dessauges-Zavadsky M., Prochaska J.X., D'odorico S., Calura F., Matteucci F.", "title_pub": "A new comprehensive set of elemental abundances in DLAs. II. Data analysis and chemical variation studies.", "first_author": "Dessauges-Zavadsky M.", "ref_biblio": [""], "bibcode": ["2006A&A...445...93D"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1051/0004-6361:20053200"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_465_339"}} {"id": "J/A+A/465/339", "title_cds": "Synthetic stellar polarization 400-1000nm", "title_create": "Socas-Navarro+ 2007", "year": "2007", "author": "Socas-Navarro H., Asensio Ramos A., Manso Sainz R.", "title_pub": "A synthetic stellar polarization atlas from 400 to 1000 nm.", "first_author": "Socas-Navarro H.", "ref_biblio": [""], "bibcode": ["2007A&A...465..339S"], "see_also": ["http://download.hao.ucar.edu/pub/PSA : Home Page"], "keyword_cds": "", "keyword_pub": "atlases - stars: atmospheres - stars: magnetic fields - line: formation - polarization - radiative transfer", "abstract": ["With the development of new polarimeters for large telescopes, the", "spectro-polarimetric study of astrophysical bodies is becoming", "feasible and, indeed, more frequent. In particular, this is permitting", "the observational study of stellar magnetic fields.", "With the aim to optimize and interpret this kind of observations, we", "have produced a spectral atlas of circular polarization in a grid of", "stellar atmospheric models with effective temperatures between 3500", "and 10000K, surface gravities log(g)=3.5-5, metallicities between", "10^-2^ and 1, and magnetic field strengths of 100, 1000 and 5000G."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1051/0004-6361:20066388"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_468_o.205"}} {"id": "J/A+A/468/205", "title_cds": "Spectra of red giants and supergiants", "title_create": "Lancon+, 2007", "year": "2007", "author": "Lancon A., Hauschildt P.H., Ladjal D., Mouhcine M.", "title_pub": "Near-IR spectra of red supergiants and giants. I- Models with solar and with mixing-induced surface abundance ratios.", "first_author": "Lancon A.", "ref_biblio": [""], "bibcode": ["2007A&A...468..205L"], "keyword_cds": "Stars, giant ; Stars, supergiant ; Spectra, infrared ; Models", "keyword_pub": "stars: fundamental parameters - stars: abundances - infrared: stars - stars: atmospheres", "abstract": ["It remains difficult to interpret the near-IR emission of young", "stellar populations. One main reason is our incomplete understanding", "of the spectra of luminous red stars. This work provides a grid of", "theoretical spectra of red giant (RG) and red supergiant (RSG) stars,", "that extends through optical and near-IR wavelengths. For the first", "time, models are also provided with modified surface abundances of C,", "N and O, as a step towards accounting for the changes that occur due", "to convective dredge-up in red supergiants or may occur at earlier", "evolutionary stages in the case of rotation. The aims are (i) to", "assess how well current models reproduce observed spectra, in", "particular in the near-IR; (ii) to quantify the effects of the", "abundance changes on the spectra; and (iii) to determine how these", "changes affect estimates of fundamental stellar parameters."], "description": ["Each FITS file in this directory contains a theoretical stellar", "spectrum. The spherical model atmospheres and the synthetic spectra", "were computed with PHOENIX version 13.11.00B as described in the", "article, with an initial wavelength sampling step of 0.01nm in the", "wavelength range of interest [510nm-2490nm]. The spectra made", "available here have been smoothed with a Gaussian with a full width", "at half maximum of 0.2nm. They are resampled with a wavelength step", "of 0.025nm."], "date_update": "14-Aug-2007", "tables": [{"name": "table1.dat", "desc": "List of the spectra ", "columns": [{"name": "Model", "desc": "Model (m15rsg, m15solar or m1solar) "}, {"name": "Mass", "desc": "Mass "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "FileName", "desc": "Name of the fits file "}]}, {"name": "m15rsg/*", "desc": "RSG-specific abundances, M=15M_{sun}_ model spectra ", "columns": []}, {"name": "m15solar/*", "desc": "Solar abundances, M=15M_{sun}_ model spectra ", "columns": []}, {"name": "m1solar/*", "desc": "Solar abundances, M=1M_{sun}_ model spectra ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_636_A2"}} {"id": "J/A+A/636/A2", "title_cds": "HII regions detected in absorption", "title_create": "Polderman+, 2020", "year": "2020", "author": "Polderman I.M., Haverkorn M., Jaffe T.R.", "title_pub": "A more detailed look at Galactic magnetic field models: using free-free absorption in HII regions.", "first_author": "Polderman I.M.", "ref_biblio": [""], "bibcode": ["2020A&A...636A...2P"], "see_also": ["J/AJ/132/242 : H II absorption regions at 74MHz (Nord+, 2006)"], "keyword_cds": "H II regions ; Magnetic fields", "keyword_pub": "cosmic rays - ISM: magnetic fields - HII regions - Galaxy: structure - radio continuum: ISM - catalogs", "abstract": ["Cosmic rays (CRs) and the Galactic magnetic field (GMF) are", "fundamental actors in many processes in the Milky Way. The observed", "interaction product of these actors is Galactic synchrotron emission", "integrated over the line of sight (LOS). A comparison to simulations", "can be made with this tracer using existing GMF models and CR density", "models. This probes the GMF strength and morphology and the CR", "density.", "Our aim is to provide insight into the Galactic CR density and the", "distribution and morphology of the GMF strength by exploring and", "explaining the differences between the simulations and observations of", "synchrotron intensity.", "At low radio frequencies HII regions become opaque due to free-free", "absorption. Using these HII regions we can measure the synchrotron", "intensity over a part of the LOS through the Galaxy. The measured", "intensity per unit path length, that is, the emissivity, for HII", "regions at different distances, allows us to probe the variation in", "synchrotron emission not only across the sky but also in the third", "dimension of distance. Performing these measurements on a large scale", "is one of the new applications of the window opened by current", "low-frequency arrays. Using a number of existing GMF models in", "conjunction with the Galactic CR modeling code GALPROP, we can", "simulate these synchrotron emissivities.", "We present an updated catalog, compiled from the literature, of", "low-frequency absorption measurements of HII regions, their distances,", "and electron temperatures. We report a simulated emissivity that shows", "a compatible trend for HII regions that are near the observer.", "However, we observe a systematically increasing synchrotron emissivity", "for HII regions that are far from the observer, which is not", "compatible with the values simulated by the GMF models and GALPROP.", "Current GMF models plus a GALPROP generated CR density model cannot", "explain low-frequency absorption measurements. One possibility is that", "distances to all HII regions catalogued at the kinematic \"far\"", "distance are erroneously determined, although this is unlikely since", "it ignores all evidence for far distances in the literature. However,", "a detection bias due to the nature of this tracer requires us to keep", "in mind that certain sources may be missed in an observation. The", "other possibilities are an enhanced emissivity in the outer Galaxy or", "a diminished emissivity in the inner Galaxy."], "description": ["A significant part of the data in the Polderman et al.", "(2019A&A...621A.127P, Cat. J/A+A/621/A127) catalog comes from the work", "of Nord et al. (2006AJ....132..242N, Cat. J/AJ/132/242; hereafter", "N06). For some of these sources, newdistance information is now", "available. Therefore, in our catalog we update both the number of", "sources from N06 and their distances in three ways."], "type": ["OC"], "data": "", "date_update": "19-Apr-2021", "tables": [{"name": "tablea1.dat", "desc": "Complete and updated catalog of HII regions detected in absorption", "columns": [{"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "Dist", "desc": "Distance from the Sun to the HII region "}, {"name": "n_Dist", "desc": "[5] Note on Dist (1) "}, {"name": "e_Dist", "desc": "rms uncertainty on Distance "}, {"name": "Tobs", "desc": "Brightness temperature derived from the measured intensity at the observing frequency"}, {"name": "n_Tobs", "desc": "[2] Note on Tobs (1) "}, {"name": "e_Tobs", "desc": "rms uncertainty on Tobs "}, {"name": "T", "desc": "Synchrotron brightness temperature of the column in front (n_T=F) or behind (n_T=B) the HII region"}, {"name": "f_T", "desc": "[a] Flag on T (1) "}, {"name": "e_T", "desc": "rms uncertainty on T "}, {"name": "n_T", "desc": "[FB] front or behind for synchrotron brightness temperature"}, {"name": "Te", "desc": "Electron temperature of the HII region "}, {"name": "e_Te", "desc": "rms uncertainty on Te "}, {"name": "n_Te", "desc": "[1,3] Note on e_Te (1) "}, {"name": "eps", "desc": "Emissivity of the column in front (n_eps=F) or behind (n_eps=B) the HII region"}, {"name": "e_eps", "desc": "rms uncertianty on eps "}, {"name": "n_eps", "desc": "[FB] front or behind for emissivity "}, {"name": "Source", "desc": "Origin paper of the data (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+A_646_A103"}} {"id": "J/A+A/646/A103", "title_cds": "YSO candidates in S169", "title_create": "Duronea+, 2021", "year": "2021", "author": "Duronea N.U., Cichowolski S., Bronfman L., Mendoza E., Finger R., Suad L.A., Corti M., Reynoso E.M.", "title_pub": "Physical characterization of S169: a prototypical IR bubble associated with the massive star-forming region IRAS 12326-6245.", "first_author": "Duronea N.U.", "ref_biblio": [""], "bibcode": ["2021A&A...646A.103D"], "see_also": ["V/114 : MSX6C Infrared Point Source Catalog (Egan+ 2003)", "II/311 : WISE All-Sky Data Release (Cutri+ 2012)", "II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008)"], "keyword_cds": "Interstellar medium ; YSOs ; Photometry, infrared", "keyword_pub": "ISM: bubbles - HII regions - ISM: molecules - ISM: kinematics and dynamics", "abstract": ["With the aim of studying the physical properties of Galactic IR", "bubbles and to explore their impact in massive star formation, we", "present a study of the IR bubble S169, associated with the massive", "star forming region IRAS 12326-6245.", "We used CO (2-1),^13^CO (2-1), C^18^O (2-1), HCN (3-2), and HCO^+^", "(3-2) line data obtained with the APEX telescope using the on-the-fly", "full sampling technique to study the properties of the molecular gas", "in the nebula and the IRAS source. To analyze the properties and", "distribution of the dust, we made use of images obtained from the", "IRAC-GLIMPSE, Herschel, and ATLASGAL archives. The properties of the", "ionized gas in the nebula were studied using radio continuum and", "H{alpha} images obtained from the SUMSS survey and SuperCOSMOS", "database, respectively. In our search for stellar and protostellar", "objects in the region, we used point source calalogs obtained from the", "MSX, WISE, GLIMPSE, 2MASS, AAVSO, ASCC-2.5V3, and GAIA databases.", "The new APEX observations allowed us to identify three molecular", "components, each one associated with different regions of the nebula,", "namely: at -39km/s (component A), -25km/s (component B), and -17km/s", "(component C). Component A is shown to be the most dense and clumpy.", "Six molecular condensations (MC1 to MC6) were identified in this", "component, with MC3 (the densest and more massive one) being the", "molecular counterpart of IRAS 12326-6245. For this source, we", "estimated an H_2_ column density up to 8x10^23^cm^-2^. An LTE analysis", "of the high density tracer lines HCO^+^ (3-2) and HCN (3-2) on this", "source, assuming 50 and 150K, respectively, indicates column densities", "of N(HCO^+^)=(5.2+/-0.1)x10^13^cm^-2^ and", "N(HCN)=(1.9+/-0.5)x10^14^cm^-2^. To explain the morphology and", "velocity of components A, B, and C, we propose a simple model", "consisting of a partially complete semisphere-like structure expanding", "at ~12km/s. The introduction of this model has led to a discussion", "about the distance to both S169 and IRAS 12326-6245, which was", "estimated to be ~2kpc. Several candidate YSOs were identified,", "projected mostly onto the molecular condensations MC3, MC4, and MC5,", "which indicates that the star-formation process is very active at the", "borders of the nebula. A comparison between observable and modeled", "parameters was not enough to discern whether the collect-and-collapse", "mechanism is acting at the edge of S169. However, other processes such", "as radiative-driven implosion or even a combination of both", "mechanisms, namely, collect-and-collapse and radiative-driven", "implosion, could be acting simultaneously in the region."], "description": ["As part of a broader project aimed at characterizing and studying the", "physical properties of Galactic IR bubbles and their surroundings, we", "present a multiwavelength analysis of the southern IR dust bubble S169", "associated with the massive star forming core IRAS 12326-6245.", "Table A1 list YSO candidates obtained from MSX, WISE, and Spitzer", "catalogs."], "object": ["12 35 31.9 -62 58 16 S169 = [CPA2006] S169"], "type": ["CCC"], "data": "", "date_update": "22-Apr-2021", "tables": [{"name": "tablea1m.dat", "desc": "YSO candidates obtained from MSX catalog ", "columns": [{"name": "Origin", "desc": "[MSX ] Source origin "}, {"name": "Seq", "desc": "[1/2] Sequential number "}, {"name": "Name", "desc": "Source name, GLLL.llll+BB.bbbb, MSX6C GLLL.llll+BB.bbbb in Simbad"}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "F8", "desc": "MSX6C 8.28um flux density "}, {"name": "F12", "desc": "MSX6C 12.13um flux density "}, {"name": "F14", "desc": "MSX6C 14.65um flux density "}, {"name": "F21", "desc": "MSX6C 21.34um flux density "}, {"name": "Note", "desc": "Notes (class, match with other YSO and with ^13^CO/CO or IR structure)"}]}, {"name": "tablea1w.dat", "desc": "YSO candidates obtained from WISE catalogs ", "columns": [{"name": "Origin", "desc": "[WISE ] Source origin "}, {"name": "Seq", "desc": "[3/50] Sequential number "}, {"name": "Name", "desc": "Source name, JHHMMSS.ss+DDMMSS.s, WISE JHHMMSS.ss+DDMMSS.s"}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "W1", "desc": "WISE W1 magnitude "}, {"name": "W2", "desc": "WISE W2 magnitude "}, {"name": "W3", "desc": "WISE W3 magnitude "}, {"name": "W4", "desc": "WISE W4 magnitude "}, {"name": "Note", "desc": "Notes (class, match with other YSO and with ^13^CO/CO or IR structure)"}]}, {"name": "tablea1s.dat", "desc": "YSO candidates obtained from Spitzer catalog ", "columns": [{"name": "Origin", "desc": "[Spitzer] Source origin "}, {"name": "Seq", "desc": "[51/74] Sequential number "}, {"name": "Name", "desc": "Source name, GLLL.llll+BB.bbbb, GLIMPSE GLLL.llll+BB.bbbb"}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "[3.6]", "desc": "Spitzer/IRAC 3.6um magnitude "}, {"name": "[4.5]", "desc": "Spitzer/IRAC 4.5um magnitude "}, {"name": "[5.8]", "desc": "Spitzer/IRAC 5.8um magnitude "}, {"name": "[8.0]", "desc": "Spitzer/IRAC 8.0um magnitude "}, {"name": "Note", "desc": "Notes (class, match with other YSO and with ^13^CO/CO or IR structure)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_101_447"}} {"id": "J/A+AS/101/447", "title_cds": "Spectral Characteristics of RATAN-600 sources", "title_create": "Bursov+ 1993", "year": "1993", "author": "Bursov N.N., Chepurnov A.V., Lipovka N.M., Soboleva N.S., Temirova A.V.", "title_pub": "The spectral characteristics of the Ratan-600 RC-catalog sources.", "first_author": "Bursov N.N.", "ref_biblio": [""], "bibcode": ["1993A&AS..101..447B"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "21-Mar-2000"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_13_133"}} {"id": "J/A+AS/13/133", "title_cds": "UBV observations of Mira variables", "title_create": "Koester+, 1974", "year": "1974", "author": "Koester D.", "title_pub": "UBV observations of Mira variables near maximum light.", "first_author": "Koester D.", "ref_biblio": [""], "bibcode": ["1974A&AS...13..133K"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["UBV observations are presented for 14 Mira variables near maximum", "light and further observations of about 15 variables made at ESO"], "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_21_109"}} {"id": "J/A+AS/21/109", "title_cds": "O-B2 stars in the Large Magellanic Cloud", "title_create": "Brunet+, 1975", "year": "1975", "author": "Brunet J.P., Imbert M., Martin N., Mianes P., Prevot L., Rebeirot E., Rousseau J.", "title_pub": "Recherches dans le Grand Nuage de Magellan. I. Un catalogue de 272 etoiles O-B2 nouvelles.", "first_author": "Brunet J.P.", "ref_biblio": [""], "bibcode": ["1975A&AS...21..109B"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_29_31"}} {"id": "J/A+AS/29/31", "title_cds": "UBV and spectral classes in Loden associations", "title_create": "Loden+, 1977", "year": "1977", "author": "Loden L.O.", "title_pub": "A study of some loose clusterings in the Southern Milky Way.", "first_author": "Loden L.O.", "ref_biblio": [""], "bibcode": ["1977A&AS...29...31L"], "see_also": ["III/40A : Spectral Survey of Southern Milky Way (Loden+ 1976)"], "keyword_cds": "Photometry, UBV ; Associations, stellar ; Spectral types", "keyword_pub": "clusters ; photometry", "description": ["The catalog contains precise coordinates and identifications for 620", "stars observed in 19 loose open clusters observed by Loden as part of", "a larger survey of similar fields. The UBV data come from the original", "publication (observations made at ESO telescopes between 1969 and", "1976), as well as the spectral types (from objective-prism spectra at", "Boyden Observatory, South Africa in 1956 and 1966). The positions and", "identifications were computed by B. Skiff (Lowell Observatory) from", "Loden's charts in November 2009.", "Although reported as sparse open clusters or cluster remnants,", "probably only NGC 4633 = Loden 623 is likely to contain more", "than a few stars that are physically related."], "type": ["OC"], "data": "", "date_update": "17-Nov-2009", "tables": [{"name": "catalog.dat", "desc": "Positions, identifications, UBV and spectral types of stars in 19 loose groupings.", "columns": [{"name": "---", "desc": "[Cl Loden] "}, {"name": "Fld", "desc": "Field number "}, {"name": "Seq", "desc": "Running number of star in field "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[MTU] Source of position (1) "}, {"name": "UCAC2", "desc": "? Designation in UAC2 catalog (I/289) "}, {"name": "CD", "desc": "Cordoba Ducrnmusterung "}, {"name": "m_CD", "desc": "[ab] Multiplicity index on CD "}, {"name": "CPD", "desc": "Cape Photographic Durchmusterung "}, {"name": "m_CPD", "desc": "[ab] Multiplicity index on CPD "}, {"name": "HD", "desc": "? HD identification (Cat. III/1345) "}, {"name": "m_HD", "desc": "[ab] Multiplicity index on CPD "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "B-V", "desc": "? Johnson (B-V) color "}, {"name": "U-B", "desc": "? Johnson (U-B) color "}, {"name": "Sp", "desc": "Spectal type "}, {"name": "Notes", "desc": "Other identifications and notes from B. Skiff "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_32_25"}} {"id": "J/A+AS/32/25", "title_cds": "Spectral types of stars along the Milky Way", "title_create": "Rydstrom+, 1978", "year": "1978", "author": "Rydstrom B.A.", "title_pub": "A spectrophotometric survey of stars along the Milky Way. IV.", "first_author": "Rydstrom B.A.", "ref_biblio": [""], "bibcode": ["1978A&AS...32...25R"], "see_also": ["B/mk: Catalogue of Stellar Spectral Classifications (Skiff, 2009-2014)"], "keyword_cds": "MK spectral classification", "keyword_pub": "narrow-band photometry ; interstellar matther ; Perseus arm", "abstract": ["In the present paper a catalogue of spectrophotometric quantities,", "spectral types, monochromatic magnitudes and colour equivalents is", "given for all stars brighter than the magnitude m_4400_=10.5 in a", "region of the Milky Way in Perseus. No absorption is found for stars", "closer than about r=100pc. The absorbing clouds are situated at", "distances closer than1 kpc and at about 2.5 kpc in the local arm and", "the Perseus arm, respectively. The space between the two arms is free", "from absorption. It is also concluded that the Perseus arm continues", "beyond l=140{deg}, containing not only hydrogen gas but also dust to", "at least l=150{deg}), while the content of OB stars decreases abruptly", "at l=140{deg}."], "data": "", "date_update": "02-Mar-2014", "tables": [{"name": "stars.dat", "desc": " ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "[0/60] Declination J2000 (seconds) "}, {"name": "r", "desc": "[TU] Origin of position (2MASS or UCAC?) "}, {"name": "Vmag", "desc": " "}, {"name": "---", "desc": "[V] "}, {"name": "SpT", "desc": "MK spectral type "}, {"name": "Comments", "desc": "B. Skiff's comments "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_36_83"}} {"id": "J/A+AS/36/83", "title_cds": "UBV photometry in Southern Milky Way", "title_create": "Loden+, 1979", "year": "1979", "author": "Loden L.O.", "title_pub": "Photometry of loose clusterings in the Southern Milky Way.", "first_author": "Loden L.O.", "ref_biblio": [""], "bibcode": ["1979A&AS...36...83L"], "keyword_cds": "Photometry, UBV ; Photometry, uvby ; MK spectral classification", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_4_51"}} {"id": "J/A+AS/4/51", "title_cds": "Catalogue of galactic southern carbon stars", "title_create": "Westerlund, 1971", "year": "1971", "author": "Westerlund B.E.", "title_pub": "A catalogue of carbon stars in the southern Milky Way.", "first_author": "Westerlund B.E.", "ref_biblio": [""], "bibcode": ["1971A&AS....4...51W"], "see_also": ["III/40 : Spectral Survey of Southern Milky Way (Loden+ 1976)", "III/43 : Luminous Stars in the Southern Milky Way (Stephenson+ 1971)", "VII/216 : H-alpha emission regions in Southern Milky Way (Rodgers+ 1960)", "J/other/SAAOC/15.53 : Southern reddened luminous stars II (Kilkenny 1993)", "J/other/SAAOC/15.65 : Southern reddened luminous stars III (Kilkenny+ 1993)", "J/other/SAAOC/15.73 : Southern reddened luminous stars IV (Spencer Jones+ 1993)"], "keyword_cds": "Stars, carbon ; Photometry, infrared", "keyword_pub": "Southern Milky Way - carbon stars - infrared survey", "abstract": ["An objective-prism survey in infrared light has been carried out of", "the Southern Milky Way from l^II^=235{deg} to l^II^=7{deg} and between", "b^II^=+/-5{deg}. The present catalogue gives positions and estimated", "visual and infrared magnitudes for 1124 carbon stars identified in the", "survey. The positions of the stars will be given on overlays to an", "Atlas of the Southern Milky Way, which is under preparation."], "data": "", "date_update": "20-Jun-2002", "tables": [{"name": "table1.dat", "desc": "Carbon stars in the Southern Milky Way ", "columns": [{"name": "[W71b]", "desc": "Sequential number "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "RAs", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "Vmag", "desc": "? V magnitude "}, {"name": "Imag", "desc": "I magnitude "}]}, {"name": "table2.dat", "desc": "Carbon stars identified by Blanco and Munch ", "columns": [{"name": "BM", "desc": "Blanco-Munch (1955BOTT....2l..17B) number (BM IV NNN)"}, {"name": "[W71b]", "desc": "Westerlund number "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_41_173"}} {"id": "J/A+AS/41/173", "title_cds": "UBV and spectral classification in the Galaxy", "title_create": "Loden+, 1980", "year": "1980", "author": "Loden L.O.", "title_pub": "Concluding observations of loose stellar clusterings in the Southern Milky Way.", "first_author": "Loden L.O.", "ref_biblio": [""], "bibcode": ["1980A&AS...41..173L"], "see_also": ["J/A+AS/44/155 :"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["UBV photometry and spectral classification have been performed on 280", "stars in the Carina-Crux-Centaurus-Norma region, suspected of", "belonging to poor open clusters or associations. The work is a", "concluding part of a large project for detecting and listing of such", "objects in order to obtain an improved concept about the true", "frequency of clusterings in the Milky Way. The result indicates that a", "majority of the suspected objects are members of various types of", "physical stellar clusterings, occasionally cluster remnants."], "object": [], "data": "", "date_update": "08-Dec-2013", "tables": [{"name": "loden4.dat", "desc": " ", "columns": [{"name": "---", "desc": "[Cl Loden] "}, {"name": "Cl", "desc": "Cluster number "}, {"name": "Seq", "desc": "Number of star in cluster in Simbad "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[MTU] Source of postiion "}, {"name": "UCAC2", "desc": "? Number in UCAC2 (Cat. I/289) "}, {"name": "CD", "desc": "Cordoba Durchmusterung identification "}, {"name": "m_CD", "desc": "[ab] "}, {"name": "CPD", "desc": "Cape Photographic Durchmusterung identification "}, {"name": "HD", "desc": "? Henry Draper Catalog identification "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "B-V", "desc": "Johnson (B-V) color index "}, {"name": "U-B", "desc": "? Johnson (U-B) color index "}, {"name": "Sp", "desc": "Spectral class (no luminosity class) "}, {"name": "Rem", "desc": "Remarks by B. Skiff "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_41_43"}} {"id": "J/A+AS/41/43", "title_cds": "Color excesses in 5 regions of Milky Way", "title_create": "Johansson, 1980", "year": "1980", "author": "Johansson K.L.V.", "title_pub": "Colour excess and stellar distribution in five selected directions of the Milky Way in Carina, Crux, Centaurus and Norma.", "first_author": "Johansson K.L.V.", "ref_biblio": [""], "bibcode": ["1980A&AS...41...43J"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_43_103"}} {"id": "J/A+AS/43/103", "title_cds": "OB stars found in a Perseus arm field", "title_create": "Wramdemark+, 1981", "year": "1981", "author": "Wramdemark S.", "title_pub": "A study of early-type stars in a Perseus arm area", "first_author": "Wramdemark S.", "ref_biblio": [""], "bibcode": ["1981A&AS...43..103W"], "keyword_cds": "Stars, early-type ; Photometry, UBV", "keyword_pub": "OB stars ; UBV{beta} photometry ; HII retgions ; galactic structure", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "22-Mar-2016"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_44_155"}} {"id": "J/A+AS/44/155", "title_cds": "Loden 28 and 915 photometry", "title_create": "Loden+, 1981", "year": "1981", "author": "Loden L.O.", "title_pub": "A photometric study of two stellar clusterings in the southern Milky Way (and a general consideration on previous and present data concerning galactic clusterings).", "first_author": "Loden L.O.", "ref_biblio": [""], "bibcode": ["1981A&AS...44..155L"], "see_also": ["J/A+AS/41/173 :"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["The paper analyzes photometrically obtained data on approximately 100", "stars and two suspected stellar clusterings in the Southern Milky Way,", "using objective-prism spectral classification methods. The", "observations, carried out with the 50cm ESO telescope, achieved", "estimated accuracy in the photometric parameters of: V:0.023,", "B-V:0.011, U-B:0.022. Strong evidence for the presence of a pronounced", "concentration of A-F (partly evolved) stars was found. One of the", "stellar clusterings found (in Carina) reveals an ordinary B", "association with an estimated 3 million years, while the second (in", "Centaurus), a very loose open cluster, is of intermediate age,", "approximately 100 million years. Conclusively it is stated that,", "wherever in the Milky Way an apparent densification of stars of a", "certain spectral type is found, there is also an enhanced probability", "of detecting a physical clustering of some kind. Moreover, it may be", "difficult to find any line of sight through the Milky Way that does", "not pass through one or more star clusterings within the nearest", "1-2kpc."], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_46_347"}} {"id": "J/A+AS/46/347", "title_cds": "BV photometry of M15 central part", "title_create": "Auriere+, 1981", "year": "1981", "author": "Auriere M., Cordoni J.-P.", "title_pub": "Position, magnitudes and color for stars of the central part of the X-ray globular cluster M 15.", "first_author": "Auriere M.", "ref_biblio": [""], "bibcode": ["1981A&AS...46..347A"], "see_also": ["J/A+AS/119/307 : Position in M15 (Le Campion+, 1996)", "J/AJ/113/1026 : Fabry-Perot Observations of M15 (Gebhardt+ 1997)", "J/AJ/124/3255 : UBV photometry in M15 (van der Marel+, 2002)"], "keyword_cds": "Clusters, globular ; X-ray sources ; Photometry, photographic", "keyword_pub": "globular cluster - X-ray source - stellar photometry", "abstract": ["Position, magnitudes and color for 734 stars in a 1'x1' square field", "centered on the X-ray globular cluster M 15 are given. The", "observations consist of long focus (about 35m) high spatial resolution", "(FWHM down to 0.55arcsec) unfiltered image tube B and V classical", "photographs of the central part of the cluster obtained with two", "specially designed cameras at the 1 meter telescope of Pic du Midi", "Observatory. The reduction procedure is a compromise between automatic", "and interactive techniques. Errors in the data relative to photometry", "as well as astrometry are discussed."], "type": ["OC"], "data": "", "date_update": "06-Jun-2006", "tables": [{"name": "position.dat", "desc": "Star positions (from Simbad) ", "columns": [{"name": "Seq", "desc": "Sequential number "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "SName", "desc": "Simbad name "}]}, {"name": "table2.dat", "desc": "Position, magnitudes and color ", "columns": [{"name": "Seq", "desc": "Sequential number, Cl* NGC 7078 AC NNN in Simbad "}, {"name": "Xpos", "desc": "X position (1) "}, {"name": "Ypos", "desc": "Y position (1) "}, {"name": "R", "desc": "Distance from star No 216 (1) "}, {"name": "Bmag", "desc": "B magnitude "}, {"name": "n_Bmag", "desc": "[)] uncertainty flag on Bmag "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "n_Vmag", "desc": "[)] uncertainty flag on Vmag "}, {"name": "B-V", "desc": "? B-V colour index "}, {"name": "ONames", "desc": "Other names (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_53_255"}} {"id": "J/A+AS/53/255", "title_cds": "Catalog of late-type supergiants in SMC", "title_create": "Prevot+, 1983", "year": "1983", "author": "Prevot L., Martin N., Maurice E., Rebeirot E., Rousseau J.", "title_pub": "A catalogue of late-type supergiant stars in the Small Magellanic Cloud.", "first_author": "Prevot L.", "ref_biblio": [""], "bibcode": ["1983A&AS...53..255P"], "keyword_cds": "", "keyword_pub": "", "abstract": ["An objective-prism survey of the Small Magellanic Cloud has been made", "on IIIaJ plates taken with the 1 m ESO Schmidt telescope and has", "resulted in the detection of nearly 200 late K and M supergiant stars.", "Most of these are new probable members of the SMC which do not appear", "in previous catalogues. The mean visual absolute magnitude of -6.0", "agrees with the visual absolute magnitude of lab-lb galactic", "supergiants of spectral types M0 to M4. The fraction of known variable", "stars found in this catalogue is barely 10 percent; this is 2.5 times", "less than the value found for the corresponding stars in the LMC. The", "catalogue provides accurate 1975 coordinates, finding charts, spectral", "types, V magnitudes, indications concerning radial velocities when", "available and designations of the stars in other catalogues."], "description": ["accurate coordinates for the PMMR red stars in and around the SMC. I", "used the published finder charts to identify the stars. The format of", "the file is the same as for 'mktypes.dat' ---> B/mk. The improved", "coordinates allow the stars to be linked with the similar list by", "Sanduleak (acronym SkKM)."], "curator": "Francois Ochsenbein [CDS]", "alias": ["PMMR"], "type": ["OC"], "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_9_163"}} {"id": "J/A+AS/9/163", "title_cds": "UBV photometry in four areas", "title_create": "Ardeberg+, 1973", "year": "1973", "author": "Ardeberg A., Sarg K., Wramdemark S.", "title_pub": "Photoelectric UBV photometry in four areas of intermediate-high galactic latitude.", "first_author": "Ardeberg A.", "ref_biblio": [""], "bibcode": ["1973A&AS....9..163A"], "keyword_cds": "", "keyword_pub": "UBV photometry ; high latitudes ; galactic structure ; interstellar absorption", "description": ["The table contains photoelectric UBV photometry for a total of 127 stars", "situated in 4 fields with 55"], "bibcode": ["1973A&AS....9..183W"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["UHA"], "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_94_245"}} {"id": "J/A+AS/94/245", "title_cds": "Morphologies of ring-shaped galaxies", "title_create": "Faundez-abans+, 1992", "year": "1992", "author": "Faundez-abans M., Hertling G., Ramirez A.C.", "title_pub": "The visual appearance of the nuclei of ring-shaped galaxies as an alternative classification criterion.", "first_author": "Faundez-abans M.", "ref_biblio": [""], "bibcode": ["1992A&AS...94..245F"], "see_also": ["J/A+AS/104/1 : Faint ring-shaped galaxies near South Pole (Faundez-Abans+ 1994", "J/ApJS/96/39 : Catalog of Southern Ringed Galaxies (Buta+, 1995)", "J/A+AS/129/357 : Morphology of peculiar ring galaxies (Faundez-Abans+ 1998)", "J/ApJS/181/572 : Collisional ring galaxies atlas (Madore+, 2009)"], "keyword_cds": "Galaxy catalogues ; Morphology", "keyword_pub": "galaxies: general ; galaxies, nuclei of ; galaxies: structure of", "abstract": ["An alternative classification of apparent ring galaxies is introduced", "concerning the morphology of the main body (nucleus). For this", "purpose, a list of probable ring galaxies has been prepared based on", "visual inspection of 58 film copies of the J-band SRC/ESO survey. The", "candidate objects have also been classified following Few and Madore's", "(1986MNRAS.222..673F) criteria."], "data": "", "date_update": "07-Dec-2013", "tables": [{"name": "table1.dat", "desc": "List of ring-shpoaed galaxies ", "columns": [{"name": "---", "desc": "[HRG] "}, {"name": "HRG", "desc": "our own designation "}, {"name": "Name", "desc": "Other identifier (ESO or other) "}, {"name": "RAh", "desc": "Right Ascension B1950 (hours) "}, {"name": "RAm", "desc": "Right Ascension B1950 (minutes) "}, {"name": "RAs", "desc": "Right Ascension B1950 (seconds) "}, {"name": "DE-", "desc": "Declination B1950 (sign) "}, {"name": "DEd", "desc": "Declination B1950 (degrees) "}, {"name": "DEm", "desc": "Declination B1950 (minutes) "}, {"name": "DEs", "desc": "Declination B1950 (seconds) "}, {"name": "RAJ.h", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAJ.m", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAJ.s", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DEJ.-", "desc": "Declination J2000 (sign) "}, {"name": "DEJ.d", "desc": "Declination J2000 (degrees) "}, {"name": "DEJ.m", "desc": "Declination J2000 (minutes) "}, {"name": "DEJ.s", "desc": "Declination J2000 (seconds) "}, {"name": "HuCl", "desc": "the estimated Hubble class from the ESO/Uppsala survey, "}, {"name": "Rt", "desc": "[OP? ] the FM ring galaxies classification, "}, {"name": "NuCl", "desc": "the estimated diffuse stellar component classification, "}, {"name": "Comments", "desc": "Comments and remarks "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_A+AS_99_1"}} {"id": "J/A+AS/99/1", "title_cds": "UBV study of open cluster NGC 5460", "title_create": "Claria+, 1993", "year": "1993", "author": "Claria J.J., Lapasset E., Bosio M.A.", "title_pub": "Further observations of stars in the open cluster NGC 5460.", "first_author": "Claria J.J.", "ref_biblio": [""], "bibcode": ["1993A&AS...99....1C"], "keyword_cds": "Photometry, UBV ; Clusters, open", "keyword_pub": "Clusters, open - Photometry, UBV, DDO, CMT1T2", "abstract": ["New photoelectric UBV photometry in the open cluster NGC 5460 is", "presented for 155 stars brighter than 14.0 mag. In addition, six", "comparatively bright red stars in the cluster field were observed in", "the DDO and Washington systems. Nearly 40 percent of the observed", "stars are found to be members or probable members. The analysis of the", "new data yields E(B-V)=0.12+/-0.03 and V(0)-M(v)=9.34+/-0.20", "(740+/-68 pc) for the cluster reddening and true distance modulus,", "respectively. An age of 1.1 x 10 exp 8 yr was derived, which places", "this cluster within the NGC 2516 age group. NGC 5460 does not probably", "contain any red giant."], "data": "", "date_update": "08-Dec-2013", "tables": [{"name": "n5460.dat", "desc": "Photometric magnitudes in the region of NGC 1904 ", "columns": [{"name": "---", "desc": "[Cl* NGC 5460 CLB] "}, {"name": "Seq", "desc": "[1/155] Star sequence number "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[UTM] Source of position "}, {"name": "Vmag", "desc": "Johnson V magnitude "}, {"name": "B-V", "desc": "Johnson B-V magnitude "}, {"name": "U-B", "desc": "? Johnson U-B magnitude "}, {"name": "Comments", "desc": "Additional comments, from B. Skiff. "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_100_569"}} {"id": "J/AJ/100/569", "title_cds": "S stars in the Northern Milky Way", "title_create": "Stephenson+, 1990", "year": "1990", "author": "Stephenson C.B.", "title_pub": "New and relatively faint S stars found in the Northern Milky Way.", "first_author": "Stephenson C.B.", "ref_biblio": [""], "bibcode": ["1990AJ....100..569S"], "keyword_cds": "Stars, S", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["CSS2"], "type": ["OC"], "doi_pub": ["10.1086/115540"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_103_263"}} {"id": "J/AJ/103/263", "title_cds": "Stephenson's highly reddened stars", "title_create": "Stephenson+, 1992", "year": "1992", "author": "Stephenson C.B.", "title_pub": "A list of highly reddened stars likely to be distant luminous stars.", "first_author": "Stephenson C.B.", "ref_biblio": [""], "bibcode": ["1992AJ....103..263S"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/116059"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_104_495"}} {"id": "J/AJ/104/495", "title_cds": "Galaxy redshifts", "title_create": "Malumuth+, 1992", "year": "1992", "author": "Malumuth E.M., Kriss G.A., Dixon W.V., Ferguson H.C., Ritchie C.", "title_pub": "Dynamics of clusters of galaxies with central dominant galaxies. I. Galaxy redshifts.", "first_author": "Malumuth E.M.", "ref_biblio": [""], "bibcode": ["1992AJ....104..495M"], "keyword_cds": "Galaxies, optical ; Redshifts", "abstract": ["Optical redshifts are presented for a sample of 638 galaxies in the", "fields of the clusters Abell 85, DC 0107-46, Abell 496, Abell 2052,", "and DC 1842-63. The velocity histograms and wedge diagrams show", "evidence for a foreground sheet of galaxies in Abell 85 and background", "sheets of galaxies in DC 0107-46 and Abell 2052. The foreground group", "projected against the center of Abell 85 found by Beers et al.", "(1991AJ....102.1581B) is confirmed. No evidence of substructure was", "found in Abell 496, Abell 2052, and DC 1842-63. The clusters have", "global velocity dispersions ranging from 551 km/s for DC 1842-63 to", "714km/s for A496, and flat dispersion profiles. Mass estimates using", "the virial theorem and the projected mass method range from 2.3x10^14^", "solar masses for DC 0107-46 to 1.1x10^15^ solar masses for A85."], "doi_pub": ["10.1086/116250"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table7.dat", "desc": "Galaxy redshifts in DC 1842-63 ", "columns": [{"name": "[MKD92]", "desc": "[1/154]+ Sequential number, [MKD92] DRCG 1842-63 NNN in Simbad"}, {"name": "n_[MKD92]", "desc": "[*] * for D or cD galaxy "}, {"name": "[D80]", "desc": "? Dressler (1980, Cat. ) number ([D80] DRCG 1842-63 NNN)"}, {"name": "[BW89]", "desc": "Bell & Whitemore (1989ApJS...70..139B) number "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "RAs", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "DEs", "desc": "Declination (1950) "}, {"name": "cz", "desc": "Heliocentric velocity "}, {"name": "e_cz", "desc": "rms uncertainty on cz "}, {"name": "r_cz", "desc": "Sources of the redshift (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_105_1206"}} {"id": "J/AJ/105/1206", "title_cds": "Exposure guide for large format CCDs", "title_create": "Tyson+, 1993", "year": "1993", "author": "TYSON N.D., GAL R.R.", "title_pub": "An exposure guide for taking twilight flatfields with large format CCDs", "first_author": "TYSON N.D.", "ref_biblio": [""], "bibcode": ["1993AJ....105.1206T"], "abstract": ["Driven by the long readout times of today's large format CCDs, we", "present an efficient method to compute an ideal sequence of exposure", "times for twilight skyflats. The procedure will allow the observer to", "maximize the number of flats that can be obtained in the rapidly", "changing surface brightness of the dusk or dawn sky."], "curator": "Patricia Bauer [CDS]", "doi_pub": ["10.1086/116505"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_106_964"}} {"id": "J/AJ/106/964", "title_cds": "BVRI photometry of NGC 185 stellar population", "title_create": "Lee+, 1993", "year": "1993", "author": "Lee M.G., Freedman W.L., Madore B.F.", "title_pub": "Stellar populations in the dwarf elliptical galaxy NGC 185.", "first_author": "Lee M.G.", "ref_biblio": [""], "bibcode": ["1993AJ....106..964L"], "keyword_cds": "Galaxies, photometry ; Photometry, UBVRI ; Photometry, CCD", "abstract": ["BVRI CCD photometry of ~5300 stars in the central (2'2x3'5) area of", "the dwarf elliptical galaxy NGC 185 in the Local Group is presented.", "The color-magnitude diagrams of NGC 185 show three distinct stellar", "populations: (1) a strong red giant branch (RGB) population, the tip", "of which is found to be at I_TRGB_=20.3+/-0.2mag, and", "(V-I)_TRGB_=1.95+/-0.05, (2) an asymptotic giant branch (AGB) located", "above the tip of the RGB, and (3) a small number of young stars having", "blue to yellow colors. The reddening of the bright foreground stars", "has been determined using the (B-V)-(V-I) diagram to be", "E(B-V)=0.19+/-0.03 mag. The distance has been estimated from the I", "magnitude of the tip of the RGB, giving (m-M)_0_=23.96+/-0.21mag for", "A_I_=0.38mag, corresponding to 620+/-60kpc. The mean metallicity of", "the RGB stars has been determined using the median color of the RGB", "stars at M_I_=-3.5mag, (V-I)_-3.5,0_=1.727mag: giving a mean", "metallicity of [Fe/H]=-1.23+/-0.16dex. The dispersion in color at", "M_I_=-3.5mag is {delta}(V-I)_-3.5_=0.12mag, implying a metallicity", "dispersion of -1.6<[Fe/H]<-0.9dex. Surface photometry of the area", "within R=50\" is also presented, showing that colors get rapidly bluer", "inside R~10\". A V luminosity function for the blue stars has been", "derived, the slope of which is very similar to that for other nearby", "galaxies. The AGB stars extend to M_bol_~-5.0mag, and Most of the AGB", "stars above the tip of the RGB are likely to belong to an", "intermediate-age population. The bolometric luminosity function of the", "red giant stars in NGC 185 is found to be very similar to that of M32."], "object": ["00 39 01.5 +48 20 27 NGC 185"], "doi_pub": ["10.1086/116697"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table3a.dat", "desc": "BVRI CCD photometry of stars in NGC 185. ", "columns": [{"name": "[LFM93a]", "desc": "Star number ([LFM93a] NNNN in Simbad) "}, {"name": "Xpos", "desc": "X position (1) "}, {"name": "Ypos", "desc": "Y position (1) "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "V-R", "desc": "? V-R colour index "}, {"name": "V-I", "desc": "? V-I colour index "}, {"name": "Imag", "desc": "? I magnitude "}]}, {"name": "table3b.dat", "desc": "Blue stars [(B-V)<0.6] in NGC 185. ", "columns": [{"name": "[LFM93a]", "desc": "Star number ([LFM93a] NNNN in Simbad) "}, {"name": "Xpos", "desc": "X position (1) "}, {"name": "Ypos", "desc": "Y position (1) "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "V-R", "desc": "? V-R colour index "}, {"name": "V-I", "desc": "? V-I colour index "}, {"name": "Imag", "desc": "? I magnitude "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_107_2184"}} {"id": "J/AJ/107/2184", "title_cds": "FK giants and supergiants photometry", "title_create": "Eggen 1994", "year": "1994", "author": "Eggen O.J.", "title_pub": "Photometry of F-K type bright giants and supergiants. III. The luminosity, reddening, and heavy element abundance of GK stars.", "first_author": "Eggen O.J.", "ref_biblio": [""], "bibcode": ["1994AJ....107.2184E"], "see_also": ["VIII/4 : Fourth Cambridge Survey (4C) (Pilkington+ 1965; Gower+1967)"], "keyword_cds": "Stars, giant ; Stars, supergiant ; Photometry ; Abundances, [Fe/H] ; Reddening ; Radial velocities", "abstract": ["The reddening, luminosity, and heavy element abundance of 250 bright", "giants and supergiants of type GK are discussed on the basis of", "4 color, DDO, RI, and Geneva photometry. Bright giants of type GK with", "age greater than 5x10^8^yr, and of type G0/3 with age greater than", "2x10^8^yr, are very scarce in the solar neighborhood. The median space", "motion vectors of the bright giants and supergiants with well", "determined space motions are", "(U, V, W)=(+10.6, -13.2, -7.7)+/-(12.3, 8.8, 8.8)km/s. The M_1 index", "for 4 color photometry, when corrected for luminosity (gravity)", "effects, is sensitive to heavy element abundance in the F type stars", "but not in those of GK type. The CN index reflects the heavy element", "abundance of the GK stars but may not be reliable for those of type", "G0/3. The available spectroscopic determinations of [Fe/H] give mixed", "results with the two largest samples (McWilliam, 1990ApJS...74.1075M;", "Brown et al, 1989ApJS...71..293B) being internally consistent but with", "a large zero-point difference. There is a similar zero-point shift in", "the peak frequency of the photometrically determined values of P[Fe/H]", "for the F type and for the GK type stars. There is little evidence for", "an appreciable galactic, radial gradient in the P[Fe/H] values. A", "previously noted correlation of the heavy element abundance index,", "{DELTA}M_1_, with the amplitude defect in the B light curves of", "Cepheids, F_B_, and interpretation of the (PLF_B_) relation as a", "(PL[Fe/H]) relation needs further investigation in light of the", "apparent sensitivity of M_1_ to Fe/H for the F stars (the domain of", "the Cepheids with P<10d) and lack of this sensitivity for the G0/3", "star (domain of the Cepheids with P>10d)."], "doi_pub": ["10.1086/117030"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "(R-I) photometry ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "m_HD", "desc": "Multiplicity index on HD "}, {"name": "Name", "desc": "Other name "}, {"name": "Rmag", "desc": "? R magnitude "}, {"name": "n_Rmag", "desc": "[V] "}, {"name": "R-I", "desc": "R-I colour index "}, {"name": "u_R-I", "desc": "Uncertainty flag on R-I "}, {"name": "DR-I", "desc": "? Mean deviation of a single observation from the mean value"}, {"name": "Nobs", "desc": "Number of observations "}]}, {"name": "table2.dat", "desc": "Previously unpublished DDO photometry (McClure, 1976AJ.....81..182M)", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "m_HD", "desc": "Multiplicity index on HD "}, {"name": "Name", "desc": "Other name "}, {"name": "m48", "desc": "m49 magnitude "}, {"name": "u_m48", "desc": "Uncertainty flag on m48 "}, {"name": "(45-48)", "desc": "45-48 colour index "}, {"name": "u_(45-48)", "desc": "Uncertainty flag on (45-48) "}, {"name": "(42-45)", "desc": "42-45 colour index "}, {"name": "u_(42-45)", "desc": "Uncertainty flag on (42-45) "}, {"name": "(41-42)", "desc": "? 41-42 colour index (1) "}, {"name": "u_(41-42)", "desc": "Uncertainty flag on (41-42) "}, {"name": "D(45-48)", "desc": "? Mean deviation of a single observation from the mean (45-48) value"}, {"name": "D(42-45)", "desc": "? Mean deviation of a single observation from the mean (42-45) value"}, {"name": "D(41-42)", "desc": "? Mean deviation of a single observation from the mean (41-42) value"}, {"name": "Nobs", "desc": "Number of observations "}]}, {"name": "table5.dat", "desc": "Photometry of early type stars in NGC 3114 (Schmidt, 1982PASP...94..232S)", "columns": [{"name": "NGC3114", "desc": "NGC 3114 NNN star number "}, {"name": "E(b-y)", "desc": "? (b-y) colour excess (1) "}, {"name": "[u-b]", "desc": "Colour index [u-b] "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "n_VMAG", "desc": "[)] Uncertainty flag on VMAG "}, {"name": "MOD", "desc": "? MOD magnitude (1) "}, {"name": "SpType", "desc": "Spectral type "}]}, {"name": "table6.dat", "desc": "Reddening, luminosity, and space motion of bright giants and supergiants near the Sun", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "n_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Cm0", "desc": "? Dereddened Cm colour index "}, {"name": "d(45-48)0", "desc": "? Dereddened (45-48) colour index "}, {"name": "d[u-b]", "desc": "? d[u-b] colour index (=[u-b]-3.80(R-I)_0_-0.240)"}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "? DDO absolute V magnitude "}, {"name": "VMAG4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "pmRA", "desc": "Proper motion in right ascension "}, {"name": "pmDE", "desc": "Proper motion in declination "}, {"name": "n_pmRA", "desc": "[)] Uncertainty flag on proper motions "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "n_RV", "desc": "[:V] "}, {"name": "Uvel", "desc": "U velocity "}, {"name": "u_Uvel", "desc": "Uncertainty flag on Uvel "}, {"name": "Vvel", "desc": "V velocity "}, {"name": "u_Vvel", "desc": "Uncertainty flag on Vvel "}, {"name": "Wvel", "desc": "W velocity "}, {"name": "u_Wvel", "desc": "Uncertainty flag on Wvel "}, {"name": "n_Uvel", "desc": "[)] Uncertainty flag on U, V, W velocities "}, {"name": "HR", "desc": "? HR (Cat. ) number "}, {"name": "SpTypeC", "desc": "Combined spectral type "}, {"name": "SpTypeO", "desc": "Observed spectral type "}, {"name": "Note", "desc": "[X] X: note in note6.dat file "}]}, {"name": "note6.dat", "desc": "Individual notes to table6.dat ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "Note", "desc": "Note "}]}, {"name": "table7.dat", "desc": "Metallicity parameters for the stars in table 5 ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "M10O", "desc": "? Observed (M_1_)_0_ metallicity index "}, {"name": "M10C", "desc": "? Computed (M_1)_0_ metallicity index (1) "}, {"name": "M10O-C", "desc": "? Observed minus computed (M_1)_0_ values (2) "}, {"name": "n_M10O-C", "desc": "[)] Uncertainty flag on M10O-C "}, {"name": "m2O", "desc": "? Observed m_2_ metallicity index "}, {"name": "m2C", "desc": "? Computed m_2_ metallicity index "}, {"name": "m2O-C", "desc": "? Observed minus computed m_2_ values (2) "}, {"name": "n_m2O-C", "desc": "[)] Uncertainty flag on m2O-C "}, {"name": "DCN", "desc": "? {DELTA}CN metallicity index (3) "}, {"name": "P[Fe/H]", "desc": "? P[Fe/H] from DCN (P[Fe/H]=5DCN-0.12) "}, {"name": "n_P[Fe/H]", "desc": "[)] Uncertainty flag on P[Fe/H] "}, {"name": "X", "desc": "Radial distance from the Sun, positive in the direction away from the galactic center"}]}, {"name": "table8.dat", "desc": "Bright giants and supergiants observed spectroscopically by McWilliams (1990ApJS...74.1075M) and Luck and Bond (1989ApJS...71..559L)", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "DCN", "desc": "{DELTA}CN metallicity index "}, {"name": "P[Fe/H]", "desc": "P[Fe/H] index "}, {"name": "D[Fe/H]", "desc": "P[Fe/H] minus [Fe/H] difference (1) "}, {"name": "n_D[Fe/H]", "desc": "[)] Uncertainty flag on D[Fe/H] "}, {"name": "TeffO", "desc": "Observed effective temperature "}, {"name": "TeffC", "desc": "Combined effective temperature "}, {"name": "TeffO-C", "desc": "TeffO minus TeffC difference "}, {"name": "r_TeffO", "desc": "[ML] Origin of TeffO value (2) "}]}, {"name": "table9.dat", "desc": "F type supergiants common to Luck & Bond (1989ApJS...71..559L) and the Geneva Photometry Catalogue (Rufener 1988, Cat. )", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "m2", "desc": "m_2_ index "}, {"name": "Del", "desc": "Del index "}, {"name": "beta", "desc": "{beta} index "}, {"name": "dDel", "desc": "{delta}Del index (=Del-3.20{beta}+8.130) "}, {"name": "dm2", "desc": "{delta}m_2_ index "}, {"name": "dm2Corr", "desc": "{delta}m_2_ index corrected for gravity effects (={delta}m_2_+0.150{delta}Del+0.125)"}, {"name": "Fe/H", "desc": "Fe/H value "}]}, {"name": "table10.dat", "desc": "Stars common to Paper II (1991AJ....102.1826E) and the Geneva Photometry Catalogue ()", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "m2", "desc": "m_2_ index "}, {"name": "Del", "desc": "Del index (=3.20{beta}-8.130) "}, {"name": "beta", "desc": "{beta} index "}, {"name": "dDel", "desc": "{delta}Del (=Del-3.20{beta}+8.130) index "}, {"name": "dm2", "desc": "{delta}m_2_ index "}, {"name": "dm2Corr", "desc": "{delta}m_2_ index corrected for gravity effects (={delta}_m_2_+0.150{delta}Del+0.125)"}, {"name": "P[Fe/H]m2", "desc": "P[Fe/H] index derived from m_2_ index "}, {"name": "P[Fe/H]M1", "desc": "P[Fe/H] index derived from M_1_ index (1) "}, {"name": "DP[Fe/H]", "desc": "P[Fe/H]m2 - P[Fe/H]M1 value (2) "}, {"name": "n_DP[Fe/H]", "desc": "[)] Uncertainty flag on DP[Fe/H] "}]}, {"name": "table11.dat", "desc": "Metallicities of bright giants and supergiants stars by Brown et al. (1989ApJS...71..293B)", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "DCN", "desc": "{DELTA}CN index "}, {"name": "TeffO", "desc": "Observed effective temperature "}, {"name": "u_TeffO", "desc": "Uncertainty flag on TeffO "}, {"name": "TeffC", "desc": "Computed effective temperature (1) "}, {"name": "TeffC_O", "desc": "Computed minus observed effective temperature "}]}, {"name": "table12.dat", "desc": "Faint SG and BG of GK type ", "columns": [{"name": "Hd", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "n_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "(R-I)0", "desc": "Dereddened (R-I) colour index "}, {"name": "Cm0", "desc": "? Dereddened C_m index "}, {"name": "d(45-48)0", "desc": "? Dereddened {delta}(54-48) index "}, {"name": "D[u-b]", "desc": "{DELTA}[u-b] index "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "? DDO absolute V magnitude "}, {"name": "VMAG4C", "desc": "4C (Cat. ) absolute V magnitude "}, {"name": "M10O", "desc": "Observed dereddened M_1_ index "}, {"name": "M10C", "desc": "Computed dereddened M_1_ index "}, {"name": "n_M10C", "desc": "[)] Uncertainty flag on M10C "}, {"name": "DCN", "desc": "? {DELTA}CN index "}, {"name": "n_DCN", "desc": "[)] Uncertainty flag on DCN "}, {"name": "P[Fe/H]", "desc": "? P[Fe/H] index from DCN (1) "}, {"name": "n_P[Fe/H]", "desc": "[)] Uncertainty flag on [Fe/H] "}, {"name": "SpTypeC", "desc": "Computed spectral type "}, {"name": "SpTypeO", "desc": "Observed spectral type "}, {"name": "r_SpTypeO", "desc": "? Reference for SpTypeO (2) "}, {"name": "X", "desc": "Radial distance from the Sun, positive in the direction away from the galactic center"}, {"name": "Note", "desc": "[X] X: individual note (3) "}]}, {"name": "table13.dat", "desc": "R type SG near NGC 2414 and NGC 2437 ", "columns": [{"name": "Star", "desc": "Star name "}, {"name": "Vmag", "desc": "V magnitude (1) "}, {"name": "b-y", "desc": "b-y colour index "}, {"name": "M1", "desc": "M_1_ colour index "}, {"name": "C1", "desc": "C_1_ colour index "}, {"name": "Rmag", "desc": "? R magnitude "}, {"name": "R-I", "desc": "R-I colour index (2) "}, {"name": "DM1", "desc": "Mean deviation of a single observation from the mean M_1_ value"}, {"name": "DC1", "desc": "Mean deviation of a single observation from the mean C_1_ value"}, {"name": "DRmag", "desc": "Mean deviation of a single observation from the mean Rmag value"}, {"name": "DR-I", "desc": "Mean deviation of a single observation from the mean R-I value"}, {"name": "Nobs", "desc": "Number of observations "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "D[u-b]", "desc": "? {delta}[u-b] colour index "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "beta", "desc": "{beta} index "}, {"name": "SpTypeC", "desc": "Computed spectral type "}, {"name": "Note", "desc": "[X] X: individual note (3) "}]}, {"name": "table14.dat", "desc": "*Stars classified as supergiants or bright giants but with photometric indices of normal galaxies", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "n_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "(R-I)0", "desc": "? Dereddened R-I colour index "}, {"name": "Cm0", "desc": "? Dereddened C_m_ index (1) "}, {"name": "D(45-48)0", "desc": "? Dereddened {Delta}(45-48) index (2) "}, {"name": "[C1]", "desc": "? [C_1_] index "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "MVDDO", "desc": "DDO absolute V magnitude "}, {"name": "MV4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "n_MV4C", "desc": "[)o] ): uncertainty flag; o: optical "}, {"name": "D(M1)0", "desc": "? Dereddened {Delta}M_1_ index "}, {"name": "n_D(M1)0", "desc": "[)] Uncertainty flag on D(M1)0 "}, {"name": "DCN", "desc": "? {Delta}CN index "}, {"name": "P[Fe/H]4C", "desc": "? P[Fe/H] index from 4C (Cat. ) "}, {"name": "n_P[Fe/H]4C", "desc": "[)] Uncertainty flag on P[Fe/H]4C "}, {"name": "P[Fe/H]DDO", "desc": "? P[Fe/H] index from DDO (=3.12DCN+0.031) "}, {"name": "SpTypeC", "desc": "Computed spectral type "}, {"name": "SpTypeO", "desc": "Observed spectral type "}, {"name": "r_SpTypeO", "desc": "? Source of spectral type (3) "}, {"name": "Note", "desc": "[XA] Individual notes (4) "}]}, {"name": "table15.dat", "desc": "Problem stars ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "n_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Cm0", "desc": "Dereddened C_m_ colour index "}, {"name": "d(45-48)0", "desc": "Dereddened {delta}(45-48) colour index "}, {"name": "n_d(45-48)0", "desc": "[)] Uncertainty flag on d(45-48)0 "}, {"name": "D[u-b]", "desc": "? {Delta}[u-y] index "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "? DDO absolute V magnitude "}, {"name": "n_VMAGDDO", "desc": "[)] Uncertainty flag on VMAGDDO "}, {"name": "VMAG4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "n_VMAG4C", "desc": "[)] Uncertainty flag on VMAG4C "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "SpTypeC", "desc": "Computed spectral type "}, {"name": "SpTypeO", "desc": "Observed spectral type "}, {"name": "Note", "desc": "[XA] Individual notes (1) "}]}, {"name": "note15.dat", "desc": "Individual notes to table15.dat ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "table16.dat", "desc": "G0/3 I stars ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E[b-y]", "desc": "! [b-y] colour excess "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Cm0", "desc": "Dereddened C_m_ index "}, {"name": "d(45-48)0", "desc": "Dereddened {delta}(45-48) index "}, {"name": "D[u-b]", "desc": "? {Delta}[u-b] index "}, {"name": "n_D[u-b]", "desc": "[)] Uncertainty flag on D[u-b] "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "DDO absolute V magnitude "}, {"name": "VMAG4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "n_VMAG4C", "desc": "[)] Uncertainty flag on VMAG4C "}, {"name": "DCN", "desc": "{Delta}CN index "}, {"name": "n_DCN", "desc": "[)] Uncertainty flag on DCN "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "References for SpType (1) "}, {"name": "Note", "desc": "[X] Individual notes (2) "}]}, {"name": "table17.dat", "desc": "Stars in table 16 with Geneva photometry ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "m2O", "desc": "Observed m_2_ index (=[B1-B2]-0.457[B2-VI]) "}, {"name": "DelO", "desc": "Observed Del index (=[U-B2]-0.832[B2-G]) "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Dm2", "desc": "{Delta}m_2_ index (=m_2_-1.95(R-I)_0_+0.695) "}, {"name": "DDel", "desc": "{Delta}Del index (=Del-1.60(R-I)_0_+0.695) "}, {"name": "m2C", "desc": "Computed m_2_ index "}, {"name": "m2O-C", "desc": "Observed minus computed m_2_ index (1) "}, {"name": "n_m2O-C", "desc": "[)] Uncertainty flag on m2O-C "}]}, {"name": "table18.dat", "desc": "G0/3 II stars ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "(R-I)0", "desc": "Dereddened R-I colour index "}, {"name": "Cm0", "desc": "Dereddened C_m_ colour index "}, {"name": "d(45-48)0", "desc": "Dereddened {delta}(45-48) colour index "}, {"name": "d[u-b]", "desc": "? {delta}[u-y] index (=[u-b]-3.80(R-I)_0_-0.240) "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGDDO", "desc": "? DDO absolute V magnitude "}, {"name": "VMAG4C", "desc": "? 4C (Cat. ) absolute V magnitude "}, {"name": "DCN", "desc": "{Delta}CN index "}, {"name": "n_DCN", "desc": "[)] Uncertainty flag on DCN "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "References to spectral type (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_108_1843"}} {"id": "J/AJ/108/1843", "title_cds": "Serendipitous EUV sources", "title_create": "McDonald+, 1994", "year": "1994", "author": "McDonald K., Craig N., Sirk M.M., Drake J.J., Fruscione A., Vallerga J.V., Malina R.F.", "title_pub": "Serendipitous EUV sources detected during the first year of the Extreme Ultraviolet Explorer right angle program.", "first_author": "McDonald K.", "ref_biblio": [""], "bibcode": ["1994AJ....108.1843M"], "keyword_cds": "Ultraviolet ; Cross identifications", "abstract": ["We report the detection of 114 extreme ultraviolet (EUV; 58-740{AA})", "sources, of which 99 are new serendipitous sources, based on", "observations made with the imaging telescopes on board the Extreme", "Ultraviolet Explorer (EUVE) during the Right Angle Program (RAP).", "These data were obtained using the survey scanners and the Deep Survey", "instrument during the first year of the spectroscopic guest observer", "phase of the mission, from January 1993 to January 1994. The data set", "consists of 162 discrete pointings whose exposure times are typically", "two orders of magnitude longer than the average exposure times during", "the EUVE all-sky survey. Based on these results, we can expect that", "EUVE will serendipitously detect approximately 100 new EUV sources per", "year, or about one new EUV source per 10 sq deg, during the guest", "observer phase of the EUVE mission. New EUV sources of note include", "one B star and three extragalactic objects. The B star (HR 2875, EUVE", "J0729-38.7) is detected in both the Lexan/B (~100{AA}) and Al/Ti/C", "(~200{AA}) bandpasses, and the detection is shown not to be a result", "of UV leaks. We suggest that we are detecting EUV and/or soft x rays", "from a companion to the B star. Three sources, EUVE J2132+10.1, EUVE", "J2343-14.9, and EUVE J2359-30.6 are identified as the active galactic", "nuclei MKN 1513, MS2340.9-1511, and 1H2354-315, respectively."], "doi_pub": ["10.1086/117197"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "EUVE right angle program source list ", "columns": [{"name": "EUVE", "desc": "EUVE name "}, {"name": "n_EUVE", "desc": "[+ b] Note on Name (1) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "Lex", "desc": "? Lexan/B count rates "}, {"name": "AlC", "desc": "? Al/Ti/C count rates "}, {"name": "Dag", "desc": "? Ti/Sb/Al count rates "}, {"name": "Tin", "desc": "? Sn/SiO count rates "}, {"name": "DSL", "desc": "? DS Lexan count rates "}, {"name": "DSA", "desc": "? DS Al/C count rates "}, {"name": "Q", "desc": "[12U] Identification quality (2) "}, {"name": "ID", "desc": "Possible optical identification "}, {"name": "Name", "desc": "Other name of ID "}, {"name": "SpType", "desc": "Spectral type of ID "}, {"name": "Type", "desc": "Type of ID (SB, Em, WD ...) "}, {"name": "Vmag", "desc": "? V or B magnitude "}, {"name": "n_Vmag", "desc": "Note on Vmag (variability or uncertainty flag) "}, {"name": "Band", "desc": "[B] B if B magnitude in Vmag column "}, {"name": "Sep", "desc": "? Separation between the EUVE RAP source and the candidate counterpart"}, {"name": "Notes", "desc": "Notes (3) "}]}, {"name": "notes.dat", "desc": "Notes to table2.dat ", "columns": [{"name": "Note", "desc": "Note abbreviation "}, {"name": "Text", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_109_2229"}} {"id": "J/AJ/109/2229", "title_cds": "South Galactic Pole stars photometry", "title_create": "Eggen 1995", "year": "1995", "author": "Eggen O.J.", "title_pub": "Stellar populations at the South Galactic Pole.", "first_author": "Eggen O.J.", "ref_biblio": [""], "bibcode": ["1995AJ....109.2229E"], "see_also": ["J/AJ/112/772 : VI photometry in South Galactic Pole (Caldwell+ 1996)", "J/A+AS/97/835 : K giants at the South Galactic Pole (Flynn+ 1993)", "V/33 : Radial velocities of stars at the North & South Galactic Poles", "II/120 : Phot and Spectrophot Investigation, SGP (Eriksson 1978)", "I/129 : Parallaxes and Proper Motions near SGP (Murray+ 1986)"], "keyword_cds": "Galactic pole, south ; Populations, stellar ; Photometry ; Proper motions ; Radial velocities", "abstract": ["Four-color, (R, I), H{beta}, and DDO photometry for some 500 stars", "with known proper motion and within 10{deg} of the South Galactic Pole", "is analyzed for reddening, luminosity, metal abundance, and space", "motion. The sample contains 275, mostly evolved, GK stars and 225 near", "main sequence, AF stars. The stars are divided into young disk and old", "disk population objects on the basis of their motion vectors and this", "also separates them into stars younger and older than 2x10^9^yr, on", "the basis of models with convective overshoot at the cores. The", "critical mass separating the two populations is 1.7M_{sun}_, which is", "also the critical mass separating the stars that develop degenerate", "helium cores and evolve to a giant luminosity that is an order of", "magnitude greater than the main sequence turnoff, and the more massive", "stars that do not form degenerate cores and maintain, as giants, their", "mean sequence luminosity. The dispersions in the W velocity, for the", "OD samples of AF and GK stars, with the addition of small samples of", "AGB stars and high latitude A stars (presumable OD, BS) at the SGP,", "define the relation ({omega}_w_=9.5+0.025|Z|(pc). The stars discussed", "here do not, generally, follow the pattern of decreasing metallicity", "with increasing Z. found by others for unevolved GK stars. The BS", "population at the NGP consists of 20% of the OD, AF stars, whereas it", "is only 4% at the SGP and this result may be associated with the fact", "that the OD/YD ratio is near 1.5 for most reliable samples, whereas it", "is only about 0.5 for the AF stars at the NGP."], "doi_pub": ["10.1086/117448"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "position.dat", "desc": "Object positions ", "columns": [{"name": "RAh", "desc": "Right ascension (2000.0) "}, {"name": "RAm", "desc": "Right ascension (2000.0) "}, {"name": "RAs", "desc": "Right ascension (2000.0) "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (2000.0) "}, {"name": "DEm", "desc": "Declination (2000.0) "}, {"name": "DEs", "desc": "? Declination (2000.0) "}, {"name": "CPC", "desc": "? CPC number "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "CD", "desc": "CD number "}, {"name": "HD", "desc": "HD number "}, {"name": "Names", "desc": "Other names "}]}, {"name": "table1.dat", "desc": "Cape Zone Catalogue stars within 10{deg} of the South Calactic Pole.", "columns": [{"name": "CPC", "desc": "Cape (Cat. ) number "}, {"name": "m_CPC", "desc": "[ABEW] Multiplicity index on CPC "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "CD", "desc": "? CD (Cat. ) number "}, {"name": "m_CD", "desc": "[AB] Multiplicity index on CPD "}, {"name": "n_CD", "desc": "Distance from the companion when no CPD number "}, {"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "m_HD", "desc": "[AB] Multiplicity index on HD "}, {"name": "Vmag", "desc": "? V magnitude "}, {"name": "n_Vmag", "desc": "[V] V for variable "}, {"name": "b-y", "desc": "? b-y colour index "}, {"name": "M1", "desc": "? M1 colour index "}, {"name": "C1", "desc": "? C1 colour index "}, {"name": "Rmag", "desc": "? R magnitude "}, {"name": "beta", "desc": "? beta colour index "}, {"name": "R-I", "desc": "? R-I colour index "}, {"name": "e_b-y", "desc": "? rms uncertainty on b-y "}, {"name": "e_M1", "desc": "? rms uncertainty on M1 "}, {"name": "e_C1", "desc": "? rms uncertainty on C1 "}, {"name": "e_R-I", "desc": "? rms uncertainty on R-I "}, {"name": "Nobs", "desc": "? Number of observations "}]}, {"name": "table2.dat", "desc": "Previously unpublished DDO photometry. ", "columns": [{"name": "Star", "desc": "Star name (HD or CD) "}, {"name": "M48", "desc": "? M48 magnitude "}, {"name": "(45-48)", "desc": "(45-48) DDO colour index "}, {"name": "u_(45-48)", "desc": "Uncertainty flag on (45-48) "}, {"name": "(42-45)", "desc": "(42-45) DDO colour index "}, {"name": "u_(42-45)", "desc": "Uncertainty flag on (42-45) "}, {"name": "(41-42)", "desc": "(41-42) DDo colour index "}, {"name": "u_(41-42)", "desc": "Uncertainty flag on (41-42) "}]}, {"name": "table3.dat", "desc": "The GK stars of the SGP ", "columns": [{"name": "CPC", "desc": "Cape number "}, {"name": "m_CPC", "desc": "[AB] Multiplicity index on CPC "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "Name", "desc": "Object name "}, {"name": "E(b-y)", "desc": "Interstellar reddening "}, {"name": "u_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "D(45-48)", "desc": "? Luminosity-dependent index from the DDO system"}, {"name": "n_D(45-48)", "desc": "[)n] ): Uncertainty flag on D(45-48) n: See text"}, {"name": "Cm0", "desc": "? Measure of the CN strength "}, {"name": "n_Cm0", "desc": "[)n] ): Uncertainty flag on Cm0 n: See text"}, {"name": "MV4C", "desc": "? Four-colour photometry V magnitude (2) "}, {"name": "u_MV4C", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "MVDDO", "desc": "? DDO photometry V magnitude (3) "}, {"name": "u_MVDDO", "desc": "[)] Uncertainty flag on MVDDO "}, {"name": "P[Fe/H]4C", "desc": "? Four-colour photometry metallicity (4) "}, {"name": "u_P[Fe/H]4C", "desc": "[)] Uncertainty flag on P[Fe/H]4C "}, {"name": "P[Fe/H]DDO", "desc": "? DDO metallicity (4) "}, {"name": "u_P[Fe/H]DDO", "desc": "[)] Uncertainty flag on P[Fe/H]DDO "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] Dash "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "u_pmRA", "desc": "[)] Uncertainty flag on pmRA and pmDE "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "n_Uvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "n_Vvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "n_Wvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Z", "desc": "? Distance from the galactic plane "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "n_SpType", "desc": "[a] Note on SpType (5) "}, {"name": "Pop", "desc": "Population (OD, YD) "}]}, {"name": "table4.dat", "desc": "Anomalous CN ", "columns": [{"name": "CPC", "desc": "Cape (Cat. ) number "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "P[Fe/H]4C", "desc": "Four-colour photometry metallicity "}, {"name": "P[Fe/H]DDO", "desc": "DDO photometry metallicity "}, {"name": "CN", "desc": "wk: CN weak star; str: CN strong star "}, {"name": "Pop", "desc": "OD: old disk, YD: young disk "}]}, {"name": "table5.dat", "desc": "YD evolved GK stars near the NGP (SA 79, 80, 81, and 82)", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "BD", "desc": "BD (Cat. ) number "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "D(45-48)0", "desc": "Dereddened {DELTA}(45-48) colour index "}, {"name": "Cm0", "desc": "Dereddened C_m_ colour index "}, {"name": "MV4C", "desc": "Four-colour photometry absolute V magnitude "}, {"name": "MVDDo", "desc": "DDO photometry absolute V magnitude "}, {"name": "P[Fe/H]4C", "desc": "Four-colour photometry metallicity "}, {"name": "P[Fe/H]DDO", "desc": "DDO photometry metallicity "}, {"name": "pmRA", "desc": "Proper motion in RA "}, {"name": "---", "desc": "[/] Dash "}, {"name": "pmDE", "desc": "Proper motion in DE "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "Uvel", "desc": "U velocity "}, {"name": "Vvel", "desc": "V velocity "}, {"name": "Wvel", "desc": "W velocity "}, {"name": "Z", "desc": "Distance from the galactic plane "}]}, {"name": "table6.dat", "desc": "Problem stars ", "columns": [{"name": "CPC", "desc": "Cape number "}, {"name": "m_CPC", "desc": "[AB] Multiplicity index on CPC "}, {"name": "n_CPC", "desc": "[X] Note on CPC (1) "}, {"name": "Name", "desc": "Object name "}, {"name": "E(b-y)", "desc": "Interstellar reddening "}, {"name": "u_E(b-y)", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "D(45-48)", "desc": "? Luminosity-dependent index from the DDO system"}, {"name": "n_D(45-48)", "desc": "[)n] ): Uncertainty flag on D(45-48) n: See text"}, {"name": "Cm0", "desc": "? Measure of the CN strength "}, {"name": "n_Cm0", "desc": "[)n] ): Uncertainty flag on Cm0 n: See text"}, {"name": "MV4C", "desc": "? Four-colour photometry V magnitude (2) "}, {"name": "u_MV4C", "desc": "[)] Uncertainty flag on E(b-y) "}, {"name": "MVDDO", "desc": "? DDO photometry V magnitude (3) "}, {"name": "u_MVDDO", "desc": "[)] Uncertainty flag on MVDDO "}, {"name": "P[Fe/H]4C", "desc": "? Four-colour photometry metallicity (4) "}, {"name": "u_P[Fe/H]4C", "desc": "[)] Uncertainty flag on P[Fe/H]4C "}, {"name": "P[Fe/H]DDO", "desc": "? DDO metallicity (4) "}, {"name": "u_P[Fe/H]DDO", "desc": "[)] Uncertainty flag on P[Fe/H]DDO "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] Dash "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "u_pmRA", "desc": "[)] Uncertainty flag on pmRA and pmDE "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "n_Uvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "n_Vvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "n_Wvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Z", "desc": "? Distance from the galactic plane "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "n_SpType", "desc": "[a] Note on SpType (5) "}, {"name": "Pop", "desc": "Population (OD, YD) "}]}, {"name": "table7.dat", "desc": "Stars at the SGP ", "columns": [{"name": "Cape", "desc": "Cape number "}, {"name": "m_Cape", "desc": "[A] Multilicity index on CPC "}, {"name": "n_Cape", "desc": "[X] Note on CPC (1) "}, {"name": "Note", "desc": "[a] Individual note (2) "}, {"name": "Name", "desc": "Other name "}, {"name": "beta", "desc": "? beta magnitude "}, {"name": "u_beta", "desc": "[)] Uncertainty flag on beta "}, {"name": "VMag", "desc": "? Absolute V magnitude "}, {"name": "u_VMag", "desc": "[)] Uncertainty flag on VMag "}, {"name": "Z", "desc": "? Distance from the galactic plane "}, {"name": "P[Fe/H]", "desc": "? Metallicity "}, {"name": "u_P[Fe/H]", "desc": "[)] Uncertainty flag on P[Fe/H] "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "n_Uvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "n_Vvel", "desc": "? Percentage of that velocity contributes to the vectors (U, V)"}, {"name": "SpType", "desc": "Spectral type "}, {"name": "pmRA", "desc": "Proper motion in RA "}, {"name": "---", "desc": "[/] Dash "}, {"name": "pmDE", "desc": "Proper motion in DE "}, {"name": "u_pmDE", "desc": "[)] Uncertainty flag on proper motions "}, {"name": "Pop", "desc": "Population (OD: old disk, YD: Young Disk) "}]}, {"name": "table8.dat", "desc": "SGP A stars with Z>700 pc ", "columns": [{"name": "Name", "desc": "Object name (1) "}, {"name": "(b-y)0", "desc": "Dereddened (b-y) colour index "}, {"name": "u_(b-y)0", "desc": "[)] Uncertainty flag on (b-y)0 "}, {"name": "VMag", "desc": "Absolute V magnitude "}, {"name": "|Z|", "desc": "Absolute distance above the plane (2) "}, {"name": "W", "desc": "Radial velocity times sin(b) (2) "}, {"name": "[Ca/H]", "desc": "? Calcium relative abundance (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_110_823"}} {"id": "J/AJ/110/823", "title_cds": "Blue stragglers in solar vicinity", "title_create": "Eggen+, 1995", "year": "1995", "author": "Eggen O.J.", "title_pub": "Blue stragglers in the solar vicinity: newborn or reborn.", "first_author": "Eggen O.J.", "ref_biblio": [""], "bibcode": ["1995AJ....110..823E"], "see_also": ["J/AJ/115/2397 : Stars in the solar region (Eggen 1998)", "J/A+AS/109/375 : Blue stragglers in open clusters (Ahumada+, 1995)"], "keyword_cds": "Stars, blue ; Photometry, Geneva ; Photometry, uvby, beta ; Rotational velocities ; Space velocities ; Effective temperatures", "abstract": ["A selected sample of 1400 A0/1 to F2/ (logTeff=3.96 to 3.82) stars", "with accurate photometric and astrometric data are discussed on the", "basis of luminosities obtained from both Stroemgren+H{beta} and Geneva", "photometry. The sample contains members of the Hyades, Sirius, and HR", "1614 superclusters, all of which show an appreciable age spread. The", "spread of 6 to 20x10^8^yr in the Hyades supercluster is reflected in a", "spread of about 6 to 10x10^8^yr in the Praesepe and Hyades clusters", "within the supercluster. Strong arguments are presented for the", "presence of a larger age spread in the noncluster supercluster members", "than in the contained clusters. The age range for members of the", "Sirius supercluster is 2 to 6x10^8^yr and nearly all of this range is", "seen in the UMa nucleus of the Sirius supercluster, contained within", "the supercluster. The HR 1614 supercluster is near 4x10^9^yr old and", "may include the old disk cluster NGC 6791. About three-quarters of", "bright A-star sample consists of young disk stars, on the basis of", "their (U, V) velocities. The Am, USPC ({delta} Sct), and A Boo stars", "represent about 10%, 6%, and 1%, respectively, of the total sample as", "well as of the young disk and old disk constituents of the sample."], "doi_pub": ["10.1086/117567"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "Stars of type A2 or later ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number (1) "}, {"name": "---", "desc": "[/] "}, {"name": "n_HR", "desc": "? When multiple HR name "}, {"name": "Q", "desc": "[AB] Note (2) "}]}, {"name": "table3.dat", "desc": "Conflict of spectroscopic and photometric luminosities", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "u_E(b-y)", "desc": "Uncertainty flag on E(b-y) "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "Uncertainty flag on V0 "}, {"name": "l_V0", "desc": "Limit flag on V0 "}, {"name": "VMAG4c", "desc": "? 4C absolute V magnitude "}, {"name": "l_VMAGg", "desc": "Limit flag on VMAGg "}, {"name": "VMAGg", "desc": "? Geneva absolute V magnitude "}, {"name": "SpType", "desc": "Spectral type (1) "}]}, {"name": "table4.dat", "desc": "Sample stars in the Hyades supercluster ", "columns": [{"name": "Group", "desc": "[CS] C: cluster, S: supercluster "}, {"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[ABC ] Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "nu", "desc": "? Proper motion in the direction of (A, D) "}, {"name": "---", "desc": "[/] "}, {"name": "tau", "desc": "? Motion perpendicular to the direction of (A, D)"}, {"name": "n_tau", "desc": "[*] Note (1) "}, {"name": "DT", "desc": "? Pecular motion, tau, in km/s "}, {"name": "X", "desc": "? Distance of the member to the Sun "}, {"name": "Vtot", "desc": "? Total velocity "}, {"name": "MOD", "desc": "? Distance modulus "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGc", "desc": "Cluster absolute V magnitude "}, {"name": "u_VMAGc", "desc": "[)] Uncertainty flag on VMAGc "}, {"name": "VMAGp", "desc": "? Photometric absolute V magnitude "}, {"name": "u_VMAGp", "desc": "Uncertainty flag on VMAGp "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "(B-V)0", "desc": "Dereddened B-V colour index "}, {"name": "RVC", "desc": "? Comparison radial velocity "}, {"name": "n_RVC", "desc": "[V] Note on RVC (2) "}, {"name": "RVO", "desc": "? Observed radial velocity "}, {"name": "n_RVO", "desc": "[V:ns] Note on RVO (2) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Note", "desc": "[X] Note in notes.dat file "}]}, {"name": "table5.dat", "desc": "USPC ({delta} Sct) variables in the Hyades supercluster", "columns": [{"name": "HR", "desc": "? HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AB ] Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "Name", "desc": "Name "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "l_vsini", "desc": "Limit flag on vsini "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "SpType", "desc": "Spectral type (only in table5.dat) "}, {"name": "beta", "desc": "{beta} index "}, {"name": "logTeff", "desc": "Effective temperature "}, {"name": "Note", "desc": "Notes "}]}, {"name": "table6.dat", "desc": "Am Stars in the Hyades supercluster ", "columns": [{"name": "HR", "desc": "? HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AB ] Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "Name", "desc": "Name "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "l_vsini", "desc": "Limit flag on vsini "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "SpType", "desc": "Spectral type (only in table5.dat) "}, {"name": "beta", "desc": "{beta} index "}, {"name": "logTeff", "desc": "Effective temperature "}, {"name": "Note", "desc": "Notes "}]}, {"name": "table7.dat", "desc": "Effective temperature of USPC, Am, and normal stars.", "columns": [{"name": "HR", "desc": "? HR (Cat. ) number "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logTeffs", "desc": "Spectrophotometric logarithmic effective temperature"}, {"name": "logTeffc", "desc": "Comparison logarithmic effective temperature "}, {"name": "DlogTeff", "desc": "logTeffs minus logTeffc (1) "}, {"name": "Type", "desc": "Stellar type "}, {"name": "Note", "desc": "Note "}]}, {"name": "table8.dat", "desc": "Am Stars in the sample but not in the Hyades or Sirius supercluster.", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AB ab] Multiplicity index on HR "}, {"name": "Name", "desc": "Name (only in table9.dat) "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "? (b-y) colour excess "}, {"name": "V0", "desc": "? Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGs", "desc": "? Stroemgren absolute V magnitude "}, {"name": "u_VMAGs", "desc": "[)] Uncertainty flag on VMAGs "}, {"name": "VMAGg", "desc": "? Geneva absolute V magnitude "}, {"name": "u_VMAGg", "desc": "[)] Uncertainty flag on VMAGg "}, {"name": "MOD", "desc": "? Distance modulus "}, {"name": "u_MOD", "desc": "[)] Uncertainty flag on MOD "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "(B-V)0", "desc": "? Dereddened B-V colour index "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Note", "desc": "[X] X: note in notes.dat file "}]}, {"name": "table9.dat", "desc": "USPC ({delta} Sct) variables in the bright A-star sample but not in the Hyades supercluster", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AB ab] Multiplicity index on HR "}, {"name": "Name", "desc": "Name (only in table9.dat) "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "? (b-y) colour excess "}, {"name": "V0", "desc": "? Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGs", "desc": "? Stroemgren absolute V magnitude "}, {"name": "u_VMAGs", "desc": "[)] Uncertainty flag on VMAGs "}, {"name": "VMAGg", "desc": "? Geneva absolute V magnitude "}, {"name": "u_VMAGg", "desc": "[)] Uncertainty flag on VMAGg "}, {"name": "MOD", "desc": "? Distance modulus "}, {"name": "u_MOD", "desc": "[)] Uncertainty flag on MOD "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "(B-V)0", "desc": "? Dereddened B-V colour index "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Note", "desc": "[X] X: note in notes.dat file "}]}, {"name": "table10.dat", "desc": "Possible Am stars in the Orion association ", "columns": [{"name": "WH", "desc": "Warren and Hesser (1978ApJS...36..497W) number "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "beta", "desc": "{beta} index "}, {"name": "VMAGs", "desc": "Stroemgren absolute V magnitude "}, {"name": "VMAGg", "desc": "? Geneva absolute V magnitude "}, {"name": "MODp", "desc": "Photometry distance modulus "}, {"name": "MODwh", "desc": "Warren and Hesser distance modulus "}, {"name": "e_MODwh", "desc": "rms uncertainty on MODwh "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Name", "desc": "Name "}]}, {"name": "table11.dat", "desc": "{lambda} Boo stars ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[AC] Multiplicity index on HR "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "VMAGs", "desc": "? Stroemgren absolute V magnitude "}, {"name": "VMAGgnv", "desc": "? Geneva absolute V magnitude "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "n_RV", "desc": "[V] Note on RV "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "u_Uvel", "desc": "[)] Uncertainty flag on Uvel "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "u_Vvel", "desc": "[)] Uncertainty flag on Vvel "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "u_Wvel", "desc": "[)] Uncertainty flag on Wvel "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "SpType", "desc": "Spectral type (1) "}, {"name": "Note", "desc": "[ab] ???????? "}]}, {"name": "table12.dat", "desc": "A2 IV stars ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[ABC] Multiplicity index on HR "}, {"name": "n_HR", "desc": "[*] Note on HR (1) "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGp", "desc": "? Photometric absolute V magnitude "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "VVel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "Note", "desc": "[hs] Note on space velocities (2) "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "logTeff", "desc": "? Effective temperature "}]}, {"name": "table13.dat", "desc": "Members of the Sirius supercluster ", "columns": [{"name": "Group", "desc": "[CS] C: cluster, S: supercluster "}, {"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "[ABC ] Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "nu", "desc": "? Proper motion in the direction of (A, D) "}, {"name": "---", "desc": "[/] "}, {"name": "tau", "desc": "? Motion perpendicular to the direction of (A, D)"}, {"name": "n_tau", "desc": "[*] Note (1) "}, {"name": "DT", "desc": "? Pecular motion, tau, in km/s "}, {"name": "X", "desc": "? Distance of the member to the Sun "}, {"name": "Vtot", "desc": "? Total velocity "}, {"name": "MOD", "desc": "? Distance modulus "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAGc", "desc": "Cluster absolute V magnitude "}, {"name": "u_VMAGc", "desc": "[)] Uncertainty flag on VMAGc "}, {"name": "VMAGp", "desc": "? Photometric absolute V magnitude "}, {"name": "u_VMAGp", "desc": "Uncertainty flag on VMAGp "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "(B-V)0", "desc": "Dereddened B-V colour index "}, {"name": "RVC", "desc": "? Comparison radial velocity "}, {"name": "n_RVC", "desc": "[V] Note on RVC (2) "}, {"name": "RVO", "desc": "? Observed radial velocity "}, {"name": "n_RVO", "desc": "[V:ns] Note on RVO (2) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Note", "desc": "[X] Note in notes.dat file "}]}, {"name": "table14.dat", "desc": "Normal old disk stars in the bright A-star sample ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "m_HR", "desc": "Multiplicity index on HR "}, {"name": "HD", "desc": "HR (Cat. ) number "}, {"name": "m_HD", "desc": "Multiplicity index on HD "}, {"name": "beta", "desc": "? {beta} index "}, {"name": "E(b-y)", "desc": "(b-y) colour excess "}, {"name": "V0", "desc": "Dereddened V magnitude "}, {"name": "u_V0", "desc": "[)] Uncertainty flag on V0 "}, {"name": "VMAG", "desc": "? Absolute V magnitude "}, {"name": "pmRA", "desc": "? Proper motion in right ascension "}, {"name": "---", "desc": "[/] "}, {"name": "pmDE", "desc": "? Proper motion in declination "}, {"name": "RV", "desc": "? Radial velocity "}, {"name": "Uvel", "desc": "? U velocity "}, {"name": "Vvel", "desc": "? V velocity "}, {"name": "Wvel", "desc": "? W velocity "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "l_vsini", "desc": "Limit flag on vsini "}, {"name": "vsini", "desc": "? Rotational velocity "}, {"name": "Note", "desc": "[X] Note in notes.dat file "}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "HR", "desc": "HR (Cat. ) number "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_110_o.2288"}} {"id": "J/AJ/110/2288", "title_cds": "Kinematics of local RR Lyrae stars. II.", "title_create": "Layden 1995", "year": "1995", "author": "Layden A.C.", "title_pub": "The metallicities and kinematics of RR Lyrae variables. II. Galactic structure and formation from local stars", "first_author": "Layden A.C.", "ref_biblio": [""], "bibcode": ["1995AJ....110.2288L"], "see_also": ["J/AJ/108/1016 : Kinematics of local RR lyrae stars I. (Layden, 1994)"], "keyword_cds": "Stars, variable ; Proper motions ; Space velocities", "abstract": ["We investigate the kinematics and spatial distribution of a sample of", "302 nearby RR Lyrae variable stars with the goal of learning more", "about the formation history and present-day structure of the galaxy.", "We find that the kinematics change abruptly at [Fe/H]~-1.0. Above", "this value, the stars exhibit kinematic properties like those of other", "tracers of the galaxy's thick disk, while below [Fe/H]=-1.3, halo", "kinematics are observed. The stars with -1.3<=[Fe/H]<=-1.0 are a", "mixture of these populations, though the fraction of thick disk RR", "Lyrae stars with [Fe/H]<=-1.0 is significantly smaller than found", "among red giant stars by other authors; we discuss several", "possibilities for this discrepancy. The RR Lyraes with [Fe/H]>-0.5", "exhibit somewhat cooler kinematics and a flatter spatial distribution", "than those of the thick disk, and may include some members of the old", "thin disk population. We find the kinematics of the halo RR Lyraes to", "be uncorrelated with abundance over the range -2.2<=[Fe/H]<=-1.0,", "and interpret this as evidence that the motions and chemical", "enrichment of gas in the early galaxy was characterized by a high", "degree of randomization, consistent with fragment accretion pictures", "of galaxy formation. We argue that the small number of thick disk", "stars with [Fe/H]<=-1.0 cannot be called upon to balance the net", "kinematics of a retrograde-rotating halo to produce the slow prograde", "rotations seen in this and other local samples; however, a hotter,", "slowly rotating, somewhat flattened second halo component may be", "consistent with kinematics both of local samples and of samples far", "from the galactic plane. We find the local density of halo RR Lyraes", "to be 11-15kpc^-3^, with a firm lower limit of 8+/-3kpc^-3^. This is", "larger than that predicted from counts of faint RR Lyraes far from the", "plane; either the flattening of the local halo is larger than c/a~0.7,", "or a two- component halo exists in which one component is quite", "flattened. We derive an exponential scale height of 0.7(+0.5)(-0.3)kpc", "and a midplane density of 10+/-4kpc^-3^ for the disk RR Lyraes with", "[Fe/H]>-1.0."], "date_update": "05-Nov-1996", "tables": [{"name": "table2.dat", "desc": "Proper motions and space velocities of 154 RR Lyrae variables", "columns": [{"name": "Star", "desc": "Star name "}, {"name": "pmRA", "desc": "Proper motion in right ascension (1) "}, {"name": "e_pmRA", "desc": "Error in pmRA "}, {"name": "pmDE", "desc": "Proper motion in declination "}, {"name": "e_pmDE", "desc": "Error in pmDE "}, {"name": "Note", "desc": "[a-d] Note flag (2) "}, {"name": "Vrho", "desc": "Rho component of space velocity (3) "}, {"name": "e_Vrho", "desc": "Error in Vrho "}, {"name": "Vphi", "desc": "Phi component of space velocity (3) "}, {"name": "e_Vphi", "desc": "Error in Vphi "}, {"name": "Vz", "desc": "z component of space velocity (3) "}, {"name": "e_Vz", "desc": "Error in Vz "}, {"name": "[Fe/H]", "desc": "Metal abundance "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_114_1365"}} {"id": "J/AJ/114/1365", "title_cds": "Physical properties of stellar systems", "title_create": "Burstein+, 1997", "year": "1997", "author": "Burstein D., Bender R., Faber S.M., Nolthenious R.", "title_pub": "Global relationships among the physical properties of stellar systems.", "first_author": "Burstein D.", "ref_biblio": [""], "bibcode": ["1997AJ....114.1365B"], "keyword_cds": "Associations, stellar", "abstract": ["The {kappa}-space three-dimensional parameter system was originally", "defined to examine the physical properties of dynamically hot", "elliptical galaxies and bulges (DHGs). The axis of {kappa}-space are", "proportional to the logarithm of galaxy mass, mass-to-light ratio, and", "a third quantity that is mainly surface brightness. In this paper, we", "define self-consistent {kappa} parameters for disk galaxies, galaxy", "groups and clusters, and globular stellar systems in the Universe."], "doi_pub": ["10.1086/118570"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Stellar system physical properties ", "columns": [{"name": "Name", "desc": "Common name for object (1) "}, {"name": "Intnum", "desc": "Internal number for object "}, {"name": "IDnum", "desc": "ID number, stellar system type (2) "}, {"name": "Dist", "desc": "Distance for object (3) "}, {"name": "logVcharO", "desc": "log of observed characteristic dynamic velocity (4)"}, {"name": "logVchaU", "desc": "log of used characteristic dynamic velocity (4)"}, {"name": "logreff", "desc": "log of effective radius used (5) "}, {"name": "logIeff", "desc": "log of effective surface brightness used (5)"}, {"name": "Stellpop", "desc": "?=-1.00 Stellar population index (6) "}, {"name": "kappa1", "desc": "Kappa_1 (7) "}, {"name": "kappa2", "desc": "Kappa_2 (7) "}, {"name": "kappa3", "desc": "Kappa_3 (7) "}, {"name": "delta2:1", "desc": "Delta_2:1 (8) "}, {"name": "delta3:1", "desc": "Delta_3:1 (8) "}, {"name": "logMasseff", "desc": "log of effective mass of object (9) "}, {"name": "logLeff", "desc": "log of effective luminosity of object (9)"}, {"name": "log(Me/Le)", "desc": "log of mass-to-light ratio within reff (9)"}, {"name": "logTeff", "desc": "log of effective temperature (9) "}, {"name": "lognb", "desc": "log of baryon number (9) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_117_1668"}} {"id": "J/AJ/117/1668", "title_cds": "Sc galaxies I photometry, optical data", "title_create": "Haynes+, 1999", "year": "1999", "author": "Haynes M.P., Giovanelli R., Salzer J.J., Wegner G., Freudling W., Da Costa L.N., Herter T., Vogt N.P.", "title_pub": "The I-band Tully-Fisher relation for Sc galaxies: optical imaging data.", "first_author": "Haynes M.P.", "ref_biblio": [""], "bibcode": ["1999AJ....117.1668H"], "see_also": ["VII/26 : Uppsala General Catalogue of Galaxies (UGC) (Nilson 1973)", "J/AJ/113/22 : Tully-Fisher Relation. I. (Giovanelli+ 1997)", "J/AJ/116/2728 : I photometry of early-type galaxies (Scodeggio+, 1998)", "J/AJ/116/2738 : Spectroscopy of early-type galaxies (Scodeggio+ 1998)", "J/A+AS/130/333 : 2112 new 21-cm line measurements (Theureau+ 1998)", "J/AJ/117/2039 : Sc galaxies I photometry, 21cm data (Haynes+, 1999)"], "keyword_cds": "Galaxy catalogs ; Galaxies, photometry", "keyword_pub": "galaxies: photometry - galaxies: spiral - techniques: spectroscopic", "abstract": ["Properties derived from the analysis of photometric I-band imaging", "observations are presented for 1727 inclined spiral galaxies, mostly", "of types Sbc and Sc. The reduction, parameter extraction, and error", "estimation procedures are discussed in detail. The asymptotic behavior", "of the magnitude curve of growth and the radial variation in", "ellipticity and position angle are used in combination with the", "linearity of the surface brightness falloff to fit the disk portion of", "the profile. Total I-band magnitudes are calculated by extrapolating", "the detected surface brightness profile to a radius of eight disk", "scale lengths. Errors in the magnitudes, typically ~0.04 mag, are", "dominated by uncertainties in the sky subtraction and disk-fitting", "procedures. Comparison is made with the similar imaging database of", "Mathewson, Ford, & Buchhorn, both as presented originally by those", "authors and after reanalyzing their digital reduction files using", "identical disk-fitting procedures. Direct comparison is made of", "profile details for 292 galaxies observed in common. Although some", "differences occur, good agreement is found, proving that the two data", "sets can be used in combination with only minor accommodation of those", "differences. The compilation of optical properties presented here is", "optimized for use in applications of the Tully-Fisher relation as a", "secondary distance indicator in studies of the local peculiar velocity", "field."], "doi_pub": ["10.1086/300817"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "stars.dat", "desc": "J2000.0 coordinates from Simbad Database ", "columns": [{"name": "RAh", "desc": "? Right ascension (J2000.0) "}, {"name": "RAm", "desc": "? Right ascension (J2000.0) "}, {"name": "RAs", "desc": "? Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "? Declination (J2000.0) "}, {"name": "DEm", "desc": "? Declination (J2000.0) "}, {"name": "DEs", "desc": "? Declination (J2000.0) "}, {"name": "Name", "desc": "Galaxy name (UGC NNNNNN or AGC NNNNNN) "}, {"name": "Simbad", "desc": "Other name taken form Simbad database "}, {"name": "table2", "desc": "Other name from table2.dat when it differs from Simbad"}, {"name": "Com", "desc": "Comments "}]}, {"name": "table2.dat", "desc": "Optical properties ", "columns": [{"name": "UGC/AGC", "desc": "UGC (Cat. ) number where applicable or else in our private database, referred to as the Arecibo General Catalog (AGC) (1)"}, {"name": "Name", "desc": "Other galaxy designation (2) "}, {"name": "RAh", "desc": "Right ascension (1950.0) "}, {"name": "RAm", "desc": "Right ascension (1950.0) "}, {"name": "RAs", "desc": "Right ascension (1950.0) "}, {"name": "DE-", "desc": "Declination sign (1950.0) "}, {"name": "DEd", "desc": "Declination (1950.0) "}, {"name": "DEm", "desc": "Declination (1950.0) "}, {"name": "DEs", "desc": "Declination (1950.0) "}, {"name": "TType", "desc": "Hubble morphological type code "}, {"name": "r23.5", "desc": "Isophotal radius measured at an I-band surface magnitude of 23.5mag/arcsec^2^"}, {"name": "r83L", "desc": "Characteristic optical radius (3) "}, {"name": "mu", "desc": "Surface magnitude at the other most detected isophote in the I-band image"}, {"name": "E0", "desc": "disk ellipticity, corrected for seeing "}, {"name": "e_E0", "desc": "rms uncertainty on E0 "}, {"name": "PA", "desc": "Mean disk position angle "}, {"name": "e_PA", "desc": "rms uncertainty on PA "}, {"name": "Imag", "desc": "Total I-band magnitude "}, {"name": "e_Imag", "desc": "rms uncertainty on Imag "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_118_1073"}} {"id": "J/AJ/118/1073", "title_cds": "Orbiting astronomical observatory catalog", "title_create": "Meade+, 1999", "year": "1999", "author": "Meade M.R.", "title_pub": "A second catalog of orbiting astronomical observatory 2 filter photometry: ultraviolet photometry of 614 stars.", "first_author": "Meade M.R.", "ref_biblio": [""], "bibcode": ["1999AJ....118.1073M"], "keyword_cds": "Photometry, ultraviolet", "keyword_pub": "catalogs - stars: general", "abstract": ["Ultraviolet photometry from the Wisconsin Experiment Package on the", "Orbiting Astronomical Observatory 2 (OAO 2) is presented for 614", "stars. Previously unpublished magnitudes from 12 filter bandpasses", "with wavelengths ranging from 1330 to 4250{AA} have been placed on the", "white dwarf model atmosphere absolute flux scale. The fluxes were", "converted to magnitudes using V=0 for F(V)=3.46x10-9ergs/cm2/s1/{AA},", "or m_{lambda}_=-2.5logF_{lambda}_-21.15. This second catalog", "effectively doubles the amount of OAO 2 photometry available in the", "literature and includes many objects too bright to be observed with", "modern space observatories."], "doi_pub": ["10.1086/300955"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "Second OAO-2 Filter Photometry Catalogue ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "n_HD", "desc": "Last digit when two number for the same object "}, {"name": "Name", "desc": "Name "}, {"name": "SpType", "desc": "Spectral classification "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "B-V", "desc": "? B-V colour index "}, {"name": "U-B", "desc": "? U-B colour index "}, {"name": "Ref", "desc": "Reference (1) "}, {"name": "Var", "desc": "[V] V: variable "}, {"name": "UV", "desc": "Other UV observations (2) "}, {"name": "4250{AA}", "desc": "? 4250{AA} filter magnitude "}, {"name": "3320{AA}", "desc": "? 3320{AA} filter magnitude "}, {"name": "2980{AA}", "desc": "? 2980{AA} filter magnitude "}, {"name": "2940{AA}", "desc": "? 2940{AA} filter magnitude "}, {"name": "2460{AA}", "desc": "? 2460{AA} filter magnitude "}, {"name": "2380{AA}", "desc": "? 2380{AA} filter magnitude "}, {"name": "2035{AA}", "desc": "? 2035{AA} filter magnitude "}, {"name": "1910{AA}", "desc": "? 1910{AA} filter magnitude "}, {"name": "1680{AA}", "desc": "? 1680{AA} filter magnitude "}, {"name": "1550{AA}", "desc": "? 1550{AA} filter magnitude "}, {"name": "1430{AA}", "desc": "? 1430{AA} filter magnitude "}, {"name": "1330{AA}", "desc": "? 1330{AA} filter magnitude "}]}, {"name": "table3.dat", "desc": "Variable-star information for OAO-2 objects ", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "m_HD", "desc": "Last digit when two number for the same object "}, {"name": "Name", "desc": "Name "}, {"name": "Var", "desc": "Variable type "}, {"name": "Amp", "desc": "? Amplitude "}, {"name": "JD", "desc": "Julian Date (-2440000) for OAO2 observations "}, {"name": "JD2", "desc": "? Julian Date (-2440000) for OAO2 observations "}, {"name": "n_JD2", "desc": "[*] Note (1) "}, {"name": "JD3", "desc": "? Julian Date (-2440000) for OAO2 observations "}, {"name": "JD4", "desc": "? Julian Date (-2440000) for OAO2 observations "}, {"name": "JD5", "desc": "? Julian Date (-2440000) for OAO2 observations "}, {"name": "JD6", "desc": "? Julian Date (-2440000) for OAO2 observations "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_118_752"}} {"id": "J/AJ/118/752", "title_cds": "BI photometry of NGC 3256 young globular clusters", "title_create": "Zepf+, 1999", "year": "1999", "author": "Zepf S.E., Ashman K.M., English J., Freeman K.C., Sharples R.M.", "title_pub": "The formation and evolution of candidate young globular clusters in NGC 3256.", "first_author": "Zepf S.E.", "ref_biblio": [""], "bibcode": ["1999AJ....118..752Z"], "keyword_cds": "Clusters, globular ; Photometry", "keyword_pub": "galaxies: formation - galaxies: individual (NGC 3256) - galaxies: interactions - galaxies: starburst - galaxies: star clusters", "mission": "HST", "abstract": ["We present images of the recent galaxy merger NGC 3256 obtained with", "the Wide Field Planetary Camera 2 of the Hubble Space Telescope in B", "and I filters. We show that there is a large population of more than", "1000 compact, bright, blue objects in this galaxy within the 7kpcx7kpc", "region studied. These objects have sizes, colors, and luminosities", "like those expected for young Galactic globular clusters, with ages", "ranging from a few to several hundred megayears. On this basis, we", "identify at least some fraction of the compact, bright, blue objects", "in NGC 3256 as young globular clusters."], "object": ["10 27 51.3 -43 54 17 NGC 3256"], "doi_pub": ["10.1086/300961"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Candidate young globular clusters in NGC 3256 ", "columns": [{"name": "RAh", "desc": "Right ascension (J2000) (1) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Bmag", "desc": "B magnitude "}, {"name": "B-I", "desc": "B-I colour index "}, {"name": "R1/2", "desc": "Size (1 pix = 8 pc) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_120_1794"}} {"id": "J/AJ/120/1794", "title_cds": "Far-UV observations of the shell in IC 2574", "title_create": "Stewart+, 2000", "year": "2000", "author": "Stewart S.G., Walter F.", "title_pub": "Ultraviolet observations of the powering source of the supergiant shell in IC 2574.", "first_author": "Stewart S.G.", "ref_biblio": [""], "bibcode": ["2000AJ....120.1794S"], "keyword_cds": "Photometry, ultraviolet ; Photometry, H-alpha ; Stars, ages ; Stars, masses", "keyword_pub": "Galaxies: Individual: IC 2574 - Galaxies: ISM - ISM: Bubbles - ISM: Structure - Ultraviolet Emission", "abstract": ["A multiband analysis of the region containing the supergiant H I shell", "in the nearby dwarf irregular galaxy IC 2574 presents evidence of a", "causal relationship between a central star cluster, the surrounding", "expanding H I shell, and secondary star formation sites on the rim of", "the H I shell. Comparisons of the far-UV (FUV, 1521 {AA}), optical", "broad band, H-alpha, X-ray, and H I morphologies suggest that the", "region is in an auspicious moment of star formation triggered by the", "central stellar cluster. The derived properties of the H I shell, the", "central stellar cluster, and the star-forming regions on the rim", "support this scenario: The kinematic age of the H I shell is <14 Myr", "and in agreement with the age of the central stellar cluster derived", "from the FUV observations (~11 Myr). An estimate for the mechanical", "energy input from supernovae and stellar winds of the central stellar", "cluster, made from FUV photometry and the derived cluster age, is", "4.1x10^52^ ergs, roughly a few times higher than the kinetic energy of", "the H I shell. The requisite energy input needed to create the H I", "shell, derived in the ``standard'' fashion from the H I observations", "(using the numerical models of Chevalier), is 2.6x10^53^ ergs, which is", "almost 1 order of magnitude higher than the estimated energy input as", "derived from the FUV data. Given the overwhelming observational", "evidence that the central cluster is responsible for the expanding H I", "shell, this discrepancy suggests that the required energy input is", "overestimated using the ``standard'' method. This may explain why some", "other searches for remnant stellar clusters in giant H I holes have", "been unsuccessful so far. Our observations also show that stellar", "clusters are indeed able to create supergiant H I shells, even at", "large galactocentric radii; a scenario that has recently been", "questioned by a number of authors."], "object": ["10 28 47 +68 28 18 NAME IC2574 SGS"], "doi_pub": ["10.1086/301584"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Observations for star-forming regions ", "columns": [{"name": "Region", "desc": "The supergiant shell region in IC 2574 (1) "}, {"name": "Bmag", "desc": "The B band magnitude (2) "}, {"name": "Halpha", "desc": "The H{alpha} flux in units of 10^-15^ ergs/cm^2^/s/{AA} (2)"}, {"name": "FUV", "desc": "The Far-UV flux in units of 10^-15^ ergs/cm^2^/s/{AA} (2)"}, {"name": "FUVmag", "desc": "The Far-UV magnitude "}, {"name": "(FUV-B)", "desc": "The (Far-UV - B) color (3) "}, {"name": "Ratio", "desc": "Logarithmic ratio of Lyman continuum photons to FUV flux (4)"}]}, {"name": "table2.dat", "desc": "Derived parameters for star-forming regions ", "columns": [{"name": "Region", "desc": "The supergiant shell region in IC 2574 (1) "}, {"name": "Age", "desc": "The mean age of the stars in the aperture "}, {"name": "LFUV", "desc": "Far-UV luminosity corrected for internal extinction and assuming a distance of 3.2 Mpc"}, {"name": "Mass", "desc": "Mass estimate based on Age "}, {"name": "EMech", "desc": "Estimate of the net mechanical energy deposited into the ISM by SN and stellar winds (2)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_122_2190"}} {"id": "J/AJ/122/2190", "title_cds": "HDF-South multicolor observations", "title_create": "Vanzella+, 2001", "year": "2001", "author": "Vanzella E., Cristiani S., Saracco P., Arnouts S., Bianchi S., D'Odorico S., Fontana A., Giallongo E., Grazian A.", "title_pub": "Multicolor observations of the Hubble Deep Field South.", "first_author": "Vanzella E.", "ref_biblio": [""], "bibcode": ["2001AJ....122.2190V"], "see_also": ["J/AJ/112/1335 : Hubble Deep Field observations (Williams+ 1996)", "J/ApJ/513/34 : HDF photometric redshifts catalog (Fernandez-Soto+, 1999)", "J/AJ/120/2206 : NTT, HDF-S and HDF-N photometric redshifts (Fontana+, 2000)", "J/A+A/375/1 : IR obs. of Chandra Deep Field + HDF-South (Saracco+, 2001)", "J/A+A/364/517 : HDF-N spiral and irregular galaxies (Rodighiero+, 2000)", "J/AJ/120/2747 : HDF-South WFPC2 observations (Casertano+, 2000)", "J/A+AS/145/111 : HDF-South catalogue of galaxies (Volonteri+, 2000)", "J/AJ/119/486 : HDF-South: STIS imaging (Gardner+, 2000)", "J/AJ/122/2205 : HDF-South K photometric redshift catalog (Rudnick+, 2001)"], "keyword_cds": "Galaxy catalogs ; Photometry, UBVRIJKLMNH", "keyword_pub": "cosmology: observations - galaxies: evolution - galaxies: statistics", "abstract": ["We present a deep multicolor (U, B, V, I, Js, H, Ks) catalog of", "galaxies in the Hubble Deep Field South, based on observations", "obtained with the HST WFPC2 (UBVI) in 1998 and VLT-ISAAC (Js, H, Ks)", "in 1999. The photometric procedures were tuned to derive a catalog", "optimized for the estimation of photometric redshifts. In particular", "we adopted a \"conservative\" detection threshold, which resulted in a", "list of 1611 objects. The behavior of the observed source counts is in", "general agreement with the previous results of Casertano et al. (2000,", "Cat. ) in the Hubble Deep Field South and Williams et", "al. (1996, Cat. ) in the Hubble Deep Field North, while", "the corresponding counts in the Hubble Deep Field North provided by", "Fernandez-Soto, Lanzetta, & Yahil (1999, Cat. ) are", "systematically lower by a factor 1.5 beyond I_AB_=26."], "doi_pub": ["10.1086/323544"], "orcid_pub": ["0000-0002-5057-135X"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table3.dat", "desc": "The Object Catalog for the HDF-S WFPC2 Field ", "columns": [{"name": "[VCS2001]", "desc": "Identification number "}, {"name": "Xpix", "desc": "X pixel position in the WFPC2 image "}, {"name": "Ypix", "desc": "Y pixel position in the WFPC2 image "}, {"name": "RAh", "desc": "Right Ascension (J2000) "}, {"name": "RAm", "desc": "Right Ascension (J2000) "}, {"name": "RAs", "desc": "Right Ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Imag", "desc": "AB magnitude in the I band "}]}, {"name": "table5.dat", "desc": "HDF-S U-Dropouts ", "columns": [{"name": "[VCS2001]", "desc": "Identification number "}, {"name": "Imag", "desc": "AB magnitude in the I band ((F814W filter) "}, {"name": "B-I", "desc": "AB (B-I) color "}, {"name": "U-B", "desc": "AB (U-B) color "}, {"name": "Xpix", "desc": "X pixel position in the WFPC2 image "}, {"name": "Ypix", "desc": "Y pixel position in the WFPC2 image "}, {"name": "RAh", "desc": "Right Ascension (J2000) "}, {"name": "RAm", "desc": "Right Ascension (J2000) "}, {"name": "RAs", "desc": "Right Ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}]}, {"name": "table6.dat", "desc": "HDF-S B Dropouts ", "columns": [{"name": "[VCS2001]", "desc": "Identification number "}, {"name": "Imag", "desc": "AB magnitude in the I band "}, {"name": "V-I", "desc": "(V-I) AB colour index "}, {"name": "B-V", "desc": "(B-V) AB colour index "}, {"name": "Xpos", "desc": "X position "}, {"name": "Ypos", "desc": "Y position "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}]}, {"name": "table7.dat", "desc": "A list of EROs in the HDF-S with (I-K)_AB_>2.7 ", "columns": [{"name": "[VCS2001]", "desc": "Identification number (1) "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "Kmag", "desc": "K AB magnitude "}, {"name": "Imag", "desc": "? I AB magnitude "}, {"name": "l_I-K", "desc": "Limit flag on I-K "}, {"name": "I-K", "desc": "(I-K) AB magnitude "}, {"name": "n_I-K", "desc": "[*] *: I-K is an upper limit in the infrared bands"}, {"name": "MType", "desc": "Morphology (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_127_3034"}} {"id": "J/AJ/127/3034", "title_cds": "Proper-motion catalog combining USNO-B and SDSS", "title_create": "Munn+, 2004", "year": "2004", "author": "Munn J.A., Monet D.G., Levine S.E., Canzian B., Pier J.R., Harris H.C., Lupton R.H., Ivezic Z., Hindsley R.B., Hennessy G.S., Schneider D.P., Brinkmann J.", "title_pub": "An improved proper-motion catalog combining USNO-B and the Sloan Digital Sky Survey.", "first_author": "Munn J.A.", "ref_biblio": [""], "bibcode": ["2004AJ....127.3034M"], "keyword_cds": "", "keyword_pub": "astrometry - catalogs", "mission": "", "abstract": ["An improved proper-motion catalog is presented, combining the USNO-B", "and Sloan Digital Sky Survey (SDSS) catalogs in the area of sky", "covered by SDSS Data Release 1 (DR1; 2099 deg^2^). USNO-B positions are", "recalibrated using SDSS galaxies, and proper motions are recomputed", "including both the USNO-B and SDSS positions. Statistical errors in", "the USNO-B proper motions are decreased by roughly 20%-30%, systematic", "errors are greatly reduced, and the proper motions are placed on an", "absolute reference frame. Requiring a match to an SDSS object removes", "the large number of false high proper motion objects in USNO-B. The", "resultant catalog is 90% complete to g<19.7, with statistical errors", "in the component proper motions of roughly 3-3.5mas/yr, substantially", "smaller systematic errors, and a contamination rate of less than 0.5%.", "A number of studies are currently underway using proper motions from", "this catalog. The catalog is available via ftp."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/383292"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_128_330"}} {"id": "J/AJ/128/330", "title_cds": "UBVRI photometry and spectroscopy in Roslund 4", "title_create": "Delgado+, 2004", "year": "2004", "author": "Delgado A.J., Miranda L.F., Fernandez M., Alfaro E.J.", "title_pub": "Photometric and spectroscopic study of stars in the field of the young open cluster Roslund 4.", "first_author": "Delgado A.J.", "ref_biblio": [""], "bibcode": ["2004AJ....128..330D"], "keyword_cds": "", "keyword_pub": "H II regions ; ISM: Herbig-Haro objects ; open clusters and associations: individual (Roslund 4); stars: emission-line, Be; stars: fundamental parameters; stars: pre-main sequence", "description": ["Images of Roslund 4 were obtained on 2003 June 30 with the 1.5m", "telescope at the Observatorio de Sierra Nevada (OSN, Granada).", "3 narrow-band filters were used: H{alpha} (656.3nm, FWHM=5.3nm),", "SII (672.3nm, FWHM=5nm), and a continuum filter (665.2nm, FWHM=5nm).", "The UBVRI photometric observations were carried out in 2000 August,", "and were calbirated wo standard fields of the Landolt catalog (1992,", "Cat. II/183)", "The spectra were taken on the nights of 2001 August 11 and 12 with the", "ISIS spectrograph attached to the WHT telescope at the ORM in La", "Palma. Detectors EEV12 and TeK4 were mounted in the blue and red arms,", "respectively. The wavelength ranges 350-500 and 635-675nm were", "observed at respective resolutions R = 10,000 and 16,000."], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/421742"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_129_2562"}} {"id": "J/AJ/129/2562", "title_cds": "NYU-VAGC catalog", "title_create": "Blanton+, 2005", "year": "2005", "author": "Blanton M.R., Schlegel D.J., Strauss M.A., Brinkmann J., Finkbeiner D., Fukugita M., Gunn J.E., Hogg D.W., Ivezic Z., Knapp G.R., Lupton R.H., Munn J.A., Schneider D.P., Tegmark M., Zehavi I.", "title_pub": "New York University Value-Added Galaxy Catalog: a galaxy catalog based on new public surveys.", "first_author": "Blanton M.R.", "ref_biblio": [""], "bibcode": ["2005AJ....129.2562B"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/429803"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_143_57"}} {"id": "J/AJ/143/57", "title_cds": "New RVs from the spectroscopic survey BRAVA (II)", "title_create": "Kunder+, 2012", "year": "2012", "author": "Kunder A., Koch A., Rich R.M., De Propris R., Howard C.D., Stubbs S.A., Johnson C.I., Shen J., Wang Y., Robin A.C., Kormendy J., Soto M., Frinchaboy P., Reitzel D.B., Zhao H., Origlia L.", "title_pub": "The bulge radial velocity assay (BRAVA). II. Complete sample and data release.", "first_author": "Kunder A.", "ref_biblio": [""], "bibcode": ["2012AJ....143...57K"], "see_also": ["VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "J/A+A/546/A57 : Spectroscopy of 400 Bulge red giants (Uttenthaler+, 2012)", "J/ApJ/733/L47 : Galaxy bulge types within 11Mpc (Fisher+, 2011)", "J/ApJ/732/108 : Abundances of 92 giants in Plaut's window (Johnson+, 2011)", "J/ApJ/691/1387 : Spectroscopy of the Galactic bar. I. (Rangwala+, 2009)", "J/A+A/486/177 : Bulge field stars from FLAMES-GIRAFFE (Zoccali+, 2008)", "J/MNRAS/348/1439 : OGLE II Galactic center proper motions (Sumi+, 2004)", "J/AJ/118/895 : Milky way and stellar distributions (Tiede+ 1999)", "J/MNRAS/246/54 : Late-type giants in Baade's window (Sharples+ 1990)", "J/AJ/89/636 : Giant M stars in Baade's Window (Blanco+, 1984)", "http://irsa.ipac.caltech.edu/ : NASA/IPAC Infrared Science Archive (IRSA)", "http://brava.astro.ucla.edu/ : The Bulge Radial Velocity Assay at University"], "keyword_cds": "Milky Way ; Stars, M-type ; Stars, giant ; Spectroscopy ; Radial velocities ; Velocity dispersion", "keyword_pub": "Galaxy: center - stars: abundances - stars: distances - stars: Population II - surveys", "abstract": ["We present new radial velocity measurements from the Bulge Radial", "Velocity Assay, a large-scale spectroscopic survey of M-type giants in", "the Galactic bulge/bar region. The sample of ~4500 new radial", "velocities, mostly in the region -10{deg}"], "bibcode": ["2017AJ....153...10M"], "see_also": ["J/ApJS/219/19 : Nearby white dwarfs from SUPERBLINK (Limoges+, 2015)", "J/MNRAS/449/3966 : Ultracool white dwarfs (Gianninas+, 2015)", "J/ApJ/730/128 : Spectroscopy of DA WD from the SDSS-DR4 (Tremblay+, 2011)", "J/ApJ/714/1037 : White dwarfs from the Kiso survey (Limoges+, 2010)", "J/ApJS/190/77 : Detailed analysis of cool WDs in the SDSS (Kilic+, 2010)", "J/A+A/466/627 : Parameters of DA white dwarfs in SDSS-DR1 (Hu+, 2007)", "J/AJ/132/1221 : VJHK and SDSS photometry of DA white dwarfs (Holberg+, 2006)", "J/AJ/131/582 : Cool white dwarfs in the SDSS (Kilic+, 2006)", "J/ApJS/156/47 : DA white dwarfs from Palomar Green Survey (Liebert+, 2005)", "J/ApJ/607/426 : Catalog of white dwarfs in SDSS-DR1 (Kleinman+, 2004)", "J/AJ/125/2621 : SDSS WD-M binary parameters (Raymond+, 2003)", "J/MNRAS/335/673 : DA white dwarfs in 2dF QSO Redshift Survey (Vennes+, 2002)", "J/ApJS/133/413 : BVRIJHK photometry of cool white dwarfs (Bergeron+, 2001)"], "keyword_cds": "Stars, dwarfs", "keyword_pub": "stars: luminosity function, mass function - white dwarfs", "abstract": ["A catalog of 8472 white dwarf (WD) candidates is presented, selected", "using reduced proper motions from the deep proper motion catalog of", "Munn et al. Candidates are selected in the magnitude range 16"], "bibcode": ["1963AJ.....68..319M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["A catalogue of spectral types and infra-red magnitudes for 920 stars", "M5 and later in an area of 9 square degrees surrounding S.A. 158", "(l=3.9deg, b=-9.0deg) is given. These data, together with similar", "unpublished data for 7069 stars nearer the galactic equator in the", "same general direction, have been analyzed for space density. The", "number of stars per 10^6^pc^3^ appears to be relatively constant", "at about 0.2 in a stratum 1kpc thick south of the galactic plane.", "Superposed on this basic layer and beginning at approximately 6kpc", "from the sun is a concentration of stars in which the density rises to", "5 or 6 times that in the basic stratum. The negative density gradient", "perpendicular to the galactic plane near the galactic center appears", "to be quite high."], "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/108980"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_69_104"}} {"id": "J/AJ/69/104", "title_cds": "Stellar space density near selected area 158", "title_create": "McCuskey, 1964", "year": "1964", "author": "McCuskey S. W.", "title_pub": "Stellar space density near selected area 158", "first_author": "McCuskey S. W.", "ref_biblio": [""], "bibcode": ["1964AJ.....69..104M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["Spectral types and photographic magnitudes for 1684 stars in", "25.2sq.deg surrounding S.A.158 are presented in a catalogue and", "identification charts. The matnitude limit of the data is about", "m_pg_=12. Color indices approximately on the (B,V) system are given", "for 275 stars. Stellar space densities are presented as a function", "of distance in table VII and Fig.3. The early A stars decrease by a", "factor of 10 between 100 and 2000pc from the sun. The yellow-red giant", "stars have approximately a constant density in this distance interval.", "A comparison of the density functions with those for the galactic", "anticenter is shown in Fig.4. General luminosity functions computed", "from the above data have mean values of log{phi}(M) for 0"], "bibcode": ["1968AJ.....73..590D"], "see_also": ["II/221 : LF"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/110666"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_76_412"}} {"id": "J/AJ/76/412", "title_cds": "UBV sequences for QSOs", "title_create": "Angione+, 1971", "year": "1971", "author": "Angione R.J.", "title_pub": "Photoelectric sequences for the brighter QSO's.", "first_author": "Angione R.J.", "ref_biblio": [""], "bibcode": ["1971AJ.....76..412A"], "keyword_cds": "Photometry, UBV ; QSOs", "keyword_pub": "", "mission": "", "description": ["UBV photoelectric sequences were measured for 22 of the brighter QSOs", "and four other objects. The results and finding charts were used to", "identify the stars observed.", "The attached plain-text list shows coordinates for stars in"], "doi_pub": ["10.1086/111136"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "angione71.dat", "desc": "Positions and photometry of stars observed ", "columns": [{"name": "Field", "desc": "File name (QSO or AGN name) "}, {"name": "Seq", "desc": "[A-G' ] Star sequence "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[UGAMS] Source of position "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "B-V", "desc": "Johnson B-V magnitude "}, {"name": "U-B", "desc": "? Johnson U-B magnitude "}, {"name": "Comments", "desc": "Additional comments, from B. Skiff. "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_78_687"}} {"id": "J/AJ/78/687", "title_cds": "Southern stars of astrophysical interest", "title_create": "Bidelman+, 1973", "year": "1973", "author": "Bidelman W.P., Macconnell D.J.", "title_pub": "The brighter stars of astrophysical interest in the southern sky.", "first_author": "Bidelman W.P.", "ref_biblio": [""], "bibcode": ["1973AJ.....78..687B"], "see_also": ["III/46 : Ap and Am Stars (Bertaud+ 1974; Bidelman+ 1973)"], "keyword_cds": "", "keyword_pub": "", "mission": "", "doi_pub": ["10.1086/111475"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "bidmac.dat", "desc": "The catalog of stars of astrophysical interest in the southern sky (Tables III to X)", "columns": [{"name": "Name", "desc": "Star name (1) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "s", "desc": "[UTMG] Source of position "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "SpType", "desc": "MK spectral type "}, {"name": "Remarks", "desc": "Remartks and notes by B. Skiff "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_79_107"}} {"id": "J/AJ/79/107", "title_cds": "Positions and Identifications in Stock 2", "title_create": "Mccuskey+, 1974", "year": "1974", "author": "Mccuskey S.W.", "title_pub": "The space density of A stars in a region in Cassiopeia.", "first_author": "Mccuskey S.W.", "ref_biblio": [""], "bibcode": ["1974AJ.....79..107M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "description": ["This list shows accarute coordinates and identifications for about 440", "stars in the region of the open cluster Stock 2 observed by McCuskey.", "Many of the stars are present in SIMBAD only by name, lacking", "coordinates altogether. I used the published charts in combination", "with computer screen-plots of stars to get coordinates in addition to", "VizieR and SIMBAD.", "The table shows the names, coordinates (nearly all from Tycho-2),", "Tycho-2 numbers, plus HD, BD, and AGK numbers as available. Many of", "the BD names were omitted by McCuskey. I copy McCuskey's photographic", "V magnitudes rounded to 0.1-mag precision---rms scatter is ~0.2 mag", "despite the claims in the text. Finally his spectral types, which", "appear to be reliable. The remarks include those given by McCuskey as", "well as descriptions of of double stars etc.", "There is much overlap in this region with spectral surveys by the", "Marseilles group, the Kiev group, Brodskaya, Stock's original cluster", "paper, and others. A few stars are included that are in the region of", "clusters besides Stock 2: NGC 743, Markarian 6, and IC 1805, among", "those I noticed.", "Additional photoelectric photometry and slit-spectra for many of the", "same stars are given in the companion paper by Pesch & McCuskey", "(1974AJ.....79..16P)."], "curator": "Francois Ochsenbein [CDS]", "alias": ["[M74]"], "doi_pub": ["10.1086/111537"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_80_208"}} {"id": "J/AJ/80/208", "title_cds": "Souther Stars embedded in nebulosity", "title_create": "van den Bergh+, 1975", "year": "1975", "author": "van den Bergh S., Herbst W.", "title_pub": "Catalogue of southern stars embedded in nebulosity.", "first_author": "van den Bergh S.", "ref_biblio": [""], "bibcode": ["1975AJ.....80..208V"], "see_also": ["VII/21 : Catalogue of Reflection Nebulae (Van den Bergh, 1966)"], "keyword_cds": "Nebulae ; Milky Way", "description": ["A survey of the Milky Way southward of the Palomar Sky Survey for the", "identification of reflection nebulae was carried out at the Cerro", "Tololo Inter-American Observatory in Chile. Plates in blue light were", "obtained at the Curtis Schmidt telescope covering a strip of plus or", "minus six degrees of the galactic equator. Red sensitive plates for", "comparison were also obtained with the same telescope covering the", "same area near the galactic plane. Observatory staff members and some", "students of the University of Toronto, Canada assisted in identifying", "stars embedded in nebulosity as shown by the plates. Although this", "catalogue roughly complements the Catalogue of Reflection Nebulae of", "van den Berg (1966AJ.....71..990V, Cat. ), the region here", "surveyed is more narrowly confined to the galactic equator."], "alias": ["VDBH", "BHe"], "doi_pub": ["10.1086/111733"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "bhe.dat", "desc": "The Catalogue (Table I of publication) ", "columns": [{"name": "BHe", "desc": "BHe id number and components as (a, b, c) "}, {"name": "IDs", "desc": "Alternate designation "}, {"name": "RAh", "desc": "Right Ascension B1950 (hours) "}, {"name": "RAm", "desc": "Right Ascension B1950 (minutes) "}, {"name": "DE-", "desc": "Declination B1950 (sign) "}, {"name": "DEd", "desc": "Declination B1950 (degrees) "}, {"name": "DEm", "desc": "Declination B1950 (minutes) "}, {"name": "Type", "desc": "Type of nebula, see Note (1) "}, {"name": "u_Type", "desc": "Uncertainty flag (:) on Type "}, {"name": "SurfBr", "desc": "Surface brightness from blue plates, Note (2) "}, {"name": "u_SurfBr", "desc": "Uncertainty flag (:) on SurfBr "}, {"name": "Color", "desc": "Coded reference to colors, see Note (3) "}, {"name": "u_Color", "desc": "Uncertainty flag (:) on Color "}, {"name": "Absorb", "desc": "Absorption in field of nebula, see Note (4) "}, {"name": "u_Absorb", "desc": "Uncertainty flag (:) on Absorb "}, {"name": "BDiaMax", "desc": "? Maximum diameter observed on blue plates "}, {"name": "u_BDiaMax", "desc": "Uncertainty flag (:) on BDiaMax "}, {"name": "RDiaMax", "desc": "? Maximum diameter observed on red plates "}, {"name": "u_RDiaMax", "desc": "Uncertainty flag (:) on RDiaMax "}, {"name": "Rem", "desc": "Note flag (*) detailed in file \"notes.dat\" "}]}, {"name": "notes.dat", "desc": "Full notes of publication for Table I ", "columns": [{"name": "BHe", "desc": "BHe id descriptor, repeated if several lines "}, {"name": "Text", "desc": "Text of note "}, {"name": "Flag", "desc": "'*' if note continues on next line "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_81_350"}} {"id": "J/AJ/81/350", "title_cds": "Dwarf late-type stars in the NGP", "title_create": "Sanduleak+, 1976", "year": "1976", "author": "Sanduleak N.", "title_pub": "Catalog of probable dwarf stars of type M3 and later in the direction of the North Galactic Pole.", "first_author": "Sanduleak N.", "ref_biblio": [""], "bibcode": ["1976AJ.....81..350S"], "keyword_cds": "Stars, late-type ; Galactic pole, north", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/111894"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_82_345"}} {"id": "J/AJ/82/345", "title_cds": "OB stars in the Coalsack region", "title_create": "Muzzio+, 1977", "year": "1977", "author": "Muzzio J.C., Orsatti A.M.", "title_pub": "Searches for faint OB stars in the Southern Milky Way. I. The Coalsack region.", "first_author": "Muzzio J.C.", "ref_biblio": [""], "bibcode": ["1977AJ.....82..345M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/112056"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_82_474"}} {"id": "J/AJ/82/474", "title_cds": "OB stars in the Vela region", "title_create": "Muzzio+, 1977", "year": "1977", "author": "Muzzio J.C., Orsatti A.M.", "title_pub": "Searches for faint OB stars in the Southern Milky Way. II. The Vela region.", "first_author": "Muzzio J.C.", "ref_biblio": [""], "bibcode": ["1977AJ.....82..474M"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/112076"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_90_418"}} {"id": "J/AJ/90/418", "title_cds": "Galaxies redshifts", "title_create": "Koo+, 1985", "year": "1985", "author": "Koo D.C.", "title_pub": "Optical multicolors : a poor person's z machine for galaxies.", "first_author": "Koo D.C.", "ref_biblio": [""], "bibcode": ["1985AJ.....90..418K"], "keyword_cds": "Redshifts ; Galaxies, photometry", "abstract": ["We explore the feasibility, limits, accuracy, and uncertainties of", "using optical broadband colors in the form of twocolor plots to", "measure the redshifts of faint galaxies. Comparison of redshifts from", "slit spectra and 4-m photographic UBVI photometry of 100 faint", "galaxies confirms that colors do yield redshifts. These galaxies of", "17-23mag in B span a wide range of intrinsic color and are thus", "unlike previous samples of faint galaxies that were largely radio or", "cluster galaxies of early (red) type. For redshifts less than 0.35,", "two-thirds of the color redshifts agree with the spectroscopic values", "to within +/-0.04 in z; for higher redshifts to z of 0.6, the errors", "increase to +/-0.06. These accuracies were achieved for blue as well", "as red galaxies, and ensure that multicolors-can serve as a poor", "person's redshift machine to study distant galaxies in clusters and", "the field."], "doi_pub": ["10.1086/113748"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table4.dat", "desc": "Redshifts and multicolor photometry ", "columns": [{"name": "Seq", "desc": "[1/116]+ Sequential number "}, {"name": "z", "desc": "? Spectroscopic redshift "}, {"name": "zUF", "desc": "Redshift determined from UF plots "}, {"name": "zUJFN", "desc": "? Redshift determined from UJFN plots "}, {"name": "J+mag", "desc": "J^+^ magnitude (1) "}, {"name": "U+-J+", "desc": "U^+^-J^+^ colour index (1) "}, {"name": "J+-F+", "desc": "J^+^-F^+^ colour index (1) "}, {"name": "F+-N+", "desc": "? F^+^-N^+^ colour index (1) "}, {"name": "Set", "desc": "Set number "}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "Group", "desc": "Group (I, II or III) "}, {"name": "Seq", "desc": "Sequential number "}, {"name": "Note", "desc": "Text of the note (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_91_530"}} {"id": "J/AJ/91/530", "title_cds": "BV photometry of faint galaxies", "title_create": "Peterson+, 1986", "year": "1986", "author": "Peterson C.J., Baumgart C.W.", "title_pub": "Blue and visual photometry of the Rubin et al. (1976) sample of faint galaxies", "first_author": "Peterson C.J.", "ref_biblio": [""], "bibcode": ["1986AJ.....91..530P"], "keyword_cds": "Galaxies, photometry ; Photometry, UBV", "abstract": ["Blue and visual multiaperture photoelectric photometry of 112 faint", "spiral galaxies from the list of Rubin et al. (1976AJ.....81..687R) is", "presented. We briefly compare total galaxy magnitudes [for an", "aperture/diameter ratio of 1.0 according to the precepts of Graham", "(1976AJ.....81..681G)] with the photographic magnitudes of the Zwicky", "et al. (1961-1968, Cat. ) Catalogue of Galaxies and Clusters of", "Galaxies. From a reanalysis for the motion of the Local Group, we find", "that use of the new galaxy magnitudes increases the difference between", "the motion vector derived from Rubin et al. and the motions derived", "from other sample galaxies and that implied by the anisotropy of the", "cosmic background radiation."], "doi_pub": ["10.1086/114032"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Kitt Peak photoelectric BV photometry of Rubin et al. (1976AJ.....81..687R) Sc I galaxies", "columns": [{"name": "Galaxy", "desc": "Galaxy designation (1) "}, {"name": "Vmag0.46", "desc": "? V magnitude over circular area of 0.46' "}, {"name": "u_Vmag0.46", "desc": "Uncertainty flag on Vmag0.46 "}, {"name": "Vmag0.94", "desc": "? V magnitude over circular area of 0.94' "}, {"name": "u_Vmag0.94", "desc": "Uncertainty flag on Vmag0.94 "}, {"name": "n_Vmag0.94", "desc": "[*] Note on Vmag0.94 (2) "}, {"name": "Vmag1.39", "desc": "? V magnitude over circular area of 1.39' "}, {"name": "u_Vmag1.39", "desc": "Uncertainty flag on Vmag1.39 "}, {"name": "n_Vmag1.39", "desc": "[*] Note on Vmag1.39 (2) "}, {"name": "Vmag1.87", "desc": "? V magnitude over circular area of 1.87' "}, {"name": "u_Vmag1.87", "desc": "Uncertainty flag on Vmag1.87 "}, {"name": "n_Vmag1.87", "desc": "[*] Note on Vmag1.87 (2) "}, {"name": "B-V0.46", "desc": "? B-V colour index over circular area of 0.46' "}, {"name": "u_B-V0.46", "desc": "Uncertainty flag on B-V0.46 "}, {"name": "B-V0.94", "desc": "? B-V colour index over circular area of 0.94' "}, {"name": "u_B-V0.94", "desc": "Uncertainty flag on B-V0.94 "}, {"name": "n_B-V0.94", "desc": "[*] Note on B-V0.94 (2) "}, {"name": "B-V1.39", "desc": "? B-V colour index over circular area of 1.39' "}, {"name": "u_B-V1.39", "desc": "Uncertainty flag on B-V1.39 "}, {"name": "n_B-V1.39", "desc": "[*] Note on B-V1.39 (2) "}, {"name": "B-V1.87", "desc": "? B-V colour index over circular area of 1.87' "}, {"name": "u_B-V1.87", "desc": "Uncertainty flag on B-V1.87 "}, {"name": "n_B-V1.87", "desc": "[*] Note on B-V1.87 (2) "}, {"name": "Nnights", "desc": "Number of separate nights on which the galaxy was observed"}, {"name": "Notes", "desc": "[G1234567] Notes (3) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_94_106"}} {"id": "J/AJ/94/106", "title_cds": "H{alpha} survey of rho Oph complex", "title_create": "Wilking+, 1987", "year": "1987", "author": "Wilking B.A., Schwartz R.D., Blackwell J.H.", "title_pub": "An H-alpha emission-line survey of the rho Ophiuchi dark cloud complex.", "first_author": "Wilking B.A.", "ref_biblio": [""], "bibcode": ["1987AJ.....94..106W"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/114452"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_95_739"}} {"id": "J/AJ/95/739", "title_cds": "Early-G dwarf stars towards SGP", "title_create": "Corbally+, 1988", "year": "1988", "author": "Corbally C.J., Garrison R.F.", "title_pub": "A search for early-G dwarf stars towards the South Galactic Pole.", "first_author": "Corbally C.J.", "ref_biblio": [""], "bibcode": ["1988AJ.....95..739C"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/114671"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_95_745"}} {"id": "J/AJ/95/745", "title_cds": "G dwarf stars at NGP", "title_create": "Corbally+, 1988", "year": "1988", "author": "Corbally C.J., Garrison R.F.", "title_pub": "A search for early-G dwarf stars the North Galactic Pole.", "first_author": "Corbally C.J.", "ref_biblio": [""], "bibcode": ["1988AJ.....95..745C"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/114672"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_99_1488"}} {"id": "J/AJ/99/1488", "title_cds": "UBVRI sequences in the Magellanic Clouds", "title_create": "Alcaino+, 1990", "year": "1990", "author": "Alcaino G., Alvarado F., Wenderoth E., Liller W.", "title_pub": "Photoelectric UBVRI sequences in the Magellanic Cloud clusters Lindsay 1, NGC 339, NGC 361, and NGC 1466.", "first_author": "Alcaino G.", "ref_biblio": [""], "bibcode": ["1990AJ.....99.1488A"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/115433"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_99_1501"}} {"id": "J/AJ/99/1501", "title_cds": "UBVRI sequences in globulars", "title_create": "Alvarado+, 1990", "year": "1990", "author": "Alvarado F., Wenderoth E., Alcaino G., Liller W.", "title_pub": "Photoelectric UBVRI sequences in the galactic globular clusters NGC 6752 and NGC 6864.", "first_author": "Alvarado F.", "ref_biblio": [""], "bibcode": ["1990AJ.....99.1501A"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/115435"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_159_50"}} {"id": "J/AJ/159/50", "title_cds": "Identifying multiple populations in M71 using CN", "title_create": "Gerber+, 2020", "year": "2020", "author": "Gerber J.M., Friel E.D., Vesperini E.", "title_pub": "Identifying multiple populations in M71 using CN.", "first_author": "Gerber J.M.", "ref_biblio": [""], "bibcode": ["2020AJ....159...50G"], "see_also": ["VII/195 : Globular Clusters in the Milky Way (Harris, 1996)", "VII/202 : Globular Clusters in the Milky Way (Harris, 1997)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+, 2003)", "J/A+AS/144/227 : BV photometry of M71 (Geffert+, 2000)", "J/AJ/125/197 : CN abundances of the 47 Tuc main sequence (Harbeck+, 2003)", "J/AJ/127/1588 : 47 Tuc main-sequence star abundances (Briley+, 2004)", "J/ApJ/638/1018 : Equivalent widths for giant stars in M13 and M71 (Yong+, 2006)", "J/A+A/486/941 : Abundances in M71 (NGC 6838) (Alves-Brito+, 2008)", "J/ApJ/687/1019 : Chandra X-ray observations of M71 (Elsner+, 2008)", "J/A+A/505/139 : Abundances red giants 17 globular clusters (Carretta+, 2009)", "J/A+A/505/117 : Abundances red giants 15 globular clusters (Carretta+, 2009)", "J/ApJ/754/L38 : Abundances & radial velocities of M13 giants (Johnson+, 2012)", "J/other/Nat/498.198 : Na abundances in NGC6752 (Campbell+, 2013)", "J/ApJ/810/148 : Red giant abundances in NGC 2808 (Carretta, 2015)", "J/AJ/149/53 : Rad. velocities 12 Milky Way globular clusters (Kimmig+, 2015)", "J/ApJ/801/125 : Carbon in red giants in GCs and dSph galaxies (Kirby+, 2015)", "J/A+A/573/A70 : UBVI photometry in 3 globular clusters (Nardiello+, 2015)", "J/ApJ/824/5 : Chemical abundances in NGC 5024 (M53) (Boberg+, 2016)", "J/AJ/151/7 : Globular & open clusters observed SDSS/SEGUE (Morrison+, 2016)", "J/AJ/156/6 : Light element abundances RGB & AGB stars in M10 (Gerber+,2018)"], "keyword_cds": "Clusters, globular; Effective temperatures; Magnitudes, absolute; Radial velocities; Stars, giant; Abundances; Stars, horizontal branch; Spectra, optical", "keyword_pub": "Globular star clusters ; Stellar astronomy ; Spectroscopy", "abstract": ["We have observed their cyanogen CN features at ~3800 and 4120{AA} as", "well as the CH band at ~4300{AA} for 145 evolved stars in the Galactic", "globular cluster M71 using the multi-object spectrograph, Hydra, on", "the Wisconsin-Indiana-Yale- NOAO-3.5 m telescope. We use these", "measurements to create two {delta}CN indices finding that both", "distributions are best fit by two populations: a CN-enhanced and", "CN-normal. We find that 42%{+/-}4% of the red giant branch stars in", "our sample are CN-enhanced. The percentage of CN-enhanced is", "40%{+/-}13% for the asymptotic giant branch and 33%{+/-}9% for the", "horizontal branch stars (HB stars), which suggests there are no", "missing second generation stars at these stages of stellar evolution.", "The two generations also separate in magnitude and color on the HB,", "which allows us to find the difference in He abundance between the two", "populations by fitting appropriate zero-age horizontal branches. The", "broad range of distances from the cluster's center covered by our", "sample allows us to study the dependence of the ratio of the number of", "first to second population stars on the distance from the cluster's", "center, and we find that this ratio does not vary radially and that", "the two populations are spatially mixed. Finally, we compare our", "identification of multiple populations with the classification based", "on the Na-O anti-correlation and the Hubble Space Telescope UV", "photometry, and we find good agreement with both methods."], "description": ["In this paper, we continue our previous work on multiple populations", "in globular clusters (GCs) (Gerberi+, 2018, J/AJ/156/6) with a sample", "size of approximately 150 stars in M71.", "We obtained 171 combined spectra of stars within a 18' by 18' grid", "around the center of M71 between four observation runs in 2014 August,", "2015 June, 2016 June, and 2017 June using the", "Wisconsin-Indiana-Yale-NOAO (WIYN) 3.5m Telescope and Hydra, a", "multi-object, fiber-fed bench spectrograph. The Bench Spectrograph was", "used with the \"600@10.1\" grating, which resulted in spectra with a", "~4.5{AA}/pixel dispersion covering a range of ~2800{AA}. The spectra", "taken during the 2014 run are centered on a wavelength of 4900{AA},", "while the spectra taken in subsequent runs are centered on a", "wavelength of 5100{AA}. Ten different configurations of fibers were", "necessary to obtain our full sample size."], "type": ["OC"], "doi_pub": ["10.3847/1538-3881/ab607e"], "orcid_pub": ["0000-0001-9583-0004"], "data": "f-v", "date_creation": "25-Mar-2020", "xmatch": "J/AJ/159/50/table1", "last_update": "26-Mar-2020", "catid": "51590050", "date_update": "26-Mar-2020", "tables": [{"name": "table1.dat", "desc": "Stars measured in M71 ", "columns": [{"name": "ID", "desc": "[2/2299] Index number (1) "}, {"name": "RAdeg", "desc": "[298.36/298.52] Right Ascension (J2000) (1) "}, {"name": "DEdeg", "desc": "[18.72/18.85] Declination (J2000) (1) "}, {"name": "HRV", "desc": "[-112/30] Heliocentric radial velocity "}, {"name": "Vmag", "desc": "[12/18] Apparent V band magnitude (1) "}, {"name": "B-V", "desc": "[0.75/1.9] The (B-V) color (1) "}, {"name": "VMAG", "desc": "[-1.7/4.2] Absolute V band magnitude assuming (m-M)v=13.728"}, {"name": "2MASS", "desc": "2MASS identifier (HHMMSSss+DDMMSSs; J2000) if any"}, {"name": "Teff", "desc": "[3485/6084] Effective temperature "}, {"name": "logg", "desc": "[0.19/4.4] log surface gravity "}, {"name": "S3839", "desc": "[-0.7/0.5]?=99.99 The S(3839) index "}, {"name": "CN4216", "desc": "[-0.07/0.5]?=99.99 The CN(4216) index "}, {"name": "CH4300", "desc": "[0.08/0.4]?=99.99 The CH(4300) index "}, {"name": "DS3839", "desc": "[-0.7/0.5]?=100.144 The {delta}S(3839) index "}, {"name": "DCN4216", "desc": "[-0.2/0.3]?=99.838 The {delta}CN(4216) index "}, {"name": "[Na/Fe]", "desc": "[-0.1/0.9]?=99.999 log Na/Fe abundance ratio "}, {"name": "[O/Fe]", "desc": "[0.05/0.8]?=99.999 log O/Fe abundance ratio "}, {"name": "r_[Na/Fe]", "desc": "? Source reference for [Na/Fe] (2) "}, {"name": "r_[O/Fe]", "desc": "? Source reference for [O/Fe] (2) "}, {"name": "OType", "desc": "Branch (3) "}, {"name": "Mm", "desc": "[y/n] Membership y=yes (146 occurrences), n=no (5 occurrences)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_159_27"}} {"id": "J/AJ/159/27", "title_cds": "LCs of the Manwe-Thorondor eclipsing system", "title_create": "Rabinowitz+, 2020", "year": "2020", "author": "Rabinowitz D.L., Benecchi S.D., Grundy W.M., Verbiscer A.J., Thirouin A.", "title_pub": "The complex rotational light curve of (385446) Manwe-Thorondor, a multicomponent eclipsing system in the Kuiper Belt.", "first_author": "Rabinowitz D.L.", "ref_biblio": [""], "bibcode": ["2020AJ....159...27R"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "B/astorb : Orbits of Minor Planets (Bowell+, 2014)", "J/A+A/380/347 : BVRI photometry of 27 Kuiper Belt Objects (Delsanti+, 2001)", "J/A+A/407/1139 : RVB photometry Kuiper-Belt obj. 1999 TD10 (Rousselot+, 2003)", "J/AJ/127/3023 : R magnitudes Kuiper Belt object 2001QG298 (Sheppard+, 2004)", "J/AJ/135/55 : NIR spectra Centaurs & Kuiper Belt objects (Barkume+, 2008)", "J/A+A/509/A94 : Lightcurves of 14 NEAs (Kwiatkowski+, 2010)", "J/A+A/511/A49 : Lightcurves of 12 NEAs (Kwiatkowski+, 2010)", "J/ApJ/720/1691 : Observations of the distant Kuiper belt (Schwamb+, 2010)", "J/A+A/546/A86 : R absolute magnitudes Kuiper Belt objects (Peixinho+, 2012)", "J/ApJ/749/10 : SDSS observations of Kuiper belt objects (Ofek, 2012)", "J/A+A/556/A8 : 100 asteroids rotational parameters (Lhotka+, 2013)", "J/A+A/562/A48 : Light curves of asteroid (25143) Itokawa (Lowry+, 2014)", "J/ApJS/227/20 : Rotation periods of asteroids using iPTF (Chang+, 2016)", "J/AJ/154/62 : Orbital parameters of Kuiper Belt objects (Volk+, 2017)", "J/AJ/154/241 : Photometry Kuiper Belt object: 2002 CC249 (Thirouin+, 2017)", "J/A+A/627/A172 : Near-Earth asteroid (1917) Cuyo opt. & IR obs. (Rozek+,2019)", "J/AJ/157/228 : Cold Classical TNOs LCs & rot. properties (Thirouin+,2019)"], "keyword_cds": "Minor planets; Solar system; Photometry, ugriz; Magnitudes, absolute", "keyword_pub": "Kuiper belt ; Light curves ; Small solar system bodies", "abstract": ["Kuiper Belt Object (385446) Manwe-Thorondor is a multiobject system", "with mutual events predicted to occur from 2014 to 2019. To detect the", "events, we observed the system at 4 epochs (UT 2016 August 25 and 26,", "2017 July 22 and 25, 2017 November 9, and 2018 October 6) in g, r, and", "VR bands using the 4m SOAR and the 8.1m Gemini South telescopes at", "Cerro Pachon, Chile, and Lowell Observatory's 4.3m Discovery Channel", "Telescope at Happy Jack, Arizona. These dates overlap the uncertainty", "range ({+/-}0.5 day) for four inferior events (Thorondor eclipsing", "Manwe). We clearly observe variability for the unresolved system with", "a double-peaked period 11.88190{+/-}0.00005hr and ~0.5mag amplitude", "together with much longer-term variability. Using a multicomponent", "model, we simultaneously fit our observations and earlier photometry", "measured separately for Manwe and Thorondor with the Hubble Space", "Telescope. Our fit suggests Manwe is bilobed, close to the \"barbell\"", "shape expected for a strengthless body with density ~0.8g/cm^3^ in", "hydrostatic equilibrium. For Manwe, we thereby derive maximum width to", "length ratio ~0.30, surface area equivalent to a sphere of diameter", "190km, geometric albedo 0.06, mass 1.4x1018kg, and spin axis oriented", "~75deg from Earth's line of sight. Changes in Thorondor's brightness", "by ~0.6mag with a ~300day period may account for the system's", "long-term variability. Mutual events with unexpectedly shallow depth", "and short duration may account for residuals to the fit. The system is", "complex, providing a challenging puzzle for future modeling efforts."], "description": ["The epoch 1 observations reported here were obtained in the Sloan", "Digital Sky Survey (SDSS) r and g bands on two consecutive nights", "(2016 August 25 and 26 UT) using the SOAR Optical Imager on the 4m", "SOAR telescope at Cerro Pachon, Chile. The imager pixel scale was", "0.154\".", "The epoch 2 observations were obtained in SDSS r and g bands on 2017", "July 22 and 25 UT using the GMOS-S imager on the 8.1m Gemini South", "telescope at Cerro Pachon, Chile. The imager pixel scale was 0.16\".", "The epoch 3 observations were obtained on 2017 November 9 UT in r band", "using the Large Monolithic Imager (LMI) on Lowell Observatory's", "Discovery Channel Telescope (DCT) at Happy Jack AZ. The LMI pixel", "scale was 0.24\".", "The epoch 4 observations were obtained on 2018 October 6 UT in a wide", "VR band, again using the LMI on the DCT.", "Table2 lists the observing circumstances for each epoch.", "Table 4 lists resolved photometry of Manwe and Thorondor previously", "obtained with the HST Wide-Field Planetary Camera2 (WFPC2) in the", "F606W band at seven different epochs from 2007 to 2013.", "Grundy+ (2014Icar..237....1G) report magnitudes for Manwe and", "Thorondor derived from these data after transforming F606W to V band", "and averaging the results from each epoch. Here we present the", "measurements without transformation or averaging."], "type": ["OC"], "doi_pub": ["10.3847/1538-3881/ab59d4"], "data": "f-v", "date_creation": "30-Mar-2020", "last_update": "16-Apr-2020", "catid": "51590027", "date_update": "31-Mar-2020", "tables": [{"name": "table1.dat", "desc": "*Binary orbital parameters for Manwe-Thorondor ", "columns": [{"name": "Per", "desc": "Manwe-Thorondor orbital period "}, {"name": "e_Per", "desc": "Error on Per "}, {"name": "a", "desc": "Manwe-Thorondor semi-major axis "}, {"name": "e_a", "desc": "Error on a "}, {"name": "e", "desc": "Manwe-Thorondor eccentricity "}, {"name": "e_e", "desc": "Error on e "}, {"name": "Msys", "desc": "System mass "}, {"name": "e_Msys", "desc": "Error on M "}, {"name": "inc", "desc": "Manwe-Thorondor inclination "}, {"name": "e_inc", "desc": "Error on inc "}, {"name": "Omega", "desc": "Manwe-Thorondor ascending node "}, {"name": "e_Omega", "desc": "Error on Omega "}]}, {"name": "table2.dat", "desc": "Observing circumstances ", "columns": [{"name": "Epoch", "desc": "[1/4] Epoch number "}, {"name": "Date", "desc": "UT observation date "}, {"name": "Tel", "desc": "Telescope used: DCT, Gemini and SOAR, 2 occurrences for each"}, {"name": "Filt", "desc": "Filter used: VR 1 occurrences, g 4 occurrences and r 5 occurrences"}, {"name": "Obs.start", "desc": "UT start time of the observation "}, {"name": "Obs.end", "desc": "UT end time of the observation "}, {"name": "Midpt", "desc": "UT event midpoint (1) "}, {"name": "Depth", "desc": "[0.05/0.66]? Event depth (1) "}, {"name": "theta", "desc": "[0.4/1.1] Solar phase angle ({Theta}) "}, {"name": "rhel", "desc": "[43.4/43.7] Heliocentric distance (r_hel_) "}, {"name": "rgeo", "desc": "[42/43] Geocentric distance (r_geo_) "}]}, {"name": "table3.dat", "desc": "Photometric observations of Manwe-Thorondor ", "columns": [{"name": "Tel", "desc": "Telescope used (1) "}, {"name": "JD", "desc": "[7625/8398] Julian Date of observation, JD-2450000 "}, {"name": "Filt", "desc": "Filter used: \"VR\" 34 occurrences, \"g\" 43 occurrences or \"r\" 148 occurrences"}, {"name": "omag", "desc": "[21.7/24.6] Observed magnitude in Filt "}, {"name": "e_omag", "desc": "[0.02/0.25] Uncertainty in omag "}, {"name": "Exp", "desc": "[150/600] Exposure time "}, {"name": "O-C", "desc": "[-0.28/0.31] Fit Residuals "}]}, {"name": "table4.dat", "desc": "F606W-band photometry of Manwe-Thorondor with HST ", "columns": [{"name": "Obs.Y", "desc": "[2007/2013] Year of observation, UT "}, {"name": "Obs.M", "desc": "Month of observation, UT "}, {"name": "Obs.D", "desc": "[4/26] Day of observation, UT "}, {"name": "JD", "desc": "[4306/6618] Julian date of observation, JD-2450000"}, {"name": "Mmag", "desc": "[23.2/24.1] Manwe HST/WFPC2 F606W magnitude "}, {"name": "f_Mmag", "desc": "[*] *: rejected measurement "}, {"name": "e_Mmag", "desc": "[0.05/0.11] Uncertainty in Mmag "}, {"name": "Tmag", "desc": "[24.2/26.1]? Thorondor HST/WFPC2 F606W magnitude "}, {"name": "f_Tmag", "desc": "[*] *: rejected measurement "}, {"name": "e_Tmag", "desc": "[0.05/0.69]? Uncertainty in Tmag "}, {"name": "M*mag", "desc": "[22.9/23.5] Pseudo magnitude for Manwe+Thorondor (1)"}, {"name": "f_M*mag", "desc": "[*] *: rejected measurement "}, {"name": "theta", "desc": "[0.08/1.21] Solar phase angle of the Manwe/Thorondor system ({Theta})"}, {"name": "Sep", "desc": "[0.03/0.33] Separation ({Delta}) "}]}, {"name": "table6.dat", "desc": "Multicomponent model parameters ", "columns": [{"name": "DiamM", "desc": "Diameter of sphere with equivalent area as Manwe"}, {"name": "DiamMVol", "desc": "Diameter of sphere with equivalent volume as Manwe"}, {"name": "DiamT", "desc": "Diameter of Thorondor "}, {"name": "MM", "desc": "Mass of Manwe "}, {"name": "MT/MM", "desc": "Upper limit to Thorondor/Manwe mass ratio (1) "}, {"name": "pM", "desc": "Albedo of Manwe "}, {"name": "pT", "desc": "Albedo of Thorondor "}, {"name": "beta", "desc": "Linear dependence on solar phase angle ({beta}) "}, {"name": "PerM", "desc": "Rotation period of Manwe "}, {"name": "t1", "desc": "Reference Julian date for absolute magnitudes "}, {"name": "rho", "desc": "Average density of the Manwe/Thorondor system ({rho})"}, {"name": "epsT", "desc": "Julian date of minimum brightness for Thorondor ({epsilon}_T_)"}, {"name": "OmegaM", "desc": "Ascending node of Manwe's equator ({Omega}) (2) "}, {"name": "incM", "desc": "Inclination of Manwe's equator (2) "}, {"name": "RotM", "desc": "Rotation angle of Manwe's long axis ({mu}) (3) "}, {"name": "aM", "desc": "Average angle between Manwe's spin and Manwe-Earth direction (<{alpha}_M_>)"}, {"name": "PerT", "desc": "Rotation period of Thorondor (single-peaked) "}, {"name": "AmpT", "desc": "Light-curve amplitude of Thorondor (peak-to-peak)"}, {"name": "gMAG", "desc": "Absolute g-band magnitude of Manwe/Thorondor (H_g_) at epoch t1"}, {"name": "rMAG", "desc": "Absolute r-band magnitude of Manwe/Thorondor (H_r_) at epoch t1"}, {"name": "MMAG", "desc": "Absolute F606W-band magnitude of Manwe (H_M_) at epoch t1"}, {"name": "TMAG", "desc": "Absolute F606W-band magnitude of Thorondor (H_T_) at epoch t1"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_159_28"}} {"id": "J/AJ/159/28", "title_cds": "Short Title", "title_create": "Abushattal+, 2020", "year": "2020", "author": "Abushattal A.A., Docobo J.A., Campo P.P.", "title_pub": "The most probable 3D orbit for spectroscopic binaries.", "first_author": "Abushattal A.A.", "ref_biblio": [""], "bibcode": ["2020AJ....159...28A"], "keyword_cds": "", "keyword_pub": "Binary stars; Spectroscopic binary stars; Visual binary stars Fundamental parameters of stars", "mission": "", "abstract": ["Binary stars are a very important source of astronomical information. Those short-period binaries observed by means of both spectroscopy and interferometry can provide, through their corresponding orbits, precise values regarding individual masses as well as orbital parallaxes. For this reason, it is fundamental to attempt to optically resolve double-lined spectroscopic binaries. In the present article, we used the elaboration of a specific algorithm in order to determine the necessary telescope aperture to resolve a concrete spectroscopic binary. To that end, using available photometric and spectroscopic information, we established a 3D model for each spectroscopic binary with an orbit from which we deduced the most probable maximum and minimum separations between the components. In this manner, using the obtained calibrations in our study, we also deduced different physical parameters of the components of each system. The methodology presented here was tested satisfactorily with a list of spectroscopic binaries that had been optically resolved and that have both the spectroscopic and visual orbits."], "object": [], "curator": "Coralie Fix [CDS]", "data": "", "date_update": "17-Mar-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_159_84"}} {"id": "J/AJ/159/84", "title_cds": "Machine-learning regression of extinction in Gaia DR2", "title_create": "Bai+, 2020", "year": "2020", "author": "Bai Yu, Liu J., Wang Y., Wang S.", "title_pub": "Machine-learning regression of extinction in the second Gaia Data Release.", "first_author": "Bai Yu", "ref_biblio": [""], "bibcode": ["2020AJ....159...84B"], "see_also": ["III/279 : RAVE 5th data release (Kunder+, 2017)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "I/349 : StarHorse, Gaia DR2 photo-astrometric distances (Anders+, 2019)", "V/146 : LAMOST DR1 catalogs (Luo+, 2015)", "J/AJ/136/2070 : SEGUE stellar parameter pipeline. III (Allende Prieto+,2008)", "J/AJ/136/2050 : SEGUE stellar parameter pipeline. II. (Lee+, 2008)", "J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009)", "J/AJ/141/89 : SEGUE stellar parameter pipeline. IV. (Smolinski+, 2011)", "J/AJ/146/133 : Stellar parameters SDSS-III APOGEE DR10 (Meszaros+, 2013)", "J/ApJ/798/122 : Abundances SEGUE Stellar Parameters Pipeline (Miller+, 2015)", "J/AJ/151/144 : ASPCAP weights 15 APOGEE chemical elements (Garcia+, 2016)", "J/MNRAS/460/3179 : APOGEE stars distance and extinction (Wang+, 2016)", "J/ApJS/229/30 : Revised stellar properties of Q1-17 Kepler (Mathur+, 2017)", "J/A+A/619/A180 : Gaia DR2 photo. sensitivity curves (Maiz Apellaniz+, 2018)", "J/AJ/158/93 : Regression of stellar temperatures in GaiaDR2 (Bai+, 2019)"], "keyword_cds": "Surveys; Extinction; Optical", "keyword_pub": "Interstellar dust extinction ; Analytical mathematics", "abstract": ["Machine learning has become a popular tool to help us make better", "decisions and predictions, based on experiences, observations, and", "analyzing patterns, within a given data set without explicit", "functions. In this paper, we describe an application of the supervised", "machine-learning algorithm to the extinction regression for the second", "Gaia data release, based on the combination of the Large Sky Area", "Multi-Object Fiber Spectroscopic Telescope, Sloan Extension for", "Galactic Understanding and Exploration, and the Apache Point", "Observatory Galactic Evolution Experiment. The derived extinction in", "our training sample is consistent with other spectrum-based estimates,", "and its standard deviation of the cross-validations is 0.0127mag. A", "blind test is carried out using the RAdial Velocity Experiment", "catalog, and the standard deviation is 0.0372mag. Such a precise", "training sample enables us to regress the extinction, E(BP-RP), for", "133 million stars in the second Gaia data release. Of these,", "106 million stars have the uncertainties less than 0.1mag, which", "suffer less bias from the external regression. We also find that there", "are high deviations between the extinctions from photometry-based", "methods, and between spectrum- and photometry-based methods. This", "implies that the spectrum-based method could bring more signal to a", "regressing model than multiband photometry, and a higher", "signal-to-noise ratio would acquire a more reliable result."], "description": ["1.38 billion sources of the Gaia DR2 (Cat. I/345) have the integrate", "fluxes from the blue and red photometer (BP and RP)", "spectrophotometers, which span 3300-6800{AA} and 6400-10500{AA},", "respectively.", "We apply the regressor and present a revised version of the E(BP-RP)", "catalog for Gaia DR2."], "type": ["MC"], "records": ["132739322 records"], "doi_pub": ["10.3847/1538-3881/ab63d5"], "orcid_pub": ["0000-0002-4740-3857"], "data": "f", "islargetable": true, "date_creation": "04-Nov-2020", "date_update": "04-Nov-2020", "tables": [{"name": "table2.sam", "desc": "Results of our regression for Gaia DR2 (Cat. I/345) (sample of 1000 sources among 132,739,322)", "columns": [{"name": "Source", "desc": "Source identifier in Gaia DR2 "}, {"name": "RAdeg", "desc": "Gaia DR2 Right Ascension (ICRS) at Ep=2015.5 (column added by the CDS)"}, {"name": "DEdeg", "desc": "Gaia DR2 Declination (ICRS) at Ep=2015.5 (column added by the CDS)"}, {"name": "E(BP-RP)", "desc": "[-0.46/2.91] Regressed redenning E(BP-RP) "}, {"name": "e_E(BP-RP)", "desc": "[0.0024/0.87] Uncertainty in E(BP-RP) "}]}, {"name": "table2.txt", "desc": "Original table from paper with IDs and regressed extinctions", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_159_217"}} {"id": "J/AJ/159/217", "title_cds": "Simulation of Nodal precession in planet pairs", "title_create": "Bailey+, 2020", "year": "2020", "author": "Bailey N., Fabrycky D.", "title_pub": "Nodal precession in closely spaced planet pairs.", "first_author": "Bailey N.", "ref_biblio": [""], "bibcode": ["2020AJ....159..217B"], "see_also": ["J/ApJS/208/22 : Transit timing variation for 12 planetary pairs (Xie, 2013)", "J/ApJ/790/146 : Planets in Kepler's multi-transiting systems (Fabrycky+, 2014)", "J/ApJS/210/25 : Transit timing variation 15 planetary pairs. II. (Xie, 2014)", "J/A+A/573/A124 : Kepler-117 (KOI-209) transit-timing variations (Bruno+, 2015)", "J/MNRAS/448/1044 : Simulation data 50 planetary model systems (Hansen+, 2015)"], "keyword_cds": "Exoplanets; Models; Binaries, orbits", "keyword_pub": "Analytical mathematics ; Ascending node ; Celestial mechanics ; Exoplanet systems ; Exoplanet dynamics ; N-body simulations ; Orbits ; Three-body problem", "abstract": ["Planet-planet perturbations can cause planet's orbital elements to", "change on secular timescales. Previous work has evaluated the nodal", "precession rate for planets in the limit of low {alpha} (semimajor", "axis ratio; 0<{alpha}<=1). Our simulations show that systems at high", "{alpha} (or low period ratio), similar to multiplanet systems found in", "the Kepler survey, have a nodal precession rate that is more strongly", "dependent on eccentricity and inclination. We present a complete", "expansion of the nodal precession rate to fourth order in the", "disturbing function and show that this analytical solution much better", "describes the simulated N-body behavior of high-{alpha} planet pairs;", "at {alpha}~0.5, the higher-order solution, on average, reduces the", "median analytical error by a factor of 7.5 from linear theory and 6.2", "from a similar expansion assuming low {alpha}. We set limits on", "eccentricity and inclination where the theory is precisely validated", "by N-body integrations, which can be useful in future secular", "treatments of planetary systems."], "data": "", "date_update": "25-Aug-2020", "tables": [{"name": "tableB1.dat", "desc": "Restricted Simulations Data ", "columns": [{"name": "Per-b", "desc": "[3.4834] Inner planet period "}, {"name": "Per-c", "desc": "[6.16/174.2] Outer planet period "}, {"name": "/Per", "desc": "[1.77/50] Period ratio "}, {"name": "e-b0", "desc": "[2.09E-16/0.07] Inner planet initial eccentricity"}, {"name": "e-c0", "desc": "[0/0.1] Outer planet initial eccentricity "}, {"name": "i-b0", "desc": "[0] Inner planet initial inclination "}, {"name": "i-c0", "desc": "[0.008/0.42] Outer planet initial inclination "}, {"name": "omega-b0", "desc": "[0.827767955] Inner planet initial argument of pericenter ({omega}_1.0_})"}, {"name": "omega-c0", "desc": "[1.0943632214] Outer planet initial argument of pericenter ({omega}_2.0_})"}, {"name": "Pern-c", "desc": "[106185/966743333] Outer planet nodal precession period fitted from simulation"}, {"name": "e_Pern-c", "desc": "[0.002/45] Standard deviation in Pern-c "}, {"name": "Texp", "desc": "[107270/17417020] Time period used to fit nodal precession period (1)"}, {"name": "Tsim", "desc": "[107270/17417020] Total time simulated "}, {"name": "Per-LL", "desc": "[211025/961145944] Analytical nodal precession period from Laplace-Lagrange linear theory"}, {"name": "Per-2nd", "desc": "[120427/966445072] Analytical nodal precession period from 2nd order expansion"}, {"name": "Per-4th", "desc": "[107816/966631850] Analytical nodal precession period from 4th order expansion"}, {"name": "figs", "desc": "? Figures where this data appears "}]}, {"name": "tableB2.dat", "desc": "Unrestricted Simulations Data ", "columns": [{"name": "Per-b", "desc": "[6.2448] Inner planet period "}, {"name": "Per-c", "desc": "[11.05/312.3] Outer planet period "}, {"name": "/Per", "desc": "[1.77/50] Period ratio "}, {"name": "e-b0", "desc": "[2.95E-7/0.9] Inner planet initial eccentricity "}, {"name": "e-c0", "desc": "[3E-7/0.9] Outer planet initial eccentricity "}, {"name": "i-b0", "desc": "[0.004/0.42] Inner planet initial inclination "}, {"name": "i-c0", "desc": "[0.001/0.23] Outer planet initial inclination "}, {"name": "omega-b0", "desc": "[-3.08/3.1] Inner planet initial argument of pericenter"}, {"name": "omega-c0", "desc": "[-1.49/2.99] Outer planet initial argument of pericenter"}, {"name": "Pern-b", "desc": "[100004/999564] Inner planet nodal precession period fitted from simulation"}, {"name": "e_Pern-b", "desc": "[0.002/999] Standard deviation in Pern-b "}, {"name": "Pern-c", "desc": "[100004/999586] Outer planet nodal precession period fitted from simulation"}, {"name": "e_Pern-c", "desc": "[0.002/993] Standard deviation in pern-c "}, {"name": "Texp", "desc": "[24.9/2547874657] Time period used to fit nodal precession period (1)"}, {"name": "Tsim", "desc": "[1105326/2547874657] Total time simulated "}, {"name": "Per-LL", "desc": "[141883/520413421] Analytical nodal precession0 period from Laplace-Lagrange linear theory"}, {"name": "Per-2nd", "desc": "[54154/600384597] Analytical nodal precession period from 2nd order expansion"}, {"name": "Per-4th", "desc": "[1696/612881431] Analytical nodal precession period from 4th order expansion"}, {"name": "figs", "desc": "? Figures where this data appears "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_160_57"}} {"id": "J/AJ/160/57", "title_cds": "IR spectra of planetary-mass brown dwarfs in IC 348", "title_create": "Luhman+, 2020", "year": "2020", "author": "Luhman+, Luhman K.L., Hapich C.J.", "title_pub": "New candidates for planetary-mass brown dwarfs in IC 348.", "first_author": "Luhman+", "ref_biblio": [""], "bibcode": ["2020AJ....160...57L"], "see_also": ["II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "II/314 : UKIDSS-DR8 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "J/A+A/337/403 : Low-mass stars evolutionary models (Baraffe+ 1998)", "J/ApJ/541/977 : HST observations of low-mass stars in IC 348 (Najita+, 2000)", "J/ApJ/593/1093 : IC 348 membership (Luhman+, 2003)", "J/ApJ/597/555 : IR photometry of IC 348 young brown dwarfs (Mainzer+, 2003)", "J/MNRAS/434/806 : Pre-main-sequence isochrones. II. SFR (Bell+, 2013)", "J/ApJ/810/158 : M,L,T dwarfs fundamental parameters & SEDs (Filippazzo+,2015)", "J/AJ/154/134 : Planetary-mass brown dwarfs in the Taurus SFR (Esplin+, 2017)", "J/AJ/154/46 : Proper motions and photo. for members of Cha I (Esplin+,2017)", "J/AJ/153/46 : Spectroscopy of candidate members in Taurus (Luhman+, 2017)", "J/ApJ/865/73 : GOBELINS. V. Kinematics of Perseus (Ortiz-Leon+, 2018)", "J/AJ/158/54 : Taurus memb. from stellar to planetary masses (Esplin+, 2019)"], "keyword_cds": "Clusters, open; Star Forming Region; Stars, brown dwarf; Spectra, infrared; Spectral types", "keyword_pub": "Brown dwarfs ; Star-forming regions ; Initial mass function ; Hubble Space Telescope", "abstract": ["We have used infrared images obtained with the Wide Field Camera 3 on", "board the Hubble Space Telescope to search for planetary-mass brown", "dwarfs in the star-forming cluster IC348. In those images, we have", "identified 12 objects that have colors indicative of spectral types", "later than M8, corresponding to masses of <~30MJup at the age of", "IC348. The four brightest candidates have been observed with", "spectroscopy, all of which are confirmed to have late types. Two of", "those candidates appear to be young, and thus are likely members of", "the cluster, while the ages and membership of the other two candidates", "are uncertain. One of the former candidates is the faintest known", "member of IC348 in extinction-corrected Ks and is expected to have a", "mass of 4-5MJup based on evolutionary models and an assumed age of", "3Myr. Four of the remaining eight candidates have ground-based", "photometry that further supports their candidacy as brown dwarfs, some", "of which are fainter (and potentially less massive) than the known", "members."], "description": ["IC348 was observed with the IR channel of Hubble's Wide Field Camera 3", "(WFC3) on several dates between 2016 December and 2017 February", "through program 14626 (M. Barsony). The camera contains a 1024x1024", "HgCdTe array in which the pixels have dimensions of ~0.135\"x0.121\".", "The inner 1014x1014 portion of the array detects light, which", "corresponds to a field of view of 136\"x123\".the total exposure times", "were 250 or 275 s for a given field and filter. WFC3 observed 48", "fields through three filters, consisting of F125W (1.1-1.4{mu}m),", "F139M (1.35-1.41{mu}m), and F160W (1.4-1.69{mu}m)."], "type": ["OC"], "data": "", "date_update": "21-Dec-2020", "tables": [{"name": "table1.dat", "desc": "Candidate members of IC 348 ", "columns": [{"name": "ID", "desc": "IC 348 IRS position-based identifier "}, {"name": "LRL", "desc": "[21460/91235] LRL designation (1) "}, {"name": "SpT", "desc": "Spectral Type "}, {"name": "Ak", "desc": "[0.1/0.2]? K band reddening "}, {"name": "Young?", "desc": "Young according to spectral features? "}, {"name": "m125", "desc": "[18.82/22.13] HST/WFPC3 F125W magnitude "}, {"name": "e_m125", "desc": "[0.02/0.03] Uncertainty in m125 "}, {"name": "m139", "desc": "[18.95/21.62] HST/WFPC3 F139M magnitude "}, {"name": "e_m139", "desc": "[0.02/0.09] Uncertainty in m139 "}, {"name": "m160", "desc": "[18.12/20.94] HST/WFPC3 F160W magnitude "}, {"name": "e_m160", "desc": "[0.02/0.02] Uncertainty in m160 "}, {"name": "Jmag", "desc": "[18.77/21.66]? J band magnitude (2) "}, {"name": "e_Jmag", "desc": "[0.02/0.12]? Uncertainty in Jmag (2) "}, {"name": "Hmag", "desc": "[17.77/20.0]? H band magnitude (2) "}, {"name": "e_Hmag", "desc": "[0.02/0.12]? Uncertainty in Hmag (2) "}, {"name": "Ksmag", "desc": "[16.98/19.09]? Ks band magnitude (2) "}, {"name": "e_Ksmag", "desc": "[0.02/0.06]? Uncertainty in Ksmag (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_160_265"}} {"id": "J/AJ/160/265", "title_cds": "", "title_create": "Hu+, 2020", "year": "2020", "author": "Hu Z., Tak H.", "title_pub": "Modeling stochastic variability in multiband time-series data.", "first_author": "Hu Z.", "ref_biblio": [""], "see_also": ["J/ApJ/698/895 : Variations in QSOs optical flux (Kelly+, 2009)", "J/ApJ/747/107 : QSO Candidates in the MACHO LMC database (Kim+, 2012)", "J/A+A/540/A132 : Optical follow-up of Q0957+561 in 2005-2010 (Shalyapin+, 2012)", "J/ApJ/806/129 : Space telescope RM project. II. Swift data (Edelson+, 2015)"], "keyword_cds": "", "keyword_pub": "Astrostatistics ; Interdisciplinary astronomy ; Astrostatistics tools", "abstract": ["In preparation for the era of time-domain astronomy with upcoming", "large-scale surveys, we propose a state-space representation of a", "multivariate damped random walk process as a tool to analyze", "irregularly-spaced multifilter light curves with heteroscedastic", "measurement errors. We adopt a computationally efficient and scalable", "Kalman filtering approach to evaluate the likelihood function, leading", "to maximum O(k^3^n) complexity, where k is the number of available", "bands and n is the number of unique observation times across the k", "bands. This is a significant computational advantage over a commonly", "used univariate Gaussian process that can stack up all multiband light", "curves in one vector with maximum O(k^3^n^3^) complexity. Using", "such efficient likelihood computation, we provide both maximum", "likelihood estimates and Bayesian posterior samples of the model", "parameters. Three numerical illustrations are presented: (I) analyzing", "simulated five-band light curves for a comparison with independent", "single-band fits; (II) analyzing five-band light curves of a quasar", "obtained from the Sloan Digital Sky Survey Stripe 82 to estimate", "short-term variability and timescale; (III) analyzing gravitationally", "lensed g- and r-band light curves of Q0957+561 to infer the time", "delay. Two R packages, Rdrw and timedelay, are publicly available to", "fit the proposed models."], "object": ["10 01 20.69 +55 53 55.6 QSO0957+561 = 8C 0958+561"], "data": "", "date_update": "11-Feb-2021", "tables": [{"name": "fig7.dat", "desc": "Light curves of doubly-lensed quasar Q0957+561 ", "columns": [{"name": "Band", "desc": "SDSS band; g or r "}, {"name": "Comp", "desc": "Lensed image component; A or B "}, {"name": "MJD", "desc": "[3443/4249] Modified Julian Date MJD-50000 "}, {"name": "mag", "desc": "[16.8/17.4] Apparent magnitude in Band "}, {"name": "e_mag", "desc": "[8.1E-03/1.6E-02] Uncertainty in mag "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_161_100"}} {"id": "J/AJ/161/100", "title_cds": "Ages and alpha-abundances of population in K2", "title_create": "Warfield+, 2021", "year": "2021", "author": "Warfield J.T., Zinn J.C., Pinsonneault M.H., Johnson J.A., Stello D., Elsworth Y., Garcia R.A., Kallinger T., Mathur S., Mosser B., Beaton R.L., Garcia-Hernandez D.A.", "title_pub": "An intermediate-age Alpha-rich galactic population in K2.", "first_author": "Warfield J.T.", "ref_biblio": [""], "bibcode": ["2021AJ....161..100W"], "see_also": ["V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)", "I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "III/284 : APOGEE-2 data from DR16 (Johnsson+, 2020)", "J/A+A/410/527 : Abundances in the Galactic disk (Bensby+, 2003)", "J/ApJ/746/16 : Modelling the convection zone (van Saders+, 2012)", "J/ApJS/215/19 : APOKASC catalog of Kepler red giants (Pinsonneault+, 2014)", "J/MNRAS/445/2758 : KIC giants Bayesian dist. & extinctions (Rodrigues+, 2014)", "J/MNRAS/452/2127 : Fundamental parameters of Kepler stars (Silva Aguirre+,2015)", "J/AJ/151/144 : ASPCAP weights for 15 APOGEE chemic. elements (Garcia+,2016)", "J/A+A/597/A30 : Seismology & spectroscopy of CoRoGEE red giants (Anders+,2017)", "J/ApJ/844/102 : KIC star prlxs from asteroseismology vs Gaia (Huber+, 2017)", "J/ApJ/835/173 : Kepler asteroseismic LEGACY sample. II. (Silva Aguirre+, 2017)", "J/ApJ/835/83 : K2 GAP data release. I. Campaign 1 (Stello+, 2017)", "J/ApJS/239/32 : APOKASC-2 catalog of Kepler evolved stars (Pinsonneault+,2018)", "J/AJ/156/18 : APOGEE DR14:Binary comp. of evolved stars (Price-Whelan+,2018)", "J/A+A/627/A173 : Abundances for 4 metal-poor stars (Valentini+, 2019)", "J/ApJS/251/23 : K2 GAP DR2: campaigns 4, 6 & 7 (Zinn+, 2020)", "J/A+A/645/A85 : Age dissection of the Milky Way discs (Miglio+, 2021)"], "keyword_cds": "Surveys; Milky Way; Stars, ages; Stars, masses; Stars, giant; Abundances; Effective temperatures; Spectra, infrared; Cross identifications", "keyword_pub": "Stellar ages ; Stellar abundances ; Asteroseismology ; Galaxy evolution ; Galaxy formation ; Milky Way formation ; Galaxy stellar content ; Red giant stars ; Surveys", "abstract": ["We explore the relationships between the chemistry, ages, and", "locations of stars in the Galaxy using asteroseismic data from the K2", "mission and spectroscopic data from the Apache Point Galactic", "Evolution Experiment survey. Previous studies have used giant stars in", "the Kepler field to map the relationship between the chemical", "composition and the ages of stars at the solar circle. Consistent with", "prior work, we find that stars with high [{alpha}/Fe] have distinct,", "older ages in comparison to stars with low [{alpha}/Fe]. We provide", "age estimates for red giant branch (RGB) stars in the Kepler field,", "which support and build upon previous age estimates by taking into", "account the effect of {alpha}-enrichment on opacity. Including this", "effect for [{alpha}/Fe]-rich stars results in up to 10% older ages for", "low- mass stars relative to corrected solar mixture calculations. This", "is a significant effect that Galactic archeology studies should take", "into account. Looking beyond the Kepler field, we estimate ages for", "735 RGB stars from the K2 mission, mapping age trends as a function of", "the line of sight. We find that the age distributions for low- and", "high-[{alpha}/Fe] stars converge with increasing distance from the", "Galactic plane, in agreement with suggestions from earlier work. We", "find that K2 stars with high [{alpha}/Fe] appear to be younger than", "their counterparts in the Kepler field, overlapping more significantly", "with a similarly aged low-[{alpha}/Fe] population. This observation", "may suggest that star formation or radial migration proceeds unevenly", "in the Galaxy."], "description": ["The spectroscopic data for this work is from the sixteenth data", "release of the APOGEE survey. This survey has been collecting", "high-resolution infrared spectra for hundreds of thousand of stars", "throughout the Milky Way. The spectroscopic data in APOGEE DR16 was", "collected with the 2.5m Sloan Foundation Telescope at the Apache Point", "Observatory in New Mexico, USA and the 2.5m du Pont Telescope at Las", "Campanas Observatory in Chile as a part of SDSS-IV. APOGEE uses twin", "R~22500 H-band spectrographs."], "type": ["GCC"], "data": "", "date_update": "13-Apr-2021", "tables": [{"name": "table3.dat", "desc": "Data for K2 campaigns 4, 6, and 7, including our ages", "columns": [{"name": "K2", "desc": "K2 object ID "}, {"name": "K2camp", "desc": "[4/7] K2 campaign field "}, {"name": "APOGEE", "desc": "APOGEE object ID "}, {"name": "Age", "desc": "[0.14/652] Median calculated stellar age "}, {"name": "e_Age", "desc": "[0/457] Lower 1-sigma deviation on stellar age"}, {"name": "E_Age", "desc": "[0/4998] Upper 1-sigma deviation on stellar age"}, {"name": "RAdeg", "desc": "[51.6/291] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-29.6/26.2] Declination (J2000) "}, {"name": "GAIA", "desc": "Object GAIA designation "}, {"name": "Teff", "desc": "[3732/5304] Corrected effective temperature from APOGEE DR16"}, {"name": "e_Teff", "desc": "[60/158] Uncertainty on Teff "}, {"name": "logg", "desc": "[0.67/3.19] Corrected log surface gravity from APOGEE DR16"}, {"name": "e_logg", "desc": "[0.03/0.12] Uncertainty on corrected logg "}, {"name": "[alpha/M]", "desc": "[0.0002/0.39] Alpha abundance from APOGEE DR16"}, {"name": "e_[alpha/M]", "desc": "[0.004/0.04] Uncertainty on [alpha/M] "}, {"name": "[Fe/H]", "desc": "[-1.9/0.43] Metallicity from APOGEE DR16 "}, {"name": "e_[Fe/H]", "desc": "[0.005/0.04] Uncertainty on [Fe/H] "}, {"name": "numax", "desc": "[6.57/207] Mean value of numax from all pipelines that returned a value from K2GAP"}, {"name": "e_numax", "desc": "[0.024/2.66] Uncertainty on numax "}, {"name": "dnu", "desc": "[1.07/16.6]? Mean value of dnu from all pipelines that returned a value from K2GAP"}, {"name": "e_dnu", "desc": "[0/0.32]? Uncertainty on dnu "}, {"name": "numax.COR", "desc": "[6.47/207]? Corrected numax from the COR pipeline from K2GAP"}, {"name": "e_numax.COR", "desc": "[0.23/3.39]? Uncertainty on numax.COR "}, {"name": "numax.A2Z", "desc": "[6.16/183]? Corrected numax from the A2Z pipeline from K2GAP"}, {"name": "e_numax.A2Z", "desc": "[0.34/23]? Uncertainty on numax.A2Z "}, {"name": "numax.BAM", "desc": "[7.07/185]? Corrected numax from the BAM pipeline from K2GAP"}, {"name": "e_numax.BAM", "desc": "[0.18/3.8]? Uncertainty on numax.BAM "}, {"name": "numax.CAN", "desc": "[7.78/176]? Corrected numax from the CAN pipeline from K2GAP"}, {"name": "e_numax.CAN", "desc": "[0.25/3.4]? Uncertainty on numax.CAN "}, {"name": "numax.BHM", "desc": "[9.94/181]? Corrected numax from the BHM pipeline from K2GAP"}, {"name": "e_numax.BHM", "desc": "[0.19/3.3]? Uncertainty on numax.BHM "}, {"name": "numax.SYD", "desc": "[7.44/207]? Corrected numax from the SYD pipeline from K2GAP"}, {"name": "e_numax.SYD", "desc": "[0.12/36]? Uncertainty on numax.SYD "}, {"name": "dnu.COR", "desc": "[1.05/16.4]? Corrected dnu from the COR pipeline from K2GAP"}, {"name": "e_dnu.COR", "desc": "[0.05/0.23]? Uncertainty on dnu.COR "}, {"name": "dnu.A2Z", "desc": "[1.23/15.5]? Corrected dnu from the A2Z pipeline from K2GAP"}, {"name": "e_dnu.A2Z", "desc": "[0.01/0.87]? Uncertainty on dnu.A2Z "}, {"name": "dnu.BAM", "desc": "[1.24/14.4]? Corrected dnu from the BAM pipeline from K2GAP"}, {"name": "e_dnu.BAM", "desc": "[0.005/1.4]? Uncertainty on dnu.BAM "}, {"name": "dnu.CAN", "desc": "[1.09/14]? Corrected dnu from the CAN pipeline from K2GAP"}, {"name": "e_dnu.CAN", "desc": "[0.009/0.36]? Uncertainty on dnu.CAN "}, {"name": "dnu.BHM", "desc": "[1.48/14.9]? Corrected dnu from the BHM pipeline from K2GAP"}, {"name": "e_dnu.BHM", "desc": "[0.05/0.95]? Uncertainty on dnu.BHM "}, {"name": "dnu.SYD", "desc": "[1.47/14.4]? Corrected dnu from the SYD pipeline from K2GAP"}, {"name": "e_dnu.SYD", "desc": "[0.02/0.84]? Uncertainty on dnu.SYD "}, {"name": "logg.SEIS", "desc": "[1.71/3.23] Asteroseismic log surface gravity"}, {"name": "e_logg.SEIS", "desc": "[0.004/0.04] Uncertainty on logg.SEIS "}, {"name": "Mass", "desc": "[0.3/3.67] Asteroseismic mass "}, {"name": "e_Mass", "desc": "[0.03/1.1]? Uncertainty on Mass "}, {"name": "Dist", "desc": "[0.33/11.4] Distance calculated from GAIA parallax from Bailer-Jones 2015"}, {"name": "e_Dist", "desc": "[0.01/7.4] Uncertainty on Dist "}, {"name": "X", "desc": "[-12.3/-1.04] Galactocentric X coordinate calculated with astropy"}, {"name": "Y", "desc": "[-4.26/1.4] Galactocentric Y coordinate calculated with astropy"}, {"name": "Z", "desc": "[-2.37/8.66] Galactocentric Z coordinate calculated with astropy"}, {"name": "R", "desc": "[1.59/12.31] Galactocentric R coordinate calculated with astropy"}]}, {"name": "table4.dat", "desc": "RGB stars in the Kepler field, including our ages ", "columns": [{"name": "KIC", "desc": "MAST Kepler Input Catalog ID "}, {"name": "APOGEE", "desc": "APOGEE object ID "}, {"name": "Age", "desc": "[0.28/150] Median calculated stellar age "}, {"name": "e_Age", "desc": "[0.02/88] Lower 1-sigma deviation on Age "}, {"name": "E_Age", "desc": "[0.03/400] Upper 1-sigma deviation on Age "}, {"name": "Age.APO", "desc": "[0.4/17.7] Calculated stellar age from Pinsonneault et al. 2018"}, {"name": "Teff", "desc": "[3942/5239] Corrected effective temperature from APOGEE DR16"}, {"name": "e_Teff", "desc": "[65/130] Uncertainty on Teff "}, {"name": "logg", "desc": "[1.41/3.35] Corrected log surface gravity from APOGEE DR16"}, {"name": "e_logg", "desc": "[0.02/0.12] Uncertainty on logg "}, {"name": "[alpha/M]", "desc": "[6e-06/0.39] Alpha abundance from APOGEE DR16"}, {"name": "e_[alpha/M]", "desc": "[0.004/0.03] Uncertainty on [alpha/M] "}, {"name": "[Fe/H]", "desc": "[-2.15/0.45] Metallicity from APOGEE DR16 "}, {"name": "e_[Fe/H]", "desc": "[0.005/0.03] Uncertainty on [Fe/H] "}, {"name": "numax", "desc": "[4.78/249] Mean value of numax from all pipelines from APOKASC2"}, {"name": "e_numax", "desc": "[0.05/7.01] Uncertainty on numax "}, {"name": "dnu", "desc": "[0.74/19.2] Mean value of dnu from all pipelines from APOKASC2, with our f_dnu_"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_161_102"}} {"id": "J/AJ/161/102", "title_cds": "VPDs and CMDs of Berkeley32, Berkeley98 and King23", "title_create": "Sariya+, 2021", "year": "2021", "author": "Sariya D.P., Jiang I.-G., Bisht D., Yadav R.K.S., Rangwal G.", "title_pub": "Astrometric and photometric investigation of three old age open clusters in the Gaia era: Berkeley 32, Berkeley 98, and King 23.", "first_author": "Sariya D.P.", "ref_biblio": [""], "bibcode": ["2021AJ....161..102S"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/AcA/41/167 : UBV photometry in Berkeley 32 (Kaluzny+, 1991)", "J/A+AS/133/387 : NGC 1817 and NGC 1807 proper motions (Balaguer-Nunnez+, 1998)", "J/A+AS/131/89 : NGC 1750 + NGC 1758 proper motions (Tian+ 1998)", "J/other/BASI/29.53 : UBVI photometry in Berkeley 32 (Richtler+, 2001)", "J/A+A/463/789 : Blue stragglers in open clusters (Ahumada+, 2007)", "J/A+A/480/79 : Abundances of giants in 5 Galactic clusters (Bragaglia+, 2008)", "J/A+A/493/959 : UBV(RI)cHalpha photometry in omega Cen (Bellini+, 2009)", "J/A+A/496/441 : Radial velocities of Berkeley 32 stars (Randich+, 2009)", "J/MNRAS/399/2146 : Orbits of open clusters in the Galaxy (Wu+, 2009)", "J/A+A/523/A48 : Gaia photometry (Jordi+, 2010)", "J/A+A/535/A30 : Chemical abundance of 12 stars open clusters (Carrera+, 2011)", "J/A+A/558/A53 : MW global survey of star clusters. II. (Kharchenko+, 2013)", "J/MNRAS/430/3350 : Proper motions and membership in NGC 3766 (Yadav+, 2013)", "J/ApJ/797/115 : HSTPROMO I. Observations and NGC7078 results (Bellini+, 2014)", "J/A+A/584/A59 : Proper motions and membership in NGC 6366 (Sariya+, 2015)", "J/A+A/593/A116 : Open clusters within 1.8 kpc of the Sun (Joshi+, 2016)", "J/AJ/153/134 : PMs and photometry of stars in NGC 3201 (Sariya+, 2017)", "J/A+A/618/A93 : Gaia DR2 open clusters in the Milky Way (Cantat-Gaudin+, 2018)", "J/other/RAA/18.126 : Membership catalog for M12 (NGC6218) stars (Sariya+, 2018)", "J/A+A/619/A155 : Open cluster kinematics with Gaia DR2 (Soubiran+, 2018)", "J/A+A/627/A35 : New open clusters Galactic anti-centre (Castro-Ginard+, 2019)"], "keyword_cds": "Clusters, open; Photometry, infrared; Optical; Proper motions; Parallaxes, trigonometric", "keyword_pub": "Hertzsprung Russell diagram ; Star clusters ; Open star clusters ; Initial mass function ; Orbit determination", "abstract": ["Using the photometric and kinematical data from Gaia Data Release 2,", "three old open clusters namely Berkeley32 (Be32), Berkeley98 (Be98),", "and King23 are investigated. The latter two of these clusters are", "poorly studied in the literature. The numbers of the most probable", "cluster members are 563, 260, and 114 for Be32, Be98, and King23,", "respectively, with membership probabilities higher than 80% and lying", "within the clusters limiting radii. Mean proper motions (PMs;", "{mu}_{alpha}_cos_{delta}_ and {mu}_{delta}_) of the clusters are", "determined as (-0.34{+/-}0.008, -1.60{+/-}0.006), (-1.34{+/-}0.007,", "-3.22{+/-}0.008), and (-0.46{+/-}0.009, -0.87{+/-}0.012)mas/yr. The", "errors mentioned in the PMs are the Gaussian fitting errors. The blue", "straggler stars (BSS) in all three old clusters were found to exhibit", "centralized radial distribution. The clusters' radii are determined as", "9.4', 12.95', and 6.6' for Be32, Be98, and King23 using radial density", "profiles. Ages of the clusters determined by isochrone fitting are", "4.90{+/-}0.22, 3.23{+/-}0.15, and 1.95{+/-}0.22Gyr. The errors given", "in the clusters ages are the internal errors. The mass function slopes", "are found to be flatter than Salpeter's value for all three clusters.", "All three clusters are found to be dynamically relaxed. Galactic", "orbits are derived for these clusters, which demonstrate that the", "studied clusters follow a circular path around the Galactic center."], "description": ["To investigate the clusters under study, we used the data from Gaia", "DR2. The ranges covered by Gaia bands, G, GBP, and GRP, in the optical", "wavelengths are 330-1050nm, 330-680nm, and 630-1050nm, respectively"], "object": ["06 58 07.20 +06 25 58.8 Berkeley 32 = Cl Berkeley 32", "22 42 39.60 +52 24 25.2 Berkeley 98 = Cl Berkeley 98", "07 21 50.16 -00 59 16.8 King 23 = Cl King 23"], "type": ["OC"], "data": "", "date_update": "14-Apr-2021", "tables": [{"name": "fig3.dat", "desc": "Vector point diagrams (VPDs) and color-magnitude diagram (CMDs) of Berkeley 32", "columns": [{"name": "Seq", "desc": "[1/4123] Sequential Number "}, {"name": "Dist", "desc": "[0.04/13] Radial distance from cluster sequence (1)"}, {"name": "plx", "desc": "[-3.78/4.18] Gaia DR2 parallax "}, {"name": "e_plx", "desc": "[0.02/1] Uncertainty in plx "}, {"name": "pmRA", "desc": "[-12/11] Gaia DR2 proper motion along RA "}, {"name": "e_pmRA", "desc": "[0.04/1] Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-12/11.6] Gaia DR2 proper motion along DE "}, {"name": "e_pmDE", "desc": "[0.03/1] Uncertainty in pmDE "}, {"name": "Gmag", "desc": "[7.73/20] Apparent Gaia DR2 G band magnitude "}, {"name": "e_Gmag", "desc": "[0.0002/0.03] Uncertainty in Gmag "}, {"name": "BPmag", "desc": "[7.66/20.8] Apparent Gaia DR2 blue passband magnitude"}, {"name": "e_BPmag", "desc": "[0.0003/0.1] Uncertainty in BPmag "}, {"name": "RPmag", "desc": "[7.39/19.2] Apparent Gaia DR2 red passband magnitude"}, {"name": "e_RPmag", "desc": "[0.0006/0.1] Uncertainty in RPmag "}, {"name": "Memb", "desc": "[0/100] Membership probability percentage "}, {"name": "RAh", "desc": "[06] Hour of Right Ascension (J2000) (2) "}, {"name": "RAm", "desc": "[57/59] Minute of Right Ascension (J2000) (2) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) (2) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) (2) "}, {"name": "DEd", "desc": "[06] Degree of Declination (J2000) (2) "}, {"name": "DEm", "desc": "[13/39] Arcminute of Declination (J2000) (2) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) (2) "}]}, {"name": "fig4.dat", "desc": "VPDs and CMDs of Berkeley 98 ", "columns": [{"name": "Seq", "desc": "[1/2835] Sequential Number "}, {"name": "Dist", "desc": "[0.27/15] Radial distance from cluster sequence (1)"}, {"name": "plx", "desc": "[-2.19/2.79] Gaia DR2 parallax "}, {"name": "e_plx", "desc": "[0.01/0.63] Uncertainty in plx "}, {"name": "pmRA", "desc": "[-3/-0.2] Gaia DR2 proper motion along RA "}, {"name": "e_pmRA", "desc": "[0.02/0.98] Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-4/-1] Gaia DR2 proper motion along DE "}, {"name": "e_pmDE", "desc": "[0.02/0.9] Uncertainty in pmDE "}, {"name": "Gmag", "desc": "[10.2/20.1] Apparent Gaia DR2 G band magnitude "}, {"name": "e_Gmag", "desc": "[0.0002/0.02] Uncertainty in Gmag "}, {"name": "BPmag", "desc": "[10.2/20.6] Apparent Gaia DR2 blue passband magnitude"}, {"name": "e_BPmag", "desc": "[0.0009/0.07] Uncertainty in BPmag "}, {"name": "RPmag", "desc": "[10.1/19.4] Apparent Gaia DR2 red passband magnitude"}, {"name": "e_RPmag", "desc": "[0.0005/0.07] Uncertainty in RPmag "}, {"name": "Memb", "desc": "[0/100] Membership probability percentage "}, {"name": "RAh", "desc": "[22] Hour of Right Ascension (J2000) (2) "}, {"name": "RAm", "desc": "[40/45] Minute of Right Ascension (J2000) (2) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) (2) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) (2) "}, {"name": "DEd", "desc": "[52] Degree of Declination (J2000) (2) "}, {"name": "DEm", "desc": "[07/38] Arcminute of Declination (J2000) (2) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) (2) "}]}, {"name": "fig5.dat", "desc": "VPDs and CMDs of King 23 ", "columns": [{"name": "Seq", "desc": "[1/1672] Sequential Number "}, {"name": "Dist", "desc": "[0.02/10] Radial distance from cluster sequence (1)"}, {"name": "plx", "desc": "[-1.87/2.69] Gaia DR2 parallax "}, {"name": "e_plx", "desc": "[0.02/0.73] Uncertainty in plx "}, {"name": "pmRA", "desc": "[-7.87/2] Gaia DR2 proper motion along RA "}, {"name": "e_pmRA", "desc": "[0.03/0.99] Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-3.98/5.85] Gaia DR2 proper motion along DE "}, {"name": "e_pmDE", "desc": "[0.03/0.95] Uncertainty in pmDE "}, {"name": "Gmag", "desc": "[7.47/19.6] Apparent Gaia DR2 G band magnitude "}, {"name": "e_Gmag", "desc": "[0.0002/0.02] Uncertainty in Gmag "}, {"name": "BPmag", "desc": "[8.35/19.9] Apparent Gaia DR2 blue passband magnitude"}, {"name": "e_BPmag", "desc": "[0.0006/0.05] Uncertainty in BPmag "}, {"name": "RPmag", "desc": "[6.59/19] Apparent Gaia DR2 red passband magnitude"}, {"name": "e_RPmag", "desc": "[0.0006/0.05] Uncertainty in RPmag "}, {"name": "Memb", "desc": "[0/100] Membership probability percentage "}, {"name": "RAh", "desc": "[07] Hour of Right Ascension (J2000) (2) "}, {"name": "RAm", "desc": "[21/23] Minute of Right Ascension (J2000) (2) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) (2) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) (2) "}, {"name": "DEd", "desc": "[0/2] Degree of Declination (J2000) (2) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) (2) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_161_106"}} {"id": "J/AJ/161/106", "title_cds": "Radial velocities of 12 Psc and HD 159062", "title_create": "Bowler+, 2021", "year": "2021", "author": "Bowler B.P., Cochran W.D., Endl M., Franson K., Brandt T.D., Dupuy T.J., MacQueen P.J., Kratter K.M., Mawet D., Ruane G.", "title_pub": "The McDonald Accelerating Stars Survey (MASS): white dwarf companions accelerating the Sun-like stars 12 Psc and HD 159062.", "first_author": "Bowler B.P.", "ref_biblio": [""], "bibcode": ["2021AJ....161..106B"], "see_also": ["II/230 : TASS Mark III photometric survey (Richmond+, 2000)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/AJ/126/2048 : NStars project: the Northern Sample. I. (Gray+, 2003)", "J/ApJS/156/47 : DA white dwarfs from the Palomar Green Survey (Liebert+, 2005)", "J/AJ/131/431 : Abundances of Galactic G dwarfs (Brewer+, 2006)", "J/AJ/132/161 : NStars project: The southern sample. I. (Gray+, 2006)", "J/MNRAS/367/1329 : Elemental abundances for 176 stars (Reddy+, 2006)", "J/ApJ/725/875 : Chromospheric activity for CPS stars (Isaacson+, 2010)", "J/ApJ/725/331 : Astrometry in the Galactic Center (Yelda+, 2010)", "J/ApJ/743/138 : Spectroscopic survey of bright white dwarfs (Gianninas+, 2011)", "J/ApJS/201/19 : Hawaii Infrared Parallax Program. I. (Dupuy+, 2012)", "J/A+A/537/A146 : Stellar models with rot. 0.8"], "bibcode": ["2021AJ....161..108S"], "see_also": ["J/A+A/529/A75 : Limb-darkening coefficients (Claret+, 2011)", "J/AJ/142/84 : 10 new transit light curves of HAT-P-13b (Fulton+, 2011)", "J/A+A/554/A28 : Qatar-1 differential light curve (Covino+, 2013)", "J/AJ/145/68 : Five new transit light curves of TrES-3 (Jiang+, 2013)", "J/A+A/555/A92 : Transit timing variations on Qatar-1 (von Essen+, 2013)", "J/A+A/563/A41 : WASP-43 OSIRIS transmission spectroscopy (Murgas+, 2014)", "J/A+A/577/A109 : Transit times of Qatar-1b (Maciejewski+, 2015)", "J/AJ/151/17 : Eight transiting light curves of WASP-43b (Jiang+, 2016)", "J/A+A/588/L6 : WASP-12 transit light curves (Maciejewski+ 2016)", "J/AJ/154/4 : Times of transits and occultations of WASP-12b (Patra+, 2017)", "J/AcA/68/371 : WASP and KELT planet transits (Maciejewski+, 2018)"], "keyword_cds": "Exoplanets; Stars, high-velocity; Photometry, RI", "keyword_pub": "Exoplanet astronomy ; Transit photometry", "abstract": ["Motivated by the unsettled conclusion on whether there are any transit", "timing variations (TTVs) for the exoplanet Qatar-1b, 10 new transit", "light curves are presented and a TTV analysis with a baseline of 1400", "epochs is performed. Because the linear model provides a good fit with", "a reduced chi-square of {chi}_red_^2^=2.59 and the false-alarm", "probabilities of the possible TTV frequencies are as large as 35%, our", "results are consistent with a null-TTV model. Nevertheless, a new", "ephemeris with a reference time of T0=2455647.63360{+/-}0.00008 (BJD)", "and a period of P=1.4200236{+/-}0.0000001day is obtained. In addition,", "the updated orbital semimajor axis and planetary radius in units of", "stellar radius are provided, and the lower limit of the modified", "stellar tidal quality factor is also determined."], "description": ["Three telescopes at different sites were employed for our transit", "observations.", "One is the 60 inch telescope (P60) of Palomar Observatory located at", "Palomar mountain in north San Diego County, California, USA. The mean", "seeing quality of the images is about 1.9\". The optical imager uses a", "2048x2048pixel^2^ CCD array camera to image roughly 13x13arcmin^2^ of", "sky.", "Another telescope we used is the 0.5m telescope, MTM-500, which", "belongs to the Crimean Astrophysical Observatory (CrAO) at Nauchny in", "Crimea (longitude 34.1{deg} east, latitude 44.32{deg} north). The", "camera mounted on MTM-500 is Apogee Alta U6 and the CCD array contains", "1024x1024pixels^2^. The field of view is about 12x12 arcmin^2^, and", "the image seeing is about 5\" (0.71\"/pixel plate scale).", "In addition, we also observed with the 2m Himalayan Chandra Telescope", "(HCT), located at Hanle, India. The observations of the Qatar-1 system", "were taken in the Bessell R-filter by gathering 60s exposures using", "the Himalaya Faint Object Spectrograph Camera (HFOSC), equipped with a", "2048x4096pixels^2^ CCD with a pixel size of 15{mu}m. The central", "2048x2048 region of the CCD used for imaging covers a field of view of", "10x10arcmin^2^ on the sky, with a scale of 0.296\"/pixel."], "object": ["20 13 31.62 +65 09 43.5 Qatar 1 = Qatar 1 (P=1.4200236d)"], "type": ["OC"], "data": "", "date_update": "16-Apr-2021", "tables": [{"name": "table2.dat", "desc": "The photometric light-curve data of this work ", "columns": [{"name": "Obs.Y", "desc": "[2014/2016] UT Year of the observation (1) "}, {"name": "Obs.M", "desc": "UT Month of the observation (1) "}, {"name": "Obs.D", "desc": "UT Day of the observation (1) "}, {"name": "BJD", "desc": "[2456912/2457635] Barycentric Julian Date; TDB "}, {"name": "Flux", "desc": "[0.968/1.02] Relative Flux in R-band "}, {"name": "e_Flux", "desc": "[0.0008/0.004] Uncertainty in RFlux "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_161_112"}} {"id": "J/AJ/161/112", "title_cds": "2012 and 2017 light curves of asteroid 2012 TC4", "title_create": "Lee+, 2021", "year": "2021", "author": "Lee H.-J., Durech J., Vokrouhlicky D., Pravec P., Moon H.-K., Ryan W., Kim M.-J., Kim C.-H., Choi Y.-J., Bacci P., Pollock J., Apitzsch R.", "title_pub": "Spin change of asteroid 2012 TC4 probably by radiation torques.", "first_author": "Lee H.-J.", "ref_biblio": [""], "bibcode": ["2021AJ....161..112L"], "see_also": ["I/317 : The PPMXL Catalog (Roeser+ 2010)", "J/A+A/529/A107 : Photometry of 4 main belt asteroids (Marciniak+, 2011)", "J/A+A/545/A131 : Photometry of 8 main belt asteroids (Marciniak+, 2012)", "J/A+A/550/L11 : Lightcurves of Near-Earth Asteroid 162173 (Kim+ 2013)", "J/A+A/559/A106 : Time-series photometry of 2012 DA14 (Terai+, 2013)", "J/A+A/562/A48 : Light curves of asteroid (25143) Itokawa (Lowry+, 2014)", "J/AJ/150/75 : Asteroid light curves from PTF survey (Waszczak+, 2015)", "J/A+A/596/A40 : Main-belt asteroids optical light curves (Szabo+, 2016)", "J/A+A/598/A63 : 2015 TB145 light curve (Mueller+, 2017)", "J/A+A/619/A123 : Lightcurves of Near-Earth Asteroid 3200 Phaethon (Kim+ 2018)", "J/ApJS/245/29 : Main-belt asteroid photometry from TESS (McNeill+, 2019)", "J/AJ/159/25 : PS1 light curves and Prots of new asteroids (Lo+, 2020)"], "keyword_cds": "Minor planets; Solar system; Photometry, infrared; Optical", "keyword_pub": "Asteroids ; Close encounters ; Near-Earth objects ; Minor planets ; Small solar system bodies", "abstract": ["Asteroid 2012TC4 is a small (~10m) near-Earth object that was observed", "during its Earth close approaches in 2012 and 2017. Earlier analyses", "of light curves revealed its excited rotation state. We collected all", "available photometric data from the two apparitions to reconstruct its", "rotation state and convex shape model. We show that light curves from", "2012 and 2017 cannot be fitted with a single set of model parameters;", "the rotation and precession periods are significantly different for", "these two data sets, and they must have changed between or during the", "two apparitions. Nevertheless, we could fit all light curves with a", "dynamically self-consistent model assuming that the spin states of", "2012TC4 in 2012 and 2017 were different. To interpret our results, we", "developed a numerical model of its spin evolution in which we included", "two potentially relevant perturbations: (I) gravitational torque due", "to the Sun and Earth and (II) radiation torque, known as the", "Yarkovsky-O'Keefe-Radzievskii-Paddack (YORP) effect. Despite our model", "simplicity, we found that the role of gravitational torques is", "negligible. Instead, we argue that the observed change of its spin", "state may be plausibly explained as a result of the YORP torque. To", "strengthen this interpretation, we verify that (I) the internal energy", "dissipation due to material inelasticity and (II) an impact with a", "sufficiently large interplanetary particle are both highly unlikely", "causes of its observed spin state change. If true, this is the first", "case where the YORP effect has been detected for a tumbling body."], "description": ["Photometric observations of 2012 TC4 from 2012 and 2017 were made", "using a variety of telescopes having apertures between 0.35 and 5m and", "equipped with CCD cameras."], "type": ["OC"], "data": "", "date_update": "19-Apr-2021", "tables": [{"name": "figb1.dat", "desc": "Light curve fits for data in 2012 ", "columns": [{"name": "JD", "desc": "Julian Date of the observation "}, {"name": "Flux", "desc": "Normalized flux "}, {"name": "Tel", "desc": "Telescope identifier (1) "}, {"name": "Date", "desc": "Observation date; YYYY/MM/DD format "}, {"name": "alpha", "desc": "Solar phase angle "}]}, {"name": "figb2.dat", "desc": "Light curve fits for data in 2012 ", "columns": [{"name": "JD", "desc": "Julian Date of the observation "}, {"name": "Flux", "desc": "Normalized flux "}, {"name": "Tel", "desc": "Telescope identifier (1) "}, {"name": "Date", "desc": "Observation date; YYYY/MM/DD format "}, {"name": "alpha", "desc": "Solar phase angle "}]}, {"name": "figb3.dat", "desc": "Light curve fits for data in 2017 ", "columns": [{"name": "JD", "desc": "Julian Date of the observation "}, {"name": "Flux", "desc": "Normalized flux "}, {"name": "Tel", "desc": "Telescope identifier (1) "}, {"name": "Date", "desc": "Observation date; YYYY/MM/DD format "}, {"name": "alpha", "desc": "Solar phase angle "}]}, {"name": "figb4.dat", "desc": "Light curve fits for data in 2017 ", "columns": [{"name": "JD", "desc": "Julian Date of the observation "}, {"name": "Flux", "desc": "Normalized flux "}, {"name": "Tel", "desc": "Telescope identifier (1) "}, {"name": "Date", "desc": "Observation date; YYYY/MM/DD format "}, {"name": "alpha", "desc": "Solar phase angle "}]}, {"name": "figb5.dat", "desc": "Light curve fits for data in 2017 ", "columns": [{"name": "JD", "desc": "Julian Date of the observation "}, {"name": "Flux", "desc": "Normalized flux "}, {"name": "Tel", "desc": "Telescope identifier (1) "}, {"name": "Date", "desc": "Observation date; YYYY/MM/DD format "}, {"name": "alpha", "desc": "Solar phase angle "}]}, {"name": "figb6.dat", "desc": "Light curve fits for data in 2017 ", "columns": [{"name": "JD", "desc": "Julian Date of the observation "}, {"name": "Flux", "desc": "Normalized flux "}, {"name": "Tel", "desc": "Telescope identifier (1) "}, {"name": "Date", "desc": "Observation date; YYYY/MM/DD format "}, {"name": "alpha", "desc": "Solar phase angle "}]}, {"name": "figb7.dat", "desc": "Light curve fits for data in 2017 ", "columns": [{"name": "JD", "desc": "Julian Date of the observation "}, {"name": "Flux", "desc": "Normalized flux "}, {"name": "Tel", "desc": "Telescope identifier (1) "}, {"name": "Date", "desc": "Observation date; YYYY/MM/DD format "}, {"name": "alpha", "desc": "Solar phase angle "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_161_119"}} {"id": "J/AJ/161/119", "title_cds": "The TESS-Keck survey. IV. Rvel for WASP-170", "title_create": "Rubenzahl+, 2021", "year": "2021", "author": "Rubenzahl R.A., Dai F., Howard A.W., Chontos A., Giacalone S., Lubin J., Rosenthal L.J., Isaacson H., Batalha N.M., Crossfield I.J.M., Dressing C., Fulton B., Huber D., Kane S.R., Petigura E.A., Robertson P., Roy A., Weiss L.M., Beard C., Hill M.L., Mayo A., Mocnik T., Murphy J.M.A., Scarsdale N.", "title_pub": "The TESS-Keck survey. IV. A retrograde, polar orbit for the ultra-low-density, Hot super-Neptune WASP-107b.", "first_author": "Rubenzahl R.A.", "ref_biblio": [""], "bibcode": ["2021AJ....161..119R"], "see_also": ["I/259 : The Tycho-2 Catalogue (Hog+, 2000)", "J/ApJS/159/141 : Spectroscopic properties of cool stars. I. (Valenti+, 2005)", "J/A+A/517/L1 : Radial velocities of WASP-8b planet (Queloz+, 2010)", "J/ApJ/723/L223 : Radial velocities of HAT-P-11 (Winn+, 2010)", "J/ApJS/225/32 : Extended abundance analysis of cool stars (Brewer+, 2016)", "J/ApJ/832/183 : Binary stellar evolution for Kepler systems (Kostov+, 2016)", "J/ApJ/836/77 : Library of high-S/N optical spectra of FGKM stars (Yee+, 2017)", "J/AJ/155/255 : Rvel and activity measurements of HAT-P-11 (Yee+, 2018)", "J/AJ/159/241 : TESS-Keck Survey I. HD332231 Radial Velocities (Dalba+, 2020)", "J/A+A/640/A73 : pi Men radial velocity curves (De Rosa+, 2020)", "J/AJ/160/259 : HPF RVs and TESS photometry of TOI-1266 (Stefansson+, 2020)", "J/AJ/161/70 : RVel for WASP-170 with HIRES & CORALIE (Piaulet+, 2021)"], "keyword_cds": "Surveys; Exoplanets; Stars, G-type; Radial velocities", "keyword_pub": "Exoplanet dynamics ; Orbit determination ; Radial velocity", "abstract": ["We measured the Rossiter-McLaughlin effect of WASP-107b during a", "single transit with Keck/HIRES. We found the sky-projected inclination", "of WASP-107b's orbit, relative to its host star's rotation axis, to be", "|{lambda}|=118_-19_^+38^degrees. This confirms the misaligned/polar", "orbit that was previously suggested from spot-crossing events and adds", "WASP-107b to the growing population of hot Neptunes in polar orbits", "around cool stars. WASP-107b is also the fourth such planet to have a", "known distant planetary companion. We examined several dynamical", "pathways by which this companion could have induced such an obliquity", "in WASP-107b. We find that nodal precession and disk dispersal-driven", "tilting can both explain the current orbital geometry while", "Kozai-Lidov cycles are suppressed by general relativity. While each", "hypothesis requires a mutual inclination between the two planets,", "nodal precession requires a much larger angle, which for WASP-107 is", "on the threshold of detectability with future Gaia astrometric data.", "As nodal precession has no stellar type dependence, but disk", "dispersal-driven tilting does, distinguishing between these two models", "is best done on the population level. Finding and characterizing more", "extrasolar systems like WASP-107 will additionally help distinguish", "whether the distribution of hot-Neptune obliquities is a dichotomy of", "aligned and polar orbits or if we are uniformly sampling obliquities", "during nodal precession cycles."], "description": ["We observed the Rossiter-McLaughlin (RM) effect for WASP-107b during a", "transit on 2020 February 26 (UTC) with (High Resolution Echelle", "Spectrometer) HIRES on the KeckI Telescope on Maunakea. Our HIRES", "observations covered the full transit duration (~2.7hr) with a ~1hour", "baseline on either side. (R=45000)"], "object": ["12 33 32.84 -10 08 46.2 WASP-107\t= WASP-107 (P=5.7214742d)"], "type": ["OC"], "data": "", "date_update": "21-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Radial velocities of WASP-107 ", "columns": [{"name": "BJD", "desc": "[2458905/2458907] Barycentric Julian Date; TDB "}, {"name": "RVel", "desc": "[-5.52/6.43] Barycentric radial velocity "}, {"name": "e_RVel", "desc": "[1.2/1.7] Uncertainty in RV "}, {"name": "Texp", "desc": "[727/900] Exposure time in seconds "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_161_120"}} {"id": "J/AJ/161/120", "title_cds": "gri photometry for 73 stars in NGC419", "title_create": "Martinez-Vazquez+, 2021", "year": "2021", "author": "Martinez-Vazquez C.E., Salinas R., Vivas A.K.", "title_pub": "Short-period variability in the globular cluster NGC419 and the SMC field.", "first_author": "Martinez-Vazquez C.E.", "ref_biblio": [""], "bibcode": ["2021AJ....161..120M"], "see_also": ["J/A+AS/122/131 : Delta Scuti rotational velocities and Teff (Solano+ 1997)", "J/AJ/115/193 : RR Lyrae V light curves (Layden, 1998)", "J/A+AS/144/469 : Delta Scuti stars (Rodriguez+, 2000)", "J/AJ/132/1630 : CaII spectro. in Magellanic Cloud clusters (Grocholski+, 2006)", "J/AJ/131/895 : Stars in the Carina dwarf spheroidal galaxy (Koch+, 2006)", "J/MNRAS/389/678 : Catalogue of extended objects Magellanic Clouds (Bica+, 2008)", "J/AJ/136/1039 : CaII index of SMC red giant branch stars (Carrera+, 2008)", "J/AJ/135/836 : Calcium triplet index in LMC stars (Carrera+, 2008)", "J/AJ/136/1703 : Ridgelines of six intermediate-age SMC clusters (Glatt+, 2008)", "J/ApJ/685/947 : SX Phe stars in Fornax. II. (Poretti+, 2008)", "J/AJ/140/328 : LMC High-amplitude delta Scuti stars (Garg+, 2010)", "J/AcA/60/1 : VI light curves of LMC delta Scuti stars (Poleski+, 2010)", "J/MNRAS/419/342 : SX Phe stars in globular clusters (Cohen+, 2012)", "J/ApJ/779/102 : Metallicities of RGB stars in dwarf galaxies (Kirby+, 2013)", "J/AJ/145/160 : Variables LMC globular clusters. III. Reticulum (Kuehn+, 2013)", "J/ApJS/208/9 : Intrinsic colors and temperatures of PMS stars (Pecaut+, 2013)", "J/AJ/146/141 : BV photometry of dwarf Cepheids in Carina (Vivas+, 2013)", "J/ApJ/780/59 : Araucaria project: eclipsing binaries in SMC (Graczyk+, 2014)", "J/ApJ/814/71 : Carina project IX: UBVI data Carina variables (Coppola+, 2015)", "J/AcA/65/233 : OGLE Magellanic Clouds anomalous Cepheids (Soszynski+, 2015)", "J/AcA/65/297 : OGLE4 LMC and SMC Cepheids (Soszynski+, 2015)", "J/MNRAS/462/4349 : Variable stars in Sculptor dSph (Martinez-Vazquez+, 2016)", "J/AcA/66/421 : Eclipsing binaries in the Magellanic System (Pawlak+, 2016)", "J/AcA/66/131 : VI light curves of SMC and LMC RR Lyrae (Soszynski+, 2016)", "J/MNRAS/473/3131 : VMC survey. XXVI. SMC RR Lyrae stars (Muraveva+, 2018)", "J/AJ/155/183 : Properties of variables in the NGC 1846 field (Salinas+, 2018)", "J/AJ/157/35 : Population pulsating variable stars in Sextans (Vivas+, 2019)"], "keyword_cds": "Clusters, globular; Stars, variable; Photometry, VRI", "keyword_pub": "Globular star clusters ; Delta Scuti variable stars ; Small Magellanic Cloud ; Variable stars", "abstract": ["Delta Scuti ({delta}Sct) stars have been extensively studied in our", "Galaxy but far less in extragalactic systems. Here we study the", "population of {delta}Sct variables in NGC419, an intermediate-age", "globular cluster of the Small Magellanic Cloud (SMC), using g, r, and", "i Gemini-S/Gemini Multi-Object Spectrograph (GMOS) time-series", "observations. Our goal is to study the role of such variables in the", "cluster extended main-sequence turnoff (MSTO). We report the discovery", "of 54 {delta}Sct stars and three eclipsing binaries in the NGC419", "field. We find only a handful of the {delta}Sct stars at the MSTO of", "NGC419, while the majority are fainter, indicating that the cluster is", "younger (<~1.2Gyr) than previously thought. Considering their radial", "distribution, we identify only six {delta}Sct stars as probable", "members of NGC419, while the 48 remaining are likely {delta}Sct stars", "of the SMC field. Cluster {delta}Sct stars appear close to the red", "edge of the MSTO, supporting the idea that the extended MSTO has its", "origin in an age spread. The 48 field {delta}Sct stars represent the", "largest detection of {delta}Sct stars made in the SMC. The period", "distribution of these newly detected {delta}Sct stars", "(0.04day<~P<~0.15day) is similar to that detected in other systems.", "The amplitude distribution (0.05mag<~{Delta}r<~0.60mag) is likely", "biased because of the lack of low-amplitude stars. We finally use the", "{delta}Sct stars to calculate distances using different", "period-luminosity relations. The average distance moduli obtained are", "18.76{+/-}0.14mag for NGC419 and 18.86{+/-}0.11mag for the SMC field,", "which agree with previous measurements."], "description": ["Time-series imaging of NGC419 was obtained with the Gemini", "Multi-Object Spectrograph (GMOS) mounted at the Gemini-S telescope at", "Cerro Pachon, Chile. Observations were carried out on the nights of", "2017 September 14, 22, and 27 as part of the Fast Turnaround program", "GS-2017B-FT-2. Observations were obtained with 2x2 binning, resulting", "in a pixel scale of 0.16pixel/arcsec. Images were obtained in Sloan", "Digital Sky Survey (SDSS) g, r, and i, with 11, 112, and 7 frames in", "total and exposure times of 120, 90, and 80s, respectively, reaching a", "signal-to-noise ratio (S/N) ~50 at the level of the main-sequence", "turnoff (MSTO)."], "type": ["OC"], "data": "", "date_update": "26-Apr-2021", "tables": [{"name": "table3.dat", "desc": "Position and mean pulsation properties of the variables stars detected and discovered in NGC419", "columns": [{"name": "ID", "desc": "Variable identifier "}, {"name": "f_ID", "desc": "[*] Flag means A{delta} Scuti star within 2r_h_ of NGC 419 (6 occurrences)"}, {"name": "RAdeg", "desc": "[16.92/17.23] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-72.93/-72.83] Declination (J2000) "}, {"name": "rmag", "desc": "[16.07/22.37] Weighted intensity-average r band magnitude (1)"}, {"name": "gmag", "desc": "[16.39/22.63] Weighted intensity-average g band magnitude (1)"}, {"name": "imag", "desc": "[16.07/22.43] Weighted intensity-average i band magnitude (1)"}, {"name": "RoMS", "desc": "[1.6/84.6] The robust median statistic value "}, {"name": "J", "desc": "[2.2/122.1] Welch-Stetson variability index "}, {"name": "Type", "desc": "Variable type (2) "}, {"name": "Per", "desc": "[0.03/251] Period "}, {"name": "u_Per", "desc": "[:] Uncertainty flag on Period "}, {"name": "rint", "desc": "[18.8/22.5]? Intensity-averaged r band magnitude (3)"}, {"name": "u_rint", "desc": "[:] Uncertainty flag on rint "}, {"name": "l_Delr", "desc": "Limit flag on Delr "}, {"name": "Delr", "desc": "[0.05/0.76]? r band amplitude "}, {"name": "u_Delr", "desc": "[:] Uncertainty flag on Delr "}, {"name": "gint", "desc": "[18.65/22.7]? Intensity-averaged g band magnitude (3)"}, {"name": "u_gint", "desc": "[:] Uncertainty flag on gint "}, {"name": "Delg", "desc": "[0.01/1.45]? g band amplitude "}, {"name": "u_Delg", "desc": "[:] Uncertainty flag on Delg "}, {"name": "iint", "desc": "[19.06/22.52]? Intensity-averaged i band magnitude (3)"}, {"name": "u_iint", "desc": "[:] Uncertainty flag on iint "}, {"name": "Deli", "desc": "[0/0.8]? i band amplitude "}, {"name": "u_Deli", "desc": "[:] Uncertainty flag on Deli "}, {"name": "OGLE", "desc": "Previous name; OGLE identifier "}]}, {"name": "table4.dat", "desc": "Photometry of the variable stars in NGC 419 ", "columns": [{"name": "ID", "desc": "Variable identifier "}, {"name": "MJDr", "desc": "[58010/58024] Modified Julian Date of r band observation at mid-exposure"}, {"name": "rmag", "desc": "[16.03/22.97] Apparent r band magnitude "}, {"name": "e_rmag", "desc": "[0.001/0.6] Uncertainty in rmag "}, {"name": "MJDg", "desc": "[58010/58024]? Modified Julian Date of g band observation at mid-exposure"}, {"name": "gmag", "desc": "[16.33/23.14]? Apparent g band magnitude "}, {"name": "e_gmag", "desc": "[0.001/0.2]? Uncertainty in gmag "}, {"name": "MJDi", "desc": "[58010/58024]? Modified Julian Date of i band observation at mid-exposure"}, {"name": "imag", "desc": "[15.91/23.19]? Apparent i band magnitude "}, {"name": "e_imag", "desc": "[0/0.26]? Uncertainty in imag "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AJ_161_126"}} {"id": "J/AJ/161/126", "title_cds": "I-band LC of the microlensing event KMT-2017-BLG-2820", "title_create": "Ryu+, 2021", "year": "2021", "author": "Ryu Y.-H., Mroz P., Gould A., Hwang K.-H., Kim H.-W., Yee J.C., Albrow M.D., Chung S.-J., Jung Y.K., Shin I.-G., Shvartzvald Y., Zang W., Cha S.-M., Kim D.-J., Kim S.-L., Lee C.-U., Lee D.-J., Lee Y., Park B.-G., Han C., Pogge R.W., Udalski A., Poleski R., Skowron J., Szymanski M.K., Soszynski I., Pietrukowicz P., Kozlowski S., Ulaczyk K., Rybicki K.A., Iwanek P.", "title_pub": "KMT-2017-BLG-2820 and the nature of the free-floating planet population.", "first_author": "Ryu Y.-H.", "ref_biblio": [""], "bibcode": ["2021AJ....161..126R"], "see_also": ["J/AcA/50/421 : OGLE-II DIA BUL_SC1 field (Wozniak, 2000)", "J/A+A/549/A147 : Abundances of microlensed bulge dwarf stars. V. (Bensby+,2013)", "J/A+A/618/A44 : Predicted microlensing events from Gaia DR2 (Bramich, 2018)", "J/AcA/68/183 : Predicted Microlensing Events for 21st Century (Bramich+, 2018)", "J/AJ/159/98 : I-band LC of microlensing event KMT-2016-BLG-1836 (Yang+, 2020)", "J/AJ/159/262 : OGLE/KMTnet VI bands photo. of OGLE-2019-BLG-0551 (Mroz+, 2020)"], "keyword_cds": "Gravitational lensing; Photometry, RI", "keyword_pub": "Gravitational microlensing", "abstract": ["We report a new free-floating planet (FFP) candidate,", "KMT-2017-BLG-2820, with Einstein radius {theta}E~6{mu}as, lens-source", "relative proper motion {mu}rel~8mas/yr, and Einstein timescale", "t_E_=6.5hr. It is the third FFP candidate found in an ongoing study of", "giant-source finite-source point-lens (FSPL) events in the KMTNet", "database and the sixth FSPL FFP candidate overall. We find no", "significant evidence for a host. Based on their timescale", "distributions and detection rates, we argue that five of these six", "FSPL FFP candidates are drawn from the same population as the six", "point-source point-lens (PSPL) FFP candidates found by Mroz et al. in", "the OGLE-IV database. The {theta}E distribution of the FSPL FFPs", "implies that they are either sub- Jovian planets in the bulge or", "super-Earths in the disk. However, the apparent \"Einstein desert\"", "(10<~{theta}E/{mu}as<~30) would argue for the latter. Whether each of", "the 12 (six FSPL and six PSPL) FFP candidates is truly an FFP or", "simply a very wide-separation planet can be determined at first", "adaptive optics (AO) light on 30m telescopes, and earlier for some. If", "the latter, a second epoch of AO observations could measure the", "projected planet- host separation with a precision of O(10au). At the", "present time, the balance of evidence favors the unbound-planet", "hypothesis."], "description": ["KMT-2017-BLG-2820 (in KMT field BLG14) was observed with KMT's three", "observatories at the Cerro Tololo Interamerican Observatory (KMTC),", "South African Astronomical Observatory (KMTS), and Siding Springs", "Observatory (KMTA). Each facility has a 1.6m telescope equipped with a", "2x2{deg} camera. Most observations were in Cousins I. In 2017, every", "10th I-band observation from KMTC was complemented by an observation", "in the Johnson V band, while this applied to only every 20th", "observation from KMTS and KMTA.", "The event also lies in OGLE field BLG653, which was observed in the", "Cousins I band with a cadence of 0.17/hr from OGLE's 1.3m telescope at", "Las Campanas Observatory, which is equipped with a 1.4deg^2^ camera."], "object": ["17 34 58.25 -28 32 51.2 KMT-2017-BLG-2820 = KMT-2017-BLG-2820"], "type": ["OC"], "data": "", "date_update": "26-Apr-2021", "tables": [{"name": "fig1.dat", "desc": "Light curve of KMT-2017-BLG-2820 ", "columns": [{"name": "Tel", "desc": "Observatory identifier (KMTA, KMTC, KMTS and OGLE) "}, {"name": "HJD", "desc": "[7792/8045] Heliocentric Julian Date; HJD-24500000 "}, {"name": "Imag", "desc": "[16.33/17.29] Apparent I band magnitude "}, {"name": "e_Imag", "desc": "[0.005/0.08] Uncertainty in Imag "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AN_298_167"}} {"id": "J/AN/298/167", "title_cds": "UBV sequence in NGC 5823", "title_create": "Schnur+, 1977", "year": "1977", "author": "Schnur G.F.O.", "title_pub": "Two UBV sequences, North and South of the galactic cluster NGC 5823.", "first_author": "Schnur G.F.O.", "ref_biblio": [""], "bibcode": ["1977AN....298..167S"], "keyword_cds": "Photometry, UBV ; Clusters, open", "keyword_pub": "", "description": ["Attached is a plain-text list for the two UBV sequences"], "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1002/asna.19772980307"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AZh_93_968"}} {"id": "J/AZh/93/968", "title_cds": "OCARS catalog second version", "title_create": "Malkin, 2016", "year": "2016", "author": "Malkin Z.M.", "title_pub": "The second version of the OCARS Catalog of Optical Characteristics of Astrometric Radio Sources.", "first_author": "Malkin Z.M.", "ref_biblio": [""], "bibcode": ["2016AZh....93..968M", "2016ARep...60..996M"], "see_also": ["J/A+A/583/A75 : Large Quasar Astrometric Catalogue 3 (LQAC-3) (Souchay+, 2015)", "http://www.gao.spb.ru/english/as/ac_vlbi/ : OCARS Home Page"], "keyword_cds": "Radio sources ; Photometry, UBVRI ; Photometry, SDSS", "abstract": ["A new version of the Optical Characteristics of Astrometric Radio", "Sources (OCARS) catalog is presented. The catalog includes a list of", "radio sources observed in astrometric and geodetic VLBI programs since", "1979, their redshifts, photometric data in 13 bands in the visible and", "near infrared, and a table indicating identifications between the OCARS", "objects and objects in other catalogs. The main sources of information", "for the OCARS catalog are the NED and SIMBAD databases, as well as a", "variety of publications. Targeted observing programs designed to", "supplement the optical data for the astrometric radio sources have", "also been organized. The catalog currently contains 9956 sources, of", "which 5449 have redshifts and 7473 have photometric data. The catalog", "is updated, on average, once every several weeks, and is continuously", "augmented with new sources and new optical data."], "description": ["Unlike the first version, supported in 2007-2015, the second version", "of the OCARS catalog includes three files:", "ocars.txt is the main file containing the source coordinates, source", "types, redshifts, and approximate magnitudes, together with commentary;", "this file corresponds to the first version of the OCARS catalog;", "ocars_m.txt contains photometric data in the 13 uUBgV rRiIzJHK bands;", "ocars_n.txt contains a table of corresponding source names in various", "catalogs; currently, only cross-identifications with IVS programs4 and", "the LQAC catalog [9] are included;", "The list of objects included in the OCARS catalog is formed from", "various astrometric and geodeticVLBI programs and catalogs in the", "following order:", "- sources in the ICRF2 [2];", "- other sources observed in the framework of IVS programs;", "- sources from the NASA Goddard VLBI group catalog5 ;", "- sources from the RFC catalog,6 which is the most complete", "astrometric catalog of radio sources, is updated each quarter, and", "contributed more than half the OCARS objects; the latest version of", "OCARS used the RFC-2016a catalog based on observations obtained in", "1980-2015 as part of IVS and other radio astrometric programs", "[19-31];", "- sources from the literature.", "Optical Characteristics of Astrometric Radio Sources (OCARS)", "~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~", "Last revised: 27-NOV-2016", "Latest update:", "- removed 30+ RFC sources not identified in NED and optics", "- removed rather long detailed statistics table, which seems to be not", "interested for most of users; it is always available on request", "- a few additions and amendments", "E-mail alerts about updates are available on request.", "URL of this file is http://www.gao.spb.ru/english/as/ac_vlbi/ocars.txt", "Supplement files:", "Optical and IR magnitudes:", "http://www.gao.spb.ru/english/as/ac_vlbi/ocars_m.txt", "Cross-identification table:", "http://www.gao.spb.ru/english/as/ac_vlbi/ocars_n.txt", "OCARS catalog in CSV format:", "http://www.gao.spb.ru/english/as/ac_vlbi/ocars.csv", "Please send comments and requests to Zinovy Malkin, malkin(at)gao.spb.ru", "----------------------------------------------------------------------------", "The Second Version of the OCARS Catalog of Optical Characteristics of", "Astrometric Radio Sources. Astronomy Reports, 2016, Vol. 60, No. 11,", "pp. 996-1005. DOI: 10.1134/S1063772916110032 If you use OCARS catalog", "in your work, please cite this publication.", "----------------------------------------------------------------------", "Brief OCARS statistics (detailed statistics is available on request)", "~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~~", "Total number of sources 11375", "+30...+90 3320 ( 29.2%)", "-30...+30 6233 ( 54.8%)", "-90...-30 1822 ( 16.0%)", "Number of sources with known type 6284 ( 55.2%)", "AGN 4704 ( 74.9%)", "quasars 3027 ( 64.3%)", "BL Lac 992 ( 21.1%)", "Seyfert 384 ( 8.2%)", "blazars 89 ( 1.9%)", "radio galaxies 1580 ( 25.1%)", "Number of sources with redshift info 5845 ( 51.4%)", "+30...+90 1803 ( 30.8%)", "-30...+30 3329 ( 57.0%)", "-90...-30 713 ( 12.2%)", "unreliable 868 ( 14.9%)", "Number of sources with known magnitude 8133 ( 71.5%)", "+30...+90 2380 ( 29.3%)", "-30...+30 4481 ( 55.1%)", "-90...-30 1272 ( 15.6%)", "Number of sources with both z and magnitude info 5803 ( 51.0%)"], "alias": ["OCARS"], "type": ["CCC"], "data": "", "date_creation": "26-Jan-2017", "date_update": "28-Feb-2017", "tables": [{"name": "ocars.dat", "desc": "OCARS catalog (13/12/2016 version) ", "columns": [{"name": "OCARS", "desc": "OCARS name (HHMM+DDd) "}, {"name": "RAh", "desc": "Right accession (J2000.0) "}, {"name": "RAm", "desc": "Right accession (J2000.0) "}, {"name": "RAs", "desc": "Right accession (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "z", "desc": "? Redshift "}, {"name": "f_z", "desc": "[abcde] Redshift flag (1) "}, {"name": "mag", "desc": "? Optical or NIR magnitude (2) "}, {"name": "Band", "desc": "Band for which magnitude was measured magnitude without a band index is an indicative, primarily NED, value usually related to the V or B bands; it is kept in this file only and not repeated in ocars_m.dat"}, {"name": "Type", "desc": "Object primary type (3) "}, {"name": "Ref", "desc": "Position reference (4) "}, {"name": "n_z", "desc": "[*] * shows that redshift is taken not from NED (see corresponding notes)"}, {"name": "Notes", "desc": "Object names and notes (5) "}]}, {"name": "ocars_m.dat", "desc": "Optical and IR magnitudes of astrometric radio sources from the OCARS catalog (13/12/2016 version)", "columns": [{"name": "OCARS", "desc": "OCARS source name (HHMM+DDd) "}, {"name": "umag", "desc": "? SDSS u magnitude "}, {"name": "u_umag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Umag", "desc": "? U magnitude "}, {"name": "Bmag", "desc": "? B magnitude "}, {"name": "u_Bmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "gmag", "desc": "? SDSS g magnitude "}, {"name": "u_gmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Vmag", "desc": "? V magnitude "}, {"name": "u_Vmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "rmag", "desc": "? SDSS r magnitude "}, {"name": "u_rmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Rmag", "desc": "? R magnitude "}, {"name": "u_Rmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "imag", "desc": "? SDSS i magnitude "}, {"name": "u_imag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Imag", "desc": "? I magnitude "}, {"name": "u_Imag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "zmag", "desc": "? SDSS z magnitude "}, {"name": "u_zmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Jmag", "desc": "? J magnitude "}, {"name": "u_Jmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Hmag", "desc": "? H magnitude "}, {"name": "u_Hmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Kmag", "desc": "? K magnitude "}, {"name": "u_Kmag", "desc": "[u] u when a value is available somewhere, but considered as wrong"}, {"name": "Gmag", "desc": "? Gaia G magnitude "}, {"name": "Notes", "desc": "Notes "}]}, {"name": "ocars_n.dat", "desc": "Cross-identification table between the OCARS and other catalogs (13/12/2016 version)", "columns": [{"name": "OCARS", "desc": "OCARS source name (HHMM+DDd) "}, {"name": "IVS", "desc": "IVS name (source name used in IVS schedules and databases)"}, {"name": "LQAC", "desc": "LQAC name (LQAC_NNN_NNN_NNN) (from Souchay et al., 2015, Cat. J/A+A/583/A75)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AcA_62_o.1"}} {"id": "J/AcA/62/1", "title_cds": "OGLE-III. Magellanic Clouds stellar proper motions", "title_create": "Poleski+, 2012", "year": "2012", "author": "Poleski R., Soszynski I., Udalski A., Szymanski M.K., Kubiak M., Pietrzynski G., Wyrzykowski L., Ulaczyk K.", "title_pub": "The Optical Gravitational Lensing Experiment. The catalog of stellar proper motions toward the Magellanic Clouds.", "first_author": "Poleski R.", "ref_biblio": [""], "bibcode": ["2012AcA....62....1P"], "see_also": ["J/MNRAS/327/601 : OGLE-II High proper motion stars (Eyer+, 2001)", "J/AcA/52/143 : OGLE high proper motion stars towards MC (Soszynski+, 2002)", "J/AcA/59/1 : LMC RR Lyrae stars VI light curves (Soszynski+, 2009)", "J/AcA/59/239 : LMC long-period variables VI light curves (Soszynski+, 2009)", "J/AcA/60/1 : LMC delta Scuti stars VI light curves (Poleski+, 2010)", "J/AcA/60/17 : SMC classical Cepheids VI light curves (Soszynski+, 2010)", "J/AcA/60/165 : SMC RR Lyrae VI light curves (Soszynski+, 2010)", "J/AcA/61/103 : LMC eclipsing binaries VI light curves (Szymanski+, 2011)", "J/AcA/61/199 : OGLE3 Magellanic Clouds high pm stars (Poleski+, 2011)", "J/AcA/61/217 : SMC long-period variables VI light curves (Soszynski+, 2011)"], "keyword_cds": "Surveys ; Magellanic Clouds ; Proper motions", "keyword_pub": "Astrometry - Catalogs - Stars: kinematics and dynamics - binaries: visual - globular clusters: individual: 47 Tuc", "abstract": ["We present a catalog of over 6.2 million stars with measured proper", "motions. All these stars are observed in the direction of the", "Magellanic Clouds within the brightness range 12"], "bibcode": ["2016AcA....66..255S"], "keyword_cds": "Surveys ; Magellanic Clouds ; Associations, stellar", "keyword_pub": "catalogs - surveys - Magellanic Clouds - galaxies: clusters: general", "abstract": ["The Magellanic System (MS), consisting of the LargeMagellanic Cloud", "(LMC), the SmallMagellanic Cloud (SMC) and the Magellanic Bridge", "(MBR), contains diverse sample of star clusters. Their spatial", "distribution, ages and chemical abundances may provide important", "information about the history of formation of the whole System. We use", "deep photometric maps derived from the images collected during the", "fourth phase of the Optical Gravitational Lensing Experiment (OGLE-IV)", "to construct the most complete catalog of star clusters in the Large", "Magellanic Cloud using the homogeneous photometric data. In this paper", "we present the collection of star clusters found in the area of about", "225 square degrees in the outer regions of the LMC. Our sample", "contains 679 visually identified star cluster candidates, 226 of which", "were not listed in any of the previously published catalogs. The new", "clusters are mainly young small open clusters or clusters similar to", "associations."], "description": ["The photometric data of the LMC fields analyzed in this paper come", "from the images gathered during the first five years (2010\u20132015) of", "the fourth phase of the OGLE project (OGLE-IV, Udalski, Szyma\u00b4nski", "and Szyma\u00b4nski 2015). The project has been conducted on the 1.3-meter", "Warsaw Telescope at the Las Campanas Observatory, equipped with the", "32-chip mosaic CCD camera, covering 1.4 square degree field with", "0.26\" per pixel scale (see the aforementioned paper for the", "details of the OGLE-IV hardware setup, observational strategy and", "photometric reductions pipeline)."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "20-Apr-2018"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_AcA_66_269"}} {"id": "J/AcA/66/269", "title_cds": "Short Title", "title_create": "Skowron+, 2016", "year": "2016", "author": "Skowron D.M., Soszynski I., Udalski A., Szymanski M.K., Pietrukowicz P., Skowron J., Poleski R., Wyrzykowski L., Ulaczyk K., Kozlowski S., Mroz P., Pawlak M.", "title_pub": "OGLE-ing the Magellanic System: Photometric metallicity from fundamental mode RR Lyrae stars.", "first_author": "Skowron D.M.", "ref_biblio": [""], "bibcode": ["2016AcA....66..269S"], "keyword_cds": "Surveys ; Magellanic Clouds", "keyword_pub": "stars: abundances \u2013 stars: statistics \u2013 stars: variables: RR Lyr \u2013 galaxies: abundances \u2013 Magellanic Clouds", "abstract": ["In an era of extensive photometric observations, the catalogs of RR", "Lyr type variable stars number tens of thousands of objects. The", "relation between the iron abundance [Fe/H] and the Fourier parameters", "of the stars light curve allows us to investigate mean metallicities", "and metallicity gradients in various stellar environments,", "independently of time-consuming spectroscopic observations. In this", "paper we use almost 6500 V- and I-band light curves of fundamental", "mode RR Lyr stars from the OGLE-IV survey to provide a relation", "between the V- and I-band phase parameter {phi}_31_ used to estimate", "[Fe/H]. The relation depends on metallicity, which limits its", "applicability. We apply this relation to metallicity formulae", "developed for the Johnson V- and the Kepler Kp-band to obtain the", "relation between [Fe/H] and {phi}_31_ for the I-band photometry. Last,", "we apply the new relation of Nemec to the OGLE-IV fundamental mode RR", "Lyr stars data and construct a metallicity map of the Magellanic", "Clouds. Median [Fe/H] is -1.39+/-0.44dex for the LMC and", "-1.77+/-0.48dex for the SMC, on the Jurcsik metallicity scale. We also", "find a metallicity gradient within the LMC with a slope of", "-0.029+/-0.002dex/kpc in the inner 5kpc and -0.030+/-0.003dex/kpc", "beyond 8kpc, and no gradient in-between (-0.019+/-0.002dex/kpc", "integrally). We do not observe a metallicity gradient in the SMC,", "although we show that the metal-rich RRab stars are more concentrated", "toward the SMC center than the metal-poor."], "description": ["For the purpose of this study we used the OGLE-IV RRab sample that", "consists of 27 258 stars in the Galactic bulge (Soszynski et al. 2014.", "Cat. J/AcA/64/177) and 27 081 in the LMC (Soszynski et al.,", "2016AcA....66..131S). We do not include the SMC RRL sample because of", "smaller number of observations in the V-band."], "object": [], "curator": "Patricia Vannier [CDS]", "orcid_pub": ["0000-0002-2335-1730", "0000-0002-2335-1730"], "data": "", "date_update": "19-Feb-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_116_592"}} {"id": "J/ApJ/116/592", "title_cds": "Cygnus photometry", "title_create": "Macrae+, 1952", "year": "1952", "author": "Macrae D.A.", "title_pub": "Stellar spectra and colors in Cygnus at galactic latitude +14 deg.", "first_author": "Macrae D.A.", "ref_biblio": [""], "bibcode": ["1952ApJ...116..592M"], "keyword_cds": "MK spectral classification; Magnitudes, photographic", "keyword_pub": "", "abstract": ["Photographic magnitudes, colors, and spectral types of 938 stars to", "limiting magnitude 12.7 are given in table3. The photometric data,", "obtained from plates taken with the Burrell telescope, are based on a", "sequence of stars in the field for which magnitudes and colors were", "determined by photoelectric means. Luminosity classes have been", "assigned to stars brighter than 11.2. A few stars of special interest", "are discussed, including one which is similar to BD+28 4211 (Op), a", "new carbon star, and three new variables, one of which is an S-type", "star."], "object": [], "alias": ["ILF-1"], "doi_pub": ["10.1086/145652"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table3.dat", "desc": " ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_119_188"}} {"id": "J/ApJ/119/188", "title_cds": "Positions and Identifications of stars in NGC 2287", "title_create": "Cox+, 1954", "year": "1954", "author": "Cox A.N.", "title_pub": "A study of the galactic cluster NGC 2287.", "first_author": "Cox A.N.", "ref_biblio": [""], "bibcode": ["1954ApJ...119..188C"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["Magnitudes and colours of 106 stars in the region od NGC 2287 (M41)", "were observed with a photoelectric photometer mounted on the 24-inch", "(133cm) Victoria telescope at the Royal Observatory, Cape of Good", "Hope. Spectral types and radial velocities were found for 22 cluster", "stars from low-dispersion spectra obtained at the McDonald", "Observatory."], "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/145809"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_120_129"}} {"id": "J/ApJ/120/129", "title_cds": "Carbon stars near the Galactic Plane", "title_create": "Nassau+, 1954", "year": "1954", "author": "Nassau J.J., Blanco V.M.", "title_pub": "Carbon stars at the galactic equator in a zone 4 degrees wide", "first_author": "Nassau J.J.", "ref_biblio": [""], "bibcode": ["1954ApJ...120..129N"], "keyword_cds": "Stars, carbon", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["CASE"], "doi_pub": ["10.1086/145888"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_125_195"}} {"id": "J/ApJ/125/195", "title_cds": "Carbon stars in Milky Way zones", "title_create": "Nassau+, 1957", "year": "1957", "author": "Nassau J.J., Blanco V.M.", "title_pub": "Carbon stars in two northern Milky Way zones.", "first_author": "Nassau J.J.", "ref_biblio": [""], "bibcode": ["1957ApJ...125..195N"], "keyword_cds": "Stars, carbon", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/146293"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_128_267"}} {"id": "J/ApJ/128/267", "title_cds": "Feige's list of underluminous hot stars", "title_create": "Feige+, 1958", "year": "1958", "author": "Feige J.", "title_pub": "A search for underluminous hot stars.", "first_author": "Feige J.", "ref_biblio": [""], "bibcode": ["1958ApJ...128..267F"], "keyword_cds": "Stars, blue", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/146541"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_176_623"}} {"id": "J/ApJ/176/623", "title_cds": "Suspected supergiant M stars", "title_create": "Albers+, 1972", "year": "1972", "author": "Albers H.", "title_pub": "Infrared surveys of the Southern Milky Way. II. Suspected supergiant M stars.", "first_author": "Albers H.", "ref_biblio": [""], "bibcode": ["1972ApJ...176..623A"], "keyword_cds": "Stars, supergiant ; Stars, late-type", "abstract": ["An infrared objective-prism survey has been carried out along the", "Southern Milky Way, suspected M-type supergiants habe been selected", "from the presence of a CN absorption feature at 790nm. A calalog of", "170 M stars showing this feature is given."], "description": ["Accurate positions from Brian Skuff (Lowell Obs.)"], "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/151664"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_241_486"}} {"id": "J/ApJ/241/486", "title_cds": "Absolute magnitudes in 116 nearby Abell clusters", "title_create": "Hoessel+, 1980", "year": "1980", "author": "Hoessel J.G., Gunn J.E., Thuan T.X.", "title_pub": "The photometry properties of brightest cluster galaxies. I. Absolute magnitudes in 116 nearby Abell clusters.", "first_author": "Hoessel J.G.", "ref_biblio": [""], "bibcode": ["1980ApJ...241..486H"], "see_also": ["VII/87 : Data on 1889 Abell's clusters of galaxies (Leir+ 1977)", "J/ApJ/566/103 : VIK' photometry and redshifts of galaxy clusters (Nelson+ 2002)"], "keyword_cds": "Clusters, galaxy ; Magnitudes, absolute ; Redshifts", "keyword_pub": "cosmology - galaxies: clusters of - galaxies: photometry - galaxies: structure", "abstract": ["Two-color aperture photometry of the brightest galaxies in a complete", "sample of nearby Abeil clusters is presented. The results are used to", "anchor the bright end of the Hubble diagram; essentially the entire", "formal error for this method is then due to the sample of distant", "clusters used. New determinations of the systematic trend of galaxy", "absolute magnitude with the cluster properties of richness and", "Bautz-Morgan type are derived. When these new results are combined", "with the Gunn and Oke data on high-redshift clusters, a formal value", "(without accounting for any evolution) of q_0_=-0.55+/-0.45 (1{sigma})", "is found."], "doi_pub": ["10.1086/158363"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Observed Properties of the Low-Redshift Sample ", "columns": [{"name": "Abell", "desc": "Abell designation (ANNNN) "}, {"name": "RA1h", "desc": "Right ascension (B1950.0) "}, {"name": "RA1m", "desc": "Right ascension (B1950.0) "}, {"name": "RA1s", "desc": "Right ascension (B1950.0) "}, {"name": "DE1-", "desc": "Declination sign (B1950.0) "}, {"name": "DE1d", "desc": "Declination (B1950.0) "}, {"name": "DE1m", "desc": "Declination (B1950.0) "}, {"name": "DE1s", "desc": "Declination (B1950.0) "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "cz", "desc": "? Heliocentric radial velocity "}, {"name": "z", "desc": "? Redshift "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "R", "desc": "Abell richness class "}, {"name": "D", "desc": "Abell distance class "}, {"name": "BM", "desc": "BM type (from Leir & van den Bergh, 1977, Cat. )"}, {"name": "logz", "desc": "? log of redshift "}, {"name": "2gam", "desc": "? Observation angular diameter "}, {"name": "radius", "desc": "? Physical radius "}, {"name": "gmag", "desc": "? g magnitude "}, {"name": "g-r", "desc": "? g-r colour index "}, {"name": "Apcor", "desc": "? Aperture correction "}, {"name": "Rcorr", "desc": "? Corrected Radius "}, {"name": "VImag", "desc": "? VI (visual intrinsic) magnitude "}, {"name": "VIMAG", "desc": "? Absolute VI magnitude "}, {"name": "Obs", "desc": "Type and number of observations (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_253_485"}} {"id": "J/ApJ/253/485", "title_cds": "High-latitude HEAO 1 A-2 sources X-ray sample", "title_create": "Piccinotti+, 1982", "year": "1982", "author": "Piccinotti G., Mushotzky R.F., Boldt E.A., Holt S.S., Marshall F.E., Serlemitsos P.J., Shafer R.A.", "title_pub": "A complete X-ray sample of the high-latitude (|b|>20{deg}) sky from HEAO 1 A-2: log N-log S and luminosity functions.", "first_author": "Piccinotti G.", "ref_biblio": [""], "bibcode": ["1982ApJ...253..485P"], "keyword_cds": "Clusters, galaxy ; X-ray sources ; Redshifts", "keyword_pub": "Galaxies, cluster of - luminosity function - X-ray sources", "abstract": ["The HEAO 1 experiment A-2 has performed a complete X-ray survey of the", "8.2sr of the sky at |b|>20{deg} down to a limiting sensitivity of", "~3.1x10^-11^ergs/cm^2^/s in the 2-10keV band. Of the 85 detected", "sources (excluding the LMC and SMC sources), 17 have been identified", "with galactic objects, 61 have been identified with extragalactic", "objects, and 7 remain unidentified. The log N -log S relation for the", "nongalactic objects is well fitted by the Euclidean relationship. We", "have used the X-ray spectra of these objects to construct the log", "N-log S relation in physical units. The complete sample of identified", "sources has been used to construct X-ray luminosity functions, using", "the absolute maximum likelihood method, for clusters of galaxies and", "active galactic nuclei."], "doi_pub": ["10.1086/159651"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Data on X-ray sources ", "columns": [{"name": "A2Name", "desc": "HEAO A-2 name (HHHMM+DDd) "}, {"name": "A1Name", "desc": "HEAO A-1 Name (1HHHMM+DDd) "}, {"name": "Flux1", "desc": "1st Scan flux, in R15ct/s (1) "}, {"name": "e_Flux1", "desc": "rms uncertainty on Flux1 "}, {"name": "l_Flux2", "desc": "Limit flag on Flux2 "}, {"name": "Flux2", "desc": "2nd Scan flus, in R15ct/s (1) "}, {"name": "e_Flux2", "desc": "? rms uncertainty on Flux2 "}, {"name": "OName", "desc": "Optical identification "}, {"name": "RAh", "desc": "Right ascension (1950.0) "}, {"name": "RAm", "desc": "Right ascension (1950.0) "}, {"name": "RAs", "desc": "Right ascension (1950.0) "}, {"name": "DE-", "desc": "Declination sign (1950.0) "}, {"name": "DEd", "desc": "Declination (1950.0) "}, {"name": "DEm", "desc": "Declination (1950.0) "}, {"name": "DEs", "desc": "Declination (1950.0) "}, {"name": "MType", "desc": "Morphological type (2) "}, {"name": "z", "desc": "? Redshift "}, {"name": "r_z", "desc": "Reference for redshift (3) "}, {"name": "CF", "desc": "Conversion factor, in 10^-11^erg/cm2/(R15ct/s) "}, {"name": "Lum1", "desc": "? 1st Scan luminosity "}, {"name": "Lum2", "desc": "? 2nd Scan luminosity "}, {"name": "Notes", "desc": "? Individual notes (4) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_264_337"}} {"id": "J/ApJ/264/337", "title_cds": "CCD photometry of Abell clusters", "title_create": "Schneider+, 1983", "year": "1983", "author": "Schneider D.P., Gunn J.E., Hoessel J.G.", "title_pub": "CCD photometry of Abell clusters. I. Magnitudes and redshifts for 84 brightest cluster galaxies.", "first_author": "Schneider D.P.", "ref_biblio": [""], "bibcode": ["1983ApJ...264..337S"], "see_also": ["VII/87 : Data on 1889 Abell's clusters of galaxies (Leir+ 1977)", "J/AJ/101/1561 : Isophotometry of ellipticals in Abell clusters (Porter+ 1991)"], "keyword_cds": "Clusters, galaxy ; Photometry, CCD ; Redshifts", "keyword_pub": "cosmology - galaxies: clusters of - galaxies: photometry", "abstract": ["A sample of 84 Abell clusters has been selected to determine how the", "luminosity of the brightest cluster galaxy varies with cluster", "parameters. The clusters are of moderate redshift (0.04"], "bibcode": ["1983ApJ...274..534M"], "keyword_cds": "Galaxy catalogs ; Morphology", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: structure", "abstract": ["We present a catalog of 137 elliptical galaxies south of -17{deg}", "declination which exhibit shell or ripple features at large distances", "from the galaxy or in the outer envelope. Some of these galaxies show", "similar features in the inner envelope when suitable high resolution", "plate material is examined. Very few of the galaxies are associated", "with radio sources. We discuss the environment of shell galaxies, and", "the proportion of ellipticals which have these features. It appears", "that about half of the galaxies with shells are isolated and most of", "the rest are members of small groups. We discuss several individual", "examples which appear to be typical of this class of galaxy and others", "which probably illustrate an evolutionary sequence."], "doi_pub": ["10.1086/161467"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "The Galaxy Catalog ", "columns": [{"name": "[MC83b]", "desc": "Reference name of the object derived from the 1950 coordinates (1)"}, {"name": "n_[MC83b]", "desc": "[*] *: Note in notes.dat file "}, {"name": "Field", "desc": "The ESO/SRC field number (see Holmberg et al., 1974A&AS...18..463H, 1974A&AS...18..491H for the nominal field centers)."}, {"name": "WDist", "desc": "The distance in mm from the eastern edge of the image on the film copies (2)"}, {"name": "NDist", "desc": "The distance in mm from the southern edge of the image on the film copies (2)"}, {"name": "RAh", "desc": "Right ascension (1950) (3) "}, {"name": "RAm", "desc": "Right ascension (1950) (3) "}, {"name": "RAs", "desc": "Right ascension (1950) (3) "}, {"name": "DE-", "desc": "Declination sign (1950) (3) "}, {"name": "DEd", "desc": "Declination (1950) (3) "}, {"name": "DEm", "desc": "Declination (1950) (3) "}, {"name": "DEs", "desc": "Declination (1950) (3) "}, {"name": "Env", "desc": "[IGC] The environment of the sample galaxy (4) "}, {"name": "Com", "desc": "Comments. "}]}, {"name": "table2.dat", "desc": "Supplementary list of galaxies with shells outside main survey", "columns": [{"name": "[MC83b]", "desc": "Reference name of the object derived from the 1950 coordinates (1)"}, {"name": "n_[MC83b]", "desc": "[*] *: Note in notes.dat file "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "RAs", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "DEs", "desc": "? Declination (1950) "}, {"name": "Com", "desc": "Comments. "}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "[MC83b]", "desc": "Reference name of the object "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_301_927"}} {"id": "J/ApJ/301/927", "title_cds": "Stephenson's late M-star catalog", "title_create": "Stephenson+, 1986", "year": "1986", "author": "Stephenson C.B.", "title_pub": "Late M stars found in a hemispheric survey.", "first_author": "Stephenson C.B.", "ref_biblio": [""], "bibcode": ["1986ApJ...301..927S"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Brian Skiff [Lowell Obs.], Francois Ochsenbein [CDS]", "alias": ["StM"], "type": ["OC"], "doi_pub": ["10.1086/163957"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_315_104"}} {"id": "J/ApJ/315/104", "title_cds": "Molecular clouds near Gould belt", "title_create": "Taylor+, 1987", "year": "1987", "author": "Taylor D.K., Dickman R.L., Scoville N.Z.", "title_pub": "Molecular clouds and the Gould belt.", "first_author": "Taylor D.K.", "ref_biblio": [""], "bibcode": ["1987ApJ...315..104T"], "see_also": ["VII/7 : Lynds' Catalogue of Dark Nebulae (LDN) (Lynds 1962)", "VII/191 : Catalogue of Southern Dark Clouds (Hartley+ 1986)", "J/ApJS/95/457 : IRAS images of nearby dark clouds (Wood+ 1994)", "J/A+AS/141/175 : Dark clouds imaging polarimetry (Sen+, 2000)"], "keyword_cds": "Molecular clouds ; Radial velocities", "keyword_pub": "galaxies: Milky Way - galaxies: structure - interstellar: molecules", "abstract": ["We investigate the relationship of the local system of molecular", "clouds to the Gould belt. A careful examination of the National", "Geographic-Palomar Observatory Sky Survey Atlas (POSS) yielded a", "catalog of dark clouds with accurately measured positions as far south", "as {delta}=-27{deg}. From a nonlinear least squares fit to these data,", "along with positions from Feitzinger and Stuwe's catalog of southern", "clouds, we find a subset of dark clouds to be distributed irregularly", "along a curve b=-3.5{deg} + 12.5{deg}sin(l-27.5{deg}) This is similar", "to the distribution of the system of O and B stars used to define the", "system.", "Radial velocities in the J=1->0 transition of carbon monoxide were", "measured for all dark clouds in our catalog using the 14 m antenna of", "the Five College Radio Astronomy Observatory. The velocity", "distribution of those clouds judged to be members of the belt", "population suggests an expansion similar to that seen in the neutral", "atomic hydrogen and OB stars. Similar expansion energies are found for", "both gas constituents, atomic and molecular, as well as for the Gould", "belt stars. The velocity-longitude data for our molecular clouds were", "fitted to a model ring expanding under the influence of Galactic", "differential rotation and interstellar drag, with poor results. We", "discuss the reasons for this.", "Because the similar expansion energies of the stellar, H I, and", "molecular gas constituents of the Gould belt are all approximately", "equal, we suggest that the belt originated in an acceleration of gas", "rather than in a violent impulse such as a blast wave from one or more", "supernovae."], "doi_pub": ["10.1086/165117"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table3.dat", "desc": "Catalog of dark clouds ", "columns": [{"name": "TDS", "desc": "Sequential number "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "RAs", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "DEs", "desc": "Declination (1950) "}, {"name": "RV", "desc": "Spectral line centroid radial velocity "}, {"name": "n_RV", "desc": "[*] *: the observed velocity implies a nonlocal cloud"}, {"name": "Belt", "desc": "Belt (Gal or Gould) "}, {"name": "LDN", "desc": "? Lynds (Cat. ) number "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_381_33"}} {"id": "J/ApJ/381/33", "title_cds": "VRI photometry of Cl 1358+6245", "title_create": "Fabricant+, 1991", "year": "1991", "author": "Fabricant D.G., McClintock J.E., Bautz M.", "title_pub": "Galaxy evolution in distant, X-ray selected clusters of galaxies. I. Cl 1358+6245.", "first_author": "Fabricant D.G.", "ref_biblio": [""], "bibcode": ["1991ApJ...381...33F"], "see_also": ["J/ApJ/498/195 : Spectroscopic survey of CL 1358+62 (Fisher+ 1998)", "J/ApJ/500/714 : Color-magnitude relation in CL 1358+62 (Van Dokkum+ 1998)", "J/ApJ/539/577 : Galaxy morphologies Cl 1358+62 (Fabricant+, 2000)"], "keyword_cds": "Clusters, galaxy ; X-ray sources ; Photometry, VRI", "keyword_pub": "galaxies: clustering - galaxies: photometry - galaxies: structure - galaxies: X-rays", "abstract": ["A photometric and spectroscopic survey of a cluster of galaxies at", "z=0.327 is presented. We have obtained V, R, and I photometry of 288", "stars and galaxies in a region 5.7'x6.5' which is approximately", "centered on the dominant galaxy at the cluster center. The photometry", "is complete to rest band M_V_=-19.5 (19kpc diameter aperture). We have", "obtained the spectra of 70 galaxies which lie within ~2' (~R_30_) of", "the cluster center, to a magnitude limit of M_V_~- 20.5; ~90% of these", "galaxies are cluster members. The large velocity dispersion of the", "cluster, 1125^+126^_-94_ km/s, is consistent with its high X-ray", "luminosity, ~7x10^44^erg/s (0.2-4.5 keV)."], "doi_pub": ["10.1086/170626"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table5.dat", "desc": "Photometric results ", "columns": [{"name": "[FMB91]", "desc": "Sequential number "}, {"name": "RAh", "desc": "Right ascension (B1950) "}, {"name": "RAm", "desc": "Right ascension (B1950) "}, {"name": "RAs", "desc": "Right ascension (B1950) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) "}, {"name": "DEm", "desc": "Declination (B1950) "}, {"name": "DEs", "desc": "Declination (B1950) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "V-R", "desc": "V-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "Type", "desc": "[sg] Classification "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_411_501"}} {"id": "J/ApJ/411/501", "title_cds": "I-band selected galaxy sample", "title_create": "Lilly, 1993", "year": "1993", "author": "Lilly S.J.", "title_pub": "A deep I-band selected galaxy sample : implications for galaxy evolution.", "first_author": "Lilly S.J.", "ref_biblio": [""], "bibcode": ["1993ApJ...411..501L"], "keyword_cds": "Infrared sources ; Galaxies, IR ; Redshifts ; Equivalent widths", "keyword_pub": "galaxies: distances and redshifts - galaxies: evolution - galaxies: formation - infrared: galaxies", "abstract": ["New spectroscopic observations of statistically complete sample of 50", "very faint I-band selected galaxies with I_AB_<22.5 show that,", "although they extend out to z~1, the redshifts are generally low,", "_obs_~0.5+/-0.1."], "doi_pub": ["10.1086/172851"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Photometric and spectroscopic data ", "columns": [{"name": "[L93]", "desc": "Identification number "}, {"name": "n_[L93]", "desc": "[fgh] Note (1) "}, {"name": "Xpos", "desc": "X position (2) "}, {"name": "Ypos", "desc": "Y position (2) "}, {"name": "Imag3", "desc": "I_AB_ magnitude in 3\" diameter aperture "}, {"name": "ImagISO", "desc": "I_AB_ magnitude in circular isophotal aperture to {mu}_AB_(I)=28"}, {"name": "z", "desc": "? Redshift "}, {"name": "n_z", "desc": "[s] s: star "}, {"name": "Q", "desc": "[A-D] Quality class (3) "}, {"name": "(V-I)", "desc": "(V-I)_AB_ colour index (4) "}, {"name": "l_EW0", "desc": "Limit flag on EW0 "}, {"name": "EW0", "desc": "? Rest-of frame equivalent width of [O II] 3727{AA}"}, {"name": "Obs", "desc": "Year of the observing season when spectroscopic observations made"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_412_479"}} {"id": "J/ApJ/412/479", "title_cds": "Intracluster gas temperatures catalog", "title_create": "David+, 1993", "year": "1993", "author": "David L.P., Slyz A., Jones C., Forman W., Vrtilek S.D.", "title_pub": "A catalog of intracluster gas temperatures.", "first_author": "David L.P.", "ref_biblio": [""], "bibcode": ["1993ApJ...412..479D"], "see_also": ["IX/13 : The 2E Catalogue (Harris+ 1994)"], "keyword_cds": "Clusters, galaxy ; X-ray sources ; Redshifts", "keyword_pub": "catalogs - galaxies: clustering - intergalactic medium - X-rays: galaxies", "abstract": ["We have searched the Einstein Monitor Proportional Counter (MPC) data", "base for observations of clusters of galaxies. By coadding the MPC", "spectra obtained during all pointed observations of clusters with IPC", "count rates greater than 0.1 counts/s, we have obtained sufficient", "photon statistics to estimate the X-ray temperature of 84 clusters.", "Combining the MPC results with EXOSAT and Ginga results reported in", "the literature yields a combined sample of 104 clusters with known", "X-ray temperatures. One of the best studied X-ray correlations between", "clusters is that between their X-ray luminosity and gas temperature.", "We show that the best-fit power-law relation for our combined cluster", "sample can be explained by the observed increase in the gas-to-stellar", "mass ratio between low- and high-temperature clusters. The statistical", "significance of any evolution in our combined X-ray sample has been", "examined and compared with the statistical properties of clusters", "culled from optical catalogs. We find that there is strong evidence", "for a decrease in the X-ray luminosity of optically rich clusters", "beyond z approximately about 0.06. This result is used to estimate the", "normalization of the primordial power spectrum of density", "fluctuations."], "doi_pub": ["10.1086/172936"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Combined Cluster Sample ", "columns": [{"name": "Cluster", "desc": "Cluster designation "}, {"name": "Notes", "desc": "[abc] Notes (1) "}, {"name": "n_Cluster", "desc": "[*] Note on cluster (2) "}, {"name": "z", "desc": "Redshift (3) "}, {"name": "NH", "desc": "Hydrogen column density "}, {"name": "T", "desc": "? Temperature "}, {"name": "u_T", "desc": "Uncertainty flag on T "}, {"name": "l_E_T", "desc": "Limit flag on E_T (rms error in E_T) "}, {"name": "E_T", "desc": "? 1{sigma} error on T (upper limit) "}, {"name": "e_T", "desc": "? 1{sigma} error on T (lower limit) "}, {"name": "l_E90T", "desc": "Limit flag on E90T "}, {"name": "E90T", "desc": "? 90% confidence limit on T (upper limit) "}, {"name": "e90T", "desc": "? 90% confidence limit on T (lower limit) "}, {"name": "F2-10kev", "desc": "Flux at 2-10keV "}, {"name": "L2-10kev", "desc": "Luminosity at 2-10keV "}, {"name": "Lbol", "desc": "Bolometric luminosity "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_459_L27"}} {"id": "J/ApJ/459/L27", "title_cds": "R136 population", "title_create": "Hunter+ 1996", "year": "1996", "author": "Hunter D.A., O'Neil E.J.JR., Lynds R., Shaya E.J., Groth E.J., Holtzman J.A", "title_pub": "The intermediate-mass population in the core of the R136 star cluster.", "first_author": "Hunter D.A.", "ref_biblio": [""], "bibcode": ["1996ApJ...459..L27H\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "stars: formation - stars: luminosity function, mass function - galaxies: star clusters", "abstract": ["R136, the compact, luminous star cluster at the center of the", "30 Doradus nebula represents an extreme mode of star formation. Yet it", "is unique among these kinds of objects in that it can be resolved into", "individual stars and the star formation process probed through the", "stellar products. In a previous paper we reported on a study of the", "intermcdiate stellar mass population in R136 and derived a stellar", "initial mass function (IMF) for intermediate-mass stars in the region", "0.5 to 4.7pc from the center of the cluster. We have now obtained", "Hubble Space Telescope images designed to probe the stellar population", "in the core (<0.5pc) of the cluster. We have measured the IMF for", "stars 5-15M_{sun}_ at radii 0.11-0.34pc, and for 4-15M_{sun}_ at", "0.34-0.46pc. Beyond 0.46pc we measure stars in mass bins from", "2.8-15M_{sun}_, as before. The slope of the stellar IMF heyond 0.5pc", "is found to be -1.0+/-0.1, which is within a few sigma of the value", "measured previously for the same annulus. The slopes of the IMFs", "become shallower at smaller radii but the uncertainties do not rule", "out an IMF that is constant with cluster radius. The lower stellar", "mass limit is 5M_{sun}_. in the cluster core. Thus R136 is found to", "be similar to less concentrated OB associations even into 0.1pc from", "the center of the cluster."], "object": ["05 38 42.8 -69 06 03 RMC 136 = HD 38268"], "curator": "James Marcout, Patricia Bauer [CDS]", "data": "", "date_update": "12-Feb-1999"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_472_509"}} {"id": "J/ApJ/472/509", "title_cds": "Lyman-alpha Forest in Q0000-26", "title_create": "Lu+ 1996", "year": "1996", "author": "Lu L., Sargent W.L.W., Womble D.S., Takada-Hidai M.", "title_pub": "The Lyman-alpha Forest at z about 4: Keck HIRES Observations of Q0000-26", "first_author": "Lu L.", "ref_biblio": [""], "bibcode": ["1996ApJ...472..509L"], "keyword_cds": "QSOs ; Redshifts ; Spectroscopy", "abstract": ["This file contains the list of absorption lines found in the spectrum", "of the z_em_=4.1 quasar Q0000-26 obtained with the 10m Keck I", "telescope. The spectrum has a resolution of 6.6km/s, with typical", "signal-to-noise ratio 25-35 per resolution element. The absorption", "lines found in the Lyman-alpha forest region has been deblended using", "the Voigt profile fitting routine VPFIT from Robert Carswell and", "colleagues; redshift, column density, and Doppler width are provided", "for each line in the list."], "object": ["00 03 22.91 -26 03 16.8 QSO 0000-26 = QSO J0003-2603"], "doi_pub": ["10.1086/526756"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "lu1.dat", "desc": "Measured wavelengths ", "columns": [{"name": "No", "desc": "Running number "}, {"name": "lambda", "desc": "Wavelength "}, {"name": "ID", "desc": "Element identification "}, {"name": "z", "desc": "Redshift "}, {"name": "e_z", "desc": "Mean error of z "}, {"name": "b", "desc": "Effective radial velocity dispersion "}, {"name": "e_b", "desc": "Mean error of b "}, {"name": "logN", "desc": "logN (column density) "}, {"name": "e_logN", "desc": "Mean error of logN "}, {"name": "Note", "desc": "? Note detailed in file \"notes.dat\" "}]}, {"name": "lu2.dat", "desc": "Redshifts ", "columns": [{"name": "No", "desc": "? Running number "}, {"name": "lambda", "desc": "? Wavelength "}, {"name": "lam_obs", "desc": "? Observed wavelength "}, {"name": "e_lambda", "desc": "? Mean error of observed wavelength "}, {"name": "ID", "desc": "Element identification "}, {"name": "z", "desc": "? Redshift "}, {"name": "Note", "desc": "? Note detailed in file \"notes.dat\" "}]}, {"name": "notes.dat", "desc": "Notes ", "columns": [{"name": "NoteNo", "desc": "[1,10]+= Note number "}, {"name": "---", "desc": "[=] "}, {"name": "Text", "desc": "Text of note "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_478_124"}} {"id": "J/ApJ/478/124", "title_cds": "NGC 1818 stellar population", "title_create": "Hunter+, 1998", "year": "1998", "author": "Hunter D.A., Light R.M., Holtzman J.A., Lynds R., O'Neil E.J., Grillmair C.J.", "title_pub": "The intermediate-mass stellar population of the Large Magellanic Cloud cluster NGC 1818 and the universality of the stellar initial mass function.", "first_author": "Hunter D.A.", "ref_biblio": [""], "bibcode": ["1998ApJ...478..124H\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "James Marcout, Patricia Bauer [CDS]", "data": "", "date_update": "08-Apr-1999"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_485_447"}} {"id": "J/ApJ/485/447", "title_cds": "Evidence of substructure in A3558", "title_create": "Dantas+ 1997", "year": "1997", "author": "Dantas C.C., de Carvalho R.R., Capelato H.V., Mazure A.", "title_pub": "Evidence of substructure in the cluster of galaxies A3558", "first_author": "Dantas C.C.", "ref_biblio": [""], "bibcode": ["1997ApJ...485..447D"], "keyword_cds": "Clusters, galaxy ; Photometry ; Radial velocities", "keyword_pub": "catalogs - galaxies: clusters: individual (A3558) - galaxies: distances and redshifts - galaxies: elliptical and lenticular, cD - galaxies: photometry", "abstract": ["We investigate the dynamical properties of the cluster of galaxies", "A3558 (Shapley 8). Studying a region of 1deg^2^(~3Mpc^2^) centered on", "the cluster cD galaxy, we have obtained a statistically complete", "photometric catalog with positions and magnitudes of 1421 galaxies", "(down to a limiting magnitude of B~21). This catalog has been matched", "to the recent velocity data obtained by Mazure et al. (1997, in prep)", "and from the literature, yielding a radial velocity catalog containing", "322 galaxies. We analyze the resulting catalog in search of", "substructure, using different statistical techniques. This analysis", "shows that the position/velocity space distribution of galaxies shows", "significant substructure. A central bimodal core, detected previously", "in a preliminary study by Dantas, de Carvalho, & Capelato (1994, in", "Proc. 29th Rencontre de Moriond, Clusters of Galaxies, p. 385) and by", "an analysis of the X-ray emission map by Slezak, Durret, & Gerbal", "(1994AJ....108.1996S), is confirmed using the adaptive kernel", "technique and wavelet analysis. We show that this central bimodal", "substructure is nevertheless composed of a projected feature,", "kinematically unrelated to the cluster, plus a group of galaxies", "probably in its initial merging phase into a relaxed core. The cD", "galaxy's velocity offset with respect to the average cluster redshift,", "reported earlier by several authors, is completely eliminated as a", "result of our dynamical analysis. The untangling of the relaxed core", "component also allows a better, more reliable determination of the", "central velocity dispersion, which in turn eliminates the \"Beta", "problem\" for A3558. The cluster also shows a \"preferential\"", "distribution of subclumps coinciding with the direction of the", "major-axis position angle of the cD galaxy and of the central X-ray", "emission ellipsoidal distribution, in agreement with the anisotropic", "merger scenario described by West (1994MNRAS.268...79W) ."], "doi_pub": ["10.1086/304458"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table.dat", "desc": "A3558 Photometric Galaxy Catalogue ", "columns": [{"name": "Num", "desc": "Galaxy number "}, {"name": "RAh", "desc": "Right Ascension (J2000) "}, {"name": "RAm", "desc": "Right Ascension (J2000) "}, {"name": "RAs", "desc": "Right Ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Bmag", "desc": "Johnson B magnitude "}, {"name": "SuArea", "desc": "? Surface area "}, {"name": "e", "desc": "Ellipticity "}, {"name": "SuBr", "desc": "Surface brightness "}, {"name": "CI", "desc": "Color Index "}, {"name": "Vel", "desc": "? Velocity "}, {"name": "e_Vel", "desc": "? Velocity error "}, {"name": "Note", "desc": "Notes (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_498_77"}} {"id": "J/ApJ/498/77", "title_cds": "Ly{alpha} absorption systems. III.", "title_create": "Chen+, 1998", "year": "1998", "author": "Chen H.-W., Lanzetta K.M., Webb J.K., Barcons X.", "title_pub": "The gaseous extent of galaxies and the origin of Ly{alpha} absorption systems. III. Hubble space telescope imaging of Ly{alpha}-absorbing galaxies at z < 1.", "first_author": "Chen H.-W.", "ref_biblio": [""], "bibcode": ["1998ApJ...498...77C"], "see_also": ["J/ApJ/559/654 : Ly{alpha} absorption systems V. (Chen+, 2001)"], "keyword_cds": "QSOs ; Redshifts ; Equivalent widths", "keyword_pub": "galaxies: clusters: general - galaxies: distances and redshifts - quasars: absorption lines", "abstract": ["We present initial results of a program to obtain and analyze Hubble", "Space Telescope (HST) Wide Field Planetary Camera 2 images of galaxies", "identified in an imaging and spectroscopic survey of faint galaxies in", "fields of HST spectroscopic target QSOs. We measure properties of 87", "galaxies, of which 33 are associated with corresponding Ly absorption", "systems and 24 do not produce corresponding Ly{alpha} absorption lines", "to within sensitive upper limits. Considering only galaxy and absorber", "pairs that are likely to be physically associated and excluding galaxy", "and absorber pairs within 3000km/s of the background QSOs leaves 26", "galaxy and absorber pairs and seven galaxies that do not produce", "corresponding Ly{alpha} absorption lines to within sensitive upper", "limits. Redshifts of the galaxy and absorber pairs range from 0.0750", "to 0.8912 with a median of 0.3718, and impact parameter separations of", "the galaxy and absorber pairs range from 12.4 to 157.4h^-1^kpc with a", "median of 62.4h^-1^kpc."], "doi_pub": ["10.1086/305554"], "orcid_pub": ["0000-0001-8813-4182"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Journal of observations ", "columns": [{"name": "Field", "desc": "Field designation "}, {"name": "RAh", "desc": "Right ascension (B1950.0) "}, {"name": "RAm", "desc": "Right ascension (B1950.0) "}, {"name": "RAs", "desc": "Right ascension (B1950.0) "}, {"name": "DE-", "desc": "Declination sign (B1950.0) "}, {"name": "DEd", "desc": "Declination (B1950.0) "}, {"name": "DEm", "desc": "Declination (B1950.0) "}, {"name": "DEs", "desc": "Declination (B1950.0) "}, {"name": "Zem", "desc": "Emission redshift "}, {"name": "Filter", "desc": "Filter "}, {"name": "TExp", "desc": "Exposition time "}, {"name": "Date", "desc": "Observation date "}]}, {"name": "table2.dat", "desc": "Journal of archival observations ", "columns": [{"name": "Field", "desc": "Field designation "}, {"name": "RAh", "desc": "Right ascension (B1950.0) "}, {"name": "RAm", "desc": "Right ascension (B1950.0) "}, {"name": "RAs", "desc": "Right ascension (B1950.0) "}, {"name": "DE-", "desc": "Declination sign (B1950.0) "}, {"name": "DEd", "desc": "Declination (B1950.0) "}, {"name": "DEm", "desc": "Declination (B1950.0) "}, {"name": "DEs", "desc": "Declination (B1950.0) "}, {"name": "Zem", "desc": "Emission redshift "}, {"name": "Filter", "desc": "Filter "}, {"name": "TExp", "desc": "Exposition time "}, {"name": "Date", "desc": "Observation date "}]}, {"name": "table4.dat", "desc": "Galaxies and Absorption Systems ", "columns": [{"name": "Field", "desc": "Galaxy field name (1) "}, {"name": "oRA", "desc": "Right Ascension offset from the QSO (1) "}, {"name": "oDE", "desc": "Declination offset from the QSO (1) "}, {"name": "z", "desc": "Galaxy redshift "}, {"name": "Rho", "desc": "Impact parameter in units of kpc/h "}, {"name": "DRad", "desc": "? Effective disk radius in units of kpc/h "}, {"name": "BRad", "desc": "? Effective bulge radius in units of kpc/h "}, {"name": "l_D/B", "desc": "Limit flag in D/B "}, {"name": "D/B", "desc": "? Disk to Bulge ratio "}, {"name": "Alpha", "desc": "? Orientation angle "}, {"name": "Inc", "desc": "? Inclination angle "}, {"name": "b/a", "desc": "? Bulge axis ratio "}, {"name": "Wmag", "desc": "? The WFPC2 apparent magnitude "}, {"name": "SB", "desc": "? Rest-frame B band mean surface brightness "}, {"name": "BMag", "desc": "? Absolute B band magnitude minus 5*log[h] "}, {"name": "zabs", "desc": "? Absorber redshift "}, {"name": "l_EqWLya", "desc": "Limit flag on EqWLya "}, {"name": "EqWLya", "desc": "? Ly{alpha} rest-frame equivalent width (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_505_L7"}} {"id": "J/ApJ/505/L7", "title_cds": "5 BAL QSO discovery", "title_create": "Brotherton+, 1998", "year": "1998", "author": "Brotherton M.S., van Breugel W., Smith R.J., Boyle B.J., Shanks T., Croom S.M., Miller L., Becker R.H.", "title_pub": "Discovery of radio-loud broad absorption line quasars using ultraviolet excess and deep radio selection.", "first_author": "Brotherton M.S.", "ref_biblio": [""], "bibcode": ["1998ApJ...505L...7B"], "keyword_cds": "QSOs ; Photometry ; Equivalent widths ; Redshifts", "keyword_pub": "quasar: absorption lines - quasar: emission lines - galaxies: general", "abstract": ["We report the discovery of five broad absorption line (BAL) QSOs in a", "complete sample of 111 ultraviolet excess (UVX) QSO candidates also", "detected in the NRAO VLA Sky Survey. All five BAL QSOs, which include", "two high-ionization BAL QSOs and three low-ionization BAL QSOs, are", "formally radio loud. Of QSOs with z>0.4, 3%+/-2% show low-ionization", "BALs, and of QSOs with z>1.5 , all radio loud, 9%+/-5% show BALs;", "these frequencies are consistent with those of optical surveys. While", "the first reported radio-loud BAL QSO, FIRST J155633.8+351758, is", "likely to be heavily dust reddened and thus less radio loud than", "indicated by its observed radio-to-optical luminosity, these QSOs are", "UVX-selected and probably free of significant dust along the line of", "sight. We point out unusual features in two of the BAL QSOs and", "discuss the significance finding these heretofore rare objects."], "doi_pub": ["10.1086/311599"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Radio-loud UVX BAL QSO properties ", "columns": [{"name": "UN", "desc": "Quasar name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "z", "desc": "Redshift "}, {"name": "Bjmag", "desc": "B_j_ magnitude (1) "}, {"name": "U-Bj", "desc": "U-Bj colour index (1) "}, {"name": "Bj-R", "desc": "Bj-R colour index (1) "}, {"name": "BMAG", "desc": "Absolute B magnitude (2) "}, {"name": "S1400MHz", "desc": "Flux density at 1400MHz "}, {"name": "e_S1400MHz", "desc": "rms uncertainty on S1400MHz "}, {"name": "logL1400MHz", "desc": "Luminosity at 1400MHz "}, {"name": "logR*", "desc": "Formal measure of radio loudness (2) (3) "}]}, {"name": "tables.tex", "desc": "LaTeX version of the tables ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_520_491"}} {"id": "J/ApJ/520/491", "title_cds": "Superclustering in Aquarius", "title_create": "Batuski+, 1999", "year": "1999", "author": "Batuski D.J., Miller C.J., Slinglend K.A., Balkowski C., Maurogordato S., Cayatte V., Felenbok P., Olowin R.", "title_pub": "Discovery of extreme examples of superclustering in Aquarius.", "first_author": "Batuski D.J.", "ref_biblio": [""], "bibcode": ["1999ApJ...520..491B"], "see_also": ["VII/4 : Abell and Zwicky Clusters of Galaxies (Abell+ 1974)", "VII/110 : Rich Clusters of Galaxies (Abell+ 1989)"], "keyword_cds": "Clusters, galaxy ; Radial velocities", "keyword_pub": "galaxies: clusters: general - galaxies: distances and redshifts", "abstract": ["The results of spectroscopic observations of 46 R>=1 clusters of", "galaxies from the Abell (Cat. ) and Abell, Corwin, & Olowin", "(hereafter ACO, Cat. ) catalogs are presented. The", "observations were conducted at the ESO 3.6 m telescope with the", "Meudon-ESO Fibre Optics Spectrograph (MEFOS) multiple-fiber", "spectrograph. Thirty-nine of the clusters lie in a 10{deg}x45{deg}", "strip of sky that contains two supercluster candidates (in Aquarius", "and Eridanus)."], "doi_pub": ["10.1086/307484"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Abell/ACO clusters observed in 10{deg} square Centered on Aquarius supercluster", "columns": [{"name": "ACO", "desc": "Cluster name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "HV", "desc": "(R+1)-weighted heliocentric velocity (1) "}, {"name": "n_HV", "desc": "[e] HV is the emission-line velocity "}, {"name": "e_HV", "desc": "rms uncertainty on HV "}, {"name": "Em", "desc": "? Object number if the subject galaxy has an emission-line velocity"}, {"name": "Note", "desc": "[ae] Note (2) "}, {"name": "Comm", "desc": "Comments "}]}, {"name": "table2.dat", "desc": "Other Abell/ACO clusters observed within 10{deg}x45{deg} strip", "columns": [{"name": "ACO", "desc": "Cluster name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "HV", "desc": "(R+1)-weighted heliocentric velocity (1) "}, {"name": "n_HV", "desc": "[e] HV is the emission-line velocity "}, {"name": "e_HV", "desc": "rms uncertainty on HV "}, {"name": "Em", "desc": "? Object number if the subject galaxy has an emission-line velocity"}, {"name": "Note", "desc": "[ae] Note (2) "}, {"name": "Comm", "desc": "Comments "}]}, {"name": "table3.dat", "desc": "Abell/ACO galaxies in Grus-Indus sample ", "columns": [{"name": "ACO", "desc": "Cluster name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "HV", "desc": "(R+1)-weighted heliocentric velocity (1) "}, {"name": "n_HV", "desc": "[e] HV is the emission-line velocity "}, {"name": "e_HV", "desc": "rms uncertainty on HV "}, {"name": "Em", "desc": "? Object number if the subject galaxy has an emission-line velocity"}, {"name": "Note", "desc": "[ae] Note (2) "}, {"name": "Comm", "desc": "Comments "}]}, {"name": "table4.dat", "desc": "Emission-line galaxy velocities ", "columns": [{"name": "ACO", "desc": "ACO name "}, {"name": "Em", "desc": "Object number "}, {"name": "Note", "desc": "[ae] Note "}, {"name": "Vem", "desc": "Emission-line velocity "}, {"name": "e_Vem", "desc": "rms uncertainty on Vem "}, {"name": "Lines", "desc": "Lines found (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_521_155"}} {"id": "J/ApJ/521/155", "title_cds": "New Cepheids and distance to NGC 4535", "title_create": "Macri+, 1999", "year": "1999", "author": "Macri L.M., Huchra J.P., Stetson P.B., Silbermann N.A., Freedman W.L., Kennicutt R.C., Mould J.R., Madore B.F., Bresolin F., Ferrarese L., Ford H.C., Graham J.A., Gibson B.K., Han M., Harding P., Hill R.J., Hoessel J.G., Hughes S.M.G., Kelson D.D., Illingworth G.D., Phelps R.L., Prosser C.F., Rawson D.M., Saha A., Sakai S., Turner A.", "title_pub": "The extragalactic distance scale key project. XVIII. The discovery of Cepheids and a new distance to NGC 4535 using the Hubble space telescope.", "first_author": "Macri L.M.", "ref_biblio": [""], "bibcode": ["1999ApJ...521..155M"], "see_also": ["J/ApJ/463/26 : Extragalactic Distance Scale Key Project. III (Kelson+ 1996)", "J/ApJ/507/655 : VI photometry of new Cepheids in NGC 2541 (Ferrarese+, 1998)", "J/ApJ/508/491 : M101 Cepheids (Stetson+, 1998)", "J/ApJ/523/540 : VI photometry of new Cepheids in NGC 3319 (Sakai+, 1999)", "J/ApJ/529/723 : VI photometry of Cepheids (Gibson+, 2000)"], "keyword_cds": "Stars, variable ; Photometry", "keyword_pub": "Cepheids - distance scale - galaxies: distances and redshifts - galaxies: individual (NGC 4535)", "abstract": ["We report on the discovery of Cepheids in the Virgo spiral galaxy NGC", "4535, based on observations made with the Wide Field and Planetary", "Camera 2 on board the Hubble Space Telescope (HST). NGC 4535 is one of", "18 galaxies observed as a part of The HST Key Project on the", "Extragalactic Distance Scale, which aims to measure the Hubble", "constant to 10% accuracy. NGC 4535 was observed over 13 epochs using", "the F555W filter, and over 9 epochs using the F814W filter. The HST", "F555W and F814W data were transformed to the Johnson V and", "Kron-Cousins I magnitude systems, respectively. Photometry was", "performed using two independent programs, DoPHOT and DAOPHOT", "II/ALLFRAME. Period-luminosity relations in the V and I bands were", "constructed using 39 high-quality Cepheids present in our set of 50", "variable candidates. We obtain a distance modulus of 31.02+/-0.26mag,", "corresponding to a distance of 16.0+/-1.9Mpc. Our distance estimate is", "based on values of {mu}_0_=18.50+/-0.10mag and E(V-I)=0.13mag for the", "distance modulus and reddening of the LMC, respectively."], "doi_pub": ["10.1086/307541"], "orcid_pub": ["0000-0002-1775-4859"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "Cepheid candidates - coordinates and classification ", "columns": [{"name": "[MHS99]", "desc": "Cepheid candidate number (CNN) "}, {"name": "Chip", "desc": "Chip number "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "Grade", "desc": "Quality grade (1) "}, {"name": "n_Grade", "desc": "[*] Stars used in the final fits (2) "}]}, {"name": "table3.dat", "desc": "Cepheid candidates - mean properties ", "columns": [{"name": "[MHS99]", "desc": "Cepheid candidate number (CNN) "}, {"name": "PerA", "desc": "Allframe period "}, {"name": "e_PerA", "desc": "rms uncertainty on PerA "}, {"name": "A", "desc": "Allframe average V magnitude "}, {"name": "e_A", "desc": "rms uncertainty on A "}, {"name": "A", "desc": "Allframe average I magnitude "}, {"name": "e_A", "desc": "rms uncertainty on A "}, {"name": "PerD", "desc": "DoPHOT period "}, {"name": "e_PerD", "desc": "rms uncertainty on PerD "}, {"name": "D", "desc": "DoPHOT average V magnitude "}, {"name": "e_D", "desc": "rms uncertainty on D "}, {"name": "D", "desc": "DoPHOT average I magnitude "}, {"name": "e_D", "desc": "rms uncertainty on D "}]}, {"name": "taba3-6.dat", "desc": "Secondary photometry stars for PC1, WF1, WF2 and WF3 ", "columns": [{"name": "Chip", "desc": "Chip (PC1, WF1, WF2 or WF3) "}, {"name": "RAh", "desc": "Right ascension (J2000.0) "}, {"name": "RAm", "desc": "Right ascension (J2000.0) "}, {"name": "RAs", "desc": "Right ascension (J2000.0) "}, {"name": "DE-", "desc": "Declination sign (J2000.0) "}, {"name": "DEd", "desc": "Declination (J2000.0) "}, {"name": "DEm", "desc": "Declination (J2000.0) "}, {"name": "DEs", "desc": "Declination (J2000.0) "}, {"name": "A", "desc": "Allframe average V magnitude "}, {"name": "e_A", "desc": "rms uncertainty on A "}, {"name": "A", "desc": "Allframe average I magnitude "}, {"name": "e_A", "desc": "rms uncertainty on A "}, {"name": "D", "desc": "DoPHOT average V magnitude "}, {"name": "e_D", "desc": "rms uncertainty on D "}, {"name": "D", "desc": "DoPHOT average I magnitude "}, {"name": "e_D", "desc": "rms uncertainty on D "}]}, {"name": "taba7-10.dat", "desc": "DoPHOT and ALLFRAME photometry ", "columns": [{"name": "[MHS99]", "desc": "Cepheid candidate number (CNN) "}, {"name": "HJD", "desc": "Heliocentric Julian date "}, {"name": "Filt", "desc": "Filter (1) "}, {"name": "mag", "desc": "Magnitude in Filt band "}, {"name": "e_mag", "desc": "rms uncertainty on mag "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_522_983"}} {"id": "J/ApJ/522/983", "title_cds": "M80 blue straggler stars", "title_create": "Ferraro+, 1999", "year": "1999", "author": "Ferraro F.R., Paltrinieri B., Rood R.T., Dorman B.", "title_pub": "Blue straggler stars: the spectacular population in M80.", "first_author": "Ferraro F.R.", "ref_biblio": [""], "bibcode": ["1999ApJ...522..983F"], "keyword_cds": "Stars, blue ; Photometry, ultraviolet", "keyword_pub": "blue stragglers - globular clusters: individual (M80) - stars: evolution - ultraviolet: stars", "mission": "HST", "abstract": ["Using Hubble Space Telescope WFPC2 observations in two ultraviolet", "(UV) filters (F225W and F336W) of the central region of the", "high-density Galactic globular cluster (GGC) M80, we have identified", "305 blue straggler stars (BSS), which represents the largest and most", "concentrated population of BSS ever observed in a GGC. We also", "identify the largest clean sample of evolved BSS yet found. The high", "stellar density alone cannot explain the BSS, and we suggest that in", "M80 we are witnessing a transient dynamical state, during which", "stellar interactions are delaying the core-collapse process leading to", "an exceptionally large population of collisional BSS."], "object": ["16 17 02.5 -22 58 30 M 80 = NGC 6093"], "doi_pub": ["10.1086/307700"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "The BSS population in M 80 ", "columns": [{"name": "Name", "desc": "BSS number (BSS NNN) (Cl* NGC 6093 BSS NNN in Simbad) (1)"}, {"name": "FPR", "desc": "FPR (1999ApJ...522..983F) identification number (Cl* NGC 6093 FPR NNNNN in Simbad)"}, {"name": "m255", "desc": "m_255_ UV magnitude "}, {"name": "Umag", "desc": "U magnitude "}, {"name": "Xpos", "desc": "X position (2) "}, {"name": "Ypos", "desc": "Y position (2) "}]}, {"name": "table2.dat", "desc": "The E-BSS population in M 80 ", "columns": [{"name": "EBSS", "desc": "E-BSS number (E-BSS NN) (Cl* NGC 6093 EBSS NN in Simbad)"}, {"name": "FPR", "desc": "FPR (1999ApJ...522..983F) identification number (Cl* NGC 6093 FPR NNNNN in Simbad)"}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "Umag", "desc": "U magnitude "}, {"name": "Xpos", "desc": "X position (1) "}, {"name": "Ypos", "desc": "Y position (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_523_87"}} {"id": "J/ApJ/523/87", "title_cds": "Shakhbazian compact galaxy groups", "title_create": "Tovmassian+, 1999", "year": "1999", "author": "Tovmassian H.M., Chavushyan V.H., Verkhodanov O.V., Tiersch H.", "title_pub": "Radio emission of Shakhbazian compact galaxy groups.", "first_author": "Tovmassian H.M.", "ref_biblio": [""], "bibcode": ["1999ApJ...523...87T"], "see_also": ["VII/89 : Compact groups of compact galaxies (Shakhbazian+ 1973-1979)", "VIII/59 : The FIRST Survey, version 1999Jul (White+ 1999)", "J/AJ/115/1693 : NRAO VLA Sky Survey (NVSS) (Condon+, 1998)"], "keyword_cds": "Clusters, galaxy ; Radio sources", "keyword_pub": "galaxies: clusters: general - radio continuum: galaxies - submillimeter - surveys", "abstract": ["We detect 353 radio sources from the NRAO VLA Sky Survey (NVSS, Cat.", ") and the FIRST Survey (Cat. ) within the", "areas of 179 Shakhbazian compact groups (ShCGs, Cat. ) of", "galaxies. Ninety-three of them are identified with galaxies in", "74 ShCGs. Six radio sources have complex structure. The radio spectra", "of 22 sources are determined. Radio luminosities of galaxies in ShCGs", "are in general higher than those of galaxies in Hickson compact groups", "(HCGs). A comparison of radio (at 1.4GHz) and FIR (at 60{mu}m) fluxes", "of ShCG galaxies with those of HCG galaxies shows that galaxies in", "ShCGs are relatively stronger emitters at radio wavelengths, while", "galaxies in HCGs have relatively stronger FIR emission. The reasons", "for such differences are discussed"], "doi_pub": ["10.1086/307726"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "List of radio identifications ", "columns": [{"name": "ShCG.G-xy", "desc": "Shakhbazian designation of the group and number of the galaxy (as labeled in the original ShCG finding charts) (1)"}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Name", "desc": "Identified radio source "}, {"name": "RArh", "desc": "Radio source right ascension (J2000) "}, {"name": "RArm", "desc": "Radio source right ascension (J2000) "}, {"name": "RArs", "desc": "Radio source right ascension (J2000) "}, {"name": "DEr-", "desc": "Radio source declination sign (J2000) "}, {"name": "DErd", "desc": "Radio source declination (J2000) "}, {"name": "DErm", "desc": "Radio source declination (J2000) "}, {"name": "DErs", "desc": "Radio source declination (J2000) "}, {"name": "S1.4GHz", "desc": "1.4GHz radio source flux density "}]}, {"name": "table2.dat", "desc": "Radio spectral indices ", "columns": [{"name": "ShCG.G-xy", "desc": "Shakhbazian designation (1) "}, {"name": "SI", "desc": "Radio spectral index "}]}, {"name": "table3.dat", "desc": "Radio luminosities ", "columns": [{"name": "ShCG.G-xy", "desc": "Shakhbazian designation (1) "}, {"name": "z", "desc": "Redshift "}, {"name": "logP1.4GHz", "desc": "Radio luminosity at 1.4GHz "}]}, {"name": "table4.dat", "desc": "List of HCG radio identifications ", "columns": [{"name": "Shk", "desc": "Shakhbazian designation (1) "}, {"name": "MType", "desc": "Morphological type "}, {"name": "Name", "desc": "Radio source designation "}, {"name": "F1.4", "desc": "1.4GHz flux "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_567_12"}} {"id": "J/ApJ/567/12", "title_cds": "Short Title", "title_create": "Author+, ", "title_pub": "Title of the paper", "first_author": "Authors", "author": "Authors", "ref_biblio": [""], "bibcode": ["2019ApJ...567...12.\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Coralie Fix [CDS]", "data": "", "date_update": "15-Oct-2019"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_616_1284"}} {"id": "J/ApJ/616/1284", "title_cds": "Automated classification of ROSAT sources", "title_create": "McGlynn+, 2004", "year": "2004", "author": "McGlynn T.A., Suchkov A.A., Winter E.L., Hanisch R.J., White R.L., Ochsenbein F., Derriere S., Voges W., Corcoran M.F., Drake S.A., Donahue M.", "title_pub": "Automated classification of ROSAT sources using heterogeneous multiwavelength source catalogs.", "first_author": "McGlynn T.A.", "ref_biblio": [""], "bibcode": ["2004ApJ...616.1284M"], "see_also": ["http://heasarc.gsfc.nasa.gov/classx/classx_classes/index.html :", "IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)", "IX/29 : ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000)", "IX/31 : The WGACAT version of ROSAT sources (White+ 2000)"], "keyword_cds": "X-ray sources", "keyword_pub": "methods: statistical - surveys - X-rays: binaries - X-rays: general - X-rays: stars", "abstract": ["We describe an online system for automated classification of X-ray", "sources, ClassX, and we present preliminary results of classification", "of the three major catalogs of ROSAT sources, ROSAT All-Sky Survey", "(RASS) Bright Source Catalog (Cat. ), RASS Faint Source Catalog", "(Cat. ), and WGACAT (Cat. ), into six class categories:", "stars, white dwarfs, X-ray binaries, galaxies, active galactic nuclei,", "and clusters of galaxies. ClassX is based on a machine-learning", "technology. It represents a system of classifiers, each classifier", "consisting of a considerable number of oblique decision trees. These", "trees are built as the classifier is \"trained\" to recognize various", "classes of objects using a training sample of sources of known object", "types. Each source is characterized by a preselected set of", "parameters, or attributes; the same set is then used as the classifier", "conducts classification of sources of unknown identity. The ClassX", "pipeline features an automatic search for X-ray source counterparts", "among heterogeneous data sets in online data archives using Virtual", "Observatory protocols; it retrieves from those archives all the", "attributes required by the selected classifier and inputs them to the", "classifier. The user input to ClassX is typically a file with target", "coordinates, optionally complemented with target IDs. The output", "contains the class name, attributes, and class probabilities for all", "classified targets."], "doi_pub": ["10.1086/424955"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table5a.dat", "desc": "Classification of RASS BSC by the RASS-X classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table5b.dat", "desc": "Classification of RASS BSC by the RASS-XOR classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table5c.dat", "desc": "Classification of RASS BSC by the WGACAT-X classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table5d.dat", "desc": "Classification of RASS BSC by the WGACAT-XOR classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table6a.dat", "desc": "Classification of WGACAT by the RASS-X classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table6b.dat", "desc": "Classification of WGACAT by the RASS-XOR classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table6c.dat", "desc": "Classification of WGACAT by the WGACAT-X classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table6d.dat", "desc": "Classification of WGACAT by the WGACAT-XOR classifier ", "columns": [{"name": "Name", "desc": "1RXS or 1WGA identification "}, {"name": "CI", "desc": "Class index "}, {"name": "P(Star)", "desc": "Probability that the source is a star "}, {"name": "P(WD)", "desc": "Probability that the source is a white dwarf "}, {"name": "P(XRB)", "desc": "Probability that the source is an X-ray binary "}, {"name": "P(Galaxy)", "desc": "Probability that the source is a galaxy "}, {"name": "P(AGN)", "desc": "Probability that the source is an AGN "}, {"name": "P(Cluster)", "desc": "Probability that the source is a Cluster "}, {"name": "Class", "desc": "Class Name "}]}, {"name": "table7a.dat", "desc": "Classification of RASS FSC by the RASS-X classifier ", "columns": [{"name": "Seq", "desc": "Sequential number of source in RASS FSC "}]}, {"name": "table7b.dat", "desc": "Classification of RASS FSC by the RASS-XOR classifier ", "columns": [{"name": "Seq", "desc": "Sequential number of source in RASS FSC "}]}, {"name": "table7c.dat", "desc": "Classification of RASS FSC by the WGACAT-X classifier ", "columns": [{"name": "Seq", "desc": "Sequential number of source in RASS FSC "}]}, {"name": "table7d.dat", "desc": "Classification of RASS FSC by the WGACAT-XOR classifier ", "columns": [{"name": "Seq", "desc": "Sequential number of source in RASS FSC "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_654_499"}} {"id": "J/ApJ/654/499", "title_cds": "H-rich white dwarfs spectropolarimetric survey", "title_create": "Kawka+, 2007", "year": "2007", "author": "Kawka A., Vennes S., Schmidt G.D., Wickramasinghe D.T., Koch R.", "title_pub": "Spectropolarimetric survey of hydrogen-rich white dwarf stars.", "first_author": "Kawka A.", "ref_biblio": [""], "bibcode": ["2007ApJ...654..499K"], "keyword_cds": "", "keyword_pub": "magnetic fields - white dwarfs", "mission": "", "abstract": ["We have conducted a survey of 61 southern white dwarfs searching for", "magnetic fields using Zeeman spectropolarimetry. Our objective is to", "obtain a magnetic field distribution for these objects and, in", "particular, to find white dwarfs with weak fields. We found one", "possible candidate (WD 0310688) that may have a weak magnetic field of", "-6.1+/-2.2kG. Next, we determine the fraction and distribution of", "magnetic white dwarfs in the solar neighborhood and investigate the", "probability of finding more of these objects based on the current", "incidence of magnetism in white dwarfs within 20 pc of the Sun. We", "have also analyzed the spectra of the white dwarfs to obtain effective", "temperatures and surface gravities."], "description": ["The data for the survey of magnetic fields in southern white dwarfs", "were acquired using the 74 inch (1.88 m) telescope at the Mount", "Stromlo Observatory with the Steward Observatory CCD", "Spectropolarimeter. The observations were conducted on 2000 October", "27-29, November 3, 5, and 25-26, and December 14, 23-28, and 31 and", "2001 January 1, 18-20, and 27 and February 17, 18, 21, 22, and 25."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/509072"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_702_506"}} {"id": "J/ApJ/702/506", "title_cds": "The Clowes-Campusano LQG Survey. I.", "title_create": "Haberzettl+, 2009", "year": "2009", "author": "Haberzettl L., Williger G.M., Lauroesch J.T., Haines C.P., Valls-Gabaud D., Harris K.A., Koekemoer A.M., Loveday J., Campusano L.E., Clowes R.G., Dave R., Graham M.J., Sochting I.K.", "title_pub": "The Clowes-Campusano Large Quasar Group Survey. I. GALEX selected sample of Lyman break galaxies at z~1.", "first_author": "Haberzettl L.", "ref_biblio": [""], "bibcode": ["2009ApJ...702..506H"], "see_also": ["VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)", "II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)", "J/A+A/533/A142 : UV-to-IR fluxes of Hickson compact groups (Bitsakis+, 2011)", "J/MNRAS/403/683 : GALEX Arecibo SDSS survey (GASS) (Catinella+, 2010)", "J/ApJ/697/1410 : Lyman break galaxies at z~1.8-2.8 (Ly+, 2009)", "J/MNRAS/392/19 : The 2dF-SDSS QSO survey (Croom+, 2009)", "J/MNRAS/380/986 : Lyman-break galaxies from GALEX (Burgarella+, 2007)", "J/AJ/133/1780 : GALEX/SDSS quasar catalog (Trammell+, 2007)", "J/MNRAS/249/218 : Group of quasars (Clowes+, 1991)", "http://www.sdss.org/ : SDSS web site"], "keyword_cds": "Galaxies, optical ; Redshifts ; Surveys ; Ultraviolet ; Photometry, SDSS", "keyword_pub": "galaxies: distances and redshifts - galaxies: evolution - large-scale structure of universe - quasars: general", "abstract": ["The nature of galaxy structures on large scales is a key observational", "prediction for current models of galaxy formation. The Sloan Digital", "Sky Survey (SDSS) and the 2dF galaxy survey have revealed a number of", "structures on 40-150h^-1^Mpc scales at low redshifts, and some even", "larger ones. To constrain galaxy number densities, luminosities, and", "stellar populations in large structures at higher redshift, we have", "investigated two sheet-like structures of galaxies at z=0.8 and 1.3", "spanning 150h^-1^ comoving Mpc embedded in large quasar groups (LQGs)", "extending over at least 200h^-1^Mpc. We present first results of an", "analysis of these sheet-like structures using two contiguous 1{deg}", "Galaxy Evolution Explorer (GALEX) fields (FUV and NUV)", "cross-correlated with optical data from the SDSS. We derive a sample", "of 462 Lyman break galaxy (LBG) candidates coincident with the sheets.", "Using the GALEX and SDSS data, we show that the overall average", "spectral energy distribution of a LBG galaxy at z~1 is flat (in", "f_{lambda}_) in the rest-frame wavelength range from 1500{AA} to", "4000{AA}, implying evolved populations of stars in the LBGs. From the", "luminosity functions we get indications for overdensities in the two", "LQGs compared to their foreground regions."], "description": ["We observed part of the Clowes-Campusano Large Quasar Group (CCLQG),", "it contains at least 18 bright quasars at 1.2 in Simbad)"}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "FUVmag", "desc": "?=99 GALEX FUV band (1538.6{AA}) magnitude "}, {"name": "e_FUVmag", "desc": "?=99 Error in FUVmag "}, {"name": "NUVmag", "desc": "GALEX NUV band (2315.7{AA}) magnitude "}, {"name": "e_NUVmag", "desc": "Error in NUVmag "}, {"name": "umag", "desc": "SDSS-DR5 u band magnitude "}, {"name": "e_umag", "desc": "Error in umag "}, {"name": "gmag", "desc": "SDSS-DR5 g band magnitude "}, {"name": "e_gmag", "desc": "Error in gmag "}, {"name": "rmag", "desc": "SDSS-DR5 r band magnitude "}, {"name": "e_rmag", "desc": "Error in rmag "}, {"name": "imag", "desc": "SDSS-DR5 i band magnitude "}, {"name": "e_imag", "desc": "Error in imag "}, {"name": "zmag", "desc": "SDSS-DR5 z band magnitude "}, {"name": "e_zmag", "desc": "Error in zmag "}, {"name": "z", "desc": "Photometric redshift "}, {"name": "e_z", "desc": "Error in z "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_716_398"}} {"id": "J/ApJ/716/398", "title_cds": "The 1998 november 14 Saturn occultation. I.", "title_create": "Harrington+, 2010", "year": "2010", "author": "Harrington J., French R.G.", "title_pub": "The 1998 november 14 occulaion of GSC 0622-00345 by Saturn. I. Techniques for ground-based stellar occultations", "first_author": "Harrington J.", "ref_biblio": [""], "bibcode": ["2010ApJ...716..398H"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Greg Schwarz [AAS], Emmanuelle Perret [CDS]", "doi_pub": ["10.1088/0004-637X/716/1/398"], "orcid_pub": ["0000-0002-8955-8531"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_750_90"}} {"id": "J/ApJ/750/90", "title_cds": "Short Title", "title_create": "Kucas+, 2012", "year": "2012", "author": "Kucas S., Karazija R., Momkauskaite A.", "title_pub": "Cascades after k-vacancy production in atoms and ions of light elements.", "first_author": "Kucas S.", "ref_biblio": [""], "bibcode": ["2012ApJ...750...90K"], "keyword_cds": "", "keyword_pub": "atomic data - atomic processes - radiation mechanisms: general - X-rays: general", "abstract": ["The results of detailed level-by-level calculations of Auger and", "radiative cascades after K-vacancy production are presented for the", "astrophysically important elements, namely Ne, Mg, Si, S, and Ar.", "Calculations are performed using the single-configuration,", "quasi-relativistic approximation. The whole isonuclear sequence of", "ions for a given element is considered. For the first time, the", "dependence of the cascade on the initial vacancy state is", "investigated. The populations are presented not only for the levels of", "the final configurations, but also for the levels of the excited", "configurations after the Auger transitions. An intense characteristic", "emission can be observed from such levels."], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/750/2/90"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_768_42"}} {"id": "J/ApJ/768/42", "title_cds": "Short Title", "title_create": "Cubillos+, 2013", "year": "2013", "author": "Cubillos P., Harrington J., Madhusudhan N., Stevenson K.B., Hardy R.A., Blecic J., Anderson D.R., Hardin M., Campo C.J.", "title_pub": "WASP-8b: characterization of a cool and eccentric exoplanet with Spitzer.", "first_author": "Cubillos P.", "ref_biblio": [""], "bibcode": ["2013ApJ...768...42C"], "keyword_cds": "", "keyword_pub": "planetary systems; stars: individual: WASP-8; techniques: photometric", "abstract": ["WASP-8b has 2.18 times Jupiter's mass and is on an eccentric (e=0.31)", "8.16 day orbit. With a time-averaged equilibrium temperature of 948K,", "it is one of the least-irradiated hot Jupiters observed with the", "Spitzer Space Telescope. We have analyzed six photometric light curves", "of WASP-8b during secondary eclipse observed in the 3.6, 4.5, and", "8.0um Infrared Array Camera bands. The eclipse depths are", "0.113%+/-0.018%, 0.069%+/-0.007%, and 0.093%+/-0.023%, respectively,", "giving respective brightness temperatures of 1552, 1131, and 938K. We", "characterized the atmospheric thermal profile and composition of the", "planet using a line-by-line radiative transfer code and a Markov-chain", "Monte Carlo sampler. The data indicated no thermal inversion,", "independently of any assumption about chemical composition. We noted", "an anomalously high 3.6{mu}m brightness temperature (1552K); by", "modeling the eccentricity-caused thermal variation, we found that this", "temperature is plausible for radiative timescales less than ~10^2^hr.", "However, as no model spectra fit all three data points well, the", "temperature discrepancy remains as an open question."], "object": [], "curator": "Greg Schwarz [AAS], Emmanuelle Perret [CDS]", "doi_pub": ["10.1088/0004-637X/768/1/42"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_779_5"}} {"id": "J/ApJ/779/5", "title_cds": "Short Title", "title_create": "Blecic+, 2013", "year": "2013", "author": "Blecic J., Harrington J., Madhusudhan N., Stevenson K.B., Hardy R.A., Cubillos P.E., Hardin M., Campo C.J., Bowman W.C., Nymeyer S., Loredo T.J., Anderson D.R., Maxted P.F.L.", "title_pub": "Thermal emission of WASP-14b revealed with three Spitzer eclipses.", "first_author": "Blecic J.", "ref_biblio": [""], "bibcode": ["2013ApJ...779....5B"], "keyword_cds": "", "keyword_pub": "eclipses; planets and satellites: atmospheres; planets and satellites: individual: WASP-14b; techniques: photometric", "abstract": ["Exoplanet WASP-14b is a highly irradiated, transiting hot Jupiter.", "Joshi et al. calculate an equilibrium temperature (T_eq_) of 1866K for", "zero albedo and reemission from the entire planet, a mass of 7.3+/-0.5", "Jupiter masses (M_J_), and a radius of 1.28+/-0.08 Jupiter radii", "(R_J_). Its mean density of 4.6g/cm3 is one of the highest known for", "planets with periods less than three days. We obtained three secondary", "eclipse light curves with the Spitzer Space Telescope. The eclipse", "depths from the best jointly fit model are 0.224%+/-0.018% at 4.5{mu}m", "and 0.181%+/-0.022% at 8.0{mu}m. The corresponding brightness", "temperatures are 2212+/-94K and 1590+/-116K. A slight ambiguity", "between systematic models suggests a conservative 3.6{mu}m eclipse", "depth of 0.19%+/-0.01% and brightness temperature of 2242+/-55K.", "Although extremely irradiated, WASP-14b does not show any distinct", "evidence of a thermal inversion. In addition, the present data", "nominally favor models with day-night energy redistribution less than", "~30%. The current data are generally consistent with oxygen-rich as", "well as carbon-rich compositions, although an oxygen-rich composition", "provides a marginally better fit. We confirm a significant", "eccentricity of e=0.087+/-0.002 and refine other orbital parameters."], "curator": "Greg Schwarz [AAS], Emmanuelle Perret [CDS]", "doi_pub": ["10.1088/0004-637X/779/1/5"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_781_116"}} {"id": "J/ApJ/781/116", "title_cds": "Short Title", "title_create": "Blecic+, 2014", "year": "2014", "author": "Blecic J., Harrington J., Madhusudhan N., Stevenson K.B., Hardy R.A., Cubillos P.E., Hardin M., Bowman O., Nymeyer S., Anderson D.R., Hellier C., Smith A.M.S., Cameron A.C.", "title_pub": "Spitzer observations of the thermal emission from WASP-43b.", "first_author": "Blecic J.", "ref_biblio": [""], "bibcode": ["2014ApJ...781..116B"], "keyword_cds": "", "keyword_pub": "eclipses - planets and satellites: atmospheres - planets and satellites: individual: WASP-43b - techniques: photometric", "abstract": ["WASP-43b is one of the closest-orbiting hot Jupiters, with a semimajor", "axis of a=0.01526+/-0.00018AU and a period of only 0.81days. However,", "it orbits one of the coolest stars with a hot Jupiter", "(T_*_=4520+/-120K), giving the planet a modest equilibrium temperature", "of T_eq_=1440+/-40K, assuming zero Bond albedo and uniform planetary", "energy redistribution. The eclipse depths and brightness temperatures", "from our jointly fit model are 0.347%+/-0.013% and 1670+/-23K at", "3.6{mu}m and 0.382%+/-0.015% and 1514+/-25K at 4.5{mu}m. The eclipse", "timings improved the estimate of the orbital period, P, by a factor of", "three (P=0.81347436+/-1.4x10^-7^days) and put an upper limit on the", "eccentricity (e=0.010_-0.007_^+0.010^). We use our Spitzer eclipse", "depths along with four previously reported ground-based photometric", "observations in the near-infrared to constrain the atmospheric", "properties of WASP-43b. The data rule out a strong thermal inversion", "in the dayside atmosphere of WASP-43b. Model atmospheres with no", "thermal inversions and fiducial oxygen-rich compositions are able to", "explain all the available data. However, a wide range of metallicities", "and C/O ratios can explain the data. The data suggest low day-night", "energy redistribution in the planet, consistent with previous studies,", "with a nominal upper limit of about 35% for the fraction of energy", "incident on the dayside that is redistributed to the nightside."], "description": ["We observed two secondary eclipses (on 2011 Jul 30 with channel", "1-3.6{mu}m, and on 2011 Jul 29 with channel 2-4.5{mu}m) of WASP-43b", "with the Spitzer IRAC camera in subarray mode (Program ID 70084)"], "object": [], "curator": "Sylvain Guehenneux [CDS]", "doi_pub": ["10.1088/0004-637X/781/2/116"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_786_133"}} {"id": "J/ApJ/786/133", "title_cds": "Short Title", "title_create": "Yu+, 2014", "year": "2014", "author": "Yu S., Pearson J.C.", "title_pub": "Terahertz measurements of the hot hydronium ion with an extended negative glow discharge.", "first_author": "Yu S.", "ref_biblio": [""], "bibcode": ["2014ApJ...786..133Y"], "keyword_cds": "", "keyword_pub": "ISM: molecules; line: identification; molecular data techniques: spectroscopic", "mission": "", "abstract": ["Terahertz absorption spectroscopy was employed to detect the ground-state inversion transitions of the hydronium ion (H_3_O^+^). The highly excited ions were created with an extended negative glow discharge through a gas mixture of 1 mtorr of H_2_O, 2 mtorr of H_2_, and 12 mtorr of Ar, which allowed observation of transitions with J and K up to 12. In total, 47 transitions were measured in the 0.9-2.0 THz region and 22 of these were observed for the first time. The experimental uncertainties range from 100 to 300 kHz, which are much better than the range 0.3-1.2 MHz reported in previous work. Differences of up to 25.6 MHz were found between the observed positions and the catalog values that have been used for Herschel data analysis of observations of Sagittarius B2(N), NGC 4418, and Arp 220. The new and improved measurements were fit to experimental accuracies with an updated Hamiltonian, and better H_3_O^+^ predictions are reported to support the proper analysis of astronomical observations by high-resolution", "spectroscopy telescopes, such as Herschel, SOFIA, and ALMA."], "object": [], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/786/2/133"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_787_166"}} {"id": "J/ApJ/787/166", "title_cds": "Short Title", "title_create": "Aliu+, 2014", "year": "2014", "author": "Aliu E., Archambault S., Aune T., Behera B., Beilicke M., Benbow W., Berger K., Bird R., Buckley J.H., Bugaev V., Cardenzana J.V., Cerruti M., Chen X., Ciupik L., Collins-hughes E., Connolly M.P., Cui W., Dumm J., Dwarkadas V.V., Errando M., Falcone A., Federici S., Feng Q., Finley J.P., Fleischhack H., Fortin P., Fortson L., Furniss A., Galante N., Gall D., Gillanders G.H., Griffin S., Griffiths S.T., Grube J., Gyuk G., Hanna D., Holder J., Hughes G., Humensky T.B., Kaaret P., Kertzman M., Khassen Y., Kieda D., Krennrich F., Kumar S., Lang M.J., Madhavan A.S., Maier G., Mccann A.J., Meagher K., Millis J., Moriarty P., Mukherjee R., Nieto D., De Bhroithe A.O., Ong R.A., Otte A.N., Pandel D., Park N., Pohl M., Popkow A., Prokoph H., Quinn J., Ragan K., Rajotte J., Ratliff G., Reyes L.C., Reynolds P.T., Richards G.T., Roache E., Rousselle J., Sembroski G.H., Shahinyan K., Sheidaei F., Smith A.W., Staszak D., Telezhinsky I., Tsurusaki K., Tucci J.V., Tyler J., Varlotta A., Vassiliev V.V., Vincent S., Wakely S.P., Ward J.E., Weinstein A., Welsing R., Wilhelm A.", "title_pub": "Investigating the TeV morphology of MGRO J1908+06 with VERITAS.", "first_author": "Aliu E.", "ref_biblio": [""], "bibcode": ["2014ApJ...787..166A"], "keyword_cds": "", "keyword_pub": "gamma rays: general gamma-ray burst: individual: (\\objac{@3946220}{MGRO J1908+06}{19 08 42.0000 +06 11 00.000},\\objac{@3946220}{VER J1907+062}{19 08 42.0000 +06 11 00.000}) pulsars: individual: \\objac{@2689987}{PSR J1907+0602}{19 07 54.7400 +06 02 16.900} ISM: supernova remnants", "mission": "", "abstract": ["We report on deep observations of the extended TeV gamma-ray source MGRO J1908+06 made with the VERITAS very high energy gamma-ray observatory. Previously, the TeV emission has been attributed to the pulsar wind nebula (PWN) of the Fermi-LAT pulsar PSR J1907+0602. We detect MGRO J1908+06 at a significance level of 14 standard deviations (14{sigma}) and measure a photon index of 2.20+/-0.10_stat_+/- 0.20_sys_. The TeV emission is extended, covering the region near PSR J1907+0602 and also extending toward SNR G40.5-0.5. When fitted with a two-dimensional Gaussian, the intrinsic extension has a standard deviation of {sigma}_src_= 0.{deg}44+/-0.{deg}02. In contrast to other TeV PWNe of similar age in which the TeV spectrum softens with distance from the pulsar, the TeV spectrum measured near the pulsar location is consistent with that measured at a position near the rim of G40.5-0.5, 0.{deg}33 away."], "object": [], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/787/2/166"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_793_127"}} {"id": "J/ApJ/793/127", "title_cds": "Short Title", "title_create": "Vogt+, 2014", "year": "2014", "author": "Vogt F.P.A., Dopita M.A., Kewley L.J., Sutherland R.S., Scharwachter J., Basurah H.M., Ali A., Amer M.A.", "title_pub": "Galaxy emission line classification using three-dimensional line ratio diagrams.", "first_author": "Vogt F.P.A.", "ref_biblio": [""], "bibcode": ["2014ApJ...793..127V"], "keyword_cds": "", "keyword_pub": "galaxies: abundances - galaxies: general - galaxies: Seyfert - galaxies: starburst - H II regions - ISM: lines and bands", "abstract": ["Two-dimensional (2D) line ratio diagnostic diagrams have become a key", "tool in understanding the excitation mechanisms of galaxies. The", "curves used to separate the different regions--H II-like or excited by", "an active galactic nucleus (AGN)--have been refined over time but the", "core technique has not evolved significantly. However, the", "classification of galaxies based on their emission line ratios really", "is a multi-dimensional problem. Here we exploit recent software", "developments to explore the potential of three-dimensional (3D) line", "ratio diagnostic diagrams. We introduce the ZQE diagrams, which are a", "specific set of 3D diagrams that separate the oxygen abundance and the", "ionization parameter of H II region-like spectra and also enable us to", "probe the excitation mechanism of the gas. By examining these new 3D", "spaces interactively, we define the ZE diagnostics, a new set of 2D", "diagnostics that can provide the metallicity of objects excited by hot", "young stars and that cleanly separate H II region-like objects from", "the different classes of AGNs. We show that these ZE diagnostics are", "consistent with the key log [N II]/H{alpha} versus log [O III]/H{beta}", "diagnostic currently used by the community. They also have the", "advantage of attaching a probability that a given object belongs to", "one class or the other. Finally, we discuss briefly why ZQE diagrams", "can provide a new way to differentiate and study the different classes", "of AGNs in anticipation of a dedicated follow-up study."], "curator": "Prepared by [AAS], Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/793/2/127"], "orcid_pub": ["0000-0002-9665-2788"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_794_145"}} {"id": "J/ApJ/794/145", "title_cds": "Short Title", "title_create": "Savcheva+, 2014", "year": "2014", "author": "Savcheva A.S., West A.A., Bochanski J.J.", "title_pub": "A new sample of cool subdwarfs from SDSS: properties and kinematics.", "first_author": "Savcheva A.S.", "ref_biblio": [""], "bibcode": ["2014ApJ...794..145S"], "keyword_cds": "", "keyword_pub": "stars: late-type; stars: low-mass; stars: statistics; subdwarfs", "mission": "", "abstract": ["We present a new sample of M subdwarfs compiled from the seventh data release of the Sloan Digital Sky Survey. With 3517 new subdwarfs, this new sample significantly increases the number of spectroscopically confirmed low-mass subdwarfs. This catalog also includes 905 extreme and 534 ultra sudwarfs. We present the entire catalog, including observed and derived quantities, and template spectra created from co-added subdwarf spectra. We show color-color and reduced proper motion diagrams of the three metallicity classes, which are shown to separate from the disk dwarf population. The extreme and ultra subdwarfs are seen at larger values of reduced proper motion, as expected for more dynamically heated populations. We determine 3D kinematics for all of the stars with proper motions. The color-magnitude diagrams show a clear separation of the three metallicity classes with the ultra and extreme subdwarfs being significantly closer to the main sequence than the ordinary subdwarfs. All subdwarfs lie below (fainter)", "and to the left (bluer) of the main sequence. Based on the average (U, V, W) velocities and their dispersions, the extreme and ultra subdwarfs likely belong to the Galactic halo, while the ordinary subdwarfs are likely part of the old Galactic (or thick) disk. An extensive activity analysis of subdwarfs is performed using H{alpha} emission, and 208 active subdwarfs are found. We show that while the activity fraction of subdwarfs rises with spectral class and levels off at the latest spectral classes, consistent with the behavior of M dwarfs, the extreme and ultra subdwarfs are basically flat."], "object": [], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/794/2/145"], "orcid_pub": ["0000-0002-5598-046X"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_794_165"}} {"id": "J/ApJ/794/165", "title_cds": "Short Title", "title_create": "Storm+, 2014", "year": "2014", "author": "Storm S., Mundy L.G., Fernandez-lopez M., Lee K.I., Looney L.W., Teuben P., Rosolowsky E., Arce H.G., Ostriker E.C., Segura-cox D.M., Pound M.W., Salter D.M., Volgenau N.H., Shirley Y.L., Chen C.-Y., Gong H., Plunkett A.L., Tobin J.J., Kwon W., Isella A., Kauffmann J., Tassis K., Crutcher R.M., Gammie C.F., Testi L.", "title_pub": "CARMA large area star formation survey: project overview with analysis of dense gas structure and kinematics in Barnard 1.", "first_author": "Storm S.", "ref_biblio": [""], "bibcode": ["2014ApJ...794..165S"], "keyword_cds": "", "keyword_pub": "ISM: clouds; ISM: kinematics and dynamics; ISM: molecules ISM: structure; stars: formation", "mission": "", "abstract": ["We present details of the CARMA Large Area Star Formation Survey (CLASSy), while focusing on observations of Barnard 1. CLASSy is a CARMA Key Project that spectrally imaged N_2_H^+^, HCO^+^, and HCN (J = 1 --> 0 transitions) across over 800 square arcminutes of the Perseus and Serpens Molecular Clouds. The observations have angular resolution near 7'' and spectral resolution near 0.16 km/s. We imaged ~150 square arcminutes of Barnard 1, focusing on the main core, and the B1 Ridge and clumps to its southwest. N_2_H^+^ shows the strongest emission, with morphology similar to cool dust in the region, while HCO^+^ and HCN trace several molecular outflows from a collection of protostars in the main core. We identify a range of kinematic complexity, with N_2_H^+^ velocity dispersions ranging from ~0.05 to 0.50 km/s across the field. Simultaneous continuum mapping at 3 mm reveals six compact object detections, three of which are new detections. A new, non-binary dendrogram algorithm is used to analyze", "dense gas structures in the N_2_H^+^ position-position-velocity (PPV) cube. The projected sizes of dendrogram-identified structures range from about 0.01 to 0.34 pc. Size-linewidth relations using those structures show that non-thermal line-of-sight velocity dispersion varies weakly with projected size, while rms variation in the centroid velocity rises steeply with projected size. Comparing these relations, we propose that all dense gas structures in Barnard 1 have comparable depths into the sky, around 0.1-0.2 pc; this suggests that overdense, parsec-scale regions within molecular clouds are better described as flattened structures rather than spherical collections of gas. Science-ready PPV cubes for Barnard 1 molecular emission are available for download."], "object": [], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/794/2/165"], "orcid_pub": ["0000-0001-9401-1357"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_797_42"}} {"id": "J/ApJ/797/42", "title_cds": "Short Title", "title_create": "Cubillos+, 2014", "year": "2014", "author": "Cubillos P., Harrington J., Madhusudhan N., Foster A.S.D., Lust N.B., Hardy R.A., Bowman M.O.", "title_pub": "A Spitzer five-band analysis of the jupiter-sized planet TrES-1.", "first_author": "Cubillos P.", "ref_biblio": [""], "bibcode": ["2014ApJ...797...42C"], "keyword_cds": "", "keyword_pub": "planetary systems - stars: individual: TrES-1 - techniques: photometric", "abstract": ["With an equilibrium temperature of 1200 K, TrES-1 is one of the", "coolest hot Jupiters observed by Spitzer. It was also the first planet", "discovered by any transit survey and one of the first exoplanets from", "which thermal emission was directly observed. We analyzed all Spitzer", "eclipse and transit data for TrES-1 and obtained its eclipse depths", "and brightness temperatures in the 3.6 {mu}m (0.083%+/-0.024%,", "1270+/-110 K), 4.5 {mu}m (0.094%+/-0.024%, 1126+/-90 K), 5.8 {mu}m", "(0.162%+/-0.042%, 1205+/-130 K), 8.0 {mu}m (0.213%+/-0.042%,", "1190+/-130 K), and 16 {mu}m (0.33%+/-0.12%, 1270+/-310 K) bands. The", "eclipse depths can be explained, within 1{sigma} errors, by a standard", "atmospheric model with solar abundance composition in chemical", "equilibrium, with or without a thermal inversion. The combined", "analysis of the transit, eclipse, and radial-velocity ephemerides", "gives an eccentricity of e = 0.033_-0.031_^+0.015^, consistent with a", "circular orbit. Since TrES-1's eclipses have low signal-to-noise", "ratios, we implemented optimal photometry and differential-evolution", "Markov Chain Monte Carlo (MCMC) algorithms in our Photometry for", "Orbits, Eclipses, and Transits pipeline. Benefits include higher", "photometric precision and ~10 times faster MCMC convergence, with", "better exploration of the phase space and no manual parameter tuning."], "object": ["19 04 09.84 +36 37 57.5 TrES-1 = NAME TrES-1b"], "curator": "Prepared by [AAS], Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1088/0004-637X/797/1/42"], "orcid_pub": ["0000-0002-1347-2600"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_81_187"}} {"id": "J/ApJ/81/187", "title_cds": "Spectral Types of 4179 stars", "title_create": "Adams+, 1935", "year": "1935", "author": "Adams W.S., Joy A.H., Humason M.L., Brayton A.M.", "title_pub": "The spectroscopic absolute magnitudes and parallaxes of 4179 stars.", "first_author": "Adams W.S.", "ref_biblio": [""], "bibcode": ["1935ApJ....81..187A"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/143628"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_827_52"}} {"id": "J/ApJ/827/52", "title_cds": "Census of YSOs in IC 348 and NGC 1333", "title_create": "Luhman+, 2016", "year": "2016", "author": "Luhman K.L., Esplin T.L., Loutrel N.P.", "title_pub": "A census of young stars and brown dwarfs in IC 348 and NGC 1333.", "first_author": "Luhman K.L.", "ref_biblio": [""], "bibcode": ["2016ApJ...827...52L"], "see_also": ["II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "J/AJ/150/175 : YSOVAR: infrared photometry in NGC 1333 (Rebull+, 2015)", "J/AJ/150/40 : The Spitzer c2d survey of clouds. XII. Perseus (Young+, 2015)", "J/ApJ/807/27 : IN-SYNC III. Radial velocities of IC348 stars (Cottaar+, 2015)", "J/ApJ/799/136 : IN-SYNC. II. Candidate young stars in NGC 1333 (Foster+, 2015)", "J/ApJ/787/107 : Spatial structure of young stellar clusters. I. (Kuhn+, 2014)", "J/ApJ/786/29 : Catalog of distances to molecular clouds (Schlafly+, 2014)", "J/MNRAS/437/906 : Cl* IC 348 H 254 VRI light curves (Ripepi+, 2014)", "J/MNRAS/434/806 : Pre-main-sequence isochrones. II. SFR (Bell+, 2013)", "J/AJ/145/66 : Spitzer light curves of YSOs in IC 348 (Flaherty+, 2013)", "J/ApJ/744/6 : SONYC census of very low-mass NGC1333 objects (Scholz+, 2012)", "J/A+A/537/A135 : X-ray view of IC348 (Stelzer+, 2012)", "J/AJ/140/1214 : NIR spectroscopic survey of class I YSOs (Connelley+, 2010)", "J/AJ/140/266 : NGC 1333 X-ray luminous YSOs properties (Winston+, 2010)", "J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)", "J/AJ/138/703 : Deep MIPS observations of IC 348 nebula (Currie+, 2009)", "J/ApJS/181/321 : Properties of Spitzer c2d dark clouds (Evans+, 2009)", "J/AJ/136/1372 : Very low-mass YSOs in NGC 1333 (Oasa+, 2008)", "J/ApJ/674/336 : Spitzer observations of NGC 1333 (Gutermuth+, 2008)", "J/ApJ/667/308 : Weak-line T Tauri in Spitzer c2d Survey. II. (Cieza+, 2007)", "J/AJ/134/411 : Properties of IC 348 members (Muench+, 2007)", "J/AJ/131/1574 : Infrared photometry of IC348 members (Lada+, 2006)", "J/AJ/127/1131 : NGC 1333 low-mass stars infrared photometry (Wilking+, 2004)", "J/ApJ/597/555 : IR photometry of IC 348 young brown dwarfs (Mainzer+, 2003)", "J/ApJ/593/1093 : IC 348 membership (Luhman+, 2003)", "J/A+A/401/543 : XMM-Newton observations of NGC 1333 (Preibisch, 2003)", "J/ApJ/575/354 : Young stellar objects in the NGC 1333 (Getman+, 2002)", "J/AJ/122/866 : X-ray sources in IC 348 from Chandra (Preibisch+, 2001)", "J/ApJ/541/977 : HST observations of low-mass stars in IC 348 (Najita+, 2000)", "J/ApJ/525/466 : Young low-mass stars & brown dwarfs in IC 348 (Luhman+, 1999)", "J/A+AS/137/305 : IC 348 proper motion catalogue (Scholz+, 1999)", "J/ApJ/497/736 : The young cluster IC 348. (Herbig, 1998)", "J/AJ/111/1964 : JHK photometry of NGC1333 (Lada+, 1996)", "J/A+AS/106/165 : Near-IR imaging photometry of NGC 1333 (Aspin+ 1994)"], "keyword_cds": "Clusters, open ; Spectra, infrared ; Photometry, infrared ; YSOs ; Cross identifications ; Proper motions ; Spectral types", "keyword_pub": "brown dwarfs; protoplanetary disks; stars: formation; stars: low-mass; stars: luminosity function, mass function; stars: pre-main sequence", "abstract": ["We have obtained optical and near-infrared spectra of candidate", "members of the star-forming clusters IC 348 and NGC 1333. We classify", "100 and 42 candidates as new members of the clusters, respectively,", "which brings the total numbers of known members to 478 and 203. We", "also have performed spectroscopy on a large majority of the previously", "known members of NGC 1333 in order to provide spectral classifications", "that are measured with the same scheme that has been applied to IC 348", "in previous studies. The new census of members is nearly complete for", "Ks<16.8 at A_J_<1.5 in IC 348 and for Ks<16.2 at A_J_<3 in NGC 1333,", "which correspond to masses of >~0.01M_{sun}_ for ages of 3Myr", "according to theoretical evolutionary models. The faintest known", "members extend below these completeness limits and appear to have", "masses of ~0.005M_{sun}_. In extinction-limited samples of cluster", "members, NGC 1333 exhibits a higher abundance of objects at lower", "masses than IC 348. It would be surprising if the initial mass", "functions of these clusters differ significantly given their similar", "stellar densities and formation environments. Instead, it is possible", "that average extinctions are lower for less massive members of", "star-forming clusters, in which case extinction-limited samples could", "be biased in favor of low-mass objects in the more heavily embedded", "clusters like NGC 1333. In the Hertzsprung-Russell diagram, the median", "sequences of IC 348 and NGC 1333 coincide with each other for the", "adopted distances of 300 and 235pc, which would suggest that they have", "similar ages. However, NGC 1333 is widely believed to be younger than", "IC 348 based on its higher abundance of disks and protostars and its", "greater obscuration. Errors in the adopted distances may be", "responsible for this discrepancy."], "description": ["We have made use of several X-ray to IR imaging surveys of IC 348 and", "NGC 1333 for identifying candidate members.", "See section 3.1 for the details.", "Unpublished images from WIRCam are also available for NGC 1333. We", "reduced all of the WIRCam images in JHKs that are available for IC 348", "and NGC 1333 from the CFHT archive, which were obtained through", "programs 07BH20 (K. Allers), 07BH12 (B. Biller), 09BD95 (L. Albert),", "O6BF23, 08BF98, and 09BF50 (J. Bouvier). The data from O6BF23 were", "those in IC 348 analyzed by Alves de Oliveira+ (2013A&A...549A.123A).", "We also reduced the Suprime-Cam images from Scholz+", "(2009ApJ...702..805S), which were retrieved from the Subaru Telescope", "data archive.", "We have obtained spectra of 152 candidate members of IC 348 and 16", "previously known members.", "We observed 130 sources with the near-IR spectrograph SpeX (R=150) at", "the NASA Infrared Telescope Facility (IRTF).", "We performed optical spectroscopy on 15 candidates (8 new members, 7", "non-members) and six known members (LRL 141, LRL 174, LRL 294, LRL", "334, LRL 366, LRL 10094) with the Inamori Magellan Areal Camera and", "Spectrograph (IMACS) on the Magellan I telescope at Las Campanas", "Observatory.", "We used the near-IR camera on the Keck I telescope (NIRC) to obtain", "low-resolution (~100) spectra of one candidate (LRL 6005) and two", "known members (LRL 1050, LRL 2103).", "We observed two and 12 candidates with the Gemini Near-Infrared Imager", "(NIRI, R=500) and the Gemini Near-Infrared Spectrograph (GNIRS, R=800),", "respectively, at the Gemini North telescope.", "In NGC 1333, we have performed spectroscopy on 55 candidate members", "and 124 known members with SpeX and 14 candidates with GNIRS.", "See section 4 for further details."], "type": ["OC"], "doi_pub": ["10.3847/0004-637X/827/1/52"], "orcid_pub": ["0000-0003-2822-2951"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Members of IC 348 ", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[42/45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31/32] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "---", "desc": "[LRL] "}, {"name": "LRL", "desc": "Name based on Luhman+ (1998ApJ...508..347L) running IDs (1)"}, {"name": "---", "desc": "<[EDJ2009] NNN> in Simbad "}, {"name": "[EDJ2009]", "desc": "? Name from Evans+ (2009, J/ApJS/181/321) "}, {"name": "---", "desc": "[CXOU] "}, {"name": "CXOU", "desc": "Name from Stelzer+ (2012, J/A+A/537/A135) "}, {"name": "A13", "desc": "Name from Alves de Oliveira+ (2013A&A...549A.123A)"}, {"name": "ONames", "desc": "Other source names "}, {"name": "SpT", "desc": "MK spectral type(s) "}, {"name": "r_SpT", "desc": "Spectral type reference (2) "}, {"name": "Spph", "desc": "Spectrograph for spectral classification (G2) "}, {"name": "Date", "desc": "Date of spectroscopy "}, {"name": "ASpT", "desc": "Adopted spectral type "}, {"name": "Aj", "desc": "[0/8]? Extinction in J band "}, {"name": "IRexc", "desc": "[yes/no ] IR excess? (3) "}, {"name": "pmRA", "desc": "[-3.5/9.4]? Proper motion in Right Ascension "}, {"name": "e_pmRA", "desc": "[0.1/6]? Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-7.9/2.6]? Proper motion in Declination "}, {"name": "e_pmDE", "desc": "[0.1/6.6]? Uncertainty in pmDE "}, {"name": "Jmag", "desc": "[6.7/20.5]? J magnitude "}, {"name": "e_Jmag", "desc": "[0.02/0.2]? Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[6.6/19]? H magnitude "}, {"name": "e_Hmag", "desc": "[0.02/0.08]? Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[6.5/18.6]? Ks magnitude "}, {"name": "e_Ksmag", "desc": "[0.01/0.2]? Uncertainty in Ksmag "}, {"name": "Ref", "desc": "JHK references (G3) "}]}, {"name": "table2.dat", "desc": "Members of NGC 1333 ", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[28/30] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[30/31] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "S74", "desc": "Name from Strom+ (1974ApJ...191..111S) "}, {"name": "---", "desc": "[ASR] "}, {"name": "ASR", "desc": "? Name from Aspin+ (1994, J/A+AS/106/165) "}, {"name": "---", "desc": "<[LAL96] NNN> in Simbad "}, {"name": "[LAL96]", "desc": "? Name from Lada+ (1996, J/AJ/111/1964) "}, {"name": "---", "desc": "<[GFT2002] NNN> in Simbad "}, {"name": "[GFT2002]", "desc": "? Name from Getman+ (2002, J/ApJ/575/354) "}, {"name": "---", "desc": "[MBO] "}, {"name": "MBO", "desc": "? Name from Wilking+ (2004, J/AJ/127/1131) "}, {"name": "---", "desc": "<[GMM2008] NNN> in Simbad "}, {"name": "[GMM2008]", "desc": "? Name from Gutermuth+ (2008, J/ApJ/674/336) "}, {"name": "---", "desc": "<[OTS2008]> in Simbad "}, {"name": "[OTS2008]", "desc": "Name(s) from Oasa+ (2008, J/AJ/136/1372) "}, {"name": "---", "desc": "<[EDJ2009] NNN> in Simbad "}, {"name": "[EDJ2009]", "desc": "? Name from Evans+ (2009, J/ApJS/181/321) "}, {"name": "S09", "desc": "Name from Scholz+ (2009ApJ...702..805S) "}, {"name": "---", "desc": "<[WMW2010] NNN> in Simbad "}, {"name": "[WMW2010]", "desc": "? Name from Winston+ (2010, J/AJ/140/266) "}, {"name": "---", "desc": "[SSTYSV] "}, {"name": "SSTYSV", "desc": "Name from Rebull+ (2015, J/AJ/150/175) "}, {"name": "ONames", "desc": "Other source names "}, {"name": "SpT", "desc": "MK spectral type(s) "}, {"name": "r_SpT", "desc": "Spectral type reference (1) "}, {"name": "Spph", "desc": "Spectrograph for spectral classification (G2) "}, {"name": "Date", "desc": "Date of spectroscopy "}, {"name": "ASpT", "desc": "Adopted spectral type "}, {"name": "Aj", "desc": "[0/14]? Extinction in J band "}, {"name": "IRexc", "desc": "IR excess? (2) "}, {"name": "MmEv", "desc": "Membership evidence (3) "}, {"name": "pmRA", "desc": "[-8.9/8.4]? Proper motion in right ascension "}, {"name": "e_pmRA", "desc": "[0/6.8]? Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-7.8/3.4]? Proper motion in declination "}, {"name": "e_pmDE", "desc": "[0/7.4]? Uncertainty in pmDE "}, {"name": "Jmag", "desc": "[8.1/20.8]? J magnitude "}, {"name": "e_Jmag", "desc": "[0.02/0.2]? Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[7.7/19.1]? H magnitude "}, {"name": "e_Hmag", "desc": "[0.02/0.08]? Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[7.1/18.2]? Ks magnitude "}, {"name": "e_Ksmag", "desc": "[0.02/0.2]? Uncertainty in Ksmag "}, {"name": "Ref", "desc": "JHK reference (G3) "}]}, {"name": "table3.dat", "desc": "Field stars in spectroscopic samples for IC 348 and NGC 1333", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[28/45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31/32] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Flag", "desc": "[y] Proper Motion Flag (1) "}, {"name": "SpT", "desc": "MK Spectral Type(s) "}, {"name": "r_SpT", "desc": "Spectral type reference(s) (2) "}, {"name": "Inst", "desc": "Telescope/Instrument "}, {"name": "Date", "desc": "Date of spectroscopy "}]}, {"name": "table4.dat", "desc": "Candidate members of IC 348 ", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[43/45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31/32] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "L98", "desc": "[596/54532] Name based on Luhman+ (1998ApJ...508..347L) running IDs; in Simbad"}, {"name": "Select", "desc": "Basis of Selection (1) "}, {"name": "Jmag", "desc": "[18.4/20.8]? WIRCam J magnitude, this work "}, {"name": "e_Jmag", "desc": "[0.03/0.07]? Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[16.4/19.8] WIRCam H magnitude, this work "}, {"name": "e_Hmag", "desc": "[0.03/0.1] Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[14.8/18.5] WIRCam Ks magnitude, this work "}, {"name": "e_Ksmag", "desc": "[0.03/0.04] Uncertainty in Ksmag "}]}, {"name": "table5.dat", "desc": "Candidate Members of NGC 1333 ", "columns": [{"name": "Name", "desc": "Source name (G1) "}, {"name": "RAh", "desc": "[3] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[28/29] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[12/29] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "S74", "desc": "Name from Strom+ (1974ApJ...191..111S) "}, {"name": "---", "desc": "[ASR] "}, {"name": "ASR", "desc": "? Name from Aspin+ (1994, J/A+AS/106/165) "}, {"name": "---", "desc": "<[LAL96] NNN> in Simbad "}, {"name": "[LAL96]", "desc": "? Name from Lada+ (1996, J/AJ/111/1964) "}, {"name": "---", "desc": "[MBO] "}, {"name": "MBO", "desc": "? Name from Wilking+ (2004, J/AJ/127/1131) "}, {"name": "---", "desc": "<[GMM2008] NNN> in Simbad "}, {"name": "[GMM2008]", "desc": "? Name from Gutermuth+ (2008, J/ApJ/674/336) "}, {"name": "---", "desc": "<[OTS2008] NNN> in Simbad "}, {"name": "[OTS2008]", "desc": "? Name from Oasa+ (2008, J/AJ/136/1372) "}, {"name": "---", "desc": "<[EDJ2009] NNN> in Simbad "}, {"name": "[EDJ2009]", "desc": "? Name from Evans+ (2009, J/ApJS/181/321) "}, {"name": "---", "desc": "<[WMW2010] NNN> in Simbad "}, {"name": "[WMW2010]", "desc": "? Name from Winston+ (2010, J/AJ/140/266) "}, {"name": "---", "desc": "[SSTYSV] "}, {"name": "SSTYSV", "desc": "Name from Rebull+ (2015, J/AJ/150/175) "}, {"name": "Select", "desc": "Basis of selection (1) "}, {"name": "Jmag", "desc": "[11.2/21.6]? J magnitude "}, {"name": "e_Jmag", "desc": "[0.02/0.2]? Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[10.1/19.7]? H magnitude "}, {"name": "e_Hmag", "desc": "[0.03/0.2]? Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[9.5/19] Ks magnitude "}, {"name": "e_Ksmag", "desc": "[0.02/0.04] Uncertainty in Ksmag "}, {"name": "Ref", "desc": "JHK reference (G3) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_829_89"}} {"id": "J/ApJ/829/89", "title_cds": "Short Title", "title_create": "Barnes+, 2016", "year": "2016", "author": "Barnes G., Leka K.D., Schrijver C.J., Colak T., Qahwaji R., Ashamari O.W., Yuan Y., Zhang J., McAteer R.T.J., Bloomfield D.S., Higgins P.A., Gallagher P.T., Falconer D.A., Georgoulis M.K., Wheatland M.S., Balch C., Dunn T., Wagner E.L.", "title_pub": "A comparison of flare forecasting methods. I. Results from the \"all-clear\" workshop.", "first_author": "Barnes G.", "ref_biblio": [""], "bibcode": ["2016ApJ...829...89B"], "keyword_cds": "", "keyword_pub": "methods: statistical; Sun: flares; Sun: magnetic fields", "abstract": ["Solar flares produce radiation that can have an almost immediate", "effect on the near-Earth environment, making it crucial to forecast", "flares in order to mitigate their negative effects. The number of", "published approaches to flare forecasting using photospheric magnetic", "field observations has proliferated, with varying claims about how", "well each works. Because of the different analysis techniques and data", "sets used, it is essentially impossible to compare the results from", "the literature. This problem is exacerbated by the low event rates of", "large solar flares. The challenges of forecasting rare events have", "long been recognized in the meteorology community, but have yet to be", "fully acknowledged by the space weather community. During the", "interagency workshop on \"all clear\" forecasts held in Boulder, CO in", "2009, the performance of a number of existing algorithms was compared", "on common data sets, specifically line-of-sight magnetic field and", "continuum intensity images from the Michelson Doppler Imager, with", "consistent definitions of what constitutes an event. We demonstrate", "the importance of making such systematic comparisons, and of using", "standard verification statistics to determine what constitutes a good", "prediction scheme. When a comparison was made in this fashion, no one", "method clearly outperformed all others, which may in part be due to", "the strong correlations among the parameters used by different methods", "to characterize an active region. For M-class flares and above, the", "set of methods tends toward a weakly positive skill score (as measured", "with several distinct metrics), with no participating method proving", "substantially better than climatological forecasts."], "doi_pub": ["10.3847/0004-637X/829/2/89"], "orcid_pub": ["0000-0003-3571-8728"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "27769.dat", "desc": "Forecasts for events with at least one C1.0 or greater flare within 24hr after the observation", "columns": [{"name": "ID", "desc": "Identifier of the data source: date, time, number of active regions and active region number"}, {"name": "Event", "desc": "yes=1, no=0 "}, {"name": "MCD1", "desc": "Part of Maximum Common Dataset #1: yes=1,no=0 "}, {"name": "MCD2", "desc": "Part of Maximum Common Dataset #2: yes=1,no=0 "}, {"name": "Beff", "desc": "Forecast probability for B_eff "}, {"name": "ASAP", "desc": "Forecast probability for ASAP "}, {"name": "BBSO", "desc": "Forecast probability for BBSO "}, {"name": "WLSG2", "desc": "? Forecast probability for WL_SG2 (blank value when NaN)"}, {"name": "NWRAMAG", "desc": "Forecast probability for NWRA MAG 2-var "}, {"name": "log(R)", "desc": "Forecast probability for log(R) "}, {"name": "GCD", "desc": "Forecast probability for GCD "}, {"name": "NWRAMCT", "desc": "Forecast probability for NWRA MCT 2-var "}, {"name": "SMART2", "desc": "Forecast probability for SMART2 "}, {"name": "EventS", "desc": "Forecast probability for Event Statistics, 10 prior"}, {"name": "McIntosh", "desc": "? Forecast probability for McIntosh (blank value when NaN)"}]}, {"name": "27825.dat", "desc": "Forecasts for events with at least one M1.0 or greater flare within 12hr after the observation", "columns": [{"name": "ID", "desc": "Identifier of the data source: date, time, number of active regions and active region number"}, {"name": "Event", "desc": "yes=1, no=0 "}, {"name": "MCD1", "desc": "Part of Maximum Common Dataset #1: yes=1,no=0 "}, {"name": "MCD2", "desc": "Part of Maximum Common Dataset #2: yes=1,no=0 "}, {"name": "Beff", "desc": "Forecast probability for B_eff "}, {"name": "ASAP", "desc": "Forecast probability for ASAP "}, {"name": "BBSO", "desc": "Forecast probability for BBSO "}, {"name": "WLSG2", "desc": "? Forecast probability for WL_SG2 (blank value when NaN)"}, {"name": "NWRAMAG", "desc": "Forecast probability for NWRA MAG 2-var "}, {"name": "log(R)", "desc": "Forecast probability for log(R) "}, {"name": "GCD", "desc": "Forecast probability for GCD "}, {"name": "NWRAMCT", "desc": "Forecast probability for NWRA MCT 2-var "}, {"name": "SMART2", "desc": "Forecast probability for SMART2 "}, {"name": "EventS", "desc": "Forecast probability for Event Statistics, 10 prior"}, {"name": "McIntosh", "desc": "? Forecast probability for McIntosh (blank value when NaN)"}]}, {"name": "27847.dat", "desc": "Forecasts for events with at least one M5.0 or greater flare within 12hr after the observation", "columns": [{"name": "ID", "desc": "Identifier of the data source: date, time, number of active regions and active region number"}, {"name": "Event", "desc": "yes=1, no=0 "}, {"name": "MCD1", "desc": "Part of Maximum Common Dataset #1: yes=1,no=0 "}, {"name": "MCD2", "desc": "Part of Maximum Common Dataset #2: yes=1,no=0 "}, {"name": "Beff", "desc": "Forecast probability for B_eff "}, {"name": "ASAP", "desc": "Forecast probability for ASAP "}, {"name": "BBSO", "desc": "Forecast probability for BBSO "}, {"name": "WLSG2", "desc": "? Forecast probability for WL_SG2 (blank value when NaN)"}, {"name": "NWRAMAG", "desc": "Forecast probability for NWRA MAG 2-var "}, {"name": "log(R)", "desc": "Forecast probability for log(R) "}, {"name": "GCD", "desc": "Forecast probability for GCD "}, {"name": "NWRAMCT", "desc": "Forecast probability for NWRA MCT 2-var "}, {"name": "SMART2", "desc": "Forecast probability for SMART2 "}, {"name": "EventS", "desc": "Forecast probability for Event Statistics, 10 prior"}, {"name": "McIntosh", "desc": "? Forecast probability for McIntosh (blank value when NaN)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_833_58"}} {"id": "J/ApJ/833/58", "title_cds": "Short Title", "title_create": "Hodges-Kluck+, 2016", "year": "2016", "author": "Hodges-Kluck E., Cafmeyer J., Bregman J.N.", "title_pub": "Ultraviolet halos around spiral galaxies. I. Morphology.", "first_author": "Hodges-Kluck E.", "ref_biblio": [""], "bibcode": ["2016ApJ...833...58H"], "keyword_cds": "", "keyword_pub": "dust, extinction; galaxies: halos; ultraviolet: galaxies", "abstract": ["We examine ultraviolet halos around a sample of highly inclined", "galaxies within 25 Mpc to measure their morphology and luminosity.", "Despite contamination from galactic light scattered into the wings of", "the point-spread function, we find that ultraviolet (UV) halos occur", "around each galaxy in our sample. Around most galaxies the halos form", "a thick, diffuse disk-like structure, but starburst galaxies with", "galactic superwinds have qualitatively different halos that are more", "extensive and have filamentary structure. The spatial coincidence of", "the UV halos above star-forming regions, the lack of consistent", "association with outflows or extraplanar ionized gas, and the strong", "correlation between the halo and galaxy UV luminosity suggest that the", "UV light is an extragalactic reflection nebula. UV halos may thus", "represent 10^6^-10^7^M_{sun}_ of dust within 2-10kpc of the disk,", "whose properties may change with height in starburst galaxies."], "doi_pub": ["10.3847/1538-4357/833/1/58"], "orcid_pub": ["0000-0002-2397-206X"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table9.dat", "desc": "Swift Mrk 501 observations ", "columns": [{"name": "uvm2", "desc": "Swift/UVOT uvm2 band observation identifier "}, {"name": "uvw1", "desc": "Swift/UVOT uvw1 band observation identifier "}, {"name": "uvw2", "desc": "Swift/UVOT uvw2 band observation identifier "}]}, {"name": "table10.dat", "desc": "All Swift and GALEX observations ", "columns": [{"name": "Name", "desc": "Galaxy identifier "}, {"name": "FUV", "desc": "GALEX/FUV observation identifier "}, {"name": "NUV", "desc": "GALEX/NUV observation identifier "}, {"name": "uvm2", "desc": "Swift/UVOT uvm2 band observation identifier "}, {"name": "uvw1", "desc": "Swift/UVOT uvw1 band observation identifier "}, {"name": "uvw2", "desc": "Swift/UVOT uvw2 band observation identifier "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_839_20"}} {"id": "J/ApJ/839/20", "title_cds": "Spectroscopy of stars along the LoS of Crater2", "title_create": "Caldwell+, 2017", "year": "2017", "author": "Caldwell N., Walker M.G., Mateo M., Olszewski E.W., Koposov S., Belokurov V., Torrealba G., Geringer-sameth A., Johnson C.I.", "title_pub": "Crater 2: an extremely cold dark matter halo.", "first_author": "Caldwell N.", "ref_biblio": [""], "bibcode": ["2017ApJ...839...20C"], "see_also": ["J/A+A/459/423 : VI and [Fe/H] of Fornax dSph RGB stars (Battaglia+, 2006)", "J/MNRAS/380/281 : Faint galactic satellites spectrosc. survey (Martin+, 2007)", "J/AJ/136/2050 : SEGUE stellar parameter pipeline. II. (Lee+, 2008)", "J/ApJ/675/201 : Radial velocities of stars near Leo I (Mateo+, 2008)", "J/MNRAS/397/1748 : Spectroscopic study of Segue 2 (Belokurov+, 2009)", "J/AJ/137/94 : Star clusters in M31 (Caldwell+, 2009)", "J/AJ/137/3100 : Radial velocities of 4 dSph galaxies (Walker+, 2009)", "J/ApJ/694/L144 : Spectroscopic study of Leo V dSph (Walker+, 2009)", "J/ApJS/191/352 : Abundances in stars of MW dwarf satellites (Kirby+, 2010)", "J/ApJ/736/146 : Radial velocities of stars in Bootes I (Koposov+, 2011)", "J/ApJ/733/46 : Velocity measurements in Segue 1 (Simon+, 2011)", "J/AJ/144/4 : Dwarf galaxies in the Local Group (McConnachie+, 2012)", "J/ApJ/768/172 : Kinematic analysis of red giant in M31 dSphs (Collins+, 2013)", "J/ApJ/779/102 : Metallicities of RGB stars in dwarf galaxies (Kirby+, 2013)", "J/ApJ/801/74 : Dark matter profiles in dwarf gal. (Geringer-Sameth+, 2015)", "J/MNRAS/448/2717 : Bayesian analysis of resolved stellar spectra", "J/MNRAS/453/690 : Fornax VST ATLAS catalogue (Bate+, 2015)", "J/MNRAS/469/621 : VST ATLAS white dwarf candidates (Gentile Fusillo+, 2017)", "http://astro.dur.ac.uk/Cosmology/vstatlas/ : VST ATLAS survey home page"], "keyword_cds": "Stars, giant ; Photometry, SDSS ; Abundances, [Fe/H]", "keyword_pub": "galaxies: dwarf; galaxies: individual (Crater 2); galaxies: kinematics and dynamics; Local Group; methods: data analysis techniques: spectroscopic", "abstract": ["We present results from MMT/Hectochelle spectroscopy of 390 red giant", "candidate stars along the line of sight to the recently discovered", "Galactic satellite Crater 2. Modeling the joint distribution of", "stellar positions, velocities, and metallicities as a mixture of", "Crater 2 and Galactic foreground populations, we identify ~62 members", "of Crater 2, for which we resolve a line-of-sight velocity dispersion", "of {sigma}_Vlos_=2.7_-0.3_^+0.3^km/s and a mean velocity of", "=87.5_-0.4_^+0.4^km/s (solar rest frame). We also resolve a", "metallicity dispersion of {sigma}_[Fe/H]_=0.22_-0.03_^+0.04^dex and a", "mean of <[Fe/H]>=-1.98_-0.1_^+0.1^dex that is 0.28+/-0.14dex poorer", "than estimated from photometry. Despite Crater 2's relatively large", "size (projected halflight radius R_h_~1kpc) and intermediate", "luminosity (M_V_~-8), its velocity dispersion is the coldest that has", "been resolved for any dwarf galaxy. These properties make Crater 2 the", "most extreme low-density outlier in dynamical as well as structural", "scaling relations among the Milky Way's dwarf spheroidals. Even so,", "under assumptions of dynamical equilibrium and negligible", "contamination by unresolved binary stars, the observed velocity", "distribution implies a gravitationally dominant dark matter halo, with", "a dynamical mass of 4.4_-0.9_^+1.2^x10^6^M_{sun}_ and a mass-to-light", "ratio of 53_-11_^+15^M_{sun}_/L_V,{sun}_ enclosed within a radius of", "~1kpc, where the equivalent circular velocity is 4.3_-0.5_^+0.5^ km/s."], "description": ["We observed Crater 2 using the Hectochelle multi-object fiber", "spectrograph on the 6.5m MMT on Mt. Hopkins, Arizona.", "On the nights of 2016 April 27 and 30 and May 11, we used", "Hectochelle's \"RV31\" filter to observe the spectral range of", "5150-5300{AA}. The effective resolution is R~32000.", "We selected red giant branch (RGB) candidates from the photometric", "catalog provided by the VLT Survey Telescope (VST) ATLAS survey", "(Shanks+ 2015MNRAS.451.4238S)."], "object": ["11 49 14 -18 24.8 Crater 2 = NAME Crater 2 (=87.5km/s)"], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aa688e"], "orcid_pub": ["0000-0003-2352-3202"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "Hectochelle Stellar Spectroscopy of Crater 2 ", "columns": [{"name": "ID", "desc": "Object identifier (Cra2-NNN) "}, {"name": "RAh", "desc": "[11] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[46/55] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[17/18] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "gmag", "desc": "[17/20.3] The g band magnitude from the VST-ATLAS catalog (SDSS AB system??)"}, {"name": "imag", "desc": "[16/20.1] The i band magnitude from the VST-ATLAS catalog (SDSS AB system??)"}, {"name": "HJD", "desc": "Heliocentric Julian Date; JD-2450000 "}, {"name": "S/N", "desc": "[0.2/18.1] Median signal-to-Noise per pixel "}, {"name": "Vlos", "desc": "[-73/370] Heliocentric rest frame line-of-sight velocity"}, {"name": "e_Vlos", "desc": "[0.3/4] Uncertainty in vlos "}, {"name": "Teff", "desc": "[4428/7309] Effective temperature "}, {"name": "e_Teff", "desc": "[25/1085] Uncertainty in Teff "}, {"name": "log(g)", "desc": "[1/6] Log surface gravity "}, {"name": "e_log(g)", "desc": "[0.06/1.4] Uncertainty in log(g) "}, {"name": "[Fe/H]", "desc": "[-3.2/1.4] Metallicity "}, {"name": "e_[Fe/H]", "desc": "[0.04/1.1] Uncertainty in [Fe/H] "}]}, {"name": "spectra.dat", "desc": "Summary of individual spectroscopic targets; table added by CDS", "columns": [{"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "FileName", "desc": "Name of the FITS file in subdirectory spectra "}]}, {"name": "spectra/*", "desc": "Individual fits files for all individual spectroscopic targets (and \"README\" file)", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_839_6"}} {"id": "J/ApJ/839/6", "title_cds": "NGC 6946 giant molecular cloud in ^12^CO (2-1)", "title_create": "Wu+, 2017", "year": "2017", "author": "Wu Y.-L., Sakamoto K., Pan H.-A.", "title_pub": "Submillimeter Array ^12^CO (2-1) imaging of the NGC 6946 giant molecular clouds.", "first_author": "Wu Y.-L.", "ref_biblio": [""], "bibcode": ["2017ApJ...839....6W"], "see_also": ["J/ApJ/551/852 : FCRAO CO survey of the outer Galaxy (Heyer+, 2001)", "J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)", "J/ApJ/661/830 : Giant molecular clouds of M33 (Rosolowsky+, 2007)", "J/ApJ/669/525 : VRI photometric standards for NGC 6946 (Welch+, 2007)", "J/ApJ/686/948 : CO in extragalactic giant molecular clouds (Bolatto+, 2008)", "J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008)", "J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008)", "J/ApJS/177/465 : X-ray variability in NGC 6946, NGC4485/90 (Fridriksson+, 2008)", "J/ApJ/699/1092 : Giant molecular clouds (SRBY) (Heyer+, 2009)", "J/ApJS/197/16 : CO observations of LMC molecular clouds (MAGMA). (Wong+, 2011)", "J/A+A/542/A108 : Giant molecular clouds in M33 (Gratier+, 2012)", "J/A+A/545/A43 : HII regions in NGC 628 and NGC 6946 (Cedres+, 2012)", "J/A+A/552/A19 : Radio-farIR correlation in NGC 6946 (Tabatabaei+, 2013)", "J/ApJ/772/107 : GMCs in nearby galaxies (Donovan Meyer+, 2013)", "J/ApJ/784/3 : The PAWS catalogs of GMCs and islands in M51 (Colombo+, 2014)", "J/ApJ/803/16 : GMCs in NGC4526 based on ^12^CO (Utomo+, 2015)"], "keyword_cds": "Molecular clouds ; Interstellar medium ; Millimetric/submm sources", "keyword_pub": "galaxies: individual (NGC 6946); galaxies: ISM; galaxies: spiral; ISM: clouds", "abstract": ["We present a ^12^CO (2-1) mosaic map of the spiral galaxy NGC 6946 by", "combining data from the Submillimeter Array and the IRAM 30m", "telescope. We identify 390 giant molecular clouds (GMCs) from the", "nucleus to 4.5kpc in the disk. GMCs in the inner 1kpc are generally", "more luminous and turbulent, some of which have luminosities", ">10^6^K.km/s.pc^2^ and velocity dispersions >10km/s. Large-scale", "bar-driven dynamics likely regulate GMC properties in the nuclear", "region. Similar to the Milky Way and other disk galaxies, GMC mass", "function of NGC 6946 has a shallower slope (index > -2) in the inner", "region, and a steeper slope (index < -2) in the outer region. This", "difference in mass spectra may be indicative of different cloud", "formation pathways: gravitational instabilities might play a major", "role in the nuclear region, while cloud coalescence might be dominant", "in the outer disk. Finally, the NGC 6946 clouds are similar to those", "in M33 in terms of statistical properties, but they are generally less", "luminous and turbulent than the M51 clouds."], "description": ["We performed a 10-pointing ^12^CO(2-1) mosaic of NGC 6946 between 2010", "June and October in the compact (CMP) and extended (EXT) array", "configurations of the Submillimeter Array (SMA), with baselines", "ranging from 6 to 180m. We also acquired complementary data with the", "sub-compact configuration (SUB) in 2012.", "We also use the IRAM 30m ^12^CO(2-1) cube of NGC 6946 presented by", "Leroy+ (2009AJ....137.4670L)."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aa68de"], "orcid_pub": ["0000-0002-4392-1446"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table3.dat", "desc": "NGC 6946 giant molecular cloud catalog ", "columns": [{"name": "Seq", "desc": "Cloud ID "}, {"name": "oRA", "desc": "Right Ascension offset w.r.t. the galactic center (1)"}, {"name": "oDE", "desc": "Declination offset w.r.t. the galactic center (1)"}, {"name": "Velc", "desc": "[-48/174] Central velocity of the cloud "}, {"name": "Rad", "desc": "[13/213] Cloud radius "}, {"name": "e_Rad", "desc": "[6/154] Uncertainty in cloud radius "}, {"name": "sigv", "desc": "[0.5/42.5] Velocity dispersion "}, {"name": "e_sigv", "desc": "[0.5/55] Uncertainty in sigv "}, {"name": "Lum", "desc": "[1.6/702] Luminosity "}, {"name": "e_Lum", "desc": "[0.7/1912] Uncertainty in luminosity "}, {"name": "Mlum", "desc": "[0.2/40.2] Luminosity mass (2) "}, {"name": "e_Mlum", "desc": "[0.1/110] Uncertainty in luminosity mass "}, {"name": "Mvir", "desc": "[0.1/1517] Virial mass "}, {"name": "e_Mvir", "desc": "[0.3/1684] Uncertainty in virial mass "}, {"name": "T", "desc": "[1.7/18.1] Peak temperature "}, {"name": "S/N", "desc": "[5/55] Signal-to-noise ratio "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_847_20"}} {"id": "J/ApJ/847/20", "title_cds": "GMOS spectrosc. obs. of 0.3"], "bibcode": ["2017ApJ...847...20W"], "see_also": ["J/ApJS/94/687 : Old stellar populations. V. (Worthey+, 1994)", "J/MNRAS/276/1341 : Spectroscopy of E and S0 galaxies (Jorgensen+, 1995)", "J/ApJS/111/377 : H{gamma} & H{delta} absorption features (Worthey+ 1997)", "J/A+A/432/381 : VLT spectroscopic survey of RX J0152.7-1357 (Demarco+, 2005)", "J/ApJ/621/673 : Line indices for 124 early-type galaxies (Thomas+, 2005)", "J/ApJ/633/174 : Spheroidals and bulge dominated galaxies (Treu+, 2005)", "J/AJ/131/1288 : Composite spectra of early-type galaxies (Bernardi+, 2006)", "J/MNRAS/382/109 : Massive galaxies in Extended Groth Strip (Trujillo+, 2007)", "J/ApJS/184/271 : Photometry of galaxies in 3 clusters (Chiboucas+, 2009)", "J/ApJ/725/1252 : Confirmed members of RX J0152.7-1357 (Demarco+, 2010)", "J/A+A/524/A6 : Evolution of spectral early-type galaxies (Saglia+, 2010)", "J/AJ/145/77 : Imaging & spectrosc. in 3 galaxy clusters (Jorgensen+, 2013)", "J/ApJ/788/72 : Observed sample of z~0.7 massive galaxies (Gallazzi+, 2014)", "J/AJ/148/117 : Imaging and spectroscopy in Lynx W (Jorgensen+, 2014)", "J/A+A/597/A122 : Cluster & field elliptical gal. at z~1.3 (Saracco+, 2017)"], "keyword_cds": "Galaxies, spectra ; Redshifts ; Velocity dispersion ; Optical ; Equivalent widths", "keyword_pub": "galaxies: evolution ; galaxies: stellar content", "abstract": ["We analyze the stellar populations and evolutionary history of", "bulge-dominated field galaxies at redshifts 0.3"], "bibcode": ["2017ApJ...850...89G"], "see_also": ["B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)", "J/MNRAS/372/1315 : UBVRI photometry of SN 2004et (Sahu+, 2006)", "J/MNRAS/394/2266 : SN 2005cs one-year photometry (Pastorello+, 2009)", "J/MNRAS/395/1409 : Type II-P SN progenitor constraints (Smartt+, 2009)", "J/ApJ/708/661 : SDSS-II SN Survey: SN.II-P standardization (D'Andrea+, 2010)", "J/AJ/139/519 : Carnegie supernova project. SNe Ia (Contreras+, 2010)", "J/AJ/139/120 : Low-redshift Type-Ia supernovae (Folatelli+, 2010)", "J/AJ/142/156 : The CSP (DR2): photometry of SNe Ia (Stritzinger+, 2011)", "J/MNRAS/433/1871 : UBVRI griz light curves of SN 2012aw (Bose+, 2013)", "J/ApJ/773/53 : Type Ia SNe spectroscopy by the CSP (Folatelli+, 2013)", "J/ApJ/763/42 : X-ray emission from 28 SNe (IIn, Ibn, SLSN-I) (Ofek+, 2013)", "J/A+A/555/A142 : Spectra of 5 Type II supernovae (Inserra+, 2013)", "J/A+A/559/A114 : Updated O3N2 and N2 abundance indicators (Marino+, 2013)", "J/A+A/555/A10 : Light curves of 5 type IIn supernovae (Taddia+, 2013)", "J/MNRAS/442/844 : BVRI light curves of type II-P supernovae (Faran+, 2014)", "J/MNRAS/438/L101 : First month on SN 2013ej (Valenti+, 2014)", "J/ApJ/788/154 : Palomar Transient Factory SNe IIn photometry (Ofek+, 2014)", "J/ApJ/789/104 : SNe IIn observations and properties (Ofek+, 2014)", "J/ApJ/799/208 : Type IIP supernovae from Pan-STARRS1 (Sanders+, 2015)", "J/ApJ/799/215 : 26 type II-Plateau supernovae parameters (Pejcha+, 2015)", "J/ApJ/807/169 : SN IIn catalog with Fermi LAT (Ackermann+, 2015)", "J/ApJ/827/90 : Spectroscopy of SNe Ib, IIb and Ic (Liu+, 2016)", "J/A+A/587/L7 : Metallicity from Type II SN from (i)PTF (Taddia+, 2016)", "J/A+A/589/A110 : SN II in host HII regions (Anderson+, 2016)", "J/AJ/151/33 : UBVRIz LCs of 51 Type II supernovae (Galbany+, 2016)", "J/MNRAS/459/3939 : Type II supernova light curves (Valenti+, 2016)", "J/ApJ/835/166 : SNe type II from CSP-I, SDSS-II, and SNLS (de Jaeger+, 2017)", "J/ApJS/233/6 : SNe II light curves + spectra from the CfA (Hicken+, 2017)", "J/A+A/611/A25 : Updated Type II supernova Hubble diagram (Gall+, 2018)", "http://csp.obs.carnegiescience.edu/ : The Carnegie Supernova Project home", "http://sngroup.oapd.inaf.it/ : Padova-Asiago Supernova Group"], "keyword_cds": "Supernovae; Radial velocities; Spectra, optical", "keyword_pub": "supernovae: general ; surveys ; techniques: photometric ; techniques: spectroscopic", "abstract": ["We present 888 visual-wavelength spectra of 122 nearby type II", "supernovae (SNe II) obtained between 1986 and 2009, and ranging", "between 3 and 363 days post-explosion. In this first paper, we outline", "our observations and data reduction techniques, together with a", "characterization based on the spectral diversity of SNe II. A", "statistical analysis of the spectral matching technique is discussed", "as an alternative to nondetection constraints for estimating SN", "explosion epochs. The time evolution of spectral lines is presented", "and analyzed in terms of how this differs for SNe of different", "photometric, spectral, and environmental properties: velocities,", "pseudo-equivalent widths, decline rates, magnitudes, time durations,", "and environment metallicity. Our sample displays a large range in", "ejecta expansion velocities, from ~9600 to ~1500km/s at 50 days", "post-explosion with a median H_{alpha}_ value of 7300km/s. This is", "most likely explained through differing explosion energies.", "Significant diversity is also observed in the absolute strength of", "spectral lines, characterized through their pseudo-equivalent widths.", "This implies significant diversity in both temperature evolution", "(linked to progenitor radius) and progenitor metallicity between", "different SNe II. Around 60% of our sample shows an extra absorption", "component on the blue side of the H_{alpha}_ P-Cygni profile", "(\"Cachito\" feature) between 7 and 120 days since explosion. Studying", "the nature of Cachito, we conclude that these features at early times", "(before ~35 days) are associated with SiII{lambda}6355, while past the", "middle of the plateau phase they are related to high velocity (HV)", "features of hydrogen lines."], "description": ["The data presented here were obtained with a large variety of", "instruments and telescopes, as shown in Table 6.", "The majority of our spectra cover the range of ~3800 to ~9500{AA}. The", "observations were performed with the Cassegrain spectrographs at 1.5m", "and 4.0m telescopes at Cerro Tololo, with the Wide Field CCD Camera", "(WFCCD) at the 2.5m du Pont Telescope, the Low Dispersion Survey", "Spectrograph (LDSS2) on the Magellan Clay 6.5m telescope and the", "Inamori Magellan Areal Camera and Spectrograph (IMACS) on the Magellan", "Baade 6.5m telescope at Las Campanas Observatory. At La Silla, the", "observations were carried out with the ESO Multi-Mode Instrument", "(EMMI) in medium resolution spectroscopy mode (at the NTT) and the ESO", "Faint Object Spectrograph and Camera (EFOSC) at the NTT and 3.6m", "telescopes. We also have three spectra for SN 2006ee obtained with the", "Boller & Chivens CCD spectrograph at the Hiltner 2.4m Telescope of the", "MDM Observatory.", "A total of 888 spectra obtained between 1986 and 2009 and ranging", "between 3 and 363 days post-explosion have been analyzed."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aa8f52"], "orcid_pub": ["0000-0002-7252-4351"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "SN II sample ", "columns": [{"name": "SN", "desc": "Supernova identifier "}, {"name": "Host", "desc": "Host galaxy identifier "}, {"name": "HRV", "desc": "[227/23100] Galaxy heliocentric recession velocity (1)"}, {"name": "f_SN", "desc": "[1/3]? Source flags (2) "}, {"name": "Type", "desc": "Host galaxy morphological Hubble types (1) "}, {"name": "E(B-V)", "desc": "[0.01/0.6] Schlafly & Finkbeiner (2011ApJ...737..103S) reddening due to dust"}]}, {"name": "table6.dat", "desc": "Spectroscopic observations information ", "columns": [{"name": "---", "desc": "[SN] "}, {"name": "SN", "desc": "Supernova identifier "}, {"name": "UTDate", "desc": "UT date of the observation, YYYY-MM-DD "}, {"name": "JD", "desc": "Julian date of observation "}, {"name": "Phase", "desc": "[3/363] Phase, in days, since explosion "}, {"name": "Tel", "desc": "Telescope code (1) "}, {"name": "Inst", "desc": "Instrument code (2) "}, {"name": "Wmin", "desc": "[2903/10603] Min Wavelength range covered, in angstroms"}, {"name": "Wmax", "desc": "[4988/26935] Max Wavelength range covered, in angstroms"}, {"name": "Res", "desc": "[0.5/39]? Spectral resolution, angstroms, from arc-lamp lines"}, {"name": "Exp", "desc": "Total exposure time, (sequence x) seconds "}, {"name": "Airmass", "desc": "[1/5.6]? Airmass at the middle of the observation "}, {"name": "flag", "desc": "[cs] Spectrum flag (3) "}, {"name": "FileName", "desc": "Name of the FITS file in subdirectory Sp; column added by CDS"}]}, {"name": "table7.dat", "desc": "Explosion epoch estimations comparison ", "columns": [{"name": "SN", "desc": "Supernova identifier "}, {"name": "JD", "desc": "? Reduced Julian date of the spectrum used to match; JD-2400000 (1)"}, {"name": "SNID", "desc": "Best Match SN template identifier (2) "}, {"name": "dt-max", "desc": "[-7/101]? Days from maximum of the template used to match"}, {"name": "dt-exp", "desc": "[3/111]? Days from explosion of the template used to match"}, {"name": "dt-avg", "desc": "[4/93]? Average obtained from the days from explosion (1)"}, {"name": "MJD-exp1", "desc": "? Explosion date obtained with matching technique (1)"}, {"name": "e_MJD-exp1", "desc": "[3/17]? Uncertainty in MJD-exp1 "}, {"name": "MJD-nod", "desc": "? Non-detection date of the SN, Modified Julian Date (1)(3)"}, {"name": "MJD-dis", "desc": "? Discovery date of the SN, Modified Julian Date (1)(3)"}, {"name": "MJD-exp2", "desc": "? Explosion date obtained from MJD-nod and MJD-dis (1)(3)"}, {"name": "e_MJD-exp2", "desc": "[1/99]? Uncertainty in MJD-exp2 "}, {"name": "diff", "desc": "[-16/65]? Difference in MJD-exp1 and MJD-exp2 (1)(3)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_857_116"}} {"id": "J/ApJ/857/116", "title_cds": "Star cluster populations of nuclear ring galaxies", "title_create": "Ma+, 2018", "year": "2018", "author": "Ma C., de Grijs R., Ho L.C.", "title_pub": "Connections between star cluster populations and their host galaxy nuclear rings.", "first_author": "Ma C.", "ref_biblio": [""], "bibcode": ["2018ApJ...857..116M"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "J/AJ/118/2071 : ESO 565-11 UBVI(c) photometry (Buta+, 1999)", "J/AJ/121/3048 : Multicolor photometry in NGC 1512 and NGC 5248 (Maoz+, 2001)", "J/AJ/123/1411 : UBVIHalpha phot. of NGC 4314 star clusters (Benedict+, 2002)", "J/MNRAS/355/1251 : Bar-induced strengths in spiral gal. (Laurikainen+, 2004)", "J/AJ/127/1982 : HST UBVI photometry of NGC 3081 inner regions (Buta+, 2004)", "J/AJ/129/2138 : Centers of early-type galaxies with HST (Lauer+, 2005)", "J/ApJ/659/1176 : Study of bars in 180 spiral galaxies (Marinova+, 2007)", "J/ApJS/174/337 : Star formation in nuclear rings (Mazzuca+, 2008)", "J/ApJ/703/1672 : Far-IR and H{alpha} fluxes in galaxies (Kennicutt+, 2009)", "J/MNRAS/431/2917 : NGC5253 star clusters age and mass (de Grijs+, 2013)", "J/A+A/551/A81 : NGC 6951 intensity and velocity maps (van der Laan+, 2013)", "J/ApJS/216/6 : Opt-NIR HST photometry of cluster cand. in M82 (Li+, 2015)", "J/MNRAS/451/3173 : Circumnuclear star-forming regions (Alvarez-Alvarez+, 2015)", "J/MNRAS/465/2820 : NGC 6951 & NGC 1512 clusters HST photom. (de Grijs+, 2017)"], "keyword_cds": "Galaxies, IR; Photometry, HST; Photometry, infrared; Morphology; Clusters, globular; Photometry, UBVRI", "keyword_pub": "galaxies: evolution ; galaxies: individual (NGC 1512) ; galaxies: star clusters: general ; galaxies: star formation ; globular clusters: general", "abstract": ["Nuclear rings are excellent laboratories for probing diverse phenomena", "such as the formation and evolution of young massive star clusters and", "nuclear starbursts, as well as the secular evolution and dynamics of", "their host galaxies. We have compiled a sample of 17 galaxies with", "nuclear rings, which are well resolved by high-resolution Hubble and", "Spitzer Space Telescope imaging. For each nuclear ring, we identified", "the ring star cluster population, along with their physical properties", "(ages, masses, and extinction values). We also determined the", "integrated ring properties, including the average age, total stellar", "mass, and current star formation rate (SFR). We find that Sb-type", "galaxies tend to have the highest ring stellar mass fraction with", "respect to the host galaxy, and this parameter is correlated with the", "ring's SFR surface density. The ring SFRs are correlated with their", "stellar masses, which is reminiscent of the main sequence of", "star-forming galaxies. There are striking correlations between", "star-forming properties (i.e., SFR and SFR surface density) and", "nonaxisymmetric bar parameters, appearing to confirm previous", "inferences that strongly barred galaxies tend to have lower ring SFRs,", "although the ring star formation histories turn out to be", "significantly more complicated. Nuclear rings with higher stellar", "masses tend to be associated with lower cluster mass fractions, but", "there is no such relation for the ages of the rings. The two youngest", "nuclear rings in our sample, NGC 1512 and NGC 4314, which have the", "most extreme physical properties, represent the young extremity of the", "nuclear ring age distribution."], "description": ["From our initial sample of 108 galaxies (mainly from Comeron+", "2010MNRAS.402.2462C) exhibiting nuclear rings, we selected those that", "had been observed and resolved by any HST camera, including the Wide", "Field Camera 3, the Wide Field and Planetary Camera 2, the Advanced", "Camera for Surveys, the Near-Infrared Camera and Multi-Object", "Spectrometer, and the Faint Object Camera. The final sample consists", "of 17 galaxies, for which we have included the relevant information in", "Table 1.", "From the Spitzer Heritage Archive, we downloaded any available", "broadband infrared images (post-basic calibrated data, with a pixel", "scale of 0.6\") observed with the Spitzer/Infrared Array Camera."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aab6b4"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Observed filter sets and basic galactic parameters of our target galaxies", "columns": [{"name": "Galaxy", "desc": "Host galaxy name "}, {"name": "Type", "desc": "Hubble Type (1) "}, {"name": "DM", "desc": "[27.5/34.3] Distance Modulus (1) "}, {"name": "Filters", "desc": "Filters "}, {"name": "Qg", "desc": "[0.02/0.5]? non-axisymmetric bar parameter, Comeron et al. (2010MNRAS.402.2462C)"}]}, {"name": "table2.dat", "desc": "*Derived NGC 1512 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table3.dat", "desc": "Basic parameters of the ring star cluster populations ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name "}, {"name": "Nclus", "desc": "[27/1064] Number of clusters in the final selected ring cluster population"}, {"name": "f", "desc": "[0.1/1] Ratio, initial to final cluster population (1)"}, {"name": "", "desc": "[7/3020] Ring cluster surface density "}, {"name": "Lim", "desc": "Limiting master filter used for the cluster selection"}, {"name": "omagLim", "desc": "[20.4/24.1] Magnitude 90% completeness limit in filter Lim"}, {"name": "logAge", "desc": "[7.4/9] log Average age of the ring cluster sample"}, {"name": "logMass", "desc": "[4.4/7.2] log Average mass of the ring cluster sample"}, {"name": "logMtot", "desc": "[5.4/7.4] log Total mass of YMCs (2) "}]}, {"name": "table4.dat", "desc": "Integrated nuclear ring properties derived in this paper", "columns": [{"name": "Galaxy", "desc": "Host galaxy name "}, {"name": "logAge", "desc": "[7.5/9.8] Log of best-fitting age "}, {"name": "e_logAge", "desc": "[0.06/3.6] Lower uncertainty in logAge "}, {"name": "E_logAge", "desc": "[0.06/1.6] Upper uncertainty in logAge "}, {"name": "logMass", "desc": "[7.1/10] Log of total stellar mass "}, {"name": "e_logMass", "desc": "[0.06/0.4] Lower uncertainty in logAge "}, {"name": "E_logMass", "desc": "[0.05/0.2] Upper uncertainty in logAge "}, {"name": "SFR", "desc": "[0.04/2.4]? Current SFR for the past 10Myr"}, {"name": "e_SFR", "desc": "[0.006/0.4]? Uncertainty for SFR "}, {"name": "SFRD", "desc": "[0.02/0.8]? Surface density "}, {"name": "e_SFRD", "desc": "[0.005/0.1]? Uncertainty for SFRD "}]}, {"name": "table5.dat", "desc": "Multi-band photometry of the ESO 565-11 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/241] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F255W", "desc": "[17.4/26.6]?=100 Integrated apparent HST/WFPC2 F255W magnitude"}, {"name": "e_F255W", "desc": "[0.1/10]?=10 Uncertainty F255W "}, {"name": "F336W", "desc": "[17.8/28.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.07/6]?=10 Uncertainty in F336W "}, {"name": "F439W", "desc": "[17.9/27.2]?=100 Integrated apparent HST/WFPC2 F439W magnitude"}, {"name": "e_F439W", "desc": "[0.06/7.2]?=10 Uncertainty in F439W "}, {"name": "F555W", "desc": "[18.4/27]?=100 Integrated apparent HST/WFPC2 F555W magnitude"}, {"name": "e_F555W", "desc": "[0.04/2.3]?=10 Uncertainty in F555W "}, {"name": "F814W", "desc": "[18.6/30.4]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/10]?=10 Uncertainty in F814W "}]}, {"name": "table6.dat", "desc": "Derived ESO 565-11 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table7.dat", "desc": "Multi-band photometry of the IC 342 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/1063] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F275W", "desc": "[16.3/25.1]?=100 Integrated apparent HST/WFC3 F275W magnitude"}, {"name": "e_F275W", "desc": "[0.05/3]?=10 Uncertainty in F275W "}, {"name": "F336W", "desc": "[15.9/28.4]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.03/9]?=10 Uncertainty in F336W "}, {"name": "F438W", "desc": "[16/27.7]?=100 Integrated apparent HST/WFC3 F438W magnitude"}, {"name": "e_F438W", "desc": "[0.02/6]?=10 Uncertainty in F438W "}, {"name": "F547M", "desc": "[16.2/29.3]?=100 Integrated apparent HST/WFC3 F547M magnitude"}, {"name": "e_F547M", "desc": "[0.02/6.3]?=10 Uncertainty in F547M "}, {"name": "F814W", "desc": "[16.9/28.6]?=100 Integrated apparent HST/WFC3 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.01/10]?=10 Uncertainty in F814W "}]}, {"name": "table8.dat", "desc": "Derived IC 342 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table9.dat", "desc": "Multi-band photometry of the NGC 1097 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/1063] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F275W", "desc": "[16.3/25.1]?=100 Integrated apparent HST/WFC3 F275W magnitude"}, {"name": "e_F275W", "desc": "[0.05/3]?=10 Uncertainty in F275W "}, {"name": "F336W", "desc": "[15.9/28.4]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.03/9]?=10 Uncertainty in F336W "}, {"name": "F438W", "desc": "[16/27.7]?=100 Integrated apparent HST/WFC3 F438W magnitude"}, {"name": "e_F438W", "desc": "[0.02/6]?=10 Uncertainty in F438W "}, {"name": "F547M", "desc": "[16.2/29.3]?=100 Integrated apparent HST/WFC3 F547M magnitude"}, {"name": "e_F547M", "desc": "[0.02/6.3]?=10 Uncertainty in F547M "}, {"name": "F814W", "desc": "[16.9/28.6]?=100 Integrated apparent HST/WFC3 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.01/10]?=10 Uncertainty in F814W "}]}, {"name": "table10.dat", "desc": "Derived NGC 1097 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table11.dat", "desc": "Multi-band photometry of the NGC 1326 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/241] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F255W", "desc": "[17.4/26.6]?=100 Integrated apparent HST/WFPC2 F255W magnitude"}, {"name": "e_F255W", "desc": "[0.1/10]?=10 Uncertainty F255W "}, {"name": "F336W", "desc": "[17.8/28.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.07/6]?=10 Uncertainty in F336W "}, {"name": "F439W", "desc": "[17.9/27.2]?=100 Integrated apparent HST/WFPC2 F439W magnitude"}, {"name": "e_F439W", "desc": "[0.06/7.2]?=10 Uncertainty in F439W "}, {"name": "F555W", "desc": "[18.4/27]?=100 Integrated apparent HST/WFPC2 F555W magnitude"}, {"name": "e_F555W", "desc": "[0.04/2.3]?=10 Uncertainty in F555W "}, {"name": "F814W", "desc": "[18.6/30.4]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/10]?=10 Uncertainty in F814W "}]}, {"name": "table12.dat", "desc": "Derived NGC 1326 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table13.dat", "desc": "Multi-band photometry of the NGC 1672 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/301] ID number "}, {"name": "RAdeg", "desc": "[71.42/71.44] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[4] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[41.7/43.5] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-59.3/-59.2] Declination in decimal degrees (J2000)"}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[59] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[14] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[44/55] Arcsecond of Declination (J2000) "}, {"name": "F330W", "desc": "[16.4/30.3]?=100 Integrated apparent HST/ACS_HRC F330W magnitude"}, {"name": "e_F330W", "desc": "[0.04/5]?=10 Uncertainty in F330W "}, {"name": "F435W", "desc": "[16.9/26.4]?=100 Integrated apparent HST/ACS F435W magnitude"}, {"name": "e_F435W", "desc": "[0.03/5.5]?=10 Uncertainty in F435W "}, {"name": "F550M", "desc": "[17.32/24.8]?=100 Integrated apparent HST/ACS F550M magnitude"}, {"name": "e_F550M", "desc": "[0.04/5.6]?=10 Uncertainty in F550M "}, {"name": "F606W", "desc": "[17.4/25.7]?=100 Integrated apparent HST/ACS F606W magnitude"}, {"name": "e_F606W", "desc": "[0.02/10]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[17.8/26.5]?=100 Integrated apparent HST/ACS F814W magnitude"}, {"name": "e_F814W", "desc": "[0.03/3.6]?=10 Uncertainty in F814W "}]}, {"name": "table14.dat", "desc": "Derived NGC 1672 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table15.dat", "desc": "Multi-band photometry of the NGC 2997 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/250] ID number "}, {"name": "RAdeg", "desc": "[146.4/146.5] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[9] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[45] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[38/39.4] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-31.2/-31.1] Declination in decimal degrees (J2000)"}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[31] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[11] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[20/35] Arcsecond of Declination (J2000) "}, {"name": "F220W", "desc": "[17.9/29.8]?=100 Integrated apparent HST/ACS_HRC F220W magnitude"}, {"name": "e_F220W", "desc": "[0.1/8.2]?=10 Uncertainty in F220W "}, {"name": "F330W", "desc": "[18.4/29]?=100 Integrated apparent HST/ACS_HRC F330W magnitude"}, {"name": "e_F330W", "desc": "[0.09/9]?=10 Uncertainty in F330W "}, {"name": "F336W", "desc": "[18.4/36.2]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.09/6.4]?=10 Uncertainty in F336W "}, {"name": "F555W", "desc": "[19.2/31.3]?=100 Integrated apparent HST F555W magnitude"}, {"name": "e_F555W", "desc": "[0.05/2]?=10 Uncertainty in F555W "}, {"name": "F606W", "desc": "[19.8/28.5]?=100 Integrated apparent HST F606W magnitude"}, {"name": "e_F606W", "desc": "[0.03/6.8]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[20.3/28.3]?=100 Integrated apparent HST F814W magnitude"}, {"name": "e_F814W", "desc": "[0.05/4.1]?=10 Uncertainty in F814W "}]}, {"name": "table16.dat", "desc": "Derived NGC 2997 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table17.dat", "desc": "Multi-band photometry of the NGC 3081 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/241] ID number "}, {"name": "RAdeg", "desc": "Right Ascension, decimal degrees (J2000) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination, decimal degrees (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F255W", "desc": "[17.4/26.6]?=100 Integrated apparent HST/WFPC2 F255W magnitude"}, {"name": "e_F255W", "desc": "[0.1/10]?=10 Uncertainty F255W "}, {"name": "F336W", "desc": "[17.8/28.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.07/6]?=10 Uncertainty in F336W "}, {"name": "F439W", "desc": "[17.9/27.2]?=100 Integrated apparent HST/WFPC2 F439W magnitude"}, {"name": "e_F439W", "desc": "[0.06/7.2]?=10 Uncertainty in F439W "}, {"name": "F555W", "desc": "[18.4/27]?=100 Integrated apparent HST/WFPC2 F555W magnitude"}, {"name": "e_F555W", "desc": "[0.04/2.3]?=10 Uncertainty in F555W "}, {"name": "F814W", "desc": "[18.6/30.4]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/10]?=10 Uncertainty in F814W "}]}, {"name": "table18.dat", "desc": "Derived NGC 3081 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/1063] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[1.8/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[1.8/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/13.1] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.8] Reddening, E(B-V) "}]}, {"name": "table19.dat", "desc": "Multi-band photometry of the NGC 3351 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/447] ID number "}, {"name": "RAdeg", "desc": "[160.9/161] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[10] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[43] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[57.3/58.3] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[11.7/11.8] Declination, decimal degrees (J2000) "}, {"name": "DEd", "desc": "[11] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[42] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[5/21] Arcsecond of Declination (J2000) "}, {"name": "F275W", "desc": "[15.6/27.2]?=100 Integrated apparent HST/WFC3 F275W magnitude"}, {"name": "e_F275W", "desc": "[0.04/9]?=10 Uncertainty in F275W "}, {"name": "F336W", "desc": "[16/36.1]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.03/10]?=10 Uncertainty in F336W "}, {"name": "F438W", "desc": "[16.5/27]?=100 Integrated apparent HST/WFC3 F438W magnitude"}, {"name": "e_F438W", "desc": "[0.03/9]?=10 Uncertainty in F438W "}, {"name": "F450W", "desc": "[16.7/27]?=100 Integrated apparent HST/WFPC2 F450W magnitude"}, {"name": "e_F450W", "desc": "[0.02/10]?=10 Uncertainty in F450W "}, {"name": "F555W", "desc": "[17/25.8]?=100 Integrated apparent HST F555W magnitude"}, {"name": "e_F555W", "desc": "[0.02/4.4]?=10 Uncertainty in F555W "}, {"name": "F606W", "desc": "[17.6/27]?=100 Integrated apparent HST F606W magnitude"}, {"name": "e_F606W", "desc": "[0.03/4]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[18.4/27.1]?=100 Integrated apparent HST F814W magnitude"}, {"name": "e_F814W", "desc": "[0.03/4.1]?=10 Uncertainty in F814W "}]}, {"name": "table20.dat", "desc": "Derived NGC 3351 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table21.dat", "desc": "Multi-band photometry of the NGC 4303 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/142] ID number "}, {"name": "RAdeg", "desc": "[185.4/185.5] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[12] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[21] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[54.7/55.2] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[4.472/4.475] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[4] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[28] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[21.8/28.6] Arcsecond of Declination (J2000) "}, {"name": "F330W", "desc": "[18.6/25.5]?=100 Integrated apparent HST/ACS_HRC F330W magnitude"}, {"name": "e_F330W", "desc": "[0.1/2.4]?=10 Uncertainty in F330W "}, {"name": "F555W", "desc": "[19.7/25.7]?=100 Integrated apparent HST/ACS F555W magnitude"}, {"name": "e_F555W", "desc": "[0.07/3.5]?=10 Uncertainty in F555W "}, {"name": "F814W", "desc": "[20/25.4]?=100 Integrated apparent HST/ACS F814W magnitude"}, {"name": "e_F814W", "desc": "[0.05/2.5]?=10 Uncertainty in F814W "}]}, {"name": "table22.dat", "desc": "Derived NGC 4303 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table23.dat", "desc": "Multi-band photometry of the NGC 4314 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/208] ID number "}, {"name": "RAdeg", "desc": "[185.631/185.636] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[12] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[22] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[31.4/32.6] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[29.893/29.898] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[29] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[53] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[35.7/51.7] Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[17.5/27.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.06/7.2]?=10 Uncertainty in F336W "}, {"name": "F439W", "desc": "[17.9/25.4]?=100 Integrated apparent HST/WFPC2 F439W magnitude"}, {"name": "e_F439W", "desc": "[0.06/1.8]?=10 Uncertainty in F439W "}, {"name": "F569W", "desc": "[18.6/26.1]?=100 Integrated apparent HST/WFPC2 F569W magnitude"}, {"name": "e_F569W", "desc": "[0.04/1.6]?=10 Uncertainty in F569W "}, {"name": "F606W", "desc": "[18.8/26.6]?=100 Integrated apparent HST/WFPC2 F606W magnitude"}, {"name": "e_F606W", "desc": "[0.03/2]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[19.4/28.3]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/6]?=10 Uncertainty in F814W "}]}, {"name": "table24.dat", "desc": "Derived NGC 4314 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table25.dat", "desc": "Multi-band photometry of the NGC 6782 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/44] ID number "}, {"name": "RAdeg", "desc": "[290.98/291] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[19] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[23] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[57/58.5] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-59.93/-59.92] Declination in decimal degrees (J2000)"}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[59] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[55] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[16/26.2] Arcsecond of Declination (J2000) "}, {"name": "F255W", "desc": "[18/24.3]?=100 Integrated apparent HST/WFPC2 F255W magnitude"}, {"name": "e_F255W", "desc": "[0.2/7.6]?=10 Uncertainty in F255W "}, {"name": "F300W", "desc": "[18.2/24.5]?=100 Integrated apparent HST/WFPC2 F300W magnitude"}, {"name": "e_F300W", "desc": "[0.09/5.5]?=10 Uncertainty in F300W "}, {"name": "F450W", "desc": "[18/23.7]?=100 Integrated apparent HST/WFPC2 F450W magnitude"}, {"name": "e_F450W", "desc": "[0.06/4.1]?=10 Uncertainty in F450W "}, {"name": "F606W", "desc": "[17.5/24.4]?=100 Integrated apparent HST/WFPC2 F606W magnitude"}, {"name": "e_F606W", "desc": "[0.04/6.6]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[17.4/24.6]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.04/2.7]?=10 Uncertainty in F814W "}]}, {"name": "table26.dat", "desc": "Derived NGC 6782 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table27.dat", "desc": "*Derived NGC 6951 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table28.dat", "desc": "Multi-band photometry of the NGC 7217 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/115] ID number "}, {"name": "RAdeg", "desc": "[331.96/331.98] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[22] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[7] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[51.4/53.3] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[31.35/31.37] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[31] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[21] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[23/43.2] Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[21.4/28.6]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.3/5.6]?=10 Uncertainty in F336W "}, {"name": "F450W", "desc": "[21.3/26]?=100 Integrated apparent HST/WFPC2 F450W magnitude"}, {"name": "e_F450W", "desc": "[0.1/1.3]?=10 Uncertainty in F450W "}, {"name": "F547M", "desc": "[19.7/27.3]?=100 Integrated apparent HST/WFPC2 F547M magnitude"}, {"name": "e_F547M", "desc": "[0.06/9.5]?=10 Uncertainty in F547M "}, {"name": "F814W", "desc": "[21.7/29.3]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.09/1.6]?=10 Uncertainty in F814W "}]}, {"name": "table29.dat", "desc": "Derived NGC 7217 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table30.dat", "desc": "Multi-band photometry of the NGC 7469 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/56] ID number "}, {"name": "RAdeg", "desc": "[345.814/345.816] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[23] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[3] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[15.5/16] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[8.873/8.875] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[8] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[52] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[25.5/28.7] Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[16.7/23.5]?=100 Integrated apparent HST F336W magnitude"}, {"name": "e_F336W", "desc": "[0.04/1.1]?=10 Uncertainty in F336W "}, {"name": "F435W", "desc": "[17/25.5]?=100 Integrated apparent HST/ACS F435W magnitude"}, {"name": "e_F435W", "desc": "[0.02/1.6]?=10 Uncertainty in F435W "}, {"name": "F550M", "desc": "[17.6/23]?=100 Integrated apparent HST/ACS F550M magnitude"}, {"name": "e_F550M", "desc": "[0.03/0.5]?=10 Uncertainty in F550M "}, {"name": "F606W", "desc": "[18/26.3]?=100 Integrated apparent HST F606W magnitude"}, {"name": "e_F606W", "desc": "[0.02/4]?=10 Uncertainty in F606W "}, {"name": "F814W", "desc": "[18.6/25.2]?=100 Integrated apparent HST F814W magnitude"}, {"name": "e_F814W", "desc": "[0.02/1.5]?=10 Uncertainty in F814W "}]}, {"name": "table31.dat", "desc": "Derived NGC 7469 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table32.dat", "desc": "Multi-band photometry of the NGC 7742 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/270] ID number "}, {"name": "RAdeg", "desc": "[356.062/356.07] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[23] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[44] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[14.9/16.6] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[10.76/10.78] Declination in decimal degrees (J2000)"}, {"name": "DEd", "desc": "[10] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[45/46] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[18.6/29.1]?=100 Integrated apparent HST/WFPC2 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.1/8.1]?=10 Uncertainty in F336W "}, {"name": "F555W", "desc": "[19.4/26]?=100 Integrated apparent HST/WFPC2 F555W magnitude"}, {"name": "e_F555W", "desc": "[0.05/10]?=10 Uncertainty in F555W "}, {"name": "F675W", "desc": "[19.6/29.3]?=100 Integrated apparent HST/WFPC2 F675W magnitude"}, {"name": "e_F675W", "desc": "[0.05/5]?=10 Uncertainty in F675W "}, {"name": "F814W", "desc": "[20.4/28.2]?=100 Integrated apparent HST/WFPC2 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.07/9]?=10 Uncertainty in F814W "}]}, {"name": "table33.dat", "desc": "Derived NGC 7742 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}, {"name": "table34.dat", "desc": "Multi-band photometry of the UGC 3789 ring cluster candidates", "columns": [{"name": "ID", "desc": "[0/80] ID number "}, {"name": "RAdeg", "desc": "[41.584/41.587] Right Ascension in decimal degrees (J2000)"}, {"name": "RAh", "desc": "[2] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[46] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "[20.2/20.7] Second of Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-30.28/-30.27] Declination in decimal degrees (J2000)"}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[30] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[16] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "[25/33] Arcsecond of Declination (J2000) "}, {"name": "F336W", "desc": "[19.3/26.5]?=100 Integrated apparent HST/WFC3 F336W magnitude"}, {"name": "e_F336W", "desc": "[0.1/4]?=10 Uncertainty in F336W "}, {"name": "F438W", "desc": "[19.4/26.7]?=100 Integrated apparent HST/WFC3 F438W magnitude"}, {"name": "e_F438W", "desc": "[0.1/8.2]?=10 Uncertainty in F438W "}, {"name": "F814W", "desc": "[20.7/27.3]?=100 Integrated apparent HST/WFC3 F814W magnitude"}, {"name": "e_F814W", "desc": "[0.1/3.1]?=10 Uncertainty in F814W "}]}, {"name": "table35.dat", "desc": "Derived UGC 3789 ring star cluster properties ", "columns": [{"name": "Galaxy", "desc": "Host galaxy name; column added by CDS "}, {"name": "ID", "desc": "[0/447] Number of the ring star cluster population"}, {"name": "logAge", "desc": "[6.6/10.2] Log, best age "}, {"name": "b_logAge", "desc": "[6.6/8.9] Log, minimum age, 1{sigma} "}, {"name": "B_logAge", "desc": "[6.6/10.2] Log, maximum age, 1{sigma} "}, {"name": "logMass", "desc": "[2.1/9.9] Log, best mass "}, {"name": "b_logMass", "desc": "[2.1/9.4] Log, minimum mass, 1{sigma} "}, {"name": "B_logMass", "desc": "[2.8/12.9] Log, maximum mass, 1{sigma} "}, {"name": "E(B-V)", "desc": "[0/1.9] Reddening, E(B-V) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_859_101"}} {"id": "J/ApJ/859/101", "title_cds": "The supenovae Ia Pantheon sample", "title_create": "Scolnic+, 2018", "year": "2018", "author": "Scolnic D.M., Jones D.O., Rest A., Pan Y.C., Chornock R., Foley R.J., Huber M.E., Kessler R., Narayan G., Riess A.G., Rodney S., Berger E., Brout D.J., Challis P.J., Drout M., Finkbeiner D., Lunnan R., Kirshner R.P., Sanders N.E., Schlafly E., Smartt S., Stubbs C.W., Tonry J., Wood-Vasey W.M., Foley M., Hand J., Johnson E., Burgett W.S., Chambers K.C., Draper P.W., Hodapp K.W., Kaiser N., Kudritzki R.P., Magnier E.A., Metcalfe N., Bresolin F., Gall E., Kotak R., McCrum M., Smith K.W.", "title_pub": "The complete light-curve sample of spectroscopically confirmed SNe Ia from Pan-STARRS1 and cosmological constraints from the combined Pantheon sample.", "first_author": "Scolnic D.M.", "ref_biblio": [""], "bibcode": ["2018ApJ...859..101S"], "see_also": ["B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)", "V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)", "J/ApJ/607/665 : Type Ia supernovae at z>1 discovered by HST (Riess+, 2004)", "J/AJ/131/527 : UBVRI light curves of 44 type Ia supernovae (Jha+, 2006)", "J/AJ/131/1648 : Type Ia supernovae at high and low redshifts (Blondin+, 2006)", "J/ApJ/659/122 : Improved distances to type Ia supernovae (Jha+, 2007)", "J/ApJ/666/674 : ESSENCE supernova survey (Miknaitis+, 2007)", "J/AJ/136/2306 : SDSS-II Supernova survey, 2005 (Holtzman+, 2008)", "J/ApJ/700/331 : Light curves of type Ia supernovae (CfA3) (Hicken+, 2009)", "J/ApJ/700/1097 : Light curve parameters of SN Ia (Hicken+, 2009)", "J/ApJS/185/32 : First-year SDSS-II SN results (Kessler+, 2009)", "J/AJ/139/519 : Carnegie supernova project. SNe Ia (Contreras+, 2010)", "J/AJ/139/120 : Low-redshift Type-Ia supernovae (Folatelli+, 2010)", "J/A+A/523/A7 : Light curves of type Ia supernovae in SNLS (Guy+, 2010)", "J/ApJ/722/566 : Host galaxies of SNIa in SDSS-II SN survey (Lampeitl+, 2010)", "J/MNRAS/406/782 : Type Ia supernovae luminosities (Sullivan+, 2010)", "J/A+A/529/L4 : Reddening law of type Ia supernovae (Chotard+, 2011)", "J/ApJS/192/1 : Light-curve parameters from the SNLS (Conley+, 2011)", "J/MNRAS/412/1419 : Nearby supernova rates (Leaman+, 2011)", "J/ApJ/731/120 : Intrinsic SN Ia light curves (Mandel+, 2011)", "J/AJ/142/156 : The CSP (DR2): photometry of SNe Ia (Stritzinger+, 2011)", "J/AJ/143/126 : Spectroscopy of 462 nearby SNe Ia (Blondin+, 2012)", "J/ApJS/200/12 : CfA4: light curves for 94 type Ia SNe (Hicken+, 2012)", "J/ApJ/746/85 : THe HST Cluster Supernova Survey. V. (Suzuki+, 2012)", "J/ApJ/750/99 : The Pan-STARRS1 photometric system (Tonry+, 2012)", "J/ApJ/763/88 : SDSS-II supernovae Ia cosmological analysis (Campbell+, 2013)", "J/ApJ/773/53 : Type Ia SNe spectroscopy by the CSP (Folatelli+, 2013)", "J/A+A/552/A124 : SNLS & SDSS SN surveys photometric calib. (Betoule+, 2013)", "J/MNRAS/433/2240 : SALT2 parameters & distances for SNe (Ganeshalingam+, 2013)", "J/A+A/568/A22 : Joint analysis of the SDSS-II & SNLS SNIa (Betoule+, 2014)", "J/MNRAS/438/1391 : Host galaxies of Type Ia SN from PTF (Pan+, 2014)", "J/ApJ/795/44 : PS1 SNe Ia (0.02"], "bibcode": ["2018ApJ...863...59E"], "see_also": ["B/eso : ESO Science Archive Catalog (ESO, 1991-2019)", "J/ApJ/633/871 : Positions & photometry of HII knots in M51 (Calzetti+, 2005)", "J/ApJ/642/158 : IRAC flux densities in IC2163 and NGC2207 (Elmegreen+, 2006)", "J/ApJ/656/770 : Mid-IR spectrum of star-forming galaxies (Smith+, 2007)", "J/ApJ/669/959 : Warm molecular hydrogen in SINGS galaxies (Roussel+, 2007)", "J/AJ/133/791 : Spitzer phot. of normal+interacting galaxies (Smith+, 2007)", "J/ApJ/693/1821 : The Spitzer infrared nearby galaxies survey (Dale+, 2009)", "J/ApJS/184/18 : Spitzer survey of young stellar clusters (Gutermuth+, 2009)", "J/A+A/505/405 : A catalogue of Spitzer dark clouds (Peretto+, 2009)", "J/ApJ/716/942 : Bulges of nearby galaxies with Spitzer (Fisher+, 2010)", "J/ApJ/772/107 : Giant molecular clouds in nearby gal. (Donovan Meyer+, 2013)", "J/MNRAS/432/2182 : FIR bright sources of M83 (Foyle+, 2013)", "J/A+A/551/A81 : NGC 6951 intensity and velocity maps (van der Laan+, 2013)", "J/A+A/553/A54 : M100 (NGC4321) HII region IRAC photometry (Chan+, 2013)", "J/ApJ/784/3 : PAWS catalogs of GMCs and islands in M51 (Colombo+, 2014)", "J/ApJS/212/18 : An atlas of UV-to-MIR galaxy SEDs (Brown+, 2014)", "J/A+A/569/A11 : G35.20-0.74N data cubes (Sanchez-Monge+, 2014)", "J/A+A/582/A86 : Catalogue of features in the S4G (Herrera-Endoqui+, 2015)", "J/ApJ/841/37 : Tori in AGNs through Spitzer/IRS (Gonzalez-Martin+, 2017)", "J/ApJ/858/90 : Radial profiles of 5 nearby galaxies (Gallagher+, 2018)", "J/A+A/609/A123 : SABOCA imaging of G304.74+01.32 (Miettinen, 2018)", "J/ApJS/234/18 : GALEX/S4G surface brightness profiles. I. (Bouquin+, 2018)", "J/ApJS/234/35 : Stellar pop. synthesis of clumps (Zaragoza-Cardiel+, 2018)", "http://irsa.ipac.caltech.edu/Missions/spitzer.html : IRSA Spitzer home page"], "keyword_cds": "Galaxies, nearby; Photometry, infrared; Interstellar medium", "keyword_pub": "galaxies: ISM; galaxies: spiral; galaxies: star formation; ISM: structure; stars: formation", "abstract": ["Spitzer Space Telescope Infrared Array Camera (IRAC) images of M100", "show numerous long filaments with regularly spaced clumps, suggesting", "the associated cloud complexes formed by large-scale gravitational", "instabilities in shocked and accumulated gas. Optical images give no", "hint of this underlying regularity. The typical spacing between", "near-infrared clumps is ~410pc, which is ~3 times the clump diameter,", "consistent with the fastest growing mode in a filament of critical", "line density. The IRAC magnitudes and colors of several hundred clumps", "are measured in the most obvious 27 filaments and elsewhere. The clump", "colors suggest that the dust is associated with diffuse gas,", "polycyclic aromatic hydrocarbon emission, and local heating from star", "formation. Neighboring clumps on the same filament have similar", "magnitudes. The existence of many clumps all along the filament", "lengths suggests that the ages of the filaments are uniform. The", "observations support a model where interstellar gas is systematically", "accumulated over lengths exceeding several kpc, forming spiral-like", "filaments that spontaneously collapse into giant clouds and stellar", "complexes. Optical wavelengths show primarily the irregular dust", "debris, HII regions, and lingering star formation downstream from", "these primal formation sites."], "description": ["The Spitzer image of M100 was examined for small bright clumps with", "central peaks and red colors. The position and flux of each clump were", "first measured in four IRAC bands."], "type": ["OC"], "doi_pub": ["10.3847/1538-4357/aacf9a"], "orcid_pub": ["0000-0002-1723-6330"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Clumps in filaments with background annulus subtracted", "columns": [{"name": "Seq", "desc": "[1/27] Filament sequential running number "}, {"name": "Fig4", "desc": "Symbol, Color in Figure 4 "}, {"name": "RAh", "desc": "[12] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[22/23] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of Declination (J2000) "}, {"name": "DEd", "desc": "[15] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[47/51] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "3.6mag", "desc": "[14.8/24] Spitzer/IRAC 3.6 band magnitude "}, {"name": "e_3.6mag", "desc": "[0.2/2.4] Uncertainty in 3.6mag "}, {"name": "4.5mag", "desc": "[14.5/22.5] Spitzer/IRAC 4.5 band magnitude "}, {"name": "e_4.5mag", "desc": "[0.2/6.4] Uncertainty in 4.5mag "}, {"name": "5.8mag", "desc": "[12.6/20.4] Spitzer/IRAC 5.8 band magnitude "}, {"name": "e_5.8mag", "desc": "[0.1/1.3] Uncertainty in 5.8mag "}, {"name": "8.0mag", "desc": "[10.9/17.8] Spitzer/IRAC 8.0 band magnitude "}, {"name": "e_8.0mag", "desc": "[0.1/1.4] Uncertainty in 8.0mag "}]}, {"name": "table2.dat", "desc": "Clumps in filaments with interclump subtracted ", "columns": [{"name": "Seq", "desc": "[1/27] Filament sequential running number "}, {"name": "Fig4", "desc": "Symbol, Color in Figure 4 "}, {"name": "RAh", "desc": "[12] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[22/23] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of Declination (J2000) "}, {"name": "DEd", "desc": "[15] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[47/51] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "3.6mag", "desc": "[14.8/24] Spitzer/IRAC 3.6 band magnitude "}, {"name": "e_3.6mag", "desc": "[0.2/2.4] Uncertainty in 3.6mag "}, {"name": "4.5mag", "desc": "[14.5/22.5] Spitzer/IRAC 4.5 band magnitude "}, {"name": "e_4.5mag", "desc": "[0.2/6.4] Uncertainty in 4.5mag "}, {"name": "5.8mag", "desc": "[12.6/20.4] Spitzer/IRAC 5.8 band magnitude "}, {"name": "e_5.8mag", "desc": "[0.1/1.3] Uncertainty in 5.8mag "}, {"name": "8.0mag", "desc": "[10.9/17.8] Spitzer/IRAC 8.0 band magnitude "}, {"name": "e_8.0mag", "desc": "[0.1/1.4] Uncertainty in 8.0mag "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_863_91"}} {"id": "J/ApJ/863/91", "title_cds": "Co-moving catalog reorganized with BANYAN & Gaia", "title_create": "Faherty+, 2018", "year": "2018", "author": "Faherty J.K., Bochanski J.J., Gagne J., Nelson O., Coker K., Smithka I., Desir D., Vasquez C.", "title_pub": "New and known moving groups and clusters identified in a Gaia co-moving catalog.", "first_author": "Faherty J.K.", "ref_biblio": [""], "bibcode": ["2018ApJ...863...91F"], "see_also": ["B/mk : Catalogue of Stellar Spectral Classifications (Skiff, 2009-)", "IX/10 : ROSAT All-Sky Bright Source Catalogue (1RXS) (Voges+ 1999)", "IX/29 : ROSAT All-Sky Survey Faint Source Catalog (Voges+ 2000)", "I/259 : The Tycho-2 Catalogue (Hog+ 2000)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "I/298 : LSPM-North Catalog (Lepine+ 2005)", "II/328 : AllWISE Data Release (Cutri+ 2013)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/ApJS/101/117 : UBVRIJHKLMNQ photometry in Taurus-Auriga (Kenyon+ 1995)", "J/AJ/130/1247 : High proper motion stars in the DSS. III (Lepine+, 2005)", "J/AJ/133/889 : Faint companions of Hipparcos stars (Lepine+, 2007)", "J/AJ/139/2566 : SLoWPoKES catalog (Dhital+, 2010)", "J/ApJS/192/2 : A Bayesian search for binaries in Hipparcos (Shaya+, 2011)", "J/MNRAS/435/1325 : Membership of the {epsilon} Cha association (Murphy+, 2013)", "J/A+A/566/A132 : Teff and L for stars in 7 open clusters (Silaj+, 2014)", "J/MNRAS/454/593 : Young moving groups in solar neighbourhood (Bell+, 2015)", "J/ApJ/799/155 : Sub-stellar companions in Taurus (Daemgen+, 2015)", "J/AJ/150/57 : SLoWPoKES-II catalog (Dhital+, 2015)", "J/ApJS/219/33 : BANYAN. VII. Candidate YMG members from BASS (Gagne+, 2015)", "J/MNRAS/447/1267 : Low-mass members of the Octans association (Murphy+, 2015)", "J/ApJ/801/L10 : XO-2N and XO-2S equivalent widths (Teske+, 2015)", "J/ApJS/225/10 : Kinematic analysis of M7-L8 dwarfs (Faherty+, 2016)", "J/ApJ/830/44 : X-ray LFs of M37 low-mass stars (Nunez+, 2016)", "J/MNRAS/461/794 : Scorpius-Centaurus K-Type Stars (Pecaut+, 2016)", "J/A+A/595/A22 : 9 new open clusters within 500pc from the Sun (Roser+, 2016)", "J/MNRAS/472/675 : Wide binaries in Tycho-Gaia: search method (Andrews+, 2017)", "J/A+A/601/A19 : Gaia DR1 open cluster members (Gaia Collaboration+, 2017)", "J/AJ/153/259 : GAMBLES extension of the SLoWPoKES catalog (Oelkers+, 2017)", "J/AJ/153/257 : Comoving stars in Gaia DR1 (Oh+, 2017)", "J/AJ/155/149 : Co-moving stars observed by Gaia (Bochanski+, 2018)", "J/ApJ/856/23 : BANYAN. XI. The BANYAN {Sigma} algorithm (Gagne+, 2018)", "J/ApJ/860/43 : BANYAN. XII. New members from Gaia-Tycho data (Gagne+, 2018)", "J/ApJ/862/138 : BANYAN. XIII. Young assoc. with Gaia DR2 (Gagne+, 2018)"], "keyword_cds": "Photometry, infrared ; Proper motions ; Associations, stellar ; Radial velocities ; Spectral types ; Ultraviolet ; X-ray sources ; Parallaxes, trigonometric ; Optical", "keyword_pub": "methods: data analysis; proper motions; stars: kinematics and dynamics; open clusters and associations: general; binaries: general", "abstract": ["We present a reorganization of the Oh+ (2017, J/AJ/153/257) wide,", "comoving catalog of 4555 groups of stars (10606 individual objects)", "identified in the Tycho Gaia Astrometric Survey (TGAS) into new and", "known coevolving groups of stars in the Milky Way. We use the BANYAN", "{Sigma} kinematic analysis tool to identify 1015 individual stars in", "the Oh+ catalog that yielded a >80% probability in 1 of 27 known", "associations (e.g., the AB Doradus moving group, Columba, Upper", "Scorpius) in the vicinity of the Sun. Among the 27 groups uncovered by", "Oh+ that had >10 connected components, we find that 4 are newly", "discovered. We use a combination of Tycho, Gaia, Two micron All Sky", "catalog, Wide Field Infrared Survey Explorer Mission, Galaxy Evolution", "Explorer, and Rontgen Satellite photometry as well as Gaia parallaxes", "to determine that these new groups are likely older than the Pleiades", "but younger than ~1Gyr. Using isochrone fitting, we find that the", "majority of these new groups have solar-type stars and solar-type", "metallicity. Among the 35 Oh+ groups with five to nine members, we", "find that 19 also appear new and comoving, with Oh+ Group 30 is", "particularly exciting as it is well within 100pc (range of 77-90pc)", "and also appears to be older than the Pleiades. For known star-forming", "regions, open clusters, and moving groups identified by Oh+, we find", "that the majority were broken up into pieces over several Oh+ groups", "(e.g., Lower Centaurus Crux members are spread over 26 Oh+ groups);", "however, we found no correlation with positions of the groups on", "color-magnitude diagrams, and therefore no substructure of the", "association correlated with the Oh+ designated group. We find that", "across the 27 groups tested by BANYAN {Sigma} there were 400 new", "members to 20 different associations uncovered by Oh+ that require", "further vetting."], "type": ["CCC"], "doi_pub": ["10.3847/1538-4357/aac76e"], "orcid_pub": ["0000-0001-6251-0573"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Oh+ (Oh17; 2017, J/AJ/153/257) with spectral type and T_eff_", "columns": [{"name": "Name", "desc": "Object identifier; Tycho or Hipparcos "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) (G1) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) (G1) "}, {"name": "SpType", "desc": "Spectral type (G1) "}, {"name": "Teff", "desc": "[2800/32000]? Effective temperature (G1) "}, {"name": "Assoc", "desc": "BANYAN group designation (G2) "}, {"name": "Prob", "desc": "[0/100] BANYAN membership probability (1) "}, {"name": "Group", "desc": "[0/4554] Oh17 group number (G3) "}]}, {"name": "table2.dat", "desc": "Oh17 with photometry ", "columns": [{"name": "Name", "desc": "Object identifier; Tycho or Hipparcos "}, {"name": "SpType", "desc": "Spectral type (G1) "}, {"name": "Bmag", "desc": "[0.02/19.6]? Tycho B band magnitude "}, {"name": "Vmag", "desc": "[0.02/18.2]? Tycho V band magnitude "}, {"name": "l_Jmag", "desc": "Upper limit flag on Jmag "}, {"name": "Jmag", "desc": "[-27.2/16.8]? 2MASS J band magnitude "}, {"name": "e_Jmag", "desc": "[0/10]? Uncertainty in Jmag "}, {"name": "l_Hmag", "desc": "Upper limit flag on Hmag "}, {"name": "Hmag", "desc": "[0.02/11.3]? 2MASS H band magnitude "}, {"name": "e_Hmag", "desc": "[0/10]? Uncertainty in Hmag "}, {"name": "l_Ksmag", "desc": "Upper limit flag on Ksmag "}, {"name": "Ksmag", "desc": "[0/11.3]? 2MASS Ks band magnitude "}, {"name": "e_Ksmag", "desc": "[0/10]? Uncertainty in Ksmag "}, {"name": "l_W1mag", "desc": "Upper limit flag on W1mag "}, {"name": "W1mag", "desc": "[0/19.5]? WISE 3.4 micron band magnitude "}, {"name": "e_W1mag", "desc": "[0.01/18.4]? Uncertainty in W1mag "}, {"name": "l_W2mag", "desc": "Upper limit flag on W2mag "}, {"name": "W2mag", "desc": "[0.02/16] WISE 4.6 micron band magnitude "}, {"name": "e_W2mag", "desc": "[0/10]? Uncertainty in W2mag "}, {"name": "l_W3mag", "desc": "Upper limit flag on W3mag "}, {"name": "W3mag", "desc": "[-0.4/13]? WISE 12 micron band magnitude "}, {"name": "e_W3mag", "desc": "[0.01/10]? Uncertainty in W3mag "}, {"name": "l_W4mag", "desc": "Upper limit flag on W4mag "}, {"name": "W4mag", "desc": "[-3.3/11.5]? WISE 22 micron band magnitude "}, {"name": "e_W4mag", "desc": "[0/8.7]? Uncertainty in W4mag "}]}, {"name": "table3.dat", "desc": "Oh17 with photometry (cont) ", "columns": [{"name": "Name", "desc": "Object identifier; Tycho or Hipparcos "}, {"name": "SpType", "desc": "Spectral type (G1) "}, {"name": "NUVmag", "desc": "[9.8/21.8]? GALEX NUV band magnitude "}, {"name": "e_NUVmag", "desc": "[0/0.5]? Uncertainty in NUVmag "}, {"name": "FUVmag", "desc": "[10.7/24.3]? GALEX FUV band magnitude "}, {"name": "e_FUVmag", "desc": "[0/2.2]? Uncertainty in FUVmag "}, {"name": "1RXS", "desc": "ROSAT bright identifier (JHHMMSS.s+DDMMs) "}, {"name": "logLBx", "desc": "[27.6/31.7]? log bright X-ray luminosity; in erg/s units"}, {"name": "e_logLBx", "desc": "[0.03/0.5]? Uncertainty in logLBx; ergs/s "}, {"name": "1RXSf", "desc": "ROSAT faint identifier (JHHMMSS.s+DDMMs) "}, {"name": "logLFx", "desc": "[27.3/31]? log faint X-ray luminosity; ergs/s "}, {"name": "e_logLFx", "desc": "[0.1/1.6]? Uncertainty in logLFx; ergs/s "}, {"name": "Group", "desc": "[0/4554] Oh17 group number (G3) "}, {"name": "Assoc", "desc": "BANYAN group designation (G2) "}, {"name": "Prob", "desc": "[0/100] BANYAN group membership probability "}]}, {"name": "table4.dat", "desc": "Oh+ (Oh17; 2017, J/AJ/153/257) sample with BANYAN {Sigma} input of known members", "columns": [{"name": "Name", "desc": "Object identifier; Tycho or Hipparcos "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) (G1) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) (G1) "}, {"name": "pmRA", "desc": "[-248/226.4] Proper motion along RA "}, {"name": "e_pmRA", "desc": "[0.01/4.7] Uncertainty in pmRA "}, {"name": "pmDE", "desc": "[-320.4/271.6] Proper motion along DE "}, {"name": "e_pmDE", "desc": "[0.01/2.7] Uncertainty in pmDE "}, {"name": "plx", "desc": "[5.7/63.4] Parallax "}, {"name": "e_plx", "desc": "[0.2/1] Uncertainty in plx "}, {"name": "RVel", "desc": "[-4.4/42.8]? Radial velocity "}, {"name": "e_RVel", "desc": "[0.8/8.3]? Uncertainty in RVel "}, {"name": "B-Grp", "desc": "BANYAN nearby group(s) designation "}, {"name": "Prob", "desc": "[81/100] BANYAN nearby membership probability "}, {"name": "Group", "desc": "[2/4103] Oh17 group number (G3) "}, {"name": "Known", "desc": "Object type (1) "}, {"name": "K-Grp", "desc": "Corresponding group(s) of investigation to Known"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_867_108"}} {"id": "J/ApJ/867/108", "title_cds": "Stellar masses and rest-frame u-g colors of SNIa", "title_create": "Jones+, 2018", "year": "2018", "author": "Jones D.O., Riess A.G., Scolnic D.M., Pan Y.-C., Johnson E., Coulter D.A., Dettman K.G., Foley M.M., Foley R.J., Huber M.E., Jha S.W., Kilpatrick C.D., Kirshner R.P., Rest A., Schultz A.S.B., Siebert M.R.", "title_pub": "Should Type Ia supernova distances be corrected for their local environments?", "first_author": "Jones D.O.", "ref_biblio": [""], "bibcode": ["2018ApJ...867..108J"], "see_also": ["V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)", "I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)", "II/358 : SkyMapper Southern Sky Survey. DR1.1 (Wolf+, 2018)", "J/AJ/131/527 : UBVRI light curves of 44 type Ia supernovae (Jha+, 2006)", "J/ApJ/700/331 : Light curves of type Ia supernovae (CfA3) (Hicken+, 2009)", "J/ApJ/700/1097 : Light curve parameters of SN Ia (Hicken+, 2009)", "J/ApJ/690/1236 : COSMOS photometric redshift catalog (Ilbert+, 2009)", "J/ApJS/185/32 : First-year SDSS-II SN results (Kessler+, 2009)", "J/AJ/139/519 : Carnegie supernova project. SNe Ia (Contreras+, 2010)", "J/AJ/139/120 : Low-redshift Type-Ia supernovae (Folatelli+, 2010)", "J/A+A/523/A7 : Light curves of type Ia supernovae in SNLS (Guy+, 2010)", "J/ApJ/722/566 : Host galaxies of SNeIa in SDSS-II SN survey (Lampeitl+, 2010)", "J/MNRAS/406/782 : Type Ia supernovae luminosities (Sullivan+, 2010)", "J/AJ/142/156 : The CSP (DR2): photometry of SNe Ia (Stritzinger+, 2011)", "J/ApJS/200/12 : CfA4: light curves for 94 type Ia SNe (Hicken+, 2012)", "J/A+A/568/A22 : Joint analysis of the SDSS-II & SNLS SNe Ia (Betoule+, 2014)", "J/MNRAS/438/1391 : Host galaxies of Type Ia SN from PTF (Pan+, 2014)", "J/ApJ/795/44 : PS1 SNe Ia (0.02~2{sigma}", "significance, local properties tend to correlate with distance", "residuals better than properties at random locations, though despite", "using the largest low-z sample to date, we cannot definitively prove", "that a local correlation is more significant than a random", "correlation. Our data hint that SNe observed by surveys that do not", "target a pre-selected set of galaxies may have a larger local mass", "step than SNe from surveys that do, an increase of 0.071+/-0.036mag", "(2.0{sigma}). We find a 3{sigma} local mass step after global mass", "correction, evidence that SNe Ia should be corrected for their local", "mass, but we note that this effect is insignificant in the targeted", "low-z sample. Only the local mass step remains significant at", ">2{sigma} after global mass correction, and we conservatively estimate", "a systematic shift in H0 measurements of -0.14km/s/Mpc with an", "additional uncertainty of 0.14km/s/Mpc, ~10% of the present", "uncertainty."], "description": ["For this analysis, we combine 216 z<0.1 SNe from the Pantheon", "compilation (Scolnic+ 2018ApJ...859..101S) with 178 SNe Ia from the", "Foundation first data release (DR1; Foley+ 2018MNRAS.475..193F).", "We measure host galaxy properties with photometry from the PS1 first", "data release (Chambers+ 2016, II/349) and the Sloan Digital Sky Survey", "Data Release 14 (SDSS DR14; Abolfathi+ 2018ApJS..235...42A).", "After all cuts, grizy images for measuring the local mass step are", "available for 273 SNe Ia. Of these SNe, 195 lie in the SDSS footprint", "and therefore have u measurements for measuring the rest-frame u-g color."], "type": ["CCC"], "doi_pub": ["10.3847/1538-4357/aae2b9"], "orcid_pub": ["0000-0002-6230-0151"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "localsn.dat", "desc": "Measurements of Hubble residuals and host galaxy properties for 273 Type Ia supernovae at z<0.1", "columns": [{"name": "SN", "desc": "Supernova Identifier "}, {"name": "RAh", "desc": "Hour of Right Ascension, Supernova (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination, Supernova (J2000) "}, {"name": "DEd", "desc": "Degree of Declination, Supernova (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "z", "desc": "[0.01/0.1] Redshift "}, {"name": "RAHh", "desc": "Hour of Right Ascension, Host Galaxy (J2000)"}, {"name": "RAHm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAHs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DEH-", "desc": "Sign of the Declination, Host Galaxy (J2000)"}, {"name": "DEHd", "desc": "Degree of Declination, Host Galaxy (J2000) "}, {"name": "DEHm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEHs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Rpar", "desc": "[0.07/5] Size- and orientation-weighted SN separation parameter (1)"}, {"name": "E(B-V)", "desc": "[0/0.2] Average galaxy reddening "}, {"name": "(u-g)loc", "desc": "[0.1/2.2]?=-99 Local (u-g) color index (2) "}, {"name": "b_(u-g)loc", "desc": "?=-99 Lower bound on local (u-g) color (2) "}, {"name": "B_(u-g)loc", "desc": "?=-99 Upper bound on local (u-g) color (2) "}, {"name": "(u-g)", "desc": "[0.2/2.2]?=-99 Global (u-g) color index (2)"}, {"name": "b_(u-g)", "desc": "?=-99 Lower bound on (u-g) (2) "}, {"name": "B_(u-g)", "desc": "?=-99 Upper bound on (u-g) (2) "}, {"name": "Massloc", "desc": "[6.7/10.8] Local mass within a 3kpc radius "}, {"name": "b_Massloc", "desc": "Lower bound on local mass density "}, {"name": "B_Massloc", "desc": "Upper bound on local mass density "}, {"name": "Mass", "desc": "[6.7/12] Global mass "}, {"name": "b_Mass", "desc": "Lower bound on global mass density "}, {"name": "B_Mass", "desc": "Upper bound on global mass density "}, {"name": "SFRloc", "desc": "[-42.5/-7.5]?=-99 local star formation rate, log(yr^-1^.kpc^-2^)"}, {"name": "b_SFRloc", "desc": "?=-99 Lower bound SFRloc "}, {"name": "B_SFRloc", "desc": "?=-99 Upper bound SFRloc "}, {"name": "SFR", "desc": "[-42.5/-7.7]?=-99 Global star formation rate, log(yr^-1^.kpc^-2^)"}, {"name": "b_SFR", "desc": "?=-99 Lower bound on SFR "}, {"name": "B_SFR", "desc": "?=-99 Upper bound on SFR "}, {"name": "Inc", "desc": "[12/70] Inclination "}, {"name": "Hres", "desc": "[-0.5/0.4] Hubble residual, {mu} "}, {"name": "e_Hres", "desc": "[0.04/0.3] Uncertainty in hubble-resid "}, {"name": "Hrescor", "desc": "[-0.2/0.2] Bias correction, hubble-resid "}, {"name": "c", "desc": "[-0.2/0.3] Tripp estimator parameter, c, light curve color parameter"}, {"name": "e_c", "desc": "[0.009/0.1] Uncertainty in c "}, {"name": "ccor", "desc": "[-0.11/0.04] Bias correction, c parameter "}, {"name": "x1", "desc": "[-2.7/2.3] Tripp estimator, x1, light curve shape parameter"}, {"name": "e_x1", "desc": "[0.02/0.9] Uncertainty in x1 "}, {"name": "x1cor", "desc": "[-0.4/1] Bias correction, x1 parameter "}, {"name": "mb", "desc": "[14/20] Tripp estimator, mb, log of the light curve amplitude"}, {"name": "e_mb", "desc": "[0.02/0.2] Uncertainty in mb "}, {"name": "mbcor", "desc": "[-0.2/0.03] Bias correction, mb parameter "}, {"name": "r-A", "desc": "[0.2/21] SExtractor galaxy ellipse parameter, A"}, {"name": "r-B", "desc": "[0.1/11.2] SExtractor galaxy ellipse parameter, B"}, {"name": "theta", "desc": "[-90/90] SExtractor galaxy ellipse parameter, {theta}"}, {"name": "Survey", "desc": "Was the survey targeted or untargeted "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_872_16"}} {"id": "J/ApJ/872/16", "title_cds": "Integrated star formation law revisited. I.", "title_create": "de los Reyes+, 2019", "year": "2019", "author": "de los Reyes M.A.C., Kennicutt R.C.", "title_pub": "Revisiting the integrated star formation law. I. Non-starbursting galaxies.", "first_author": "de los Reyes M.A.C.", "ref_biblio": [""], "bibcode": ["2019ApJ...872...16D"], "see_also": ["II/328 : AllWISE Data Release (Cutri+ 2013)", "VII/155 : Third Reference Cat. of Bright Galaxies (RC3) (de Vaucouleurs+ 1991)", "J/A+AS/115/407 : Short WSRT HI observations of spiral galaxies (Rhee+, 1996)", "J/A+A/324/877 : HI properties of spiral & irregular galaxies (Broeils+, 1997)", "J/A+A/370/765 : HI synthesis observations in UMa cluster (Verheijen+, 2001)", "J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)", "J/A+A/442/137 : HI observations of WHISP disk galaxies (Noordermeer+, 2005)", "J/ApJS/164/81 : Spectrophotometry of nearby galaxies (Moustakas+, 2006)", "J/PASP/119/994 : MIPS 24um calibrators (Engelbracht+, 2007)", "J/ApJS/173/185 : GALEX UV atlas of nearby galaxies (Gil de Paz+, 2007)", "J/ApJ/671/333 : Aperture photometry in NGC 5194 (Kennicutt+, 2007)", "J/ApJS/173/538 : XUV-Disk galaxies in the Local Universe (Thilker+, 2007)", "J/ApJS/178/247 : H{alpha} and [NII] survey in local 11 Mpc (Kennicutt+, 2008)", "J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008)", "J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008)", "J/ApJ/703/517 : The Spitzer Local Volume Legacy: IR photometry (Dale+, 2009)", "J/ApJ/706/599 : H{alpha} and UV SFR in the local volume (Lee+, 2009)", "J/ApJS/190/233 : Spectroscopy & abundances of SINGS gal. (Moustakas+, 2010)", "J/PASP/122/1397 : Spitzer Survey of Stellar Structure in Gal. (Sheth+, 2010)", "J/ApJS/192/6 : A GALEX UV imaging survey of nearby galaxies (Lee+, 2011)", "J/ApJ/733/87 : Star formation efficiency in galaxies (Shi+, 2011)", "J/MNRAS/414/940 : ATLAS3D project. IV. (Young+, 2011)", "J/MNRAS/423/197 : MIPS photometry for Herschel SAG2 Programs (Bendo+, 2012)", "J/A+A/544/A101 : GALEX obs. of Herschel Reference Survey (Cortese+, 2012)", "J/AJ/144/134 : LITTLE THINGS survey of nearby dwarf galaxies (Hunter+, 2012)", "J/ApJ/771/59 : S^4^G face-on gal. surface brightnesses (Munoz-Mateos+, 2013)", "J/A+A/564/A65 : Cold gas data of Herschel Reference Survey (Boselli+, 2014)", "J/MNRAS/445/899 : LVL SEDs and physical properties (Cook+, 2014)", "J/A+A/566/A71 : HI study of 18 nearby dwarf galaxies (Lelli+, 2014)", "J/A+A/569/A124 : GUViCS. Ultraviolet Source Catalogs (Voyer+, 2014)", "J/ApJS/220/6 : Updated catalog of GALEX nearby galaxies (Bai+, 2015)", "J/ApJ/805/31 : IR-Rad luminosities & surface densities of gal. (Liu+, 2015)"], "keyword_cds": "Galaxies, photometry; Ultraviolet; Infrared; Abundances; References; Radio sources", "keyword_pub": "galaxies: dwarf ; galaxies: spiral ; galaxies: star formation", "abstract": ["We use new and updated gas- and dust-corrected star formation rate", "(SFR) surface densities to revisit the integrated star formation law", "for local \"quiescent\" spiral, dwarf, and low surface brightness", "galaxies. Using UV-based SFRs with individual IR-based dust", "corrections, we find that \"normal\" spiral galaxies alone define a", "tight {Sigma}_(HI+H2)-{Sigma}_SFR_ relation described by an", "n=1.41_-0.07_^+0.07^ power law with a dispersion of 0.28_-0.02_^+0.02^", "(errors reflect fitting and statistical uncertainties). The SFR", "surface densities are only weakly correlated with HI surface", "densities alone, exhibiting a stronger and roughly linear correlation", "with H_2_ surface densities, similar to what is seen in spatially", "resolved measurements of disks. However, many dwarf galaxies lie below", "the star formation law defined by spirals, suggesting a low-density", "threshold in the integrated star formation law. We consider", "alternative scaling laws that better describe both spirals and dwarfs.", "Our improved measurement precision also allows us to determine that", "much of the scatter in the star formation law is intrinsic, and we", "search for correlations between this intrinsic scatter and secondary", "physical parameters. We find that dwarf galaxies exhibit second-order", "correlations with the total gas fraction, stellar mass surface", "density, and dynamical time, which may explain much of the scatter in", "the star formation law. Finally, we discuss various systematic", "uncertainties that should be kept in mind when interpreting any study", "of the star formation law, particularly the X(CO) conversion factor", "and the diameter chosen to define the star-forming disk in a galaxy."], "type": ["CCC"], "doi_pub": ["10.3847/1538-4357/aafa82"], "orcid_pub": ["0000-0002-4739-046X"], "data": "f-v", "date_creation": "10-Aug-2020", "xmatch": "J/ApJ/872/16/sample", "last_update": "12-Oct-2020", "catid": "18720016", "date_update": "10-Aug-2020", "tables": [{"name": "table1.dat", "desc": "General properties of sample ", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Dist", "desc": "[0.5/75.4]? Distance (1) "}, {"name": "Bmag", "desc": "[4.16/15.8]? Apparent B-band (AB) magnitude (2)"}, {"name": "e_Bmag", "desc": "[0.04/0.99]? Mean error on Bmag (2) "}, {"name": "B-V", "desc": "[0.21/1.07]? B-V color index (2) "}, {"name": "e_B-V", "desc": "[0.01/0.19]? Mean error B-V (2) "}, {"name": "MType", "desc": "Galaxy type; s=spiral, d=dwarf "}, {"name": "PA", "desc": "[-75/203] Position angle (2) "}, {"name": "E(B-V)", "desc": "[0.01/0.8] Reddening E(B-V) (3) "}, {"name": "Diam25", "desc": "[25/11433]? D25 diameter (2) "}, {"name": "DiamHa", "desc": "[8/5940] D(Halpha) diameter (4) "}, {"name": "b/a", "desc": "[0.1/1.0]? Axis ratio measured from B-band isophotes (2)"}]}, {"name": "table2.dat", "desc": "UV photometric data ", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "l_UVmag", "desc": "[0/1] Upper limit flag on UVmag; 1=yes, 0=no "}, {"name": "UVmag", "desc": "[8.2/20.7]? GALEX apparent UV magnitude "}, {"name": "e_UVmag", "desc": "[0.1/1]? Mean error on UVmag "}, {"name": "r_UVmag", "desc": "[401/408]? Reference for UVmag (see refs.dat file) "}, {"name": "tUV", "desc": "[87/21177.4]? Exposure time (5) "}, {"name": "Tile", "desc": "GALEX tile name (5) "}, {"name": "f_UVmag", "desc": "[0/1]? NUV flag; 1=only NUV available; 0=FUV used (5)"}]}, {"name": "table3.dat", "desc": "IR photometric data ", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "l_IRflux", "desc": "[0/1] Upper limit flag on IR flux; 1=yes, 0=no "}, {"name": "IRflux", "desc": "[1.9e-05/139]? 24um IR flux density "}, {"name": "e_IRflux", "desc": "[0.0001/23]? Mean error on IRflux "}, {"name": "r_IRflux", "desc": "[301/404] Reference for IRflux (see refs.dat file)"}, {"name": "tIR", "desc": "[146.8/1404.7]? Exposure time (s) (6) "}, {"name": "Survey", "desc": "For Spitzer MIPS images, name of survey (7) "}, {"name": "Nfr", "desc": "[99/558]? For AllWISE images, number of frames "}, {"name": "CoaddID", "desc": "For AllWISE images, the co-add ID "}]}, {"name": "table4.dat", "desc": "SFRs, gas masses, and SFR and gas surface densities; from erratum published in 2019, ApJ, 878, 74", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "l_logSFR", "desc": "[0/1]? Upper limit flag on logSFR (1=yes)"}, {"name": "logSFR", "desc": "[-4.5/1.5]? Log uncorrected SFR "}, {"name": "e_logSFR", "desc": "[0.02/0.4]? Mean error on logSFR "}, {"name": "l_logSFRc", "desc": "[0/1]? Upper limit flag on logSFRc (1=yes)"}, {"name": "logSFRc", "desc": "[-5.4/1.5]? Log dust-corrected SFR "}, {"name": "e_logSFRc", "desc": "[0.02/0.5]? Mean error on logSFRcorr "}, {"name": "logSigSFRc", "desc": "[-5.7/1.2]? Log dust-corrected SFR surface density"}, {"name": "logSigHI", "desc": "[-0.3/1.5]? Log HI surface density (8) "}, {"name": "r_logSigHI", "desc": "Reference for logSigHI (see refs.dat file)"}, {"name": "l_logSigH2", "desc": "[0/1] Upper limit flag on logSigH2 (1=yes)"}, {"name": "logSigH2", "desc": "[-1.3/3.5]? Log H2 surface density (8) "}, {"name": "r_logSigH2", "desc": "Reference for logSigH2 (see refs.dat file)"}]}, {"name": "table5.dat", "desc": "Other properties of sample ", "columns": [{"name": "Seq", "desc": "[1/307] Running index number "}, {"name": "Name", "desc": "Galaxy ID preferred by NED (G1) "}, {"name": "Mass", "desc": "[5.8/11.5]? Log stellar mass "}, {"name": "r_Mass", "desc": "[501/503]? Reference for stellar mass (see refs.dat file)"}, {"name": "Z", "desc": "[7.3/9.2]? Gas-phase metallicity; 12+log[O/H]"}, {"name": "r_Z", "desc": "[601/605]? Reference for Z (see refs.dat file)"}, {"name": "C42", "desc": "[1.7/6.7]? Concentration index "}, {"name": "tDyn", "desc": "[0.2/17.4]? Dynamical time (9) "}, {"name": "vRot", "desc": "[0.6/43]? Rotational velocity (9) "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "[1/605] Reference code "}, {"name": "Auth", "desc": "First author's name(s) "}, {"name": "BibCode", "desc": "Bibcode of the reference "}, {"name": "Comm", "desc": "Comment "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_872_89"}} {"id": "J/ApJ/872/89", "title_cds": "Solar energetic particle (SEP) events with GOES", "title_create": "Kahler+, 2019", "year": "2019", "author": "Kahler S.W., Ling A.G.", "title_pub": "Suprathermal ion backgrounds of solar energetic particle events.", "first_author": "Kahler S.W.", "ref_biblio": [""], "bibcode": ["2019ApJ...872...89K"], "see_also": ["J/ApJ/709/1238 : Solar Coronal Mass Ejection (Yeates+, 2010)", "J/ApJ/757/94 : Solar flares observed with GOES and AIA (Aschwanden, 2012)", "J/ApJ/759/69 : Solar electron events 1995-2005 with WIND/3DP (Wang+, 2012)", "J/ApJ/774/L27 : Solar flares predictors (Yang+, 2013)", "J/A+A/574/A37 : Movies of 2012-10-16 solar flare (Dalmasse+, 2015)", "J/ApJ/831/105 : Global energetics of solar flares. IV. CME (Aschwanden, 2016)", "J/ApJ/845/36 : Complex network for solar active regions (Daei+, 2017)", "J/ApJ/847/115 : The solar flare complex network (Gheibi+, 2017)", "J/ApJ/868/124 : ICMEs events from 1998 to 2011 with ACE and WIND (Feng+, 2018)", "J/A+A/640/A17 : GLE integral intensities (Usoskin+, 2020)", "http://umbra.nascom.nasa.gov/SEP : : Solar Proton Events list from NOAA", "http://st4a.stelab.nagoya-u.ac.jp/hinode_flare/ : Hinode Flare Catalog", "http://www.lmsal.com/hek/index.html : Heliophysics Events Knowledgebase"], "keyword_cds": "Sun; Stars, flare", "keyword_pub": "acceleration of particles ; Sun: coronal mass ejections (CMEs) ; Sun: flares ; Sun: particle emission", "abstract": ["Gradual solar energetic particle (SEP) events result from the", "acceleration of low-energy suprathermal seed particles to high", "(E>10MeV/nuc) energies by shocks driven by coronal mass ejections", "(CMEs). Several studies suggest connections between suprathermal", "particles measured in situ at 1au and the seed particles accelerated", "near the Sun to E>10MeV. We correlate E>10MeV SEP event peak", "intensities (Ip) with suprathermal H and He intensities at each of two", "energies averaged over four periods around the SEP onsets in the", "Geostationary Operational Environmental Satellite spacecraft during", "the period of 1998-2016. The 201 SEP events are sorted into four", "groups by their associated solar source longitudes and are further", "separated between events in transient CMEs and in normal solar wind", "(SW). The mean Ip in CME SW that is larger than in normal SW that was", "found earlier is confirmed. The suprathermals significantly correlate", "(correlation coefficients CCs~0.4-0.6) with the SEP Ip from the 0{deg}", "to W40{deg} range, but only weakly (CC~0.0-0.3) with SEP events from", "the well-connected W41{deg} to W83{deg} range. Eastern hemisphere SEP", "intensities are uncorrelated (CC~0.0) with suprathermals in normal SW", "but are well correlated (CC~0.4-0.7) for those in transient CME SW,", "which we interpret with a simple model involving perpendicular shock", "acceleration of the suprathermals. The in situ B field magnitude shows", "no correlation with SEP intensities for any longitude range or", "timescale. These results confirm that tracking suprathermal", "intensities at 1 au can be useful in forecasting the Ip of SEP events."], "description": ["We compiled a list of E>10MeV solar energetic particle (SEP) events", "observed with the Energetic Particle Sensors on board the", "Geostationary Operational Environmental Satellite (GOES) from 1998", "through 2016. See Section 2 for further details."], "type": ["OC"], "data": "", "date_update": "04-Aug-2020", "tables": [{"name": "table1.dat", "desc": "E>10MeV solar energetic particle (SEP) events ", "columns": [{"name": "Event.Y", "desc": "[1998/2016] Year of the event (1) "}, {"name": "Event.M", "desc": "Month of the event "}, {"name": "Event.D", "desc": "Day of the event "}, {"name": "---", "desc": "[/] "}, {"name": "Onset", "desc": "Hour of event onset (unit????) "}, {"name": "Ip", "desc": "[1.4/8000] Peak intensity (2) "}, {"name": "Time", "desc": "UT time of flare peak; Day/hour "}, {"name": "Loc", "desc": "Location of flare "}, {"name": "CME", "desc": "Coronal Mass Ejection Solar Wind event? Y=yes "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_872_206"}} {"id": "J/ApJ/872/206", "title_cds": "Blue horizontal branch stars in the VVV data", "title_create": "Montenegro+, 2019", "year": "2019", "author": "Montenegro K., Minniti D., Alonso-Garcia J., Hempel M., Saito R.K., Beers T.C., Brown D.", "title_pub": "VVV Survey of blue horizontal branch stars in the bulge-halo transition region of the Milky Way.", "first_author": "Montenegro K.", "ref_biblio": [""], "bibcode": ["2019ApJ...872..206M"], "see_also": ["B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)", "II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "II/337 : VISTA Variables in the Via Lactea Survey DR1 (Saito+, 2012)", "II/348 : VISTA Variable in the Via Lactea Survey DR2 (Minniti+, 2017)", "II/364 : VIRAC. The VVV Infrared Astrometric Catalogue (Smith+, 2019)", "J/AJ/87/1515 : UBV photometry of AB stars in halo (Pier, 1982)", "J/ApJS/67/461 : Candidate field horizontal-branch stars catalog (Beers+, 1988)", "J/ApJS/103/433 : Horizontal-branch and A-type star catalog. II (Beers+ 1996)", "J/A+A/431/143 : Field HB stars in the Galaxy (Christlieb+, 2005)", "J/ApJS/168/277 : HK-Survey field horizontal-branch candidates (Beers+, 2007)", "J/AJ/135/564 : Photometry and spectroscopy of BHB candidates (Brown+, 2008)", "J/ApJ/684/1143 : BHB candidates in the Milky Way (Xue+, 2008)", "J/AJ/137/4377 : List of SEGUE plate pairs (Yanny+, 2009)", "J/A+A/522/A88 : Photometric identification of BHB stars (Smith+, 2010)", "J/AJ/141/83 : Kepler Mission. I. Eclipsing binaries in DR1 (Prsa+, 2011)", "J/ApJ/731/119 : BHB candidates in Sagittarius stream (Ruhland+, 2011)", "J/AJ/149/99 : VVV globulars. I. 2MASS-GC02, Terzan 10 (Alonso-Garcia+, 2015)", "J/A+A/591/A145 : VVV Survey outer bulge RRab stars (Gran+, 2016)", "J/A+A/587/A124 : Metal-poor stars towards the Galactic bulge (Koch+, 2016)", "http://horus.roe.ac.uk/vsa/ : VSA - VISTA Science Archive"], "keyword_cds": "Binaries, eclipsing; Milky Way; Stars, horizontal branch; Photometry, infrared", "keyword_pub": "binaries: eclipsing ; Galaxy: bulge ; stars: horizontal-branch", "abstract": ["We characterize the population of blue horizontal branch (BHB) stars", "in the bulge-halo transition region of the Milky Way using the VISTA", "Variables in the Via Lactea (VVV) ESO Public Survey data. The", "selection of BHB stars is made using the globular cluster M22 as a", "reference standard and constructing color-magnitude and color-color", "diagrams with specific cuts in the ZYJHKs near-infrared passbands. A", "total of 12554 BHB stars were detected, in a region within", "-10.0{deg}<=lw=10.2{deg} and -10.2{deg}<=b<=-8.0{deg}. We provide", "accurate coordinates and near-IR photometry for this sample of BHB", "stars. We searched for overdensities of stars with sizes similar to", "those of known globular clusters and stellar streams. By comparing", "real data with Monte Carlo simulations, we conclude that the few", "overdensities detected are of low significance. We also constructed", "Ks-band light curves for the BHB stars to study their variability.", "Taking an average of 52 epochs to calculate periods and amplitudes, we", "identify hundreds of candidate eclipsing binaries and a dozen", "pulsating stars. Finally, we made some comparisons with results", "obtained in a previous study for RR Lyrae variable stars in this same", "region."], "description": ["The VISTA Variables in the Via Lactea (VVV) is a public near-IR survey", "of the inner Milky Way (Minniti+ 2010NewA...15..433M ;", "Catelan+ 2011rrls.conf..145C and Saito+ 2012A&A...537A.107S), whose", "coordinates have subarcsecond accuracy (Smith+ 2018, II/364), a", "necessary requirement in this high stellar density region. The VVV", "observations were taken with the near-IR camera VIRCAM at the 4m", "Visible and Infrared Survey Telescope for Astronomy (VISTA) located at", "ESO Cerro Paranal Observatory.", "The observations are made using the ZYJHKs filters and consist of two", "epochs in ZYJH, taken at the beginning and the end of the survey, in", "years 2010 and 2015, respectively, plus multiple epochs in the Ks", "band. The Ks-band variability campaign was carried out between 2010", "and 2016, obtaining a total of about 75 observations per field in the", "VVV bulge area.", "We search for variability by constructing light curves of all the blue", "horizontal branch (BHB) stars in our sample. See Section 4."], "type": ["OC"], "data": "", "date_update": "11-Aug-2020", "tables": [{"name": "table2.dat", "desc": "Complete parameters for the first category eclipsing binaries", "columns": [{"name": "---", "desc": "[VVV] "}, {"name": "VVV", "desc": "[515455684844/515723445466] VVV survey identifier number"}, {"name": "RAh", "desc": "[17/18] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[23/42] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Per", "desc": "[0.1/18.2] Binary period "}, {"name": "KsAmp", "desc": "[0.15/1.1] The K_s_ band amplitude "}, {"name": "Zmag", "desc": "[13.2/16.8] Apparent Z band magnitude "}, {"name": "Ymag", "desc": "[13.3/17.2] Apparent Y band magnitude "}, {"name": "Jmag", "desc": "[13/16.8] Apparent J band magnitude "}, {"name": "Hmag", "desc": "[12.8/16.6] Apparent H band magnitude "}, {"name": "Ksmag", "desc": "[12.8/16.7] Apparent K_s_ band magnitude "}, {"name": "Class", "desc": "Classification code (1) "}]}, {"name": "table3.dat", "desc": "Complete parameters for the second category of eclipsing binaries", "columns": [{"name": "---", "desc": "[VVV] "}, {"name": "VVV", "desc": "[515455684844/515723445466] VVV survey identifier number"}, {"name": "RAh", "desc": "[17/18] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[23/42] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Per", "desc": "[0.1/18.2] Binary period "}, {"name": "KsAmp", "desc": "[0.15/1.1] The K_s_ band amplitude "}, {"name": "Zmag", "desc": "[13.2/16.8] Apparent Z band magnitude "}, {"name": "Ymag", "desc": "[13.3/17.2] Apparent Y band magnitude "}, {"name": "Jmag", "desc": "[13/16.8] Apparent J band magnitude "}, {"name": "Hmag", "desc": "[12.8/16.6] Apparent H band magnitude "}, {"name": "Ksmag", "desc": "[12.8/16.7] Apparent K_s_ band magnitude "}, {"name": "Class", "desc": "Classification code (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_871_103"}} {"id": "J/ApJ/871/103", "title_cds": "Catalog of 563 stars in the Galactic Center", "title_create": "Gautam+, 2019", "year": "2019", "author": "Gautam A.K., Do T., Ghez A.M., Morris M.R., Martinez G.D., Hosek M.W., Lu J.R., Sakai S., Witzel G., Jia S., Becklin E.E., Matthews K.", "title_pub": "An adaptive optics survey of stellar variability at the Galactic center.", "first_author": "Gautam A.K.", "ref_biblio": [""], "bibcode": ["2019ApJ...871..103G"], "see_also": ["J/ApJ/470/864 : JHKL photometry of the Galactic Center (Blum+, 1996)", "J/ApJ/523/248 : Variable stars in the Galactic center (Ott+, 1999)", "J/A+A/373/608 : Early-type stars towards Galactic Center. II. (Dufton+,2001)", "J/A+A/426/81 : Kinematic analysis of the Minispiral (Paumard+, 2004)", "J/A+A/433/117 : L- & M-band imaging of the Galactic Center (Viehmann+, 2005)", "J/MNRAS/370/1979 : JHKs photometry T2Cs in globular clusters (Matsunaga+, 2006)", "J/ApJ/643/1011 : Early-type stars in the center of the Galaxy (Paumard+,2006)", "J/ApJ/659/1241 : Stellar variability in Galactic Center (Rafelski+, 2007)", "J/ApJ/697/1741 : Warped disks of YSOs in Galactic center (Bartko+, 2009)", "J/ApJ/703/1323 : Spectroscopy of stars in Galaxy's nuclear cluster (Do+ 2009)", "J/MNRAS/399/1709 : Near-infrared survey of Miras (Matsunaga+, 2009)", "J/ApJ/723/1195 : SAGE AGB candidates (Riebel+, 2010)", "J/A+A/511/A18 : NIR observations of stars near SgrA* (Schoedel+, 2010)", "J/ApJ/725/331 : Astrometry in the Galactic Center (Yelda+, 2010)", "J/A+A/537/A146 : Stellar models (rotation 0.8"], "bibcode": ["2019ApJ...886...20Y"], "see_also": ["J/ApJS/166/298 : Spectral cat. of bright BATSE gamma-ray bursts (Kaneko+, 2006)", "J/ApJ/756/112 : Fermi/GBM GRB time-resolved spectral analysis (Lu+, 2012)", "J/ApJS/216/32 : Localizations of GRBs with Fermi GBM (Connaughton+, 2015)", "J/A+A/588/A135 : Fermi/GBM GRB time-resolved spectral catalog (Yu+, 2016)", "J/ApJS/223/28 : The third Fermi/GBM GRB catalog (6yr) (Bhat+, 2016)", "http://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html : Fermi GBM burst"], "keyword_cds": "GRB", "keyword_pub": "catalogs ; gamma-ray burst: general ; methods: statistical", "abstract": ["We performed time-resolved spectroscopy on a sample of 38 single", "pulses from 37 gamma-ray bursts detected by the Fermi/Gamma-ray Burst", "Monitor during the first 9yr of its mission. For the first time a", "fully Bayesian approach is applied. A total of 577 spectra are", "obtained and their properties studied using two empirical photon", "models, namely the cutoff power law (CPL) and Band model. We present", "the obtained parameter distributions, spectral evolution properties,", "and parameter relations. We also provide the result files containing", "this information for usage in further studies. It is found that the", "CPL model is the preferred model, based on the deviance information", "criterion and the fact that it consistently provides constrained", "posterior density maps. In contrast to previous works, the high-energy", "power-law index of the Band model, {beta}, has in general a lower", "value for the single pulses in this work. In particular, we", "investigate the individual spectrum in each pulse, that has the", "largest value of the low-energy spectral indexes, {alpha}. For these", "38 spectra, we find that 60% of the {alpha} values are larger than", "-2/3, and thus incompatible with synchrotron emission. Finally, we", "find that the parameter relations show a variety of behaviors. Most", "noteworthy is the fact that the relation between {alpha} and the", "energy flux is similar for most of the pulses, independent of any", "evolution of the other parameters."], "description": ["In summary, we have defined a sample of 38 single pulses from 37 GRBs", "out of 2050 Fermi/GBM detected bursts from 2008 July until 2017 March.", "A total of 577 time-resolved spectra were obtained and their spectral", "properties investigated using a fully Bayesian method."], "type": ["OC"], "data": "", "date_update": "31-Mar-2021", "tables": [{"name": "table1.dat", "desc": "GRB, detectors, source and background intervals used in the analysis", "columns": [{"name": "Fermi", "desc": "[81009140/170114917] GRB identifier ( in Simbad)"}, {"name": "Det", "desc": "Detectors (1) "}, {"name": "b_delTs", "desc": "[-5/160] Source lower range {Delta}T_src_ "}, {"name": "B_delTs", "desc": "[9/200] Source upper range {Delta}T_src_ "}, {"name": "b_delTb1", "desc": "[-40/100] First background lower range {Delta}T_bkg,1_"}, {"name": "B_delTb1", "desc": "[-15/150] First background upper range {Delta}T_bkg,1_"}, {"name": "b_delTb2", "desc": "[0/250]? Second background lower range {Delta}T_bkg,2_"}, {"name": "B_delTb2", "desc": "[30/300]? Second background upper range {Delta}T_bkg,2_"}, {"name": "b_delTb3", "desc": "[0/60]? Third background lower range {Delta}T_bkg,3_"}, {"name": "B_delTb3", "desc": "[80/80]? Third background upper range {Delta}T_bkg,3_"}, {"name": "N", "desc": "[8/30] The number of time bins using Bayesian blocks across the source interval"}, {"name": "Ns", "desc": "[5/19] The number of time bins with statistical significance of at least 20"}, {"name": "a-Ep", "desc": "{alpha}-E_p_ type (2) "}, {"name": "r(a-Ep)", "desc": "[-0.86/0.93] Spearman's rank coefficient for {alpha}-E_p_"}, {"name": "F-Ep", "desc": "[1/3] F-E_p_ type (2) "}, {"name": "r(F-Ep)", "desc": "[-0.83/0.95] Spearman's rank coefficient for F-E_p_"}, {"name": "F-a", "desc": "[1/3] F-{alpha} type (2) "}, {"name": "r(F-a)", "desc": "[-0.71/0.98] Spearman's rank coefficient for F-{alpha}"}, {"name": "Evol", "desc": "Evolutionary trend of the peak energy (3) "}]}, {"name": "table3.dat", "desc": "Time-resolved spectral analysis results ", "columns": [{"name": "---", "desc": "[GRB] "}, {"name": "Fermi", "desc": "GRB identifier "}, {"name": "---", "desc": "[;] "}, {"name": "m_Fermi", "desc": "Pulse identifier "}, {"name": "tStart", "desc": "[-5/194] Start time of Bayesian block time bin"}, {"name": "tStop", "desc": "[-4/200] Stop time of Bayesian block time bin"}, {"name": "S", "desc": "[-4.4/197] Significance of the bin "}, {"name": "K", "desc": "[0.009/737] Best-fit CPL normalization parameter"}, {"name": "E_K", "desc": "[0.0002/427] Upper uncertainty in K "}, {"name": "e_K", "desc": "[0.007/401] Lower uncertainty in K "}, {"name": "alpha", "desc": "[-2.9/0.5] Best-fit CPL low-energy power-law index"}, {"name": "E_alpha", "desc": "[0/0.7] Uncertainty in alpha "}, {"name": "e_alpha", "desc": "[0.02/1.1] Uncertainty in alpha "}, {"name": "Ec", "desc": "[14/44331] Best-fit CPL cutoff energy "}, {"name": "E_Ec", "desc": "[0.8/13666] Upper uncertainty in Ec "}, {"name": "e_Ec", "desc": "[2.1/35094] Lower uncertainty in Ec "}, {"name": "Ep", "desc": "[-4024/57237] Derived CPL peak energy "}, {"name": "E_Ep", "desc": "[0.04/17645] Upper uncertainty in Ep "}, {"name": "e_Ep", "desc": "[0.2/45310] Lower uncertainty in Ep "}, {"name": "F", "desc": "[1e-9/2.6e-5] Derived CPL energy flux; erg/s/cm^2^"}, {"name": "E_F", "desc": "[1e-8/0.00011] Upper uncertainty in F "}, {"name": "e_F", "desc": "[1e-9/1.3e-5] Lower uncertainty in F "}, {"name": "K-B", "desc": "[0.0008/405] Best-fit BAND normalization parameter"}, {"name": "E_K-B", "desc": "[2e-5/154] Upper uncertainty in K-B "}, {"name": "e_K-B", "desc": "[0.0005/402] Lower uncertainty in K-B "}, {"name": "alpha-B", "desc": "[-1.8/2.5] Best-fit BAND low-energy power-law index"}, {"name": "E_alpha-B", "desc": "[0.01/3.3] Upper uncertainty in alpha-B"}, {"name": "e_alpha-B", "desc": "[0/3.1] Lower uncertainty in alpha-B "}, {"name": "Beta-B", "desc": "[-4.7/-1.6] Best-fit BAND high-energy power-law index"}, {"name": "E_Beta-B", "desc": "[0.03/1.7] Upper uncertainty in Beta-B"}, {"name": "e_Beta-B", "desc": "[0/1.7] Lower uncertainty in Beta-B "}, {"name": "Ep-B", "desc": "[10.4/8499] Derived BAND peak energy "}, {"name": "E_Ep-B", "desc": "[0.08/2007] Upper uncertainty in Ep-B "}, {"name": "e_Ep-B", "desc": "[0.4/4879] Lower uncertainty in Ep-B "}, {"name": "F-B", "desc": "[4.2e-9/0.96]? Derived BAND energy flux; erg/s/cm^2^ (1)"}, {"name": "E_F-B", "desc": "[6.2e-8/87]? Upper uncertainty in F-B (1)"}, {"name": "e_F-B", "desc": "[9.4e-10/8.5e-6]? Lower uncertainty in F-B (1)"}, {"name": "DeltaDIC", "desc": "[-145665983/3843] Difference in deviance information criterion between CPL and BAND"}, {"name": "PDIC", "desc": "[-1123/3] Effective number of CPL parameters"}, {"name": "PDIC-B", "desc": "[-145665980/4] Effective number of BAND parameters"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_27"}} {"id": "J/ApJ/886/27", "title_cds": "SNIIP progenitors. I. LMC giant comparison sample", "title_create": "Wagle+, 2019", "year": "2019", "author": "Wagle G.A., Ray A., Dev A., Raghu A.", "title_pub": "Type IIP supernova progenitors and their explodability. I. Convective overshoot, blue loops, and surface composition.", "first_author": "Wagle G.A.", "ref_biblio": [""], "bibcode": ["2019ApJ...886...27W"], "see_also": ["J/A+AS/96/269 : Stellar Models from 0.8 to 120 Msolar (Schaller+, 1992)", "J/A+A/466/277 : VLT-FLAMES survey of massive stars (Hunter+, 2007)", "J/A+A/496/841 : VLT-FLAMES survey of massive stars (Hunter+, 2009)", "J/MNRAS/395/1409 : Type II-P SN progenitor constraints (Smartt+, 2009)", "J/A+A/545/A43 : HII regions in NGC 628 and NGC 6946 (Cedres+, 2012)", "J/ApJ/749/177 : Yellow and red supergiants in the LMC (Neugent+, 2012)", "J/AJ/154/102 : LMC blue supergiants spectroscopic obs. (Urbaneja+, 2017)"], "keyword_cds": "Supernovae; Stars, giant; Spectral types; Extinction; Colors; Models; Photometry, UBV; Infrared sources", "keyword_pub": "Core-collapse supernovae ; Stellar evolutionary models ; Computational methods ; Massive stars ; Stellar convective zones ; Type II supernovae ; Blue loop ; Supergiant stars", "abstract": ["We present the evolution of massive star progenitors of supernovae of", "type IIP. We take the example of the nearby and well-studied SN2013ej.", "We explore how convective overshoot affects the stellar structure,", "surface abundances, and effective temperature of massive stars, using", "the Modules for Experiments in Stellar Astrophysics. In particular,", "models with moderate overshoot (f=0.02-0.031) show the presence of", "blue loops in the Hertzsprung-Russell diagram with a red to blue", "excursion (log_10_[Teff/K] from <3.6 to >4.0) and transition back to", "red, during the core helium-burning phase. Models with overshoot", "outside this range of f values kept the star in the red supergiant", "state throughout the post-helium-ignition phases. The surface CNO", "abundance shows enrichment post-main-sequence and again around the", "time when helium is exhausted in the core. These evolutionary changes", "in surface CNO abundance are indistinguishable in the currently", "available observations due to large observational uncertainties.", "However, these observations may distinguish between the ratio of", "surface nitrogen to oxygen at different evolutionary stages of the", "star. We also compare the effects of convective overshoot on various", "parameters related to likelihood of explosion of a star as opposed to", "collapse to a black hole. These parameters are the compactness", "parameter, M_4_, and {mu}_4_. The combination {mu}_4_xM_4_, and", "{mu}_4_ have similar variations with f and both peak at f=0.032. We", "find that all of our 13M_{sun}_ models are likely to explode."], "description": ["In Section 4, we outline the method of selection of observational data", "of supergiants to compare with our model calculations in the", "Hertzsprung-Russell diagram (HRD) and the evolution of surface", "composition.", "In brief, the stars plotted in Figure 1 include red supergiant (RSG)", "and yellow supergiant (YSG) candidates selected from", "Neugent+ (2012, J/ApJ/749/177) and blue supergiant (BSG) candidates", "selected from Urbaneja+ (2017, J/AJ/154/102).", "We selected 323 YSG+RSG candidates that belong to the Large Magellanic", "Cloud (LMC; labeled Category 1) and had the spectral type reported in", "Neugent+ (2012, J/ApJ/749/177). We then restricted the RSG candidates", "within the luminosity range 4.2"], "bibcode": ["2019ApJ...886...33L"], "see_also": ["VIII/82 : 2nd Epoch Molonglo Galactic Plane Survey (MGPS-2) (Murphy+, 2007)", "II/328 : AllWISE Data Release (Cutri+ 2013)", "J/ApJ/269/352 : Quasar evolution (Schmidt+, 1983)", "J/ApJS/95/1 : Atlas of Quasar Energy Distributions (Elvis+ 1994)", "J/ApJ/613/682 : AGN central masses & broad-line region sizes (Peterson+, 2004)", "J/ApJ/640/579 : Near-infrared spectra of 27 SDSS quasars (Glikman+, 2006)", "J/PASP/119/994 : MIPS 24um calibrators (Engelbracht+, 2007)", "J/ApJ/666/806 : SED of Spitzer quasars (QUEST) (Netzer+, 2007)", "J/AJ/136/2373 : Type 2 quasars from SDSS (Reyes+, 2008)", "J/ApJ/696/870 : Catalina Real-time Transient Survey (CRTS) (Drake+, 2009)", "J/ApJ/698/895 : Variations in QSOs optical flux (Kelly+, 2009)", "J/AJ/142/3 : 1.4GHz observations of Stripe 82 (Hodge+, 2011)", "J/ApJ/788/159 : 17 Seyfert 1 galaxies light curves (Koshida+, 2014)", "J/ApJ/792/30 : NEOWISE magnitudes for near-Earth objects (Mainzer+, 2014)", "J/A+A/561/L8 : BRJK photometry of Seyfert galaxy WPVS48 (Pozo Nunez+, 2014)", "J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)", "J/ApJS/214/23 : IR spectra and photometry of z<0.5 quasars (Shi+, 2014)", "J/ApJS/216/17 : AKARI 2.5-5um spectra of nearby Type-1 AGNs (Kim+, 2015)", "J/AJ/149/11 : Spectra of candidate standard stars in mid-IR (Sloan+, 2015)", "J/ApJ/801/127 : 3.6um, 4.5um, B & V light curves of NGC 6418 (Vazquez+, 2015)", "J/ApJ/831/168 : 6GHz JVLA obs. of low-z SDSS quasars (Kellermann+, 2016)", "J/ApJS/224/26 : SEDs of Roma BZCAT blazars (Mao+, 2016)", "J/ApJ/836/186 : Continuum-band lags in SDSS QSOs from PS1 obs. (Jiang+, 2017)", "J/ApJ/841/76 : Intrinsic far-IR SED of luminous AGNs (Lyu+, 2017)", "J/MNRAS/471/59 : Intrinsic AGN SEDs in PG quasars (Lani+, 2017)", "J/A+A/620/A137 : CCD B,V,R,I,Ha photometry of 3C120 (Ramolla+, 2018)"], "keyword_cds": "Active gal. nuclei; Photometry, infrared; Redshifts; Surveys", "keyword_pub": "Active galactic nuclei ; Quasars ; Radio loud quasars ; Radio quiet quasars ; Infrared astronomy ; Reverberation mapping ; Time series analysis ; Dust continuum emission ; Extragalactic astronomy ; Supermassive black holes ; Infrared galaxies", "abstract": ["The continued operation of the Wide-field Infrared Survey Explorer", "(WISE), combined with several ground-based optical transient surveys", "(e.g., CRTS, ASAS-SN, and PTF), offers an unprecedented opportunity to", "explore the dust structures in luminous active galactic nuclei (AGNs).", "We use these data for a mid-IR dust reverberation mapping (RM) study", "of 87 archetypal Palomar-Green quasars at z<~0.5. To cope with various", "contaminations of the photometry data and the sparse time sampling of", "the light curves, procedures to combine these data sets and retrieve", "the dust RM signals have been developed. We find that ~70% of the", "sample (with a completeness correction up to 95%) has convincing", "mid-IR time lags in the WISE W1 (~3.4{mu}m) and W2 (~4.5{mu}m) bands,", "and they are proportional to the square root of the AGN luminosity.", "Combined with previous K-band (~2.2{mu}m) RM results in the", "literature, the inferred dust emission size ratios are", "R_K_:R_W1_:R_W2_=0.6:1:1.2. Under simple assumptions, we put", "preliminary constraints on the projected dust surface density at these", "bands and reveal the possibly different torus structures among", "hot-dust-deficient, warm-dust-deficient, and normal quasars from the", "reverberation signals. With multi-epoch Spitzer data and later WISE", "photometry, we also explore AGN IR variability at 10-24{mu}m over a", "5yr timescale. Except for blazars and flat-spectrum radio sources, the", "majority of AGNs have typical variation amplitudes at 24{mu}m of no", "more than 10% of that in the W1 band, indicating that the dust", "reverberation signals damp out quickly at longer wavelengths. In", "particular, steep-spectrum radio quasars also lack strong 24{mu}m", "variability, consistent with the unification picture of radio-loud", "AGNs."], "description": ["We collected optical photometry of the Palomar-Green (PG) quasars from", "the Catalina Real-Time Transient Survey (CRTS;", "Drake+ 2009, J/ApJ/696/870). This program utilizes two Steward", "Observatory telescopes, a 1.5m telescope on Mt. Lemmon, Arizona, and a", "0.68m telescope on Mt. Bigelow, Arizona. Both survey the northern sky,", "covering timescales from minutes to years. We gathered the 2005-2013", "photometry values from the public archive of the second data release.", "We also utilized the V-band optical data from the All-Sky Automated", "Survey for Supernovae (ASAS-SN; Shappee+, 2014, J/ApJ/788/48), which", "are publicly available at the ASAS-SN light-curve servers", "(Kochanek+ 2017PASP..129j4502K). The data were obtained through a", "global network of 20 14cm diameter telescopes (camera lenses) with", "commercial-level CCD cameras that have observed nearly the entire sky", "continuously since 2012.", "Finally, we gathered the optical time-sequence photometry for the PG", "quasars from the Palomar Transient Factory (PTF; Law+ 2009PASP..121.1395L)", "Data Release 3 (DR3), which includes all data collected during the", "survey from 2009 March to 2012 December and some selected data", "obtained from 2013 to 2015 January. This survey was done with the", "Palomar 48 inch (1.2m) Samuel Oschin Telescope with a typical 2.0\"", "FWHM imaging resolution.", "We gathered all of the single-epoch profile-fit photometry", "measurements in the W1 (~3.4um) and W2 (~4.6um) bands from the WISE", "and NEOWISE missions, up to the NEOWISE 2019 Data Release, from the", "NASA/IPAC Infrared Science Archive. Typically, these data cover a time", "period from 2010 January to 2018 December with a 3yr gap between 2011", "and 2014. Each object was observed for 12-13 epochs, with 10-20 exposures", "acquired within each epoch.", "To test for variability at {lambda}>20um, we obtained MIPS 24um", "measurements (PID 40053 and PID 50099; PI: George Rieke) of a", "heterogeneous sample of quasars that had been measured at the same", "wavelength by Spitzer for various previous observing programs. All of", "the observations were conducted during the Spitzer cryogenic mission", "from 2004 to 2009 and sample a time interval of 3-4yr.", "To extend the time sampling to 2010, we collected WISE W4 measurements", "at 22um for 136 of these objects from the ALLWISE Source Catalog.", "Low-resolution (R~60-130) mid-IR spectroscopic observations of all 87", "PG quasars were obtained using the Spitzer IRS."], "type": ["OC"], "data": "", "date_update": "01-Apr-2021", "tables": [{"name": "table2.dat", "desc": "Quasar flux measurements at 24 microns and the variability results for 139 sources", "columns": [{"name": "Name", "desc": "Quasar identifier "}, {"name": "z", "desc": "[0.003/0.5]? Redshift "}, {"name": "JD", "desc": "[3058.1/5409] Julian Date; JD-2450000 "}, {"name": "f_JD", "desc": "[a] Flag on JD (1) "}, {"name": "F24", "desc": "[1.1/2882.8]? The 24 micron flux density "}, {"name": "e_F24", "desc": "[0.2/65.3]? Uncertainty in F24 "}, {"name": "StDev", "desc": "[0/71.1]? Standard deviation of flux density change "}, {"name": "Comm", "desc": "Comments "}, {"name": "Flag", "desc": "[bcdef] Flag (1) "}]}, {"name": "table4.dat", "desc": "Summary of the mid-IR reverberation properties ", "columns": [{"name": "Name", "desc": "Quasar identifier "}, {"name": "z", "desc": "[0.03/0.47] Redshift "}, {"name": "SED", "desc": "IR SED type from Lyu+ 2017ApJ...835..257L "}, {"name": "Lbol", "desc": "[10.6/13.4] AGN bolometric luminosity (1) "}, {"name": "loge-s", "desc": "[-2.88/1.09] DRW model amplitude (log_e_({sigma})) (2)"}, {"name": "loge-t", "desc": "[2.66/7.74] DRW model timescale (log_e_({tau})) (2)"}, {"name": "delt", "desc": "[79.6/2607.5] IR dust time-lag (observed frame) from WISE W1-band light curves"}]}, {"name": "table5.dat", "desc": "PG quasar variability at 12 and 22 microns ", "columns": [{"name": "Name", "desc": "Quasar identifier (1) "}, {"name": "MJD-12", "desc": "[52989.7/55387.5] Modified Julian Date of 12 micron observation"}, {"name": "F12", "desc": "[10/478.2]? WISE (W3) 12um flux density "}, {"name": "e_F12", "desc": "[0.27/15]? Uncertainty in F12 "}, {"name": "StDev-12", "desc": "[-4.8/6.4]? Standard deviation of 12um flux density change"}, {"name": "DelM-W3", "desc": "[0/0.3]? WISE W3 band magnitude change "}, {"name": "MJD-22", "desc": "[52989.7/55387.5]? Modified Julian Date of 22 micron observation"}, {"name": "F22", "desc": "[12/893]? WISE (W4) 22um flux density "}, {"name": "e_F22", "desc": "[0.7/19.1]? Uncertainty in F22 "}, {"name": "StDev-22", "desc": "[-2.6/10.3]? Standard deviation of 22um flux density change"}, {"name": "DelM-W4", "desc": "[0/0.4]? WISE W4 band magnitude change "}, {"name": "Comm", "desc": "Comment "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_40"}} {"id": "J/ApJ/886/40", "title_cds": "Most luminous SPIRITS IR transients follow-up obs.", "title_create": "Jencson+, 2019", "year": "2019", "author": "Jencson J.E., Kasliwal M.M., Adams S.M., Bond H.E., De K., Johansson J., Karambelkar V., Lau R.M., Tinyanont S., Ryder S.D., Cody A.M., Masci F.J., Bally J., Blagorodnova N., Castellon S., Fremling C., Gehrz R.D., Helou G., Kilpatrick C.D., Milne P.A., Morrell N., Perley D.A., Phillips M.M., Smith N., van Dyk S.D., Williams R.E.", "title_pub": "The SPIRITS sample of luminous infrared transients: uncovering hidden supernovae and dusty stellar outbursts in nearby galaxies.", "first_author": "Jencson J.E.", "ref_biblio": [""], "bibcode": ["2019ApJ...886...40J"], "see_also": ["J/ApJ/469/355 : Teff, B-V and BC relation (Flower, 1996)", "J/AJ/126/1607 : IRAS Revised Bright Galaxy Sample (Sanders+, 2003)", "J/A+A/465/71 : 21cm observations of 452 galaxies (Theureau+, 2007)", "J/ApJ/705/1364 : MIR catalog of point sources in M33 (Thompson+, 2009)", "J/MNRAS/408/181 : CN2002ch UBVRI and ugriz light curves (Pastorello+, 2010)", "J/PASP/122/1397 : Spitzer Survey of Stellar Structure in Gal. (Sheth+, 2010)", "J/ApJ/743/118 : BVRIJHK phot. of the 2008 OT in NGC 300 (Humphreys+, 2011)", "J/A+A/532/A104 : Hubble flow around Fornax cluster (Nasonova+, 2011)", "J/ApJ/771/59 : Surface brightness of S4G face-on gal. (Munoz-Mateos+, 2013)", "J/AJ/146/86 : Cosmicflows-2 catalog (Tully+, 2013)", "J/ApJ/788/L21 : Measured photometry of SN 2014J from HST (Amanullah+, 2014)", "J/MNRAS/444/527 : Tully-Fisher distances for Spitzer galaxies (Sorce+, 2014)", "J/A+A/584/A62 : SUDARE VST-OmegaCAM search SN rates (Cappellaro+, 2015)", "J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. (Riess+, 2016)", "J/ApJ/834/107 : Follow-up photometry of M101 OT2015-1 (Blagorodnova+, 2017)", "J/ApJ/839/88 : 14 unusual IR transients with Spitzer (Kasliwal+, 2017)", "J/ApJS/228/5 : Spitzer phot. of ~1million stars in M31 & M15 (Khan, 2017)", "J/ApJ/866/87 : VLA 22GHz water masers obs. in NGC6334I-MM1 (Brogan+, 2018)", "J/ApJ/861/63 : Type IIP SN 2016bkv LCs and spectra (Hosseinzadeh+, 2018)", "J/ApJ/853/62 : Optical & NIR spectra and LCs of SN2016ija (Tartaglia+, 2018)", "J/ApJ/877/110 : SPIRITS cat. of IR long period variables (Karambelkar+, 2019)", "J/ApJS/241/38 : A comprehensive analysis of Spitzer SNe (Szalai+, 2019)", "J/A+A/623/A173 : SNe/SNRs in starburst galaxy Arp 220 (Varenius+, 2019)"], "keyword_cds": "Infrared sources; Supernovae; Surveys; Extinction; Photometry, infrared; Spectra, infrared; Optical", "keyword_pub": "dust, extinction ; infrared: general ; stars: massive ; supernovae: general ; supernovae: individual (SPIRITS 14buu, SPIRITS 15c, SPIRITS 15ud, SPIRITS 16ix, SPIRITS 16tn, SPIRITS 17lb)", "abstract": ["We present a systematic study of the most luminous (MIR [Vega", "magnitudes] brighter than -14) infrared (IR) transients discovered by", "the SPitzer InfraRed Intensive Transients Survey (SPIRITS) between", "2014 and 2018 in nearby galaxies (D<35Mpc). The sample consists of", "nine events that span peak IR luminosities of M_[4.5],peak_ between", "-14 and -18.2, show IR colors between 0.2<([3.6]-[4.5])<3.0, and fade", "on timescales between 55d12) show multiple, luminous IR outbursts over several years and", "have directly detected, massive progenitors in archival imaging. With", "analyses of extensive, multiwavelength follow-up, we suggest the", "following possible classifications: five obscured core-collapse", "supernovae (CCSNe), two erupting massive stars, one luminous red nova,", "and one intermediate-luminosity red transient. We define a control", "sample of all optically discovered transients recovered in SPIRITS", "galaxies and satisfying the same selection criteria. The control", "sample consists of eight CCSNe and one Type Iax SN. We find that 7 of", "the 13 CCSNe in the SPIRITS sample have lower bounds on their", "extinction of 2"], "bibcode": ["2019ApJ...886...42D"], "see_also": ["VII/259 : 6dF galaxy survey final redshift release (Jones+, 2009)", "J/ApJS/98/477 : Optical spectral atlas of Seyfert nuclei (Ho+ 1995)", "J/ApJS/115/185 : 3C 390.3 BVRI and H photometry (Dietrich+, 1998)", "J/A+A/369/57 : Monitoring Mkn 279 in BVRI & H{beta} (Santos-Lleo+, 2001)", "J/ApJ/613/682 : AGN masses & broad-line region sizes (Peterson+, 2004)", "J/ApJS/164/81 : Spectrophotometry of nearby galaxies (Moustakas+, 2006)", "J/ApJ/667/131 : Mass function of active black holes (Greene+, 2007)", "J/ApJ/683/L115 : Intermediate-line region in quasars (Hu+, 2008)", "J/ApJ/687/78 : FeII emission in quasars (Hu+, 2008)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/ApJ/755/60 : Reverberation mapping for 5 Seyfert 1 galaxies (Grier+, 2012)", "J/MNRAS/431/836 : Type 1 AGN at low z. III. (Stern+, 2013)", "J/ApJ/782/45 : SEAMBHs. I. Mrk 142, Mrk 335 and IRAS F12397+3333 (Du+, 2014)", "J/ApJ/795/38 : Phot./sp. measurements for KA1858+4850 (Pei+, 2014)", "J/ApJ/795/149 : Reverberation mapping of NGC 7469 (Peterson+, 2014)", "J/ApJ/793/108 : SEAMBHs. II. Continuum and Hbeta LCs (Wang+, 2014)", "J/ApJS/217/26 : Lick AGN monitoring 2011: light curves (Barth+, 2015)", "J/ApJ/806/22 : SEAMBHs IV. H{beta} time lags (Du+, 2015)", "J/ApJ/806/129 : Space telescope RM project. II. Swift data (Edelson+, 2015)", "J/ApJS/216/4 : SDSS-RM project: technical overview (Shen+, 2015)", "J/ApJ/804/L15 : SDSS-DR7 broad-line QSOs (Sun+, 2015)", "J/ApJ/825/126 : SEAMBHs. V. The third year (Du+, 2016)", "J/ApJ/818/L14 : RM AGNs accretion rates and BH masses (Du+, 2016)", "J/ApJ/827/118 : A new reverberation mapping campaign on NGC 5548 (Lu+, 2016)", "J/ApJ/818/30 : Lag measurements for z<0.8 QSOs from SDSS-RM (Shen+, 2016)", "J/ApJ/840/97 : Optical RM campaign of 5 AGNs (Fausnaugh+, 2017)", "J/ApJ/851/21 : SDSS RM project first year of observations (Grier+, 2017)", "J/ApJ/837/131 : Space telescope RM project. V. NGC5548 (Pei+, 2017)", "J/ApJ/866/133 : Continuum-H{beta} LCs of 5 Seyfert 1 (De Rosa+, 2018)", "J/ApJ/869/142 : Monitoring AGNs with H{beta} Asymmetry (MAHA). I. (Du+, 2018)", "J/ApJ/856/6 : SEAMBHs IX. 10 new H{beta} light curves (Du+, 2018)", "J/A+A/620/A118 : Highly Accreting Quasars: SDSS Low z Catalog (Negrete+, 2018)", "J/ApJ/876/49 : 10yr reverberation mapping campaign for 3C273 (Zhang+, 2019)"], "keyword_cds": "Active gal. nuclei; Equivalent widths; Black holes; Spectroscopy; Optical", "keyword_pub": "Active galactic nuclei ; Active galaxies ; Reverberation mapping ; Supermassive black holes ; Quasars", "abstract": ["The radius-luminosity (R_H{beta}_-L_5100_) relationship of active", "galactic nuclei (AGNs) established by the reverberation mapping (RM)", "observations has been widely used as a single-epoch black hole mass", "estimator in the research of large AGN samples. However, the recent RM", "campaigns discovered that the AGNs with high-accretion rates show", "shorter time lags by factors of a few comparing with the predictions", "from the R_H{beta}-L_5100_ relationship. The explanation of the", "shortened time lags has not been finalized yet. We collect eight", "different single-epoch spectral properties to investigate how the", "shortening of the time lags correlates with those properties and to", "determine the origin of the shortened lags. We find that the flux", "ratio between FeII and H{beta} emission lines shows the most prominent", "correlation, thus confirming that accretion rate is the main driver", "for the shortened lags. In addition, we establish a new scaling", "relation including the relative strength of FeII emission. This new", "scaling relation can provide less biased estimates of the black hole", "mass and accretion rate from the single-epoch spectra of AGNs."], "type": ["CCC"], "data": "", "date_update": "09-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Reverberation mapped AGNs and their results ", "columns": [{"name": "ID", "desc": "Object identifier (1) "}, {"name": "f_ID", "desc": "[*] Flag on ID (2) "}, {"name": "tauHb", "desc": "[1.4/252] H{beta} time lag "}, {"name": "e_tauHb", "desc": "[0.3/62] Lower uncertainty in tauHb "}, {"name": "E_tauHb", "desc": "[0.4/61] Upper uncertainty in tauHb "}, {"name": "logL5100", "desc": "[41.54/45.92] Log luminosity at 5100{AA} in erg/s units"}, {"name": "e_logL5100", "desc": "[0.01/0.6] Uncertainty in logL5100 "}, {"name": "FWHM", "desc": "[778/13211] Full-Width at Half-Maximum "}, {"name": "e_FWHM", "desc": "[1/2203] Uncertainty in FWHM "}, {"name": "logMbh", "desc": "[5.42/9.2] Log Black Hole mass "}, {"name": "e_logMbh", "desc": "[0.03/0.9] Lower uncertainty in logMbh "}, {"name": "E_logMbh", "desc": "[0.03/0.4] Upper uncertainty in logMbh "}, {"name": "logMdot", "desc": "[-3.4/2.9] Log accrection rate "}, {"name": "e_logMdot", "desc": "[0.13/1.1] Lower uncertainty in logMdot "}, {"name": "E_logMdot", "desc": "[0.12/1.4] Upper uncertainty in logMdot "}, {"name": "logLHb", "desc": "[39.72/44.11] Log H{beta} luminosity; in erg/s units"}, {"name": "e_logLHb", "desc": "[0.01/0.4] Uncertainty in logLHb "}, {"name": "EW(Hb)", "desc": "[31.8/321.1] H{beta} equivalent width; in Angstroms units"}, {"name": "e_EW(Hb)", "desc": "[1.3/112.2] Uncertainty in EW (Hb) "}, {"name": "logLO3", "desc": "[39.49/43.24] Log [O III] luminosity; in erg/s units"}, {"name": "e_logLO3", "desc": "[0.02/0.3] Uncertainty in logLO3 "}, {"name": "EW(O3)", "desc": "[2.8/1638] The [O III] equivalent width; in Angstroms units"}, {"name": "e_EW(O3)", "desc": "[0.2/439] Uncertainty in EW (O3) "}, {"name": "Ref", "desc": "Reference code(s) (see refs.dat file) "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference code "}, {"name": "BibCode", "desc": "Bibcode of the reference "}, {"name": "Auth", "desc": "First author's name "}, {"name": "Comm", "desc": "Catalog's reference in VizieR "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_48"}} {"id": "J/ApJ/886/48", "title_cds": "Radio & opt/NIR counterparts of S2COSMOS submm galaxies", "title_create": "An+, 2019", "year": "2019", "author": "An F.X., Simpson J.M., Smail I., Swinbank A.M., Ma C., Liu D., Lang P., Schinnerer E., Karim A., Magnelli B., Leslie S., Bertoldi F., Chen C.-C., Geach J.E., Matsuda Y., Stach S.M., Wardlow J.L., Gullberg B., Ivison R.J., Ao Y., Coogan R.T., Thomson A.P., Chapman S.C., Wang R., Wang W.-H., Yang Y., Asquith R., Bourne N., Coppin K., Hine N.K., Ho L.C., Hwang H.S., Kato Y., Lacaille K., Lewis A.J.R., Oteo I., Scholtz J., Sawicki M., Smith D.", "title_pub": "Multi-wavelength properties of radio- and machine-learning-identified counterparts to submillimeter sources in S2COSMOS.", "first_author": "An F.X.", "ref_biblio": [""], "bibcode": ["2019ApJ...886...48A"], "see_also": ["II/298 : AKARI/FIS All-Sky Survey Point Source Catalogues (ISAS/JAXA, 2010)", "J/MNRAS/238/1171 : Optical/IR obs. of Radio Galaxies and QSOs (Dunlop+, 1989)", "J/ApJ/622/772 : Redshift survey of submillimeter galaxies (Chapman+, 2005)", "J/MNRAS/372/1621 : SCUBA Half-Degree Extragalactic Survey. II (Coppin+, 2006)", "J/ApJS/172/29 : XMM-Newton survey in COSMOS field. I. (Hasinger+, 2007)", "J/MNRAS/380/199 : SCUBA Half-Degree Extragalactic Survey. III (Ivison+, 2007)", "J/ApJ/707/1201 : LABOCA ECDFS Submillimeter Survey (LESS) (Weiss+, 2009)", "J/ApJ/716/348 : The XMM-Newton survey of the COSMOS field (Brusa+, 2010)", "J/ApJS/188/384 : The VLA-COSMOS survey. IV. (Schinnerer+, 2010)", "J/MNRAS/411/373 : Catalog of AKARI Deep Field South (Clements+, 2011)", "J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011)", "J/MNRAS/415/3831 : AzTEC/ASTE source catalogue (Aretxaga+, 2011)", "J/MNRAS/426/1845 : AzTEC survey of the SHADES fields. II. (Michalowski+, 2012)", "J/ApJ/768/91 : ALMA observations of LESS submm galaxies (Hodge+, 2013)", "J/A+A/556/A55 : Multi-color phot. of star-forming galaxies (Ilbert+, 2013)", "J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)", "J/ApJ/788/125 : ALMA survey of ECDFS submillimeter galaxies (Simpson+, 2014)", "J/MNRAS/442/577 : Selected ALESS submm gal. radio properties (Thomson+, 2014)", "J/ApJ/817/34 : C-COSMOS Legacy multiwavelength cat. (Marchesi+, 2016)", "J/ApJS/222/1 : Faint ALMA 1.2mm sources down to ~0.02mJy (Fujimoto+, 2016)", "J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016)", "J/ApJ/820/82 : S2CLS: multiwavelength counterparts to SMGs (Chen+, 2016)", "J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)", "J/MNRAS/465/1789 : SCUBA-2 Cosmology Legacy Survey (Geach+, 2017)", "J/ApJ/837/139 : SUPER GOODS. I. Ultradeep SCUBA-2 survey (Cowie+, 2017)", "J/ApJ/839/58 : ALMA submm galaxies multi-wavelength data (Simpson+, 2017)", "J/ApJ/840/78 : Redshift survey of ALMA SMGs in ECDFS (Danielson+, 2017)", "J/A+A/602/A1 : VLA-COSMOS 3 GHz Large Project (Smolcic+, 2017)", "J/A+A/602/A2 : VLA-COSMOS 3 GHz Large Project. II. (Smolcic+, 2017)", "J/ApJ/853/172 : \"Super-deblended\" dust emission in galaxies. I. (Liu+, 2018)", "J/ApJ/880/43 : S2COSMOS: SCUBA-2 submm sources in COSMOS (Simpson+, 2019)", "J/ApJS/244/40 : A3COSMOS. I. ALMA continuum photometry catalogs (Liu+, 2019)", "http://sites.google.com/view/a3cosmos : A3COSMOS home page"], "keyword_cds": "Millimetric/submm sources; Galaxies, radio; Cross identifications; Infrared sources; Redshifts", "keyword_pub": "Observational astronomy; Starburst galaxies; High-redshift galaxies Galaxy formation; Galaxy evolution; Submillimeter astronomy Clustering", "abstract": ["We identify multi-wavelength counterparts to 1147 submillimeter", "sources from the S2COSMOS SCUBA-2 survey of the COSMOS field by", "employing a recently developed radio+machine-learning method trained", "on a large sample of Atacama Large Millimeter/submillimeter Array", "(ALMA)-identified submillimeter galaxies (SMGs), including 260 SMGs", "identified in the AS2COSMOS pilot survey. In total, we identify 1222", "optical/near-infrared (NIR)/radio counterparts to the 897 S2COSMOS", "submillimeter sources with S_850_>1.6mJy, yielding an overall", "identification rate of (78+/-9)%. We find that (22+/-5)% of S2COSMOS", "sources have multiple identified counterparts. We estimate that", "roughly 27% of these multiple counterparts within the same SCUBA-2", "error circles very likely arise from physically associated galaxies", "rather than line-of-sight projections by chance. The photometric", "redshift of our radio+machine-learning-identified SMGs ranges from", "z=0.2 to 5.7 and peaks at z=2.3+/-0.1. The AGN fraction of our sample", "is (19+/-4)%, which is consistent with that of ALMA SMGs in the", "literature. Comparing with radio/NIR-detected field galaxy population", "in the COSMOS field, our radio+machine-learning-identified", "counterparts of SMGs have the highest star formation rates and stellar", "masses. These characteristics suggest that our identified counterparts", "of S2COSMOS sources are a representative sample of SMGs at z<~3. We", "employ our machine-learning technique to the whole COSMOS field and", "identified 6877 potential SMGs, most of which are expected to have", "submillimeter emission fainter than the confusion limit of our", "S2COSMOS surveys (S_850um_<~1.5mJy). We study the clustering", "properties of SMGs based on this statistically large sample, finding", "that they reside in high-mass dark matter halos", "((1.2+/-0.3)x10^13^h^-1^M_{sun}_), which suggests that SMGs may be the", "progenitors of massive ellipticals we see in the local universe."], "description": ["The 850um SCUBA-2 COSMOS survey (S2COSMOS) was carried out with the", "East Asian Observatory's James Clerk Maxwell Telescope (JCMT) between", "2016 January and 2017 June. The full details of observations, data", "reduction, and catalog are described in Simpson+ (2019, J/ApJ/880/43).", "We have completed an ALMA Cycle 4 pilot study of the brightest 160", "single-dish submillimeter sources from S2COSMOS", "(Project ID: 2016.1.00463.S). The ALMA follow-up observations were", "taken in Band 7 (870um) in 2018 April and May. See Section 2.2.1.", "We use additional ALMA archival data in the COSMOS field to construct", "our training set.", "The COSMOS field is one of the largest extragalactic fields with a", "rich ancillary data set.", "The radio data we use in this work are from the VLA-COSMOS 3GHz Large", "Project (Smolcic+ 2017, J/A+A/602/A1), which were taken with the Karl", "G. Jansky Very Large Array (VLA) at 3GHz.", "The COSMOS2015 catalog (Laigle+ 2016, J/ApJS/224/24) from the", "UltraVISTA-DR2 surveys are used to identify optical/NIR counterparts", "for both ALMA submillimeter galaxies and S2COSMOS submillimeter", "sources and are then used to construct a training set and a test", "sample for the machine-learning analyses.", "See Section 2.3."], "type": ["OC"], "data": "", "date_update": "09-Apr-2021", "tables": [{"name": "table2.dat", "desc": "Radio+machine-learning identified counterparts to S2COSMOS sources", "columns": [{"name": "---", "desc": "[S2COS850] "}, {"name": "---", "desc": "[.] "}, {"name": "S2COS850", "desc": "Short ID (S2COS850) of S2COSMOS source from Simpson+ 2009, J/ApJ/880/43"}, {"name": "RAdeg", "desc": "[149.3/150.9] Right ascension of S2COSMOS source (J2000)"}, {"name": "DEdeg", "desc": "[1.5/3] Declination of S2COSMOS source (J2000) "}, {"name": "RANdeg", "desc": "?=-99 RA of the NIR counterpart (J2000) "}, {"name": "DENdeg", "desc": "?=-99 DEC of the NIR counterpart (J2000) "}, {"name": "Cl-XGB", "desc": "Classification by machine-learning (1) "}, {"name": "RARdeg", "desc": "?=-99 RA of the radio counterpart (J2000) "}, {"name": "DERdeg", "desc": "?=-99 DEC of the radio counterpart (J2000) "}, {"name": "Cl-Rad", "desc": "Classification by radio identification (2) "}, {"name": "zphot", "desc": "[0/5.6]?=-99 Photometric redshift from COSMOS2015 catalog"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_61"}} {"id": "J/ApJ/886/61", "title_cds": "OGLE-III, MCPS and HST VI obs. of LMC & SMC", "title_create": "Yuan+, 2019", "year": "2019", "author": "Yuan W., Riess A.G., Macri L.M., Casertano S., Scolnic D.M.", "title_pub": "Consistent calibration of the tip of the red giant branch in the Large Magellanic Cloud on the Hubble Space Telescope photometric system and a redetermination of the Hubble constant.", "first_author": "Yuan W.", "ref_biblio": [""], "bibcode": ["2019ApJ...886...61Y"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "II/322 : OGLE-III. Magellanic Clouds stellar proper motions (Poleski+, 2012)", "II/351 : VISTA Magellanic Survey (VMC) catalog (Cioni+, 2011)", "J/AcA/49/223 : BVI photometry of OGLE LMC Cepheids (Udalski+, 1999)", "J/AcA/49/437 : BVI photometry of OGLE SMC Cepheids (Udalski+, 1999)", "J/PASP/111/812 : V(RI)C Phot of Cepheids in Magellanic Clouds (Barnes+ 1999)", "J/AJ/123/3216 : BV photometry of variable stars in SMC (Sharpee+, 2002)", "J/AJ/123/855 : Magellanic Clouds Photometric Survey: the SMC (Zaritsky+, 2002)", "J/AJ/128/1606 : Magellanic Clouds Phot. Survey (MCPS): LMC (Zaritsky+, 2004)", "J/MNRAS/353/705 : OGLE Variables in Magellanic Clouds (Ita+, 2004)", "J/MNRAS/361/1055 : BVI photometry of LMC Be stars (Sabogal+, 2005)", "J/A+A/430/421 : Reddening in LMC bar region (Subramaniam, 2005)", "J/AJ/131/407 : BV photometry of stars in the LMC (Kaluzny+, 2006)", "J/AcA/58/163 : VI light curves of LMC classical Cepheids (Soszynski+, 2008)", "J/AcA/59/239 : VI light curves of LMC long-period variables (Soszynski+, 2009)", "J/AcA/59/1 : VI light curves of LMC RR Lyrae stars (Soszynski+, 2009)", "J/AcA/61/199 : OGLE3 Magellanic Clouds High PM stars (Poleski+, 2011)", "J/ApJ/730/119 : HST/WFC3 observations of Cepheids in SN Ia hosts (Riess+, 2011)", "J/AJ/142/61 : RGB stars in LMC outer disk (Carrera+, 2011)", "J/AcA/63/159 : LMC OGLE-III Shallow Survey variable stars (Ulaczyk+, 2013)", "J/AJ/149/117 : LMC infrared survey. I. Photometry of Cepheids (Macri+, 2015)", "J/AcA/65/297 : OGLE4 LMC and SMC Cepheids (Soszynski+, 2015)", "J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. (Riess+, 2016)", "J/AJ/153/154 : LMC NIR survey. IV. Type II Cepheid variables (Bhardwaj+, 2017)", "J/ApJ/845/146 : The Carnegie-Chicago Hubble Program. II. IC 1613 (Hatt+, 2017)", "J/AJ/154/149 : LMC NIR synoptic survey. V. NIR phot. of Miras (Yuan+, 2017)", "J/ApJ/860/1 : Radial velocity measurements of 20 EBs in LMC (Graczyk+, 2018)", "J/ApJ/876/85 : HST observations for LMC Cepheids (Riess+, 2019)"], "keyword_cds": "Magellanic Clouds; Stars, giant; Photometry, HST; Photometry, VRI", "keyword_pub": "Distance indicators ; Cosmology ; Large Magellanic Cloud ; Hubble Space Telescope ; Small Magellanic Cloud", "abstract": ["We present a calibration of the tip of the red giant branch (TRGB) in", "the Large Magellanic Cloud (LMC) on the Hubble Space Telescope", "(HST)/ACS F814W system. We use archival HST observations to derive", "blending corrections and photometric transformations for two", "ground-based wide-area imaging surveys of the Magellanic Clouds. We", "show that these surveys are biased bright by up to ~0.1mag in the", "optical due to blending, and that the bias is a function of local", "stellar density. We correct the LMC TRGB magnitudes from", "Jang & Lee (2017ApJ...835...28J) and use the geometric distance from", "Pietrzynski+ (2019Natur.567..200P) to obtain an absolute TRGB", "magnitude of M_F814W_=-3.97+/-0.046mag. Applying this calibration to", "the TRGB magnitudes from Freedman+ (2019ApJ...882...34F) in SN Ia", "hosts yields a value for the Hubble constant of", "H_0_=72.4+/-2.0km/s/Mpc for their TRGB+SNe Ia distance ladder. The", "difference in the TRGB calibration and the value of H_0_ derived here", "and by Freedman+ primarily results from their overestimate of the LMC", "extinction, caused by inconsistencies in their different sources of", "TRGB photometry for the Magellanic Clouds. Using the same source of", "photometry (OGLE) for both Clouds and applying the aforementioned", "corrections yields a value for the LMC I-band TRGB extinction that is", "lower by 0.06mag, consistent with independent OGLE reddening maps", "used by us and by Jang & Lee to calibrate TRGB and determine H0."], "description": ["In order to obtain the ground-to-HST correction for the TRGB in the", "LMC, we analyzed two commonly used ground-based photometric catalogs,", "OGLE-III (Udalski+ 2008AcA....58...89U) and", "the MCPS (Zaritsky+ 2004, J/AJ/128/1606), as well as archival HST", "observations of 12 LMC fields that are covered by these ground-based", "surveys.", "We used MAST to retrieve archival HST ACS F814W and F555W observations", "(spanning 2003 Aug 8 to 2004 Jun 2) of 13 fields that are covered by", "the aforementioned ground surveys. These fields are centered on", "globular clusters NGC 1755, 1756, 1801, 1854, 1858, 1872, 1903, 1943,", "1953, 1983, 2010, 2056, and 2107, but the majority of each frame", "covers non-cluster stars."], "type": ["OC"], "data": "", "date_update": "12-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Summary of HST observations ", "columns": [{"name": "Field", "desc": "[1755/2107] NGC number "}, {"name": "Date", "desc": "Date of observation (UT) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "ExpV", "desc": "[20/170] F555W exposure time "}, {"name": "ExpI", "desc": "[20/120] F814W exposure time "}]}, {"name": "table2.dat", "desc": "HST photometry for the 12 LMC fields ", "columns": [{"name": "---", "desc": "[n] "}, {"name": "Field", "desc": "NGC identifier for HST fields "}, {"name": "ID", "desc": "[1000160/13086534] Internal photometry ID "}, {"name": "RAdeg", "desc": "[73.66/85.95] Right ascension (J2000) (1) "}, {"name": "DEdeg", "desc": "[-70.86/-68.16] Declination (J2000) (1) "}, {"name": "F814Wmag", "desc": "[14.49/17.5] HST/ACS F814W magnitude (2) "}, {"name": "e_F814Wmag", "desc": "[0.001/0.05] 1{sigma} uncertainty in F814Wmag "}, {"name": "F555Wmag", "desc": "[14.3/24.3] HST/ACS F555W magnitude "}, {"name": "e_F555Wmag", "desc": "[0.001/0.3] 1{sigma} uncertainty in F555Wmag "}]}, {"name": "table6.dat", "desc": "SMC tip of the red giant branch (TRGB)-like stars ", "columns": [{"name": "RAdeg", "desc": "[5.77/20.11] Right ascension (J2000) "}, {"name": "DEdeg", "desc": "[-74.8/-71.26] Declination (J2000) "}, {"name": "V-OGLE", "desc": "[16.26/16.82] OGLE V magnitude "}, {"name": "I-OGLE", "desc": "[14.85/15.05] OGLE I magnitude "}, {"name": "V-MCPS", "desc": "[15.4/20.01] MCPS V magnitude "}, {"name": "I-MCPS", "desc": "[14.3/15.7] MCPS I magnitude "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_75"}} {"id": "J/ApJ/886/75", "title_cds": "Search for GW signals associated with GRBs", "title_create": "Abbott+, 2019", "year": "2019", "author": "Abbott B.P., Abbott R., Abbott T.D., Abraham S., Acernese F., Ackley K., Adams C., Adhikari R.X., Adya V.B., Affeldt C., Agathos M., Agatsuma K., Aggarwal N., Aguiar O.D., Aiello L., Ain A., Ajith P., Allen G., Allocca A., Aloy M.A., Altin P.A., Amato A., Anand S., Ananyeva A., Anderson S.B., Anderson W.G., Angelova S.V., Antier S., Appert S., Arai K., Araya M.C., Areeda J.S., Arene M., Arnaud N., Aronson S.M., Ascenzi S., Ashton G., Aston S.M., Astone P., Aubin F., Aufmuth P., AultONeal K., Austin C., Avendano V., Avila-Alvarez A., Babak S., Bacon P., Badaracco F., Bader M.K.M., Bae S., Baird J., Baker P.T., Baldaccini F., Ballardin G., Ballmer S.W., Bals A., Banagiri S., Barayoga J.C., Barbieri C., Barclay S.E., Barish B.C., Barker D., Barkett K., Barnum S., Barone F., Barr B., Barsotti L., Barsuglia M., Barta D., Bartlett J., Bartos I., Bassiri R., Basti A., Bawaj M., Bayley J.C., Bazzan M., Becsy B., Bejger M., Belahcene I., Bell A.S., Beniwal D., Benjamin M.G., Berger B.K., Bergmann G., Bernuzzi S., Berry C.P.L., Bersanetti D., Bertolini A., Betzwieser J., Bhandare R., Bidler J., Biggs E., Bilenko I.A., Bilgili S.A., Billingsley G., Birney R., Birnholtz O., Biscans S., Bischi M., Biscoveanu S., Bisht A., Bitossi M., Bizouard M.A., Blackburn J.K., Blackman J., Blair C.D., Blair D.G., Blair R.M., Bloemen S., Bobba F., Bode N., Boer M., Boetzel Y., Bogaert G., Bondu F., Bonnand R., Booker P., Boom B.A., Bork R., Boschi V., Bose S., Bossilkov V., Bosveld J., Bouffanais Y., Bozzi A., Bradaschia C., Brady P.R., Bramley A., Branchesi M., Brau J.E., Breschi M., Briant T., Briggs J.H., Brighenti F., Brillet A., Brinkmann M., Brockill P., Brooks A.F., Brooks J., Brown D.D., Brunett S., Buikema A., Bulik T., Bulten H.J., Buonanno A., Buskulic D., Buy C., Byer R.L., Cabero M., Cadonati L., Cagnoli G., Cahillane C., Bustillo J.C., Callister T.A., Calloni E., Camp J.B., Campbell W.A., Canepa M., Cannon K.C., Cao H., Cao J., Carapella G., Carbognani F., Caride S., Carney M.F., Carullo G., Diaz J.C., Casentini C., Caudill S., Cavaglia M., Cavalier F., Cavalieri R., Cella G., Cerda-Duran P., Cesarini E., Chaibi O., Chakravarti K., Chamberlin S.J., Chan M., Chao S., Charlton P., Chase E.A., Chassande-Mottin E., Chatterjee D., Chaturvedi M., Cheeseboro B.D., Chen H.Y., Chen X., Chen Y., Cheng H.-P., Cheong C.K., Chia H.Y., Chiadini F., Chincarini A., Chiummo A., Cho G., Cho H.S., Cho M., Christensen N., Chu Q., Chua S., Chung K.W., Chung S., Ciani G., Cieslar M., Ciobanu A.A., Ciolfi R., Cipriano F., Cirone A., Clara F., Clark J.A., Clearwater P., Cleva F., Coccia E., Cohadon P.-F., Cohen D., Colleoni M., Collette C.G., Collins C., Colpi M., Cominsky L.R., Constancio M., Conti L., Cooper S.J., Corban P., Corbitt T.R., Cordero-Carrion I., Corezzi S., Corley K.R., Cornish N., Corre D., Corsi A., Cortese S., Costa C.A., Cotesta R., Coughlin M.W., Coughlin S.B., Coulon J.-P., Countryman S.T., Couvares P., Covas P.B., Cowan E.E., Coward D.M., Cowart M.J., Coyne D.C., Coyne R., Creighton J.D.E., Creighton T.D., Cripe J., Croquette M., Crowder S.G., Cullen T.J., Cumming A., Cunningham L., Cuoco E., Canton T.D., Dalya G., D'Angelo B., Danilishin S.L., D'Antonio S., Danzmann K., Dasgupta A., Da Silva Costa C.F., Datrier L.E.H., Dattilo V., Dave I., Davier M., Davis D., Daw E.J., DeBra D., Deenadayalan M., Degallaix J., De Laurentis M., Deleglise S., Del Pozzo W., DeMarchi L.M., Demos N., Dent T., De Pietri R., De Rosa R., De Rossi C., DeSalvo R., de Varona O., Dhurandhar S., Diaz M.C., Dietrich T., Di Fiore L., DiFronzo C., Di Giorgio C., Di Giovanni F., Di Giovanni M., Di Girolamo T., Di Lieto A., Ding B., Di Pace S., Di Palma I., Di Renzo F., Divakarla A.K., Dmitriev A., Doctor Z., Donovan F., Dooley K.L., Doravari S., Dorrington I., Downes T.P., Drago M., Driggers J.C., Du Z., Ducoin J.-G., Dupej P., Durante O., Dwyer S.E., Easter P.J., Eddolls G., Edo T.B., Effler A., Ehrens P., Eichholz J., Eikenberry S.S., Eisenmann M., Eisenstein R.A., Errico L., Essick R.C., Estelles H., Estevez D., Etienne Z.B., Etzel T., Evans M., Evans T.M., Fafone V., Fairhurst S., Fan X., Farinon S., Farr B., Farr W.M., Fauchon-Jones E.J., Favata M., Fays M., Fazio M., Fee C., Feicht J., Fejer M.M., Feng F., Fernandez-Galiana A., Ferrante I., Ferreira E.C., Ferreira T.A., Fidecaro F., Fiori I., Fiorucci D., Fishbach M., Fisher R.P., Fishner J.M., Fittipaldi R., Fitz-Axen M., Fiumara V., Flaminio R., Fletcher M., Floden E., Flynn E., Fong H., Font J.A., Forsyth P.W.F., Fournier J.-D., Vivanco F.H., Frasca S., Frasconi F., Frei Z., Freise A., Frey R., Frey V., Fritschel P., Frolov V.V., Fronze G., Fulda P., Fyffe M., Gabbard H.A., Gadre B.U., Gaebel S.M., Gair J.R., Gammaitoni L., Gaonkar S.G., Garcia-Quiros C., Garufi F., Gateley B., Gaudio S., Gaur G., Gayathri V., Gemme G., Genin E., Gennai A., George D., George J., Gergely L., Ghonge S., Ghosh A., Ghosh A., Ghosh S., Giacomazzo B., Giaime J.A., Giardina K.D., Gibson D.R., Gill K., Glover L., Gniesmer J., Godwin P., Goetz E., Goetz R., Goncharov B., Gonzalez G., Castro J.M.G., Gopakumar A., Gossan S.E., Gosselin M., Gouaty R., Grace B., Grado A., Granata M., Grant A., Gras S., Grassia P., Gray C., Gray R., Greco G., Green A.C., Green R., Gretarsson E.M., Grimaldi A., Grimm S.J., Groot P., Grote H., Grunewald S., Gruning P., Guidi G.M., Gulati H.K., Guo Y., Gupta A., Gupta A., Gupta P., Gustafson E.K., Gustafson R., Haegel L., Halim O., Hall B.R., Hall E.D., Hamilton E.Z., Hammond G., Haney M., Hanke M.M., Hanks J., Hanna C., Hannam M.D., Hannuksela O.A., Hansen T.J., Hanson J., Harder T., Hardwick T., Haris K., Harms J., Harry G.M., Harry I.W., Hasskew R.K., Haster C.J., Haughian K., Hayes F.J., Healy J., Heidmann A., Heintze M.C., Heitmann H., Hellman F., Hello P., Hemming G., Hendry M., Heng I.S., Hennig J., Heurs M., Hild S., Hinderer T., Hochheim S., Hofman D., Holgado A.M., Holland N.A., Holt K., Holz D.E., Hopkins P., Horst C., Hough J., Howell E.J., Hoy C.G., Huang Y., Hubner M.T., Huerta E.A., Huet D., Hughey B., Hui V., Husa S., Huttner S.H., Huynh-Dinh T., Idzkowski B., Iess A., Inchauspe H., Ingram C., Inta R., Intini G., Irwin B., Isa H.N., Isac J.-M., Isi M., Iyer B.R., Jacqmin T., Jadhav S.J., Jani K., Janthalur N.N., Jaranowski P., Jariwala D., Jenkins A.C., Jiang J., Johnson D.S., Jones A.W., Jones D.I., Jones J.D., Jones R., Jonker R.J.G., Ju L., Junker J., Kalaghatgi C.V., Kalogera V., Kamai B., Kandhasamy S., Kang G., Kanner J.B., Kapadia S.J., Karki S., Kashyap R., Kasprzack M., Katsanevas S., Katsavounidis E., Katzman W., Kaufer S., Kawabe K., Keerthana N.V., Kefelian F., Keitel D., Kennedy R., Key J.S., Khalili F.Y., Khan I., Khan S., Khazanov E.A., Khetan N., Khursheed M., Kijbunchoo N., Kim C., Kim J.C., Kim K., Kim W., Kim W.S., Kim Y.-M., Kimball C., King P.J., Kinley-Hanlon M., Kirchhoff R., Kissel J.S., Kleybolte L., Klika J.H., Klimenko S., Knowles T.D., Koch P., Koehlenbeck S.M., Koekoek G., Koley S., Kondrashov V., Kontos A., Koper N., Korobko M., Korth W.Z., Kovalam M., Kozak D.B., Kramer C., Kringel V., Krishnendu N., Krolak A., Krupinski N., Kuehn G., Kumar A., Kumar P., Kumar R., Kumar R., Kuo L., Kutynia A., Kwang S., Lackey B.D., Laghi D., Lai K.H., Lam T.L., Landry M., Lane B.B., Lang R.N., Lange J., Lantz B., Lanza R.K., Lartaux-Vollard A., Lasky P.D., Laxen M., Lazzarini A., Lazzaro C., Leaci P., Leavey S., Lecoeuche Y.K., Lee C.H., Lee H.K., Lee H.M., Lee H.W., Lee J., Lee K., Lehmann J., Lenon A.K., Leroy N., Letendre N., Levin Y., Li A., Li J., Li K.J.L., Li T.G.F., Li X., Lin F., Linde F., Linker S.D., Littenberg T.B., Liu J., Liu X., Llorens- Monteagudo M., Lo R.K.L., London L.T., Longo A., Lorenzini M., Loriette V., Lormand M., Losurdo G., Lough J.D., Lousto C.O., Lovelace G., Lower M.E., Luck H., Lumaca D., Lundgren A.P., Lynch R., Ma Y., Macas R., Macfoy S., MacInnis M., Macleod D.M., Macquet A., Hernandez I.M., Magana-Sandoval F., Magee R.M., Majorana E., Maksimovic I., Malik A., Man N., Mandic V., Mangano V., Mansell G.L., Manske M., Mantovani M., Mapelli M., Marchesoni F., Marion F., Marka S., Marka Z., Markakis C., Markosyan A.S., Markowitz A., Maros E., Marquina A., Marsat S., Martelli F., Martin I.W., Martin R.M., Martinez V., Martynov D.V., Masalehdan H., Mason K., Massera E., Masserot A., Massinger T.J., Masso-Reid M., Mastrogiovanni S., Matas A., Matichard F., Matone L., Mavalvala N., McCann J.J., McCarthy R., McClelland D.E., McCormick S., McCuller L., McGuire S.C., McIsaac C., McIver J., McManus D.J., McRae T., McWilliams S.T., Meacher D., Meadors G.D., Mehmet M., Mehta A.K., Meidam J., Villa E.M., Melatos A., Mendell G., Mercer R.A., Mereni L., Merfeld K., Merilh E.L., Merzougui M., Meshkov S., Messenger C., Messick C., Messina F., Metzdorff R., Meyers P.M., Meylahn F., Miani A., Miao H., Michel C., Middleton H., Milano L., Miller A.L., Millhouse M., Mills J.C., Milovich-Goff M.C., Minazzoli O., Minenkov Y., Mishkin A., Mishra C., Mistry T., Mitra S., Mitrofanov V.P., Mitselmakher G., Mittleman R., Mo G., Moffa D., Mogushi K., Mohapatra S.R.P., Molina-Ruiz M., Mondin M., Montani M., Moore C.J., Moraru D., Morawski F., Moreno G., Morisaki S., Mours B., Mow-Lowry C.M., Muciaccia F., Mukherjee A., Mukherjee D., Mukherjee S., Mukherjee S., Mukund N., Mullavey A., Munch J., Muniz E.A., Muratore M., Murray P.G., Nardecchia I., Naticchioni L., Nayak R.K., Neil B.F., Neilson J., Nelemans G., Nelson T.J.N., Nery M., Neunzert A., Nevin L., Ng K.Y., Ng S., Nguyen C., Nguyen P., Nichols D., Nichols S.A., Nissanke S., Nocera F., North C., Nuttall L.K., Obergaulinger M., Oberling J., O'Brien B.D., Oganesyan G., Ogin G.H., Oh J.J., Oh S.H., Ohme F., Ohta H., Okada M.A., Oliver M., Oppermann P., Oram R.J., O'Reilly B., Ormiston R.G., Ortega L.F., O'Shaughnessy R., Ossokine S., Ottaway D.J., Overmier H., Owen B.J., Pace A.E., Pagano G., Page M.A., Pagliaroli G., Pai A., Pai S.A., Palamos J.R., Palashov O., Palomba C., Pan H., Panda P.K., Pang P.T.H., Pankow C., Pannarale F., Pant B.C., Paoletti F., Paoli A., Parida A., Parker W., Pascucci D., Pasqualetti A., Passaquieti R., Passuello D., Patil M., Patricelli B., Payne E., Pearlstone B.L., Pechsiri T.C., Pedersen A.J., Pedraza M., Pedurand R., Pele A., Penn S., Perego A., Perez C.J., Perigois C., Perreca A., Petermann J., Pfeiffer H.P., Phelps M., Phukon K.S., Piccinni O.J., Pichot M., Piergiovanni F., Pierro V., Pillant G., Pinard L., Pinto I.M., Pirello M., Pitkin M., Plastino W., Poggiani R., Pong D.Y.T., Ponrathnam S., Popolizio P., Powell J., Prajapati A.K., Prasad J., Prasai K., Prasanna R., Pratten G., Prestegard T., Principe M., Prodi G.A., Prokhorov L., Punturo M., Puppo P., Purrer M., Qi H., Quetschke V., Quinonez P.J., Raab F.J., Raaijmakers G., Radkins H., Radulesco N., Raffai P., Raja S., Rajan C., Rajbhandari B., Rakhmanov M., Ramirez K.E., Ramos-Buades A., Rana J., Rao K., Rapagnani P., Raymond V., Razzano M., Read J., Regimbau T., Rei L., Reid S., Reitze D.H., Rettegno P., Ricci F., Richardson C.J., Richardson J.W., Ricker P.M., Riemenschneider G., Riles K., Rizzo M., Robertson N.A., Robinet F., Rocchi A., Rolland L., Rollins J.G., Roma V.J., Romanelli M., Romano R., Romel C.L., Romie J.H., Rose C.A., Rose D., Rose K., Rosinska D., Rosofsky S.G., Ross M.P., Rowan S., Rudiger A., Ruggi P., Rutins G., Ryan K., Sachdev S., Sadecki T., Sakellariadou M., Salafia O.S., Salconi L., Saleem M., Samajdar A., Sammut L., Sanchez E.J., Sanchez L.E., Sanchis- Gual N., Sanders J.R., Santiago K.A., Santos E., Sarin N., Sassolas B., Sathyaprakash B.S., Sauter O., Savage R.L., Schale P., Scheel M., Scheuer J., Schmidt P., Schnabel R., Schofield R.M.S., Schonbeck A., Schreiber E., Schulte B.W., Schutz B.F., Scott J., Scott S.M., Seidel E., Sellers D., Sengupta A.S., Sennett N., Sentenac D., Sequino V., Sergeev A., Setyawati Y., Shaddock D.A., Shaffer T., Shahriar M.S., Shaner M.B., Sharma A., Sharma P., Shawhan P., Shen H., Shink R., Shoemaker D.H., Shoemaker D.M., Shukla K., ShyamSundar S., Siellez K., Sieniawska M., Sigg D., Singer L.P., Singh D., Singh N., Singhal A., Sintes A.M., Sitmukhambetov S., Skliris V., Slagmolen B.J.J., Slaven-Blair T.J., Smith J.R., Smith R.J.E., Somala S., Son E.J., Soni S., Sorazu B., Sorrentino F., Souradeep T., Sowell E., Spencer A.P., Spera M., Srivastava A.K., Srivastava V., Staats K., Stachie C., Standke M., Steer D.A., Steinke M., Steinlechner J., Steinlechner S., Steinmeyer D., Stevenson S.P., Stocks D., Stone R., Stops D.J., Strain K.A., Stratta G., Strigin S.E., Strunk A., Sturani R., Stuver A.L., Sudhir V., Summerscales T.Z., Sun L., Sunil S., Sur A., Suresh J., Sutton P.J., Swinkels B.L., Szczepanczyk M.J., Tacca M., Tait S.C., Talbot C., Tanner D.B., Tao D., Tapai M., Tapia A., Tasson J.D., Taylor R., Tenorio R., Terkowski L., Thomas M., Thomas P., Thondapu S.R., Thorne K.A., Thrane E., Tiwari S., Tiwari S., Tiwari V., Toland K., Tonelli M., Tornasi Z., Torres- Forne A., Torrie C.I., Toyra D., Travasso F., Traylor G., Tringali M.C., Tripathee A., Trovato A., Trozzo L., Tsang K.W., Tse M., Tso R., Tsukada L., Tsuna D., Tsutsui T., Tuyenbayev D., Ueno K., Ugolini D., Unnikrishnan C.S., Urban A.L., Usman S.A., Vahlbruch H., Vajente G., Valdes G., Valentini M., van Bakel N., van Beuzekom M., van den Brand J.F.J., Van Den Broeck C., Vander-Hyde D.C., van der Schaaf L., VanHeijningen J.V., van Veggel A.A., Vardaro M., Varma V., Vass S., Vasuth M., Vecchio A., Vedovato G., Veitch J., Veitch P.J., Venkateswara K., Venugopalan G., Verkindt D., Vetrano F., Vicere A., Viets A.D., Vinciguerra S., Vine D.J., Vinet J.-Y., Vitale S., Vo T., Vocca H., Vorvick C., Vyatchanin S.P., Wade A.R., Wade L.E., Wade M., Walet R., Walker M., Wallace L., Walsh S., Wang H., Wang J.Z., Wang S., Wang W.H., Wang Y.F., Ward R.L., Warden Z.A., Warner J., Was M., Watchi J., Weaver B., Wei L.-W., Weinert M., Weinstein A.J., Weiss R., Wellmann F., Wen L., Wessel E.K., Wessels P., Westhouse J.W., Wette K., Whelan J.T., Whiting B.F., Whittle C., Wilken D.M., Williams D., Williamson A.R., Willis J.L., Willke B., Winkler W., Wipf C.C., Wittel H., Woan G., Woehler J., Wofford J.K., Wright J.L., Wu D.S., Wysocki D.M., Xiao S., Xu R., Yamamoto H., Yancey C.C., Yang L., Yang Y., Yang Z., Yap M.J., Yazback M., Yeeles D.W., Yu H., Yu H., Yuen S.H.R., Zadrozny A.K., Zadrozny A., Zanolin M., Zelenova T., Zendri J.-P., Zevin M., Zhang J., Zhang L., Zhang T., Zhao C., Zhao G., Zhou M., Zhou Z., Zhu X.J., Zucker M.E., Zweizig J., (The LIGO Scientific Collaboration and the Virgo Collaboration), Aptekar R.L., Boynton W.V., Frederiks D.D., Golenetskii S.V., Golovin D.V., Hurley K., Kozlova A.V., Litvak M.L., Mitrofanov I.G., Sanin A.B., Svinkin D.S., (The IPN Collaboration), Carotenuto F., Krishnan B.", "title_pub": "Search for gravitational-wave signals associated with gamma-ray bursts during the second observing run of Advanced LIGO and Advanced Virgo.", "first_author": "Abbott B.P.", "ref_biblio": [""], "bibcode": ["2019ApJ...886...75A"], "see_also": ["J/ApJ/715/1438 : Gravitational-wave bursts with GRBs (Abbott+, 2010)", "J/ApJ/760/12 : LIGO/Virgo gravitational-wave bursts with GRBs (Abadie+, 2012)", "J/ApJS/211/13 : The second Fermi/GBM GRB catalog (4yr) (von Kienlin+, 2014)", "J/ApJS/223/28 : The third Fermi/GBM GRB catalog (6yr) (Bhat+, 2016)", "J/ApJ/829/7 : Third Swift/BAT GRB catalog (past ~11yrs) (BAT3) (Lien+, 2016)", "http://gcn.gsfc.nasa.gov/gcn3_archive.html : GCN circulars archive", "http://swift.gsfc.nasa.gov/results/batgrbcat/ : Swift/BAT GRB online catalog", "http://swift.gsfc.nasa.gov/archive/grb_table/ : Swift GRBs online catalog", "http://heasarc.gsfc.nasa.gov/W3Browse/fermi/fermigbrst.html : Fermi/GBM online"], "keyword_cds": "GRB; Gravitational wave", "keyword_pub": "Burst astrophysics ; Gamma-ray bursts ; Gravitational wave astronomy ; Gravitational wave sources ; Gravitational waves ; High energy astrophysics ; LIGO", "abstract": ["We present the results of targeted searches for gravitational-wave", "transients associated with gamma-ray bursts during the second", "observing run of Advanced LIGO and Advanced Virgo, which took place", "from 2016 November to 2017 August. We have analyzed 98 gamma-ray", "bursts using an unmodeled search method that searches for generic", "transient gravitational waves and 42 with a modeled search method that", "targets compact-binary mergers as progenitors of short gamma-ray", "bursts. Both methods clearly detect the previously reported binary", "merger signal GW170817, with p-values of <9.38x10^-6^ (modeled) and", "3.1x10^-4^ (unmodeled). We do not find any significant evidence for", "gravitational-wave signals associated with the other gamma-ray bursts", "analyzed, and therefore we report lower bounds on the distance to each", "of these, assuming various source types and signal morphologies. Using", "our final modeled search results, short gamma-ray burst observations,", "and assuming binary neutron star progenitors, we place bounds on the", "rate of short gamma-ray bursts as a function of redshift for z<=1. We", "estimate 0.07-1.80 joint detections with Fermi-GBM per year for the", "2019-20 LIGO-Virgo observing run and 0.15-3.90 per year when current", "gravitational-wave detectors are operating at their design sensitivities."], "type": ["CCC"], "data": "", "date_update": "12-Apr-2021", "tables": [{"name": "table3.dat", "desc": "Information and limits on associated GW emission for each of the analyzed GRBs", "columns": [{"name": "Name", "desc": "GRB name "}, {"name": "f_Name", "desc": "Flag on Name (1) "}, {"name": "Time", "desc": "UTC time "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "Inst", "desc": "Instrument whose sky localization was used for the purposes of analysis"}, {"name": "Type", "desc": "Source type "}, {"name": "Network", "desc": "GW detector network used in the analysis of each GRB (2)"}, {"name": "f_Network", "desc": "Flag on Network (1) "}, {"name": "BNS", "desc": "[9/171]? The 90% confidence exclusion distance to the GRB (D_90_) for BNS scenario"}, {"name": "NS-BH-g", "desc": "[22/254]? The 90% confidence exclusion distance to the GRB (D_90_) for generic NS-BH scenario"}, {"name": "NS-BH-a", "desc": "[0/304]? The 90% confidence exclusion distance to the GRB (D_90_) for aligned-spin NS-BH scenario"}, {"name": "ADI-A", "desc": "[3/58]? The 90% confidence exclusion distance to the GRB (D_90_) for ADI-A scenario"}, {"name": "CSG", "desc": "[14/166]? The 90% confidence exclusion distance to the GRB (D_90_) for CSG GW burst at 150Hz scenario with total radiated energy E_GW_=M_{sun}_c^2^"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_93"}} {"id": "J/ApJ/886/93", "title_cds": "SAMP. III. Opt. LCs and spectra of two AGNs", "title_create": "Rakshit+, 2019", "year": "2019", "author": "Rakshit S., Woo J.-H., Gallo E., Hodges-Kluck E., Shin J., Jeon Y., Bae H.-J., Baldassare V., Cho H., Cho W., Foord A., Kang D., Kang W., Karouzos M., Kim M., Kim T., Le H.A.N., Park D., Park S., Son D., Sung H.-I., Bennert V.N., Malkan M.A.", "title_pub": "The Seoul National University AGN Monitoring Project. II. BLR size and black hole mass of two AGNs.", "first_author": "Rakshit S.", "ref_biblio": [""], "bibcode": ["2019ApJ...886...93R"], "see_also": ["VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)", "V/139 : SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)", "J/ApJ/613/682 : AGN central masses & broad-line region sizes (Peterson+, 2004)", "J/ApJS/152/251 : Indo-US library of coude feed stellar spectra (Valdes+, 2004)", "J/ApJ/716/993 : LAMP: reverberation mapping of H and He lines (Bentz+, 2010)", "J/ApJS/189/15 : FeII emission in a sample of AGN spectra (Kovacevic+, 2010)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/ApJ/755/60 : Reverberation mapping for 5 Seyfert 1 galaxies (Grier+, 2012)", "J/ApJ/782/45 : SEAMBHs. I. Mrk 142, Mrk 335, and IRAS F12397+3333 (Du+, 2014)", "J/ApJS/217/26 : Lick AGN monitoring 2011: light curves (Barth+, 2015)", "J/ApJ/806/22 : SEAMBHs IV. H{beta} time lags (Du+, 2015)", "J/ApJS/216/4 : SDSS-RM project: technical overview (Shen+, 2015)", "J/ApJ/825/126 : SEAMBHs. V. The third year (Du+, 2016)", "J/ApJ/818/30 : Lag measurements for 15 z<0.8 QSOs from SDSS-RM (Shen+, 2016)", "J/ApJ/840/97 : Optical RM campaign of 5 AGNs (Fausnaugh+, 2017)", "J/ApJ/851/21 : SDSS RM project first year of observations (Grier+, 2017)", "J/ApJ/837/131 : Space telescope RM project. V. NGC5548 (Pei+, 2017)", "J/ApJ/856/6 : SEAMBHs IX. 10 new H{beta} light curves (Du+, 2018)", "J/ApJ/865/56 : Emission line & R-band continuum LCs of 17 QSOs (Lira+, 2018)", "J/ApJ/870/123 : Swift optical & UV flux of four AGNs (Edelson+, 2019)", "J/ApJ/876/49 : A 10yr reverberation mapping campaign for 3C273 (Zhang+, 2019)"], "keyword_cds": "Active gal. nuclei; Photometry, UBV; Spectra, optical", "keyword_pub": "galaxies: active ; galaxies: kinematics and dynamics ; quasars: emission lines", "abstract": ["Active galactic nuclei (AGNs) show a correlation between the size of", "the broad line region and the monochromatic continuum luminosity at", "5100{AA}, allowing black hole mass estimation based on single-epoch", "spectra. However, the validity of the correlation is yet to be clearly", "tested for high-luminosity AGNs. We present the first reverberation", "mapping results of the Seoul National University AGN Monitoring", "Project (SAMP), which is designed to focus on luminous AGNs for", "probing the high end of the size-luminosity relation. We report time", "lag measurements of two AGNs, namely, 2MASSJ10261389+5237510 and", "SDSSJ161911.24+501109.2, using the light curves obtained over an", "~1000d period with an average cadence of 10 and 20d, respectively, for", "photometry and spectroscopy monitoring. Based on a cross-correlation", "analysis and H{beta} line width measurements, we determine the H{beta}", "lag as 41.8_-6.0_^+4.9^ and 52.6_-14.7_^+17.6^ days in the observed", "frame, and black hole mass as 3.65_-0.57_^+0.49^x10^7^M_{sun}_ and", "23.02_-6.56_^+7.81^x10^7^M_{sun}_, respectively, for 2MASS J1026 and", "SDSS J1619."], "description": ["Photometric observations were carried out at three different", "telescopes:", "(I) MDM 1.3m, located at Kitt Peak, Tucson, Arizona, USA, was used on", "2017 February 23 and 2018 November 6 in Johnson 4\" B filter.", "(II) Lemmonsan Optical Astronomy Observatory (LOAO) 1m, located on", "Mt. Lemmon, Tucson, Arizona, USA, was used in the B-band filter.", "(III) MDM 2.4m was used on 2017 March 20-April 8 and December 8-9).", "In total 110 and 101 epochs of B-band photometric observations were", "carried out for 2MASS J10261389+5237510 and SDSS J161911.24+501109.2,", "respectively, between 2015 November and 2018 July.", "Spectroscopic observations were carried out at two telescopes:", "(I) Shane 3m telescope, located at the Lick observatory on", "Mt. Hamilton, California, USA, using the Kast double spectrograph", "(R~624).", "(II) MDM 2.4m observations were carried out with a spectral coverage", "of 3970-6870{AA} and R=617."], "object": ["10 26 13.91 +52 37 51.3 2MASS J1026 = 2MASS J10261389+5237510", "16 19 11.25 +50 11 09.2 2MASS J1619 = SDSS J161911.24+501109.2"], "type": ["OC"], "data": "", "date_update": "13-Apr-2021", "tables": [{"name": "table2.dat", "desc": "Photometric data ", "columns": [{"name": "ID", "desc": "Source identifier "}, {"name": "JD", "desc": "[2457327.97/2458304.85] Julian Date "}, {"name": "Bmag", "desc": "[17.3/18.5] Apparent B band magnitude "}, {"name": "e_Bmag", "desc": "[0.004/0.1] Uncertainty in Bmag "}, {"name": "Tel", "desc": "Telescope identifier (1) "}]}, {"name": "table3.dat", "desc": "Spectroscopic data ", "columns": [{"name": "ID", "desc": "Source identifier "}, {"name": "JD", "desc": "[2457413.75/2458313.9] Julian Date "}, {"name": "F5100", "desc": "[0.09/0.32] Monochromatic flux at 5100{AA} in 10^-15^erg/s/cm^2^/{AA} units"}, {"name": "e_F5100", "desc": "[0.001/0.007] Uncertainty in F5100 "}, {"name": "FHb", "desc": "[12.94/28.4] H{beta} line flux in units of 10^-15^erg/s/cm^2^"}, {"name": "e_FHb", "desc": "[0.15/1.8] Uncertainty in FHb "}, {"name": "FHg", "desc": "[4/9.9] H{gamma} line flux in units of 10^-15^erg/s/cm^2^"}, {"name": "e_FHg", "desc": "[0.06/0.71] Uncertainty in FHg "}, {"name": "Tel", "desc": "Telescope identifier (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_99"}} {"id": "J/ApJ/886/99", "title_cds": "HST observations in the region of 3 SNR", "title_create": "Li+, 2019", "year": "2019", "author": "Li C.-J., Kerzendorf W.E., Chu Y.-H., Chen T.-W., Do T., Gruendl R.A., Holmes A., Ishioka R., Leibundgut B., Pan K.-C., Ricker P.M., Weisz D.", "title_pub": "Search for surviving companions of progenitors of young LMC SN Ia remnants.", "first_author": "Li C.-J.", "ref_biblio": [""], "bibcode": ["2019ApJ...886...99L"], "see_also": ["VII/232 : Nebulae in the Magellanic Clouds (Davies+ 1976)", "J/AJ/128/1606 : Magellanic Clouds Phot. Survey: the LMC (Zaritsky+, 2004)", "J/ApJ/779/L6 : 3D kinematic obs. of stars in Galactic Centre (Do+, 2013)", "J/MNRAS/439/354 : Sources around Tycho's Supernova 1572 (Bedin+, 2014)", "J/ApJS/215/9 : PHAT X. UV-IR photometry of M31 stars (Williams+, 2014)", "J/ApJ/808/106 : NIR spec. obs. in the Galactic Center (Stostad+, 2015)", "J/MNRAS/464/194 : Metallicity distribution in the GC (Feldmeier-Krause+, 2017)", "J/A+A/602/A85 : SN 1998bw MUSE datacube (Kruehler+, 2017)"], "keyword_cds": "Supernova remnants; Photometry, HST; Photometry, UBVRI; Interstellar medium; Magellanic Clouds", "keyword_pub": "Interstellar medium ; Type Ia supernovae ; Supernova remnants ; Companion stars ; Large Magellanic Cloud", "abstract": ["We have used two methods to search for surviving companions of Type Ia", "supernova progenitors in three Balmer-dominated supernova remnants in", "the Large Magellanic Cloud: 0519-69.0, 0505-67.9 (DEM L71), and", "0548-70.4. In the first method, we use the Hubble Space Telescope", "photometric measurements of stars to construct color-magnitude", "diagrams (CMDs) and compare positions of stars in the CMDs with those", "expected from theoretical post-impact evolution of surviving", "main-sequence or helium star companions. No obvious candidates of", "surviving companions are identified in this photometric search. Future", "models for surviving red giant companions or with different explosion", "mechanisms are needed for thorough comparisons with these observations", "in order to make more definitive conclusions. In the second method, we", "use Multi Unit Spectroscopic Explorer observations of 0519-69.0 and", "DEM L71 to carry out spectroscopic analyses of stars in order to use", "large peculiar radial velocities as diagnostics of surviving", "companions. We find a star in 0519-69.0 and a star in DEM L71 moving", "at radial velocities of 182+/-0km/s and 213+/-0km/s, respectively,", "more than 2.5{sigma} from the mean radial velocity of the underlying", "stellar population, 264 and 270km/s, respectively. These stars need", "higher-quality spectra to investigate their abundances and rotation", "velocities to determine whether they are indeed surviving companions", "of the supernova progenitors."], "description": ["We have obtained new HST images of SNR 0519-69.0, DEM L71, and", "SNR0548-70.4, using the UVIS channel of Wide Field Camera 3 (WFC3) in", "Program 13282 (PI: Chu). For SNR 0519-69.0, new images were obtained", "with only the F475W and F814W filters because HST F550M and F658N", "images taken with the Advanced Camera for Surveys (ACS) are available", "in the Hubble Legacy Archive.", "SNR 0519-69.0, DEM L71, and SNR 0548-70.4 were observed with the", "Advanced CCD Imaging Spectrometer (ACIS) of the Chandra X-ray", "Observatory for Program 01500024 (PI: Holt; 39.2ks), Program 01500900", "(PI: Hughes; 45.6ks), and Program 02500872 (PI: Borkowski; 59.3ks),", "respectively.", "MUSE observations of SNR 0519-69.0 and DEM L71 were obtained with the", "Very Large Telescope (VLT) UT4 of the European Southern Observatory", "(ESO) on 2015 November 16 and 2016 January 17 for Program 096.D-0352(A)", "(PI: Leibundgut)."], "type": ["OC"], "data": "", "date_update": "12-Apr-2021", "tables": [{"name": "table1.dat", "desc": "HST observations ", "columns": [{"name": "SNR", "desc": "SNR designation "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "Filt", "desc": "Filter "}, {"name": "Inst", "desc": "HST instrument "}, {"name": "Date", "desc": "Date of observation (UT) "}, {"name": "Exp", "desc": "[750/4757] Exposure time "}, {"name": "PI", "desc": "PI name "}, {"name": "PID", "desc": "[12017/13282] HST proposal ID "}]}, {"name": "table4.dat", "desc": "Stars brighter than V=23mag near central region in the SNR 0519-69.0", "columns": [{"name": "Seq", "desc": "[1/973] Internal stellar index number within SNR"}, {"name": "RAh", "desc": "[5] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[5/47] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[67/70] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Bmag", "desc": "[17/23.6] Apparent B band magnitude "}, {"name": "e_Bmag", "desc": "[0/0.02] Uncertainty in Bmag "}, {"name": "Vmag", "desc": "[16.59/23.02] Apparent V band magnitude "}, {"name": "e_Vmag", "desc": "[0/0.02] Uncertainty in Vmag "}, {"name": "Imag", "desc": "[14.97/22.3] Apparent I band magnitude "}, {"name": "e_Imag", "desc": "[0/0.02] Uncertainty in Imag "}, {"name": "B-V", "desc": "[0/0.81] The (B-V) color index "}, {"name": "e_B-V", "desc": "[0/0.02] Uncertainty in B-V "}, {"name": "V-I", "desc": "[0.06/2.83] The (V-I) color index "}, {"name": "e_V-I", "desc": "[0/0.02] Uncertainty in V-I "}, {"name": "Rad", "desc": "[0.6/40] Distance to site of SN explosion "}]}, {"name": "table6.dat", "desc": "Stars brighter than V=23mag near central region in the DEML71", "columns": [{"name": "Seq", "desc": "[1/973] Internal stellar index number within SNR"}, {"name": "RAh", "desc": "[5] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[5/47] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[67/70] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Bmag", "desc": "[17/23.6] Apparent B band magnitude "}, {"name": "e_Bmag", "desc": "[0/0.02] Uncertainty in Bmag "}, {"name": "Vmag", "desc": "[16.59/23.02] Apparent V band magnitude "}, {"name": "e_Vmag", "desc": "[0/0.02] Uncertainty in Vmag "}, {"name": "Imag", "desc": "[14.97/22.3] Apparent I band magnitude "}, {"name": "e_Imag", "desc": "[0/0.02] Uncertainty in Imag "}, {"name": "B-V", "desc": "[0/0.81] The (B-V) color index "}, {"name": "e_B-V", "desc": "[0/0.02] Uncertainty in B-V "}, {"name": "V-I", "desc": "[0.06/2.83] The (V-I) color index "}, {"name": "e_V-I", "desc": "[0/0.02] Uncertainty in V-I "}, {"name": "Rad", "desc": "[0.6/40] Distance to site of SN explosion "}]}, {"name": "table9.dat", "desc": "Stars brighter than V=23mag near central region in the SNR 0548-70.4", "columns": [{"name": "Seq", "desc": "[1/973] Internal stellar index number within SNR"}, {"name": "RAh", "desc": "[5] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[5/47] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[67/70] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Bmag", "desc": "[17/23.6] Apparent B band magnitude "}, {"name": "e_Bmag", "desc": "[0/0.02] Uncertainty in Bmag "}, {"name": "Vmag", "desc": "[16.59/23.02] Apparent V band magnitude "}, {"name": "e_Vmag", "desc": "[0/0.02] Uncertainty in Vmag "}, {"name": "Imag", "desc": "[14.97/22.3] Apparent I band magnitude "}, {"name": "e_Imag", "desc": "[0/0.02] Uncertainty in Imag "}, {"name": "B-V", "desc": "[0/0.81] The (B-V) color index "}, {"name": "e_B-V", "desc": "[0/0.02] Uncertainty in B-V "}, {"name": "V-I", "desc": "[0.06/2.83] The (V-I) color index "}, {"name": "e_V-I", "desc": "[0/0.02] Uncertainty in V-I "}, {"name": "Rad", "desc": "[0.6/40] Distance to site of SN explosion "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_102"}} {"id": "J/ApJ/886/102", "title_cds": "ALMA obs. of 70um dark high-mass clumps (ASHES)", "title_create": "Sanhueza+, 2019", "year": "2019", "author": "Sanhueza P., Contreras Y., Wu B., Jackson J.M., Guzman A.E., Zhang Q., Li S., Lu X., Silva A., Izumi N., Liu T., Miura R.E., Tatematsu K., Sakai T., Beuther H., Garay G., Ohashi S., Saito M., Nakamura F., Saigo K., Veena V.S., Nguyen-Luong Q., Tafoya D.", "title_pub": "The ALMA survey of 70um dark High-mass clumps in Early Stages (ASHES). I. Pilot survey: clump fragmentation.", "first_author": "Sanhueza P.", "ref_biblio": [""], "bibcode": ["2019ApJ...886..102S"], "see_also": ["J/A+A/291/943 : Protostellar cores (Ossenkopf+, 1994)", "J/A+A/430/137 : Close visual companions in Scorpius OB2 (Kouwenhoven+, 2005)", "J/ApJ/641/389 : Millimetric observations of IRDC cores (Rathborne+, 2006)", "J/ApJ/639/227 : MSX IRDC candidate catalog (Simon+, 2006)", "J/ApJ/651/L125 : H2O masers associated with IR dark cloud cores (Wang+, 2006)", "J/A+A/462/L17 : Dense cores in interstellar molecular clouds (Alves+, 2007)", "J/A+A/505/405 : A catalogue of Spitzer dark clouds (Peretto+, 2009)", "J/ApJS/197/25 : MALT90 pilot survey (Foster+, 2011)", "J/A+A/530/A118 : G29.96-0.02 and G35.20-1.74 1mm and 3mm maps (Pillai+, 2011)", "J/MNRAS/424/1925 : Spectrocopic Binarity of O and B type stars (Chini+, 2012)", "J/ApJ/756/60 : A 3mm line survey in 37 IR dark clouds (Sanhueza+, 2012)", "J/A+A/544/A146 : ATLASGAL cold high-mass clumps with NH_3_ (Wienen+, 2012)", "J/A+A/549/A45 : ATLASGAL Compact Source Catalog: 330500M_{sun}_), cold (<=15K), 3.6-70{mu}m dark prestellar clump", "candidates, embedded in infrared dark clouds, were carefully selected", "in the pilot survey to be observed with the Atacama Large", "Millimeter/submillimeter Array (ALMA). We have mosaicked each clump", "(~1arcmin^2^) in continuum and line emission with the 12m, 7m, and", "Total Power (TP) arrays at 224GHz (1.34mm), resulting in ~1.2\"", "resolution (~4800au, at the average source distance). As the first", "paper in the series, we concentrate on the continuum emission to", "reveal clump fragmentation. We detect 294 cores, from which 84 (29%)", "are categorized as protostellar based on outflow activity or \"warm", "core\" line emission. The remaining 210 (71%) are considered prestellar", "core candidates. The number of detected cores is independent of the", "mass sensitivity range of the observations and, on average, more", "massive clumps tend to form more cores. We find a large population of", "low-mass (<1M_{sun}_) cores and no high-mass (>30M_{sun}_) prestellar", "cores (maximum mass 11M_{sun}_). From the prestellar core mass", "function, we derive a power-law index of 1.17+/-0.10, which is", "slightly shallower than Salpeter. We used the minimum spanning tree", "(MST) technique to characterize the separation between cores and their", "spatial distribution, and to derive mass segregation ratios. While", "there is a range of core masses and separations detected in the", "sample, the mean separation and mass per clump are well explained by", "thermal Jeans fragmentation and are inconsistent with turbulent Jeans", "fragmentation. Core spatial distribution is well described by", "hierarchical subclustering rather than centrally peaked clustering.", "There is no conclusive evidence of mass segregation. We test several", "theoretical conditions and conclude that overall, competitive", "accretion and global hierarchical collapse scenarios are favored over", "the turbulent core accretion scenario."], "description": ["For the ALMA Survey of 70{mu}m dark High-mass clumps in Early Stages", "(ASHES) pilot survey, 11 infrared dark cloud (IRDC) clumps were", "selected from the Millimetre Astronomy Legacy Team 90GHz Survey", "(MALT90; Foster+ 2011, J/ApJS/197/25 and 2013PASA...30...38F ;", "Jackson+ 2013PASA...30...57J). MALT90 was built on the ATLASGAL 870um", "catalogs (Schuller+ 2009A&A...504..415S and Contreras+ 2013,", "J/A+A/549/A45), from which a sample of 3246 high-mass clumps was", "selected for follow-up in 16 spectral lines. Only 18 sources satisfy", "all the selection conditions, and 11 were observed in this pilot", "survey. The 12th target in the ASHES pilot survey is G028.273-00.167,", "which is in the first quadrant and was not covered in MALT90. This", "IRDC satisfies all requirements and has been well studied in the past", "by Sanhueza+ (2012, J/ApJ/756/60 ; 2013ApJ...773..123S and", "2017ApJ...841...97S).", "Observations of the 12 IRDCs were carried out with ALMA on different", "days during Cycle 3 (Project ID: 2015.1.01539.S; PI: Sanhueza) and a", "resubmission for Cycle 4 (Project ID: 2016.1.01246.S; PI: Sanhueza).", "The data sets consist of observations in band 6 (~224GHz; 1.34mm) with", "the main 12m array, the Atacama Compact 7m Array (ACA; Morita Array),", "and the total power (TP)."], "type": ["OC"], "data": "", "date_update": "14-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Physical properties of the prestellar, high-mass clump candidates", "columns": [{"name": "AGAL", "desc": "IRDC clump designation (GLLL.lll+BB.bbb) (1) "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) (2) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) (2) "}, {"name": "DEd", "desc": "Degree of declination (J2000) (2) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "Vlsr", "desc": "[-87.8/80] LSR velocity of the gas "}, {"name": "sigma", "desc": "[0.56/3.04] Velocity dispersion (3) "}, {"name": "Dist", "desc": "[2.9/5.4] Distance used for clump selection "}, {"name": "Tdust", "desc": "[10.3/15] Dust temperature used for clump selection"}, {"name": "Mass", "desc": "[580/5200] Mass used for clump selection "}, {"name": "Ref", "desc": "Reference (4) "}, {"name": "Rcl-pc", "desc": "[0.36/0.74] Clump radius in pc (5) "}, {"name": "Rcl", "desc": "[19/37] Clump radius in arcsec (5) "}, {"name": "Mcl", "desc": "[520/3120] Clump mass (6) "}, {"name": "Sigcl", "desc": "[0.1/1.1] Clump surface density ({Sigma}_cl_=M_cl_/{pi}R_cl_^2^)"}, {"name": "Vol", "desc": "[0.9/13] Volume density (7) "}]}, {"name": "table3.dat", "desc": "Core parameters obtained from dendrograms ", "columns": [{"name": "AGAL", "desc": "IRDC Clump Name "}, {"name": "Core", "desc": "ALMA Core Name (ALMANN within Clump or EdgeN: see Note G1)"}, {"name": "RAh", "desc": "[15/18] Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "[0/51] Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "[4/54] Degree of Declination (J2000) "}, {"name": "DEm", "desc": "[8/48] Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "F224GHz", "desc": "[0.2/14.8] Peak Flux; primary beam corrected"}, {"name": "S224GHz", "desc": "[0.2/52.8] Integrated Flux; primary beam corrected"}, {"name": "Rad", "desc": "[0.27/2.46] Radius in arcsec "}, {"name": "Cl", "desc": "[0/3] Core Classification (1) "}, {"name": "Edge", "desc": "[0/1] Core at edge of images are not used for analysis (G1)"}]}, {"name": "table4.dat", "desc": "Calculated properties for the whole core sample ", "columns": [{"name": "AGAL", "desc": "IRDC Clump Name "}, {"name": "Core", "desc": "ALMA Core Name "}, {"name": "Mass", "desc": "[0.12/30.4] Core Mass "}, {"name": "Radius", "desc": "[900/9670] Core calculated radius in au "}, {"name": "nH2", "desc": "[0.2/26.2] Core Volume Density "}, {"name": "Sigma", "desc": "[0.08/4.78] Core Surface Density "}, {"name": "NH2pk", "desc": "[0.12/9.52] Peak Column Density "}, {"name": "Edge", "desc": "Core at edge of images are not used for analysis (G1)"}]}, {"name": "table5.dat", "desc": "Overall properties per clump of the embedded ALMA cores", "columns": [{"name": "AGAL", "desc": "IRDC Clump Name "}, {"name": "Sens", "desc": "[0.03/0.2] 1{sigma} mass sensitivity "}, {"name": "Nc", "desc": "[13/39] Number of cores "}, {"name": "b_Mass", "desc": "[0.1/1.5] Minimum core mass "}, {"name": "B_Mass", "desc": "[2.7/30.4] Maximum core mass "}, {"name": "Mass", "desc": "[0.87/5] Mean Mass "}, {"name": "Rad", "desc": "[1810/4810] Radius "}, {"name": "nH2", "desc": "[0.6/9] Mean number density (n(H_2_)) "}, {"name": "Sig", "desc": "[0.18/1.7] Mean surface density ({Sigma}) "}, {"name": "NH2pk", "desc": "[2.1/16.4] Mean peak column density (N_peak_(H_2_))"}, {"name": "Npre", "desc": "Number of prestellar cores "}, {"name": "---", "desc": "[/] "}, {"name": "Npro", "desc": "Number of protostellar cores "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_124"}} {"id": "J/ApJ/886/124", "title_cds": "Completed KMOS^3D^ survey NIR obs.", "title_create": "Wisnioski+, 2019", "year": "2019", "author": "Wisnioski E., Schreiber N.M.F., Fossati M., Mendel J.T., Wilman D., Genzel R., Bender R., Wuyts S., Davies R.L., Ubler H., Bandara K., Beifiori A., Belli S., Brammer G., Chan J., Davies R.I., Fabricius M., Galametz A., Lang P., Lutz D., Nelson E.J., Momcheva I., Price S., Rosario D., Saglia R., Seitz S., Shimizu T., Tacconi L.J., Tadaki K., van Dokkum P.G., Wuyts E.", "title_pub": "The KMOS^3D^ survey: Data Release and final survey paper.", "first_author": "Wisnioski E.", "ref_biblio": [""], "bibcode": ["2019ApJ...886..124W"], "see_also": ["II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "J/A+A/437/883 : K20 survey: spectroscopic catalogue (Mignoli+, 2005)", "J/A+A/455/107 : 3D spectroscopy with VLT/GIRAFFE (Flores+, 2006)", "J/ApJS/179/124 : Subaru/XMM-Newton deep survey (SXDS) III. (Ueda+, 2008)", "J/A+A/478/83 : GOODS-South Field VLT/FORS2 redshifts. III. (Vanzella+, 2008)", "J/ApJ/706/1364 : SINS survey of high-redshift gal. (Forster Schreiber+, 2009)", "J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011)", "J/ApJ/735/86 : NEWFIRM MBS: photometric catalogs (Whitaker+, 2011)", "J/ApJS/195/10 : The CDF-S survey: 4Ms source catalogs (Xue+, 2011)", "J/ApJS/201/30 : The Chandra COSMOS survey. III. (Civano+, 2012)", "J/MNRAS/425/2116 : Arizona CDFS Environment Survey, ACES (Cooper+, 2012)", "J/ApJS/203/24 : Structural param. of galaxies in CANDELS (van der Wel+, 2012)", "J/A+A/549/A63 : GMASS photometry (Kurk+, 2013)", "J/ApJ/768/74 : PHIBSS: CO obs. of star-forming galaxies (Tacconi+, 2013)", "J/ApJ/796/7 : NIR spectral analysis of star-forming galaxies (Genzel+, 2014)", "J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014)", "J/A+A/582/A21 : Merging galaxies (mis)alignments (Barrera-Ballesteros+, 2015)", "J/MNRAS/456/1195 : KMOS AGN Survey at High redshift (KASHz) (Harrison+, 2016)", "J/ApJS/225/27 : 3D-HST Survey: grism spectra master catalog (Momcheva+, 2016)", "J/ApJ/827/74 : [NII]/H{alpha} ratio in galaxies with KMOS^3D^ (Wuyts+, 2016)", "J/ApJ/835/153 : Galaxy environment in 3D-HST fields (z=0.5-3) (Fossati+, 2017)", "J/MNRAS/467/1965 : KMOS Redshift One Spectroscopic Survey (Harrison+, 2017)", "J/ApJ/842/121 : Tully-Fisher relation with KMOS^3D^ (Ubler+, 2017)", "J/A+A/613/A72 : AS1063 and MACS1206-08 datacubes (Girard+, 2018)", "http://www.mpe.mpg.de/ir/KMOS3D : KMOS^3D^ home page"], "keyword_cds": "Galaxies, spectra; Surveys; Redshifts; Magnitudes, absolute; Velocity dispersion; Spectra, infrared; Optical", "keyword_pub": "Disk galaxies ; Emission line galaxies ; Galaxy evolution ; High-redshift galaxies ; Surveys ; Galaxy kinematics", "abstract": ["We present the completed KMOS^3D^ survey, an integral field", "spectroscopic survey of 739 log(M_*_/M_{sun}_)>9 galaxies at 0.6=3 resolution elements along the kinematic major axis. The", "detection fraction of H{alpha} is a strong function of both color and", "offset from the main sequence, with the detected and nondetected", "samples exhibiting different spectral energy distribution shapes.", "Comparison of H{alpha} and UV+IR star formation rates reveal that dust", "attenuation corrections may be underestimated by 0.5dex at the highest", "masses (log(M_*_/M_{sun}_)>10.5). We confirm our first year results of", "a high rotation-dominated fraction (monotonic velocity gradient and", "v_rot_/{sigma}_0_>3.36^0.5^) of 77% for the full KMOS^3D^ sample. The", "rotation-dominated fraction is a function of both stellar mass and", "redshift, with the strongest evolution measured over the redshift", "range of the survey for galaxies with log(M_*_/M_{sun}_)<10.5."], "description": ["Observations with the multi-IFU K-band Multi Object Spectrograph", "(KMOS) at the VLT took place in Visitor Mode over 75 guaranteed time", "nights between 2013 October and 2018 April (ESO periods 92-101).", "The spectral resolution of KMOS (R~3000-4000) varies for the 24", "different IFUs."], "type": ["OC"], "data": "", "date_update": "19-Apr-2021", "tables": [{"name": "table5.dat", "desc": "The KMOS^3D^ galaxy catalog ", "columns": [{"name": "ID", "desc": "KMOS^3D^ unique identifier "}, {"name": "Field", "desc": "Field identifier (COS=COSMOS, GS=GOODS-S or U=UDS)"}, {"name": "S14", "desc": "[779/46938]?=99999 Identifier from Skelton+ 2014, J/ApJS/214/24 (G1)"}, {"name": "Target", "desc": "KMOS^3D^ original targeting identifier (1) "}, {"name": "File", "desc": "Name of the FITS file in subdirectory cubes "}, {"name": "P", "desc": "[0/1] Primary target flag (2) "}, {"name": "Add", "desc": "[0/1] Additional galaxies detected flag (G2)"}, {"name": "Seg", "desc": "[-1/3] Segmentation flag (3) "}, {"name": "q_z", "desc": "[0/1] Redshift quality flag (4) "}, {"name": "RAdeg", "desc": "[34.23/150.21] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-27.93/2.48] Declination (J2000) "}, {"name": "zTar", "desc": "[0.38/2.83] Best known redshift at time of observation from 3D-HST"}, {"name": "Band", "desc": "Observing KMOS band "}, {"name": "Exp", "desc": "[80/1615] Total exposure time "}, {"name": "FWHM", "desc": "[0.3/0.93] FWHM of Moffat model PSF; minor axis"}, {"name": "z", "desc": "[0.38/2.7]?=-9999 Measured KMOS3D redshift "}, {"name": "Res", "desc": "[0/5209]?=-9999 Estimated spectral resolution (5)"}, {"name": "Ksmag", "desc": "[18.5/25.5] Apparent Ks AB magnitude from 3D-HST catalogs"}, {"name": "UMag", "desc": "[-23.91/-16.4] Absolute rest frame U band AB magnitude from Skelton+ 2014, J/ApJS/214/24"}, {"name": "VMag", "desc": "[-24.4/-18] Absolute rest frame V band AB magnitude from Skelton+ 2014, J/ApJS/214/24"}, {"name": "JMag", "desc": "[-25.14/-18.3] Absolute rest frame J band AB magnitude from Brammer+ 2012"}, {"name": "SFR", "desc": "[0.01/1202] Star Formation Rate (6) "}, {"name": "f_SFR", "desc": "[1/5] Flag indication type on SFR (7) "}, {"name": "M*", "desc": "[8.38/11.68] Stellar mass (8) "}, {"name": "Av", "desc": "[0/2.9] V band dust attenuation from SED modeling"}, {"name": "ReffH", "desc": "[0.028/3.92] CANDELS H band major axis effective radius"}, {"name": "e_ReffH", "desc": "[0/0.6]?=-999 Uncertainty in ReffH "}, {"name": "Q", "desc": "[0.005/1] CANDELS H band axis ratio "}, {"name": "e_Q", "desc": "[0.001/0.3]?=-999 Uncertainthy in Q "}, {"name": "HFlag", "desc": "[1/2] Source of H band data (9) "}]}, {"name": "table6.dat", "desc": "KMOS^3D^ H{alpha} flux catalog ", "columns": [{"name": "ID", "desc": "KMOS^3D^ Unique identifier "}, {"name": "Field", "desc": "Field identifier "}, {"name": "S14", "desc": "[779/46938]?=99999 Skelton identifier (G1) "}, {"name": "RAdeg", "desc": "[34.23/150.21] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-27.93/2.48] Declination (J2000) "}, {"name": "Ap", "desc": "[1.5] Aperture radius (always \"1.5\") "}, {"name": "z", "desc": "[0.6/2.7]? Redshift (vacuum) from H{alpha} line fit (1)"}, {"name": "e_z", "desc": "[0/0.0006]? Uncertainty in z "}, {"name": "sigma", "desc": "[0/1540]? Velocity dispersion (2) "}, {"name": "e_sigma", "desc": "[0/166]? Uncertainty in sigma (3) "}, {"name": "FHa", "desc": "[0.069/259458]? H{alpha} flux density (2) "}, {"name": "e_FHa", "desc": "[0/34]? Uncertainty in FHa (3) "}, {"name": "FCor", "desc": "[1/4] Aperture flux correction "}, {"name": "Flag", "desc": "[-3/2] Quality fit flag (0=reliable fit) (4) "}]}, {"name": "cubes/*", "desc": "All KMOS^3D^ data cubes in FITS format ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_150"}} {"id": "J/ApJ/886/150", "title_cds": "VRI and K-band light curves of type 1 AGNs", "title_create": "Minezaki+, 2019", "year": "2019", "author": "Minezaki T., Yoshii Y., Kobayashi Y., Sugawara S., Sakata Yu, Enya K., Koshida S., Tomita H., Suganuma M., Aoki T., Peterson B.A.", "title_pub": "Reverberation measurements of the inner radii of the dust tori in quasars.", "first_author": "Minezaki T.", "ref_biblio": [""], "bibcode": ["2019ApJ...886..150M"], "see_also": ["II/183 : UBVRI Photometric Standards (Landolt 1992)", "VII/223 : The 2dF QSO Redshift Survey. V. The 10k catalogue (Croom+ 2001)", "J/ApJ/269/352 : Quasar evolution (Schmidt+, 1983)", "J/AJ/109/1498 : Large Bright Quasar Survey VI (LBQS) (Hewett+, 1995)", "J/ApJ/663/81 : SED of hard X-ray selected AGN in XMDS (Polletta+, 2007)", "J/ApJ/698/895 : Variations in QSOs optical flux (Kelly+, 2009)", "J/ApJ/709/1257 : Spitzer-IRS spectra of Seyfert galaxies. II. (Tommasin+, 2010)", "J/ApJS/207/19 : Hard X-ray survey from Swift-BAT 6yrs (Baumgartner+, 2013)", "J/ApJS/206/4 : SED & bolometric corrections for QSOs (Krawczyk+, 2013)", "J/MNRAS/439/1648 : Subarcsecond mid-infrared atlas of local AGN (Asmus+, 2014)", "J/ApJ/788/159 : 17 Seyfert 1 galaxies light curves (Koshida+, 2014)", "J/A+A/561/L8 : BRJK photometry of Seyfert galaxy WPVS48 (Pozo Nunez+, 2014)", "J/ApJ/801/127 : 3.6um, 4.5um, B & V light curves of NGC 6418 (Vazquez+, 2015)", "J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray (Ricci+, 2017)", "J/A+A/620/A137 : CCD B,V,R,I,Ha photometry of 3C120 (Ramolla+, 2018)"], "keyword_cds": "Active gal. nuclei; QSOs; Photometry, VRI; Photometry, infrared", "keyword_pub": "Active galactic nuclei ; Quasars ; Dust continuum emission ; Cosmological parameters", "abstract": ["We present the results of a dust-reverberation survey of quasars at", "redshifts z<0.6. We found a delayed response of the K-band flux", "variation after the optical flux variation in 25 out of 31 targets,", "and obtained the lag time between them for 22 targets. Combined with", "the results for nearby Seyfert galaxies, we provide the largest", "homogeneous collection of K-band dust-reverberation data for 36 type 1", "active galactic nuclei (AGNs). This doubles the sample and includes", "the most distant AGN and the largest lag so far measured. We estimated", "the optical luminosity of the AGN component of each target using three", "different methods: spectral decomposition, the flux-variation-gradient", "method, and image decomposition. We found a strong correlation between", "the reverberation radius for the innermost dust torus and the optical", "luminosity over a range of approximately four orders of magnitude in", "luminosity, as is already known for Seyfert galaxies. We estimated the", "luminosity distances of the AGNs based on their dust-reverberation", "lags, and found that the data in the redshift-distance diagram are", "consistent with the current standard estimates of the cosmological", "parameters. We also present the radius-luminosity relations for", "isotropic luminosity indicators such as the hard X-ray (14-195keV),", "[OIV]25.89{mu}m, and mid-infrared (12{mu}m) continuum luminosities,", "which are applicable to obscured AGNs."], "description": ["In this paper, we report the results for 31 type 1 AGNs monitored by", "the Multicolor Active Galactic Nuclei (MAGNUM) project", "(Yoshii 2002ntto.conf..235Y and Yoshii+ 2003AAS...202.3803Y).", "We conducted monitoring observations using a multicolor imaging", "photometer (MIP) mounted on the MAGNUM 2m telescope at the Haleakala", "Observatories in Hawaii. The MIP is capable of simultaneous imaging in", "one optical band (selected from among U, B, V, R, and I) and one", "near-infrared band (selected from among Y, J, H, and K)."], "type": ["OC"], "data": "", "date_update": "20-Apr-2021", "tables": [{"name": "table1.dat", "desc": "List of targets and monitoring parameters ", "columns": [{"name": "ID", "desc": "Identifier (Truncated name) "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "z", "desc": "[0.06/0.6] Heliocentric redshift from NED "}, {"name": "Opt", "desc": "Optical observing band (V, R or I) (1) "}, {"name": "NIR", "desc": "NIR observing band (always K) (1) "}, {"name": "Start", "desc": "Starting date of observation (UT) "}, {"name": "---", "desc": "[-] "}, {"name": "End", "desc": "Ending date of observation (UT) "}, {"name": "Nobs", "desc": "[12/134] Number of observations "}, {"name": "Tint", "desc": "[6/112] Median monitoring interval "}, {"name": "Name", "desc": "Full name of the source "}]}, {"name": "table2.dat", "desc": "Light curve data ", "columns": [{"name": "ID", "desc": "Identifier (Truncated name) "}, {"name": "Band", "desc": "Observing band (V, R, I or K) "}, {"name": "MJD", "desc": "[52117.45/54330.62] Observation Date "}, {"name": "Flux", "desc": "[44/19712] Flux in Band (1) "}, {"name": "e_Flux", "desc": "[0.4/324] Uncertainty in Flux "}]}, {"name": "table5.dat", "desc": "Optical AGN fluxes and luminosities ", "columns": [{"name": "ID", "desc": "Identifier (Truncated name) "}, {"name": "Opt", "desc": "Optical observing band (V, R or I) "}, {"name": "Flux", "desc": "[10/5878]? Optical flux of the AGN in Band "}, {"name": "e_Flux", "desc": "[0.4/161]? Flux downwards uncertainty "}, {"name": "E_Flux", "desc": "[0.4/161]? Flux upwards uncertainty "}, {"name": "logL", "desc": "[42.6/45.43]? Log of the V-band luminosity of the AGN in erg/s units"}, {"name": "e_logL", "desc": "[0.005/0.3]? LogL downwards uncertainty "}, {"name": "E_logL", "desc": "[0.005/0.4]? LogL upwards uncertainty "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_152"}} {"id": "J/ApJ/886/152", "title_cds": "ZTF early observations of Type Ia SNe. I. LCs", "title_create": "Yao+, 2019", "year": "2019", "author": "Yao Y., Miller A.A., Kulkarni S.R., Bulla M., Masci F.J., Goldstein D.A., Goobar A., Nugent P., Dugas A., Blagorodnova N., Neill J.D., Rigault M., Sollerman J., Nordin J., Bellm E.C., Cenko S.B., De K., Dhawan S., Feindt U., Fremling C., Gatkine P., Graham M.J., Graham M.L., Ho A.Y.Q., Hung T., Kasliwal M.M., Kupfer T., Laher R.R., Perley D.A., Rusholme B., Shupe D.L., Soumagnac M.T., Taggart K., Walters R., Yan L.", "title_pub": "ZTF early observations of Type Ia supernovae. I. Properties of the 2018 sample.", "first_author": "Yao Y.", "ref_biblio": [""], "bibcode": ["2019ApJ...886..152Y"], "see_also": ["B/sn : Asiago Supernova Catalogue (Barbon et al., 1999-)", "J/AJ/137/3731 : ESSENCE high-redshift supernova (Foley+, 2009)", "J/ApJ/700/331 : Light curves of type Ia supernovae (CfA3) (Hicken+, 2009)", "J/ApJ/716/712 : HST light curves of six SNe and Union2 (Amanullah+, 2010)", "J/AJ/139/519 : Carnegie supernova project. SNe Ia (Contreras+, 2010)", "J/ApJS/190/418 : Light curves for 165 SNe (Ganeshalingam+, 2010)", "J/A+A/526/A28 : SDSS-II supernovae NTT and NOT spectroscopy (Oestman+, 2011)", "J/AJ/142/156 : The CSP (DR2): photometry of SNe Ia (Stritzinger+, 2011)", "J/AJ/143/126 : Spectroscopy of 462 nearby Type Ia SNe (Blondin+, 2012)", "J/ApJS/200/12 : CfA4: light curves for 94 type Ia SNe (Hicken+, 2012)", "J/MNRAS/425/1789 : Berkeley supernova Ia program. I. (Silverman+, 2012)", "J/A+A/568/A22 : Joint analysis of the SDSS-II & SNLS SNe Ia (Betoule+, 2014)", "J/MNRAS/446/3895 : The rising light curves of Type Ia supernovae (Firth+, 2015)", "J/ApJ/826/56 : HST/WFC3 obs. of Cepheids in SN Ia host gal. (Riess+, 2016)", "J/AJ/154/211 : The CSP (DR3): photometry of low-z SNIa (Krisciunas+, 2017)", "J/ApJ/870/L1 : K2 obs. of type Ia supernova SN 2018oh (Dimitriadis+, 2019)", "J/ApJ/870/13 : K2 LC alternative analysis of ASASSN-18bt (Shappee+, 2019)", "http://www.wis-tns.org/ : Transient Name Server (TNS) home page"], "keyword_cds": "Supernovae; Photometry; Optical; Extinction", "keyword_pub": "Type Ia supernovae ; Sky surveys ; Catalogs ; Supernovae ; Surveys ; Photometry", "abstract": ["Early-time observations of Type Ia supernovae (SNe Ia) are essential", "to constrain the properties of their progenitors. In this paper, we", "present high-quality light curves of 127 SNe Ia discovered by the", "Zwicky Transient Facility (ZTF) in 2018. We describe our method to", "perform forced point-spread function photometry, which can be applied", "to other types of extragalactic transients. With a planned cadence of", "six observations per night (three g + three r), all of the 127 SNe Ia", "are detected in both g and r bands more than 10 days (in the rest", "frame) prior to the epoch of g-band maximum light. The redshifts of", "these objects range from z=0.0181 to 0.165; the median redshift is", "0.074. Among the 127 SNe, 50 are detected at least 14 days prior to", "maximum light (in the rest frame), with a subset of nine objects being", "detected more than 17 days before g-band peak. This is the largest", "sample of young SNe Ia collected to date; it can be used to study the", "shape and color evolution of the rising light curves in unprecedented", "detail. We discuss six peculiar events in this sample: one 02cx-like", "event ZTF18abclfee (SN2018crl), one Ia-CSM SN ZTF18aaykjei", "(SN2018cxk), and four objects with possible super-Chandrasekhar mass", "progenitors: ZTF18abhpgje (SN2018eul), ZTF18abdpvnd (SN2018dvf),", "ZTF18aawpcel (SN2018cir), and ZTF18abddmrf (SN2018dsx)."], "description": ["With the Zwicky Transient Facility (ZTF), we are undertaking a", "high-cadence survey with six epochs per night (three g + three r).", "This experiment is conducted over a large area of the sky (~2500deg^2^)", "and thus enables large-number statistics. In this study, we focus on a", "special subset of SNe Ia that were discovered more than 10 days prior", "to maximum light. Our large (127 objects), homogeneous sample of young", "SNe Ia was constructed within the first year of operations by ZTF", "in 2018.", "The ZTF camera is mounted on the 48 inch Samuel Oschin Telescope (P48)", "at Palomar Observatory. ZTF divides its observing time between public", "surveys (40%), partnership surveys (40%), and Caltech surveys (20%).", "Bellm+ (2019PASP..131f8003B) provide details of the ZTF surveys."], "type": ["OC"], "data": "", "date_update": "20-Apr-2021", "tables": [{"name": "sample.dat", "desc": "General information and photometric properties of 127 SNe Ia (Tables 2 and 3)", "columns": [{"name": "ZTF", "desc": "ZTF Name "}, {"name": "RAdeg", "desc": "[12.52/348.53] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[21.38/79.06] Declination (J2000) "}, {"name": "Name", "desc": "SN IAU name from the Transient Name Server (TNS)"}, {"name": "TNS", "desc": "TNS Internal Name, indicating the discovery group"}, {"name": "Tel", "desc": "Followup telescope (s) (1) "}, {"name": "Phase", "desc": "Spectroscopic phase(s) at followup (1) "}, {"name": "Subtype", "desc": "Ia Subtype (2) "}, {"name": "z", "desc": "[0.018/0.17] Redshift (3) "}, {"name": "E(B-V)", "desc": "[0.006/0.12] Forground Galactic extinction from Schlafly & Finkbeiner (2011ApJ...737..103S)"}, {"name": "tgmax", "desc": "[58243.79/58396.52] Epoch of g-band maximum light, Modified Julian Date (4)"}, {"name": "e_tgmax", "desc": "[0/1.5] Uncertainty in tgmax "}, {"name": "Delm15g", "desc": "[0.4/1.7]? Decline within 15d from maximum in g band (4)"}, {"name": "e_Delm15g", "desc": "[0/0.1]? Uncertainty in Delm15g "}, {"name": "x1", "desc": "[-2.6/4.2] Light curve shape parameter, x1, from SALT2 fitting (salt2x1)"}, {"name": "e_x1", "desc": "[0/1.1] Uncertainty in x1 "}, {"name": "c", "desc": "[-0.2/0.7] Light curve color, c, from SALT2 fitting (salt2c)"}, {"name": "e_c", "desc": "[0/0.2] Uncertainty in c "}]}, {"name": "table5.dat", "desc": "P48 photometry of 127 SNe Ia ", "columns": [{"name": "ZTF", "desc": "ZTF name of the supernova "}, {"name": "JD", "desc": "Julian Date "}, {"name": "PID", "desc": "[1/3] Program identifier (programid) "}, {"name": "Field", "desc": "[584/1824] ZTF field identifier (fieldid) (1) "}, {"name": "CCD", "desc": "[1/16] CCD identifier (from 1 to 16) (ccdid) (1) "}, {"name": "qID", "desc": "[1/4] Quadrant (CCD-amplifier) identifier (from 1 to 4) (1)"}, {"name": "Filt", "desc": "[1/2] Filter identifier (1=g_ZTF_, 2=r_ZTF_) (filterid) (2)"}, {"name": "Seeing", "desc": "[1.19/4] Photometric seeing (FWHM) at the Palomar Observatory at the time of observation"}, {"name": "ZP", "desc": "[22.63/28.64] Photometric zero-point "}, {"name": "e_ZP", "desc": "[5.3e-7/0.018] ZP uncertainty (zp_unc) "}, {"name": "Flux", "desc": "[-3728/19044] Forced PSF-fit flux for the difference image (DN units) (fmcmc) (3)"}, {"name": "e_Flux", "desc": "[11/710] Flux uncertainty (fmcmc_unc) "}, {"name": "C", "desc": "[-999/200.3] History offset in the baseline region (DN units) (4)"}, {"name": "Chi2", "desc": "[-999/3.3] Square root of the reduced chi-square statistics (chi2_nu) (4)"}]}, {"name": "table5.fits", "desc": "Table 5 in original FITS format ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_886_L14"}} {"id": "J/ApJ/886/L14", "title_cds": "Gemini/FLAMINGOS-2 NIR spectra of V1047 Cen", "title_create": "Geballe+, 2019", "year": "2019", "author": "Geballe T.R., Banerjee D.P.K., Evans A., Gehrz R.D., Woodward C.E., Mroz P., Udalski A., Munari U., Starrfield S., Page K.L., Sokolovsky K., Hambsch F.-J., Myers G., Aydi E., Buckley D.A.H., Walter F., Wagner R.M.", "title_pub": "Infrared spectroscopy of the recent outburst in V1047 Cen (Nova Centauri 2005).", "first_author": "Geballe T.R.", "ref_biblio": [""], "bibcode": ["2019ApJ...886L..14G"], "see_also": ["B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-2014)", "B/gemini : The Gemini Observation Log (CADC, 2001-)", "I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "J/A+A/453/635 : Modelling Galactic Interstellar Extinction (Marshall+, 2006)", "J/AJ/141/121 : V446 Her V light curves (Honeycutt+, 2011)", "J/ApJS/197/31 : Swift X-ray obs. of classical novae. II. (Schwarz+, 2011)", "J/A+A/554/A123 : Near-IR catalog of novae in VVV survey area (Saito+, 2013)", "J/MNRAS/440/2036 : VPHAS+ survey synthetic colours (Drew+, 2014)", "J/ApJ/788/164 : Known Galactic classical novae (Pagnotta+, 2014)", "J/MNRAS/465/3011 : VVV high amplitude NIR var. stars (Contreras Pena+, 2017)", "J/A+A/647/A169 : VVV survey near-infrared colour catalog (Herpich+, 2021)"], "keyword_cds": "Novae; Spectra, infrared", "keyword_pub": "Cataclysmic variable stars ; Infrared sources", "abstract": ["Fourteen years after its eruption as a classical nova (CN), V1047 Cen", "(Nova Cen 2005) began an unusual re-brightening in 2019 April. The", "amplitude of the brightening suggests that this is a dwarf nova (DN)", "eruption in a CN system. Very few CNe have had DN eruptions within", "decades of the main CN outburst. The 14yr separating the CN and DN", "eruptions of V1047 Cen is the shortest of all instances recorded thus", "far. Explaining this rapid succession of CN and DN outbursts in", "V1047 Cen may be challenging within the framework of standard theories", "for DN outbursts. Following a CN eruption, the mass accretion rate is", "believed to remain high (dM/dt~10^-8^M_{sun}_/yr) for a few centuries,", "due to the irradiation of the secondary star by the still-hot surface", "of the white dwarf. Thus a DN eruption is not expected to occur during", "this high mass accretion phase as DN outbursts, which result from", "thermal instabilities in the accretion disk, and arise during a regime", "of low mass accretion rate (dM/dt~10^-10^M_{sun}_/yr). Here we present", "near-infrared spectroscopy to show that the present outburst is most", "likely a DN eruption, and discuss the possible reasons for its early", "occurrence. Even if the present re-brightening is later shown to be", "due to a cause other than a DN outburst, the present study provides", "invaluable documentation of this unusual event."], "description": ["Spectra of V1047 Cen were obtained at the 8.1m Gemini South Telescope", "using its facility spectrograph FLAMINGOS-2 on 2019 Jun 30/Jul 1 and", "2019 Aug 1/2 in the wavelength range 0.9-1.8um (JH grism; R~200 to", "~1100 at 1.3-1.4um) and 1.9-2.5um with the R3K grism (R~1200 to 3200", "near 2.2um)."], "object": ["13 20 49.74 -62 37 50.5 NOVA Cen 2005 = V* V1047 Cen"], "type": ["OC"], "data": "", "date_update": "21-Apr-2021", "tables": [{"name": "fig2.dat", "desc": "The 0.9-2.5 micron spectra of V1047 Cen obtained on 2019 June 30/July 1 and 2019 August 1/2", "columns": [{"name": "Date", "desc": "Date code (1) "}, {"name": "Band", "desc": "[JK] Band corresponding to spectral coverage (2) "}, {"name": "lambda", "desc": "[0.89/2.51] Wavelength "}, {"name": "Flux", "desc": "[1.36e-14/6.76e-13] Observed flux "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_893_46"}} {"id": "J/ApJ/893/46", "title_cds": "The fourth Fermi-GBM GRB catalog: 10 years", "title_create": "von Kienlin+, 2020", "year": "2020", "author": "von Kienlin A., Meegan C.A., Paciesas W.S., Bhat P.N., Bissaldi E., Briggs M.S., Burns E., Cleveland W.H., Gibby M.H., Giles M.M., Goldstein A., Hamburg R., Hui C.M., Kocevski D., Mailyan B., Malacaria C., Poolakkil S., Preece R.D., Roberts O.J., Veres P., Wilson-Hodge C.A.", "title_pub": "The fourth Fermi-GBM gamma-ray burst catalog: a decade of data.", "first_author": "von Kienlin A.", "ref_biblio": [""], "bibcode": ["2020ApJ...893...46V"], "see_also": ["J/ApJS/199/18 : The Fermi GBM catalog (Paciesas+, 2012)", "J/ApJS/207/39 : IPN supplement to the Fermi GBM (Hurley+, 2013)", "J/ApJS/211/13 : The second Fermi/GBM GRB catalog (4yr) (von Kienlin+, 2014)", "J/MNRAS/448/2624 : List of isolated emission episodes in GRB (Charisi+, 2015)", "J/ApJS/218/11 : The 5yr Fermi/GBM magnetar burst catalog (Collazzi+, 2015)", "J/ApJS/216/32 : Localizations of GRBs with Fermi GBM (Connaughton+, 2015)", "J/ApJS/223/28 : The third Fermi/GBM GRB catalog (6yr) (Bhat+, 2016)", "J/ApJ/818/18 : Jet angle & gamma-ray energetic estimations (Goldstein+, 2016)", "J/ApJ/826/37 : Fermi/GBM obs. of V404 Cygni 2015 outburst (Jenke+, 2016)", "J/A+A/588/A135 : Fermi/GBM GRB time-resolved spectral catalog (Yu+, 2016)", "J/ApJS/229/31 : IPN supplement to the 2nd Fermi GBM catalog (Hurley+, 2017)", "J/ApJ/886/20 : Bayesian time-resolved spectra of Fermi GBM pulses (Yu+, 2019)"], "keyword_cds": "GRB", "keyword_pub": "Catalogs ; Gamma-ray bursts", "mission": "Fermi", "abstract": ["We present the fourth in a series of catalogs of gamma-ray bursts", "(GRBs) observed with Fermi's Gamma-ray Burst Monitor (Fermi-GBM). It", "extends the six year catalog by four more years, now covering the 10yr", "time period from trigger enabling on 2008 July 12 to 2018 July 11.", "During this time period GBM triggered almost twice a day on transient", "events, 2356 of which we identified as cosmic GRBs. Additional trigger", "events were due to solar flare events, magnetar burst activities, and", "terrestrial gamma-ray flashes. The intention of the GBM GRB catalog", "series is to provide updated information to the community on the most", "important observables of the GBM-detected GRBs. For each GRB the", "location and main characteristics of the prompt emission, the", "duration, peak flux, and fluence are derived. The latter two", "quantities are calculated for the 50-300keV energy band, where the", "maximum energy release of GRBs in the instrument reference system is", "observed and also for a broader energy band from 10-1000keV,", "exploiting the full energy range of GBM's low-energy detectors.", "Furthermore, information is given on the settings of the triggering", "criteria and exceptional operational conditions during years 7 to 10", "in the mission. This fourth catalog is an official product of the", "Fermi-GBM science team, and the data files containing the complete", "results are available from the High-Energy Astrophysics Science", "Archive Research Center."], "description": ["Fermi-GBM is one of two instruments on the Fermi Gamma-ray Space", "Telescope, which was launched on 2008 June 11. GBM is made up of two", "types of scintillation detectors, 12 NaI(Tl) detectors, sensitive from", "8keV to ~1MeV, and two BGO detectors, sensitive from 200keV to 40MeV."], "alias": ["Fermi GBM"], "type": ["OC"], "data": "", "date_update": "31-Mar-2021", "tables": [{"name": "table3.dat", "desc": "Trigger modification history ", "columns": [{"name": "Date", "desc": "Observation date "}, {"name": "Time", "desc": "Observation time; yyyy/DOY:hh:mm:ss UT "}, {"name": "Command", "desc": "Command "}, {"name": "Reason", "desc": "Reason "}]}, {"name": "table4.dat", "desc": "GRB triggers: locations and trigger characteristics ", "columns": [{"name": "Fermi", "desc": "Trigger identifier (bnYYMMDDddd) "}, {"name": "f_Fermi", "desc": "[A-Cb-z] Flag on Fermi (1) "}, {"name": "GRB", "desc": "Gamma-ray burst identifier (GRB YYMMDDA) "}, {"name": "Obs", "desc": "UT time of the observation "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "Error", "desc": "[0/68.1] Position error "}, {"name": "Loc", "desc": "Location source "}, {"name": "Al", "desc": "[0/56] Algorithm (2) "}, {"name": "Time", "desc": "[0/8192] Timescale "}, {"name": "Energy", "desc": "Energy range "}, {"name": "Other", "desc": "Other detection(s) (3) "}]}, {"name": "table5.dat", "desc": "GRB durations (50-300keV) ", "columns": [{"name": "Fermi", "desc": "Trigger identifier "}, {"name": "f_Fermi", "desc": "Flag on Fermi (1) "}, {"name": "Det", "desc": "Detectors Used "}, {"name": "T90", "desc": "[0.008/829] Duration between 5% and 95% of maximum fluence"}, {"name": "e_T90", "desc": "[0.02/54] Uncertainty in T90 "}, {"name": "T90st", "desc": "[-808/189] Start of T_90_ burst duration "}, {"name": "T50", "desc": "[0.008/737] Duration between 25% and 75% of maximum fluence"}, {"name": "e_T50", "desc": "[0.01/40] Uncertainty in T50 "}, {"name": "T50st", "desc": "[-737/223] Start of T_50_ burst duration "}]}, {"name": "table6.dat", "desc": "GRB fluence & peak flux (10-1000keV) ", "columns": [{"name": "Fermi", "desc": "Trigger identifier "}, {"name": "Fluence", "desc": "[2.5e-8/0.0025] Fluence; erg/cm^2^ "}, {"name": "e_Fluence", "desc": "[3.6e-9/1.5e-5] Uncertainty in Fluence "}, {"name": "PF64", "desc": "[1.4/3055] Peak flux on the 0.064s timescale "}, {"name": "e_PF64", "desc": "[0.3/4476] Uncertainty in PF64 "}, {"name": "PF256", "desc": "[0.8/1211] Peak flux on the 0.256s timescale "}, {"name": "e_PF256", "desc": "[0.1/1119] Uncertainty in PF256 "}, {"name": "PF1024", "desc": "[0.2/1052] Peak flux on the 1.024s timescale "}, {"name": "e_PF1024", "desc": "[0.09/280] Uncertainty in PF1024 "}]}, {"name": "table7.dat", "desc": "GRB fluence & peak flux (50-300keV) ", "columns": [{"name": "Fermi", "desc": "Trigger identifier "}, {"name": "Fluence", "desc": "[1.3e-8/0.00082] Fluence; erg/cm^2^ "}, {"name": "e_Fluence", "desc": "[1.5e-9/1.4e-6] Uncertainty in Fluence "}, {"name": "PF64", "desc": "[0.08/577] Peak flux on the 0.064s timescale "}, {"name": "e_PF64", "desc": "[0.04/21] Uncertainty in PF64 "}, {"name": "PF256", "desc": "[0.03/557] Peak flux on the 0.256s timescale "}, {"name": "e_PF256", "desc": "[0.02/7] Uncertainty in PF256 "}, {"name": "PF1024", "desc": "[0.01/497] Peak flux on the 1.024s timescale "}, {"name": "e_PF1024", "desc": "[0.01/2.1] Uncertainty in PF1024 "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_873_35"}} {"id": "J/ApJ/873/35", "title_cds": "Gemini GNIRS NIR spectroscopy of 50 QSOs at z>~5.7", "title_create": "Shen+, 2019", "year": "2019", "author": "Shen Y., Wu J., Jiang L., Banados E., Fan X., Ho L.C., Riechers D.A., Strauss M.A., Venemans B., Vestergaard M., Walter F., Wang F., Willott C., Wu X.-B., Yang J.", "title_pub": "Gemini GNIRS near-infrared spectroscopy of 50 quasars at z>=5.7.", "first_author": "Shen Y.", "ref_biblio": [""], "bibcode": ["2019ApJ...873...35S"], "see_also": ["II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "II/359 : The VISTA Hemisphere Survey (VHS) catalog DR4.1 (McMahon+, 2013)", "II/343 : VIKING catalogue data release 2 (Edge+, 2016)", "VII/283 : The Million Quasars (Milliquas) catalog (6.3) (Flesch, 2019)", "J/ApJ/613/682 : AGN central masses & broad-line reg. sizes (Peterson+, 2004)", "J/ApJS/166/470 : SDSS-Spitzer type I QSOs IR photometry (Richards+, 2006)", "J/AJ/135/2453 : Sample of BL Lac objects from SDSS & FIRST (Plotkin+, 2008)", "J/ApJ/680/169 : SDSS DR5 virial black hole masses (Shen+, 2008)", "J/ApJ/699/782 : High-redshift SDSS-DR5 QSOs (Diamond-Stanic+, 2009)", "J/ApJ/692/758 : BAL QSOs in SDSS-DR5 (Gibson+, 2009)", "J/ApJ/699/800 : Mass functions of active black holes (Vestergaard+, 2009)", "J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010)", "J/MNRAS/410/860 : Redshift dependence of BAL QSOs (Allen+, 2011)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/ApJ/746/169 : Luminosity function of broad-line quasars (Shen+, 2012)", "J/ApJ/753/125 : NIR spectroscopy follow-up of 60 SDSS-DR7 QSOs (Shen+, 2012)", "J/ApJ/761/112 : High-z MgII absorption QSOs with FIRE (Matejek+, 2012)", "J/ApJ/761/184 : IR luminosities for dusty AGNs and QSOs (Weedman+, 2012)", "J/MNRAS/435/3306 : Candidate type II QSOs in SDSS III (Alexandroff+, 2013)", "J/ApJ/764/45 : Luminosity function of broad-line QSOs. II. (Kelly+, 2013)", "J/ApJ/805/122 : X-ray properties of PHL1811 analogs and WLQs (Luo+, 2015)", "J/ApJS/227/11 : PS1 z>5.6 quasars follow-up (Banados+, 2016)", "J/ApJ/817/55 : NIR spectroscopy of 1.54.5 QSOs with SDSS and WISE. I. Opt. spectra (Wang+, 2016)", "J/MNRAS/465/2120 : Correcting CIV-based virial BH masses (Coatman+, 2017)", "J/ApJ/861/37 : Luminous WISE quasars in SDSS Stripe 82 (Glikman+, 2018)", "J/ApJ/871/258 : ELQS in SDSS. III. Full ELQS quasar cat. (Schindler+, 2019)"], "keyword_cds": "Spectra, infrared; QSOs; Redshifts; Line Profiles; Equivalent widths; Black holes; Surveys", "keyword_pub": "black hole physics; galaxies: active; line: profiles; quasars: general; surveys", "abstract": ["We report initial results from a large Gemini program to observe", "z>~5.7 quasars with GNIRS near-IR spectroscopy. Our sample includes", "50 quasars with simultaneous ~0.85-2.5{mu}m spectra covering the", "rest-frame ultraviolet and major broad emission lines from Ly{alpha}", "to MgII. We present spectral measurements for these quasars and", "compare with their lower redshift counterparts at z=1.5-2.3. We find", "that when quasar luminosity is matched, there are no significant", "differences between the rest-UV spectra of z>~5.7 quasars and the", "low-z comparison sample. High-z quasars have similar continuum and", "emission line properties and occupy the same region in the black hole", "mass and luminosity space as the comparison sample, accreting at an", "average Eddington ratio of ~0.3. There is no evidence for", "super-Eddington accretion or hypermassive (>10^10^M_{sun}_) black", "holes within our sample. We find a mild excess of quasars with weak", "CIV lines relative to the control sample. Our results, corroborating", "earlier studies but with better statistics, demonstrate that these", "high-z quasars are already mature systems of accreting supermassive", "black holes operating with the same physical mechanisms as those at", "lower redshifts."], "description": ["A Gemini-GNIRS survey (Gemini Large and Long Program LLP-7) was", "conducted to obtain near-IR YJHK simultaneous spectroscopy for a", "sample of 50 quasars at z>~5.7 during the 15B-17A semesters.", "The configuration had provided simultaneous spectral coverage of", "~0.85-2.5um at a spectral resolution R~650."], "type": ["OC"], "data": "", "date_update": "12-Aug-2020", "tables": [{"name": "table1.dat", "desc": "Sample summary ", "columns": [{"name": "Fig", "desc": "Figure 3 object number; column added by CDS "}, {"name": "ID", "desc": "Object ID of the GNIRS sample "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "zold", "desc": "[5.7/6.43] Original redshift from the discovery paper"}, {"name": "zsys", "desc": "[5.637/6.42] Improved systemic redshift "}, {"name": "e_zsys", "desc": "[0.005/0.06] Uncertainty in zsys "}, {"name": "Jmag", "desc": "[17.7/21.2]? J band magnitude "}, {"name": "e_Jmag", "desc": "[0.01/0.3]? Uncertainty in Jmag "}, {"name": "Hmag", "desc": "[17/19.5]? H band magnitude "}, {"name": "e_Hmag", "desc": "[0.03/0.2]? Uncertainty in Hmag "}, {"name": "Ksmag", "desc": "[16.1/18.4]? Ks band magnitude "}, {"name": "e_Ksmag", "desc": "[0.03/0.3]? Uncertainty in Ksmag "}, {"name": "r_Jmag", "desc": "Jmag reference (1) "}, {"name": "r_zold", "desc": "[1/18] Discovery reference (2) "}, {"name": "Comm", "desc": "Comment "}]}, {"name": "table3.dat", "desc": "*Catalog ", "columns": [{"name": "ID", "desc": "Object ID of the GNIRS sample "}, {"name": "zold", "desc": "[5.7/6.43] Original redshift from the discovery paper (ZFIT)"}, {"name": "zSys", "desc": "[5.633/6.43] Improved systemic redshift "}, {"name": "e_zSys", "desc": "[0.005/0.06] zSys uncertainty (ZSYS_ERR) "}, {"name": "zMgII", "desc": "[5.95/6.43]?=- Redshift based on broad MgII "}, {"name": "e_zMgII", "desc": "[0.005/0.08]?=- zMgII uncertainty (ZMGII_ERR)"}, {"name": "zCIII", "desc": "[5.59/6.03]?=- Redshift based on the CIII] complex"}, {"name": "e_zCIII", "desc": "[0.005/0.09]?=- zCIII uncertainty (ZCIII_ERR)"}, {"name": "zCIV", "desc": "[5.63/6.36]?=- Redshift based on broad CIV "}, {"name": "e_zCIV", "desc": "[0.009/0.11] zCIV uncertainty (ZCIV_ERR) "}, {"name": "zSiIV", "desc": "[5.69/6.33] Redshift based on broad SiIV/OIV]"}, {"name": "e_zSiIV", "desc": "[0.01/0.06] zSiIV uncertainty (ZSIIV_ERR) "}, {"name": "logL1350", "desc": "[45.2/47.1] Continuum luminosity at restframe 1350{AA}; in erg/s units"}, {"name": "e_logL1350", "desc": "[0.0019/0.5] logL1350 uncertainty (LOGL1350_ERR)"}, {"name": "logL1700", "desc": "[45.19/47.03] Continuum luminosity at restframe 1700{AA}; in erg/s units"}, {"name": "e_logL1700", "desc": "[0.001/0.3] logL1700 uncertainty (LOGL1700_ERR)"}, {"name": "logL3000", "desc": "[45.2/47.02] Continuum luminosity at restframe 3000{AA}; in erg/s units"}, {"name": "e_logL3000", "desc": "[0.001/0.12]LogL3000 uncertainty (LOGL3000_ERR)"}, {"name": "logLBol", "desc": "[45.9/47.8] Log of bolometric luminosity (1) "}, {"name": "e_logLBol", "desc": "[0.001/0.12] logLBol uncertainty (LOGLBOL_ERR)"}, {"name": "pkMgII", "desc": "[2754/2820.2]?=0 MgII peak wavelength in {AA} (MGIIa)"}, {"name": "FWHMMgII", "desc": "[1411/10127]?=0 MgII FWHM (MGIIb) "}, {"name": "logLMgII", "desc": "[43.5/45]?=0 log of MgII line luminosity in erg/s (MGIIc)"}, {"name": "EWMgII", "desc": "[10.8/140]?=0 MgII restframe EW in {AA} (MGIId)"}, {"name": "FMgII", "desc": "[2754/2821]?=0 Top 50% of MgII flux centroid in {AA} (MGIIe)"}, {"name": "pkCIII", "desc": "[1851/1938]?=0 Peak wavelength for the entire CIII] complex (CIII], SiIII], AlIII) in {AA} (CIII_ALLa)"}, {"name": "FWHMCIII", "desc": "[796/35298]?=0 CIII] complex FWHM (CIII_ALLb)"}, {"name": "logLCIII", "desc": "[44/46]?=0 log of CIII] complex luminosity in erg/s (CIII_ALLc)"}, {"name": "EWCIII", "desc": "[9.5/726]?=0 CIII] complex restframe EW in {AA} (CIII_ALLd)"}, {"name": "FCIII", "desc": "[1851/1938]?=0 Top 50% of CIII] complex flux centroid in {AA} (CIII_ALLe)"}, {"name": "pkCIV", "desc": "[1524/1553] Peak wavelength for the entire CIV line (CIVa)"}, {"name": "FWHMCIV", "desc": "[1826/28275] CIV line FWHM (CIVb) "}, {"name": "logLCIV", "desc": "[43.5/45.4] log of CIV line luminosity in erg/s (CIVc)"}, {"name": "EWCIV", "desc": "[2.9/318] CIV restframe EW in {AA} (CIVd) "}, {"name": "FCIV", "desc": "[1524/1553] Top 50% of CIV line flux centroid in {AA} (CIVe)"}, {"name": "pkSiIV", "desc": "[1375/1403] Peak wavelength for the 1400{AA} complex (SiIV, OIV) in {AA} (SIIV_OIVa)"}, {"name": "FWHMSiIV", "desc": "[1411/35298]?=0 SiIV complex restframe EW in {AA} (SIIV_OIVb)"}, {"name": "logLSiIV", "desc": "[42.5/45.4]?=0 log of SiIV complex luminosity in erg/s (SIIV_OIVc)"}, {"name": "EWSiIV", "desc": "[0.7/48.1]?=0 SiIV complex restframe EW in {AA} (SIIV_OIVd)"}, {"name": "FSiIV", "desc": "[1376/1403] Top 50% of SiIV complex flux centroid in {AA} (SIIV_OIVe)"}, {"name": "e_pkMgII", "desc": "[0.5/31]?=- pkMgII uncertainty (MGII_ERRa) "}, {"name": "e_FWHMMgII", "desc": "[115/8519]?=- FWHMMgII uncertainty (MGII_ERRb)"}, {"name": "e_logLMgII", "desc": "[0.01/1.6]?=- logLMgII uncertainty (MGII_ERRc)"}, {"name": "e_EWMgII", "desc": "[0.9/17865]?=- EWMgII uncertainty (MGII_ERRd)"}, {"name": "e_FMgII", "desc": "[0.4/31]?=- FMgII uncertainty (MGII_ERRe) "}, {"name": "e_pkCIII", "desc": "[0.3/39]?=- pkCIII uncertainty (CIII_ALL_ERRa)"}, {"name": "e_FWHMCIII", "desc": "[184/16907]?=- FWHMCIII uncertainty (CIII_ALL_ERRb)"}, {"name": "e_logLCIII", "desc": "[0.01/2.4]?=- logLCIII uncertainty (CIII_ALL_ERRc)"}, {"name": "e_EWCIII", "desc": "[0.5/1.2e+6]?=- EWCIII uncertainty (CIII_ALL_ERRd)"}, {"name": "e_FCIII", "desc": "[0.3/39]?=- FCIII uncertainty (CIII_ALL_ERRe)"}, {"name": "e_pkCIV", "desc": "[0.2/23] pkCIV uncertainty (CIV_ERRa) "}, {"name": "e_FWHMCIV", "desc": "[110/16680] FWHMCIV uncertainty (CIV_ERRb) "}, {"name": "e_logLCIV", "desc": "[0.01/0.5] logLCIV uncertainty (CIV_ERRc) "}, {"name": "e_EWCIV", "desc": "[0.8/422] EWCIV uncertainty (CIV_ERRd) "}, {"name": "e_FCIV", "desc": "[0.2/21] FCIV uncertainty (CIV_ERRe) "}, {"name": "e_pkSiIV", "desc": "[0.005/11.5]?=0 pkSiIV uncertainty (SIIV_OIV_ERRa)"}, {"name": "e_FWHMSiIV", "desc": "[272/16943]?=0 FWHMSiIV uncertainty (SIIV_OIV_ERRb)"}, {"name": "e_logLSiIV", "desc": "[0.01/22]?=0 logLSiIV uncertainty (SIIV_OIV_ERRc)"}, {"name": "e_EWSiIV", "desc": "[0.3/106]?=0 EWSiIV uncertainty (SIIV_OIV_ERRd)"}, {"name": "e_FSiIV", "desc": "[0.03/11.2]?=0 FSiIV uncertainty (SIIV_OIV_ERRe)"}, {"name": "LogBHCIV", "desc": "[8.1/11]?=0 Single-epoch virial BH mass based on CIV (Vestergaard & Peterson 2006ApJ...641..689V) (LOGBH_CIV_VP06)"}, {"name": "e_LogBHCIV", "desc": "[0.02/4.5]?=- LogBHCIV uncertainty (LOGBH_CIV_VP06_ERR)"}, {"name": "LogBHMgII", "desc": "[8.3/10]?=0 Single-epoch virial BH mass based on MgII (Shen+ 2011, J/ApJS/194/45) (LOGBH_MGII_S11)"}, {"name": "e_LogBHMgII", "desc": "[0.018/3.3]?=- LogBHMgII uncertainty (LOGBH_MGII_S11_ERR)"}, {"name": "LogBH", "desc": "[8.1/10.8]?=0 Adopted fiducial BH mass; based on MgII if available, otherwise based on CIV"}, {"name": "e_LogBH", "desc": "[0.01/4.5]?=- LogBH uncertainty (LOGBH_ERR) "}, {"name": "LogEdd", "desc": "[-1.7/0.6]?=- Eddington ratio based on the fiducial BH mass (LOGEDD_RATIO)"}, {"name": "e_LogEdd", "desc": "[0.019/4.5]?=- LogEdd uncertainty (LOGEDD_RATIO_ERR)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_875_111"}} {"id": "J/ApJ/875/111", "title_cds": "HST/COS spectra toward HeII-transparent QSOs", "title_create": "Worseck+, 2019", "year": "2019", "author": "Worseck G., Davies F.B., Hennawi J.F., Prochaska J.X.", "title_pub": "The evolution of the HeII-ionizing background at redshifts 2.3"], "bibcode": ["2019ApJ...875..111W"], "see_also": ["B/hst : HST Archived Exposures Catalog (STScI, 2007)", "VII/286 : SDSS quasar catalog, fourteenth data release (Paris+, 2018)", "J/ApJ/596/768 : Optical depths in 19 QSOs (Schaye+, 2003)", "J/ApJ/690/1181 : UV-bright quasars (Syphers+, 2009)", "J/ApJS/185/20 : UV-bright quasars (Syphers+, 2009)", "J/ApJ/728/23 : GALEX UV-bright high-redshift quasars (Worseck+, 2011)", "J/ApJS/206/4 : SEDs for luminous QSOs (Krawczyk+, 2013)", "J/ApJ/768/105 : z~5 QSO lum. function from SDSS Stripe 82 (McGreer+, 2013)", "J/ApJ/814/40 : Nearby galaxy filaments with UV obs. (Wakker+, 2015)", "J/ApJ/818/113 : HST observations of QSOs with medium spectra (Neeleman+, 2016)", "J/ApJ/837/106 : UV bckg photoionization & photoheating rates (Onorbe+, 2017)", "J/ApJ/847/81 : HeII photoionization rates of quasars (Schmidt+, 2017)", "J/ApJS/230/6 : HST/COS & STIS absorption-line spectrosc. II. (Keeney+, 2017)", "J/ApJ/863/92 : LAE cand. at z~5.7 in the QSO J0148+0600 field (Becker+, 2018)", "J/AJ/155/131 : z~5 QSO luminosity function from the CFHTLS (McGreer+, 2018)", "J/ApJ/852/22 : Ly{alpha} forest power spectrum at 1.8~3 HeII sightlines at", "z>3.5, and study the redshift evolution and sightline-to-sightline", "variance of {tau}_eff_ in 24 HeII sightlines. We confirm an increase", "of the median {tau}_eff_ from ~2 at z=2.7 to {tau}_eff_>~5 at z>3, and", "a scatter in {tau}_eff_ that increases with redshift. The z>3.5 HeII", "absorption is predominantly saturated, but isolated narrow", "({Delta}v<650km/s) transmission spikes indicate patches of reionized", "helium. We compare our measurements to predictions for a range of UV", "background models applied to outputs of a large-volume (146 comoving", "Mpc)^3^ hydrodynamical simulation by forward-modeling our sample's", "quality and size. At z>2.74, the variance in {tau}_eff_ significantly", "exceeds expectations for a spatially uniform UV background, but is", "consistent with a fluctuating radiation field sourced by variations in", "the quasar number density and the mean free path in the", "post-reionization IGM. We develop a method to infer the approximate", "median HeII photoionization rate {Gamma}_HeII_ of a fluctuating UV", "background from the median {tau}_eff_, finding a factor ~5 decrease in", "{Gamma}_HeII_ between z~2.6 and z~3.1. At z~3.1,", "{Gamma}_HeII_=[9.1_-1.2_^+1.1^(stat)_-3.4_^+2.4^(sys)]x10^-16^s^-1^", "corresponds to a median HeII fraction of ~2.5%, indicating that our", "data probe the tail end of HeII reionization."], "description": ["Target selection was performed mainly by applying color cuts to", "combined catalogs of wide-field multiwavelength photometry. The quasar", "candidates were verified with low-resolution (R~200) optical", "spectroscopy, mainly with the Calar Alto Faint Object Spectrograph", "(CAFOS) at the Calar Alto 2.2m telescope and the Kast spectrometer at", "the Lick 3m Shane Telescope during several campaigns (2010-2015).", "Unambiguous redshifts were measured from broad emission lines", "(typically HI Ly{alpha} and CIV).", "In HST Cycles 20 and 22, we used the FUV-sensitive Cosmic Origins", "Spectrograph (COS) to obtain follow-up spectroscopy of eight", "3.12.7 quasars ", "columns": [{"name": "ID", "desc": "Quasar identifier "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "zEm", "desc": "[2.7/4] Quasar emission redshift "}, {"name": "PID", "desc": "[9350/13875] HST Program identifier "}, {"name": "Inst", "desc": "Instrument "}, {"name": "R", "desc": "[1000/16000] Spectral resolution at {lambda}=1150{AA} (R={lambda}/FWHM)"}, {"name": "Exp", "desc": "[4739/50993] Exposure time "}, {"name": "S/N", "desc": "[0/19] Signal-to-Noise ratio per pixel (1) "}, {"name": "F1500", "desc": "[0.5/21.6] Continuum flux density at 1500 Angstroms; in units of 10^-16^erg/cm^2^/s/{AA}"}, {"name": "alpha", "desc": "[-7.4/-0.4] Power-law spectral index (2) "}, {"name": "zAbs", "desc": "[0.13/0.9]? Intervening H I absorber redshift "}, {"name": "l_logNHI", "desc": "[<=~ ] Limit or uncertainty flag on logNHI "}, {"name": "logNHI", "desc": "[15.8/21.2]? Log intervening HI absorber column density"}, {"name": "f_logNHI", "desc": "b = blend "}, {"name": "Ref", "desc": "Data reference code (3) "}]}, {"name": "table5.dat", "desc": "Cumulative distributions of {tau}_eff_ in redshift ranges", "columns": [{"name": "zmin", "desc": "[2.3/3.7] Minimum redshift of the taueff subsample "}, {"name": "zmax", "desc": "[2.5/4] Maximum redshift of the taueff subsample "}, {"name": "taueff", "desc": "[1/6] Effective optical depth value ({tau}_eff_) "}, {"name": "F", "desc": "[0/1] Cumulative distribution function of taueff (F(<{tau}_eff_))"}, {"name": "l_taueff", "desc": "[0/1]? Limit flag on taueff (1) "}]}, {"name": "table7.dat", "desc": "Measured {tau}_eff_ in new or reanalyzed spectra (Table 1)", "columns": [{"name": "ID", "desc": "Quasar identifier "}, {"name": "z", "desc": "[2.56/3.84] Redshift "}, {"name": "taueff", "desc": "[1/6] Effective optical depth value ({tau}_eff_) "}, {"name": "E_taueff", "desc": "[0.02/1.2]? Upper statistical uncertainty in taueff (1)"}, {"name": "e_taueff", "desc": "[0/0.7] Lower statistical uncertainty in taueff "}, {"name": "upSys", "desc": "[0/1.4] Upper systematic uncertainty in taueff "}, {"name": "loSys", "desc": "[0/0.3] Lower systematic uncertainty in taueff "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_885_3"}} {"id": "J/ApJ/885/3", "title_cds": "Short Title", "title_create": "Shipp+, 2019", "year": "2019", "author": "Shipp N., Li T.S., Pace A.B., Erkal D., Drlica-wagner A., Yanny B., Belokurov V., Wester W., Koposov S.E., Kuehn K., Lewis G.F., Simpson J.D., Wan Z., Zucker D.B., Martell S.L., Wang M.Y., (the S5 Collaboration)", "title_pub": "Proper motions of stellar streams discovered in the Dark Energy Survey.", "first_author": "Shipp N.", "ref_biblio": [""], "bibcode": ["2019ApJ...885....3S"], "keyword_cds": "", "keyword_pub": "Stellar kinematics; Milky Way Galaxy; Milky Way stellar halo Local Group; Galaxy structure", "mission": "", "abstract": ["We cross-match high-precision astrometric data from Gaia DR2 with accurate multiband photometry from the Dark Energy Survey (DES) DR1 to confidently measure proper motions for nine stellar streams in the DES footprint: Aliqa Uma, ATLAS, Chenab, Elqui, Indus, Jhelum, Phoenix, Tucana III, and Turranburra. We determine low-confidence proper-motion measurements for four additional stellar streams: Ravi, Wambelong, Willka Yaku, and Turbio. We find evidence for a misalignment between stream tracks and the systemic proper motion of streams that may suggest a systematic gravitational influence from the Large Magellanic Cloud (LMC). These proper motions, when combined with radial velocity measurements, will allow for detailed orbit modeling that can be used to constrain properties of the LMC and its effect on nearby streams, as well as global properties of the Milky Way's gravitational potential."], "object": [], "curator": "Coralie Fix [CDS]", "data": "", "date_update": "17-Mar-2021"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJ_879_125"}} {"id": "J/ApJ/879/125", "title_cds": "", "title_create": "Zucker+, 2019", "year": "2019", "author": "Zucker C., Speagle J.S., Schlafly E.F., Green G.M., Finkbeiner D.P., Goodman A.A., Alves J.", "title_pub": "A Large Catalog of Accurate Distances to Local Molecular Clouds: The Gaia DR2 Edition.", "first_author": "Zucker C.", "bibcode": [""], "bibcode": ["2019ApJ...884L..42K"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "V/153 : LAMOST DR4 catalogs (Luo+, 2018)", "J/ApJS/192/2 : A Bayesian search for binaries in Hipparcos (Shaya+, 2011)", "J/other/RAA/11.924 : Atmospheric parameters for 771 stars (Wu+, 2011)", "J/AJ/144/102 : Wide companions to Hipparcos stars (Tokovinin+, 2012)", "J/A+A/583/A85 : Binaries in beta Pic moving group (Alonso-Floriano+, 2015)", "J/MNRAS/472/675 : Wide bin. in Tycho-Gaia: search method (Andrews+, 2017)", "J/AJ/153/259 : GAMBLES extension of the SLoWPoKES cat. (Oelkers+, 2017)", "J/AJ/153/257 : Comoving stars in Gaia DR1 (Oh+, 2017)", "J/MNRAS/473/5393 : Wide binaries in Tycho-Gaia (Andrews+, 2018)", "J/AJ/155/149 : Co-moving stars observed by Gaia (Bochanski+, 2018)", "J/AJ/157/78 : Multiple star syst. from Gaia DR2 (Jimenez-Esteban+, 2019)"], "keyword_cds": "Stars, double and multiple; Abundances, [Fe/H]; Proper motions; Radial velocities; Stars, distances", "keyword_pub": "Galaxy: evolution ; Galaxy: kinematics and dynamics ; open clusters and associations: general", "abstract": ["It is challenging to reliably identify stars that were born together", "outside of actively star-forming regions and bound stellar systems.", "However, conatal stars should be present throughout the Galaxy, and", "their demographics can shed light on the clustered nature of star", "formation and the dynamical state of the disk. In previous work we", "presented a set of simulations of the Galactic disk that followed the", "clustered formation and dynamical evolution of 4 billion individual", "stars over the last 5Gyr. The simulations predict that a high fraction", "of comoving stars with physical and 3D velocity separation of", "{Delta}r<20pc and {Delta}v<1.5km/s are conatal. In this Letter, we use", "Gaia DR2 and LAMOST DR4 data to identify and study comoving pairs. We", "find that the distribution of relative velocities and separations of", "pairs in the data is in good agreement with the predictions from the", "simulation. We identify 111 comoving pairs in the solar neighborhood", "with reliable astrometric and spectroscopic measurements. These pairs", "show a strong preference for having similar metallicities when", "compared to random field pairs. We therefore conclude that these pairs", "were very likely born together. The simulations predict that conatal", "pairs are born in clusters that follow the overall cluster mass", "function and in relatively young (<1Gyr) star clusters. Gaia will", "eventually deliver well-determined metallicities for the brightest", "stars, enabling the identification of thousands of conatal pairs due", "to disrupting star clusters in the solar neighborhood."], "type": ["CCC"], "data": "", "date_update": "30-Mar-2021", "tables": [{"name": "star1.dat", "desc": "Co-moving pairs in Gaia DR2 + LAMOST DR4 -- primary star data", "columns": [{"name": "Gaia", "desc": "Gaia DR2 identifier (gidp) "}, {"name": "Xgal", "desc": "[-8.96/-7.68] Galactocentric X (xp) "}, {"name": "Ygal", "desc": "[-0.37/0.58] Galactocentric Y (yp) "}, {"name": "Zgal", "desc": "[-0.37/0.52] Galactocentric Z (zp) "}, {"name": "VX", "desc": "[-61.9/74.6] Galactocentric VX (vxp) "}, {"name": "VY", "desc": "[189.9/280.1] Galactocentric VY (vyp) "}, {"name": "VZ", "desc": "[-34.5/25.6] Galactocentric VZ (vzp) "}, {"name": "RAdeg", "desc": "[0.3/358.8] Right ascension (J2000) (rap) "}, {"name": "DEdeg", "desc": "[-7.4/57.8] Declination (J2000) (decp) "}, {"name": "plx", "desc": "[1/10.7] Parallax (parallaxp) "}, {"name": "pmRA", "desc": "[-70/352] Proper motion in right ascension (pmrap)"}, {"name": "pmDE", "desc": "[-76/50] Proper motion in declination (pmdecp) "}, {"name": "RV", "desc": "[-67/52] Radial velocity (rvp) "}, {"name": "Gmag", "desc": "[9/13.3] Gaia G-band magnitude (Gmagp) "}, {"name": "BP-RP", "desc": "[0.4/1.8] BP-RP color index (bp_rpp) "}, {"name": "obsid", "desc": "LAMOST observation ID (obsidp) "}, {"name": "snru", "desc": "[0.3/203] SNR in u-band (snrup) "}, {"name": "snrg", "desc": "[14/598] SNR in g-band (snrgp) "}, {"name": "snrr", "desc": "[34/999] SNR in r-band (snrrp) "}, {"name": "snri", "desc": "[40/999] SNR in i-band (snrip) "}, {"name": "snrz", "desc": "[24/999] SNR in z-band (snrzp) "}, {"name": "Teff", "desc": "[3901/7580] LAMOST effective temperature (teffp)"}, {"name": "e_Teff", "desc": "[8/287] Teff uncertainty (teff_errp) "}, {"name": "logg", "desc": "[2.7/4.9] Log of surface gravity (loggp) "}, {"name": "[Fe/H]", "desc": "[-0.7/0.6] Metallicity (fehp) "}, {"name": "e_[Fe/H]", "desc": "[0.007/0.3] Uncertainty in [Fe/H] (feherrp) "}, {"name": "Sep", "desc": "[0.002/0.02] 3D separation (dr) "}, {"name": "delV", "desc": "[0.3/1.5] 3D velocity difference (dv) "}, {"name": "Conn", "desc": "[2] Connectivity (2=mutually exclusive) "}, {"name": "dfeh", "desc": "[0.002/0.9] Difference in [Fe/H] for pair (dfeh)"}, {"name": "dteff", "desc": "[1.4/198.3] Difference in effective temperature for pair (dteff)"}, {"name": "RUWE", "desc": "[0.7/1.7] Re-normalised unit weight error "}, {"name": "Nvis", "desc": "[8/21] Number of visibility periods (nvs) "}, {"name": "Nrvt", "desc": "[3/27] Number of radial velocity transits (rvnbs)"}, {"name": "Dist", "desc": "[93/878] Distance to star (dists) "}]}, {"name": "star2.dat", "desc": "Co-moving pairs in Gaia DR2 + LAMOST DR4 -- secondary star data", "columns": [{"name": "Gaia", "desc": "Gaia DR2 identifier (gidp) "}, {"name": "Xgal", "desc": "[-8.96/-7.68] Galactocentric X (xp) "}, {"name": "Ygal", "desc": "[-0.37/0.58] Galactocentric Y (yp) "}, {"name": "Zgal", "desc": "[-0.37/0.52] Galactocentric Z (zp) "}, {"name": "VX", "desc": "[-61.9/74.6] Galactocentric VX (vxp) "}, {"name": "VY", "desc": "[189.9/280.1] Galactocentric VY (vyp) "}, {"name": "VZ", "desc": "[-34.5/25.6] Galactocentric VZ (vzp) "}, {"name": "RAdeg", "desc": "[0.3/358.8] Right ascension (J2000) (rap) "}, {"name": "DEdeg", "desc": "[-7.4/57.8] Declination (J2000) (decp) "}, {"name": "plx", "desc": "[1/10.7] Parallax (parallaxp) "}, {"name": "pmRA", "desc": "[-70/352] Proper motion in right ascension (pmrap)"}, {"name": "pmDE", "desc": "[-76/50] Proper motion in declination (pmdecp) "}, {"name": "RV", "desc": "[-67/52] Radial velocity (rvp) "}, {"name": "Gmag", "desc": "[9/13.3] Gaia G-band magnitude (Gmagp) "}, {"name": "BP-RP", "desc": "[0.4/1.8] BP-RP color index (bp_rpp) "}, {"name": "obsid", "desc": "LAMOST observation ID (obsidp) "}, {"name": "snru", "desc": "[0.3/203] SNR in u-band (snrup) "}, {"name": "snrg", "desc": "[14/598] SNR in g-band (snrgp) "}, {"name": "snrr", "desc": "[34/999] SNR in r-band (snrrp) "}, {"name": "snri", "desc": "[40/999] SNR in i-band (snrip) "}, {"name": "snrz", "desc": "[24/999] SNR in z-band (snrzp) "}, {"name": "Teff", "desc": "[3901/7580] LAMOST effective temperature (teffp)"}, {"name": "e_Teff", "desc": "[8/287] Teff uncertainty (teff_errp) "}, {"name": "logg", "desc": "[2.7/4.9] Log of surface gravity (loggp) "}, {"name": "[Fe/H]", "desc": "[-0.7/0.6] Metallicity (fehp) "}, {"name": "e_[Fe/H]", "desc": "[0.007/0.3] Uncertainty in [Fe/H] (feherrp) "}, {"name": "Sep", "desc": "[0.002/0.02] 3D separation (dr) "}, {"name": "delV", "desc": "[0.3/1.5] 3D velocity difference (dv) "}, {"name": "Conn", "desc": "[2] Connectivity (2=mutually exclusive) "}, {"name": "dfeh", "desc": "[0.002/0.9] Difference in [Fe/H] for pair (dfeh)"}, {"name": "dteff", "desc": "[1.4/198.3] Difference in effective temperature for pair (dteff)"}, {"name": "RUWE", "desc": "[0.7/1.7] Re-normalised unit weight error "}, {"name": "Nvis", "desc": "[8/21] Number of visibility periods (nvs) "}, {"name": "Nrvt", "desc": "[3/27] Number of radial velocity transits (rvnbs)"}, {"name": "Dist", "desc": "[93/878] Distance to star (dists) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_102_411"}} {"id": "J/ApJS/102/411", "title_cds": "Neutrino Energy Loss in Stellar Interiors. VII", "title_create": "Itoh+ 1996", "year": "1996", "author": "Itoh N., Hayashi H., Nishikawa A., Kohyama Y.", "title_pub": "Neutrino Energy Loss in Stellar Interiors. VII. Pair, Photo-, Plasma, Bremsstrahlung, and Recombination Neutrino Processes.", "first_author": "Itoh N.", "ref_biblio": [""], "bibcode": ["1996ApJS..102..411I\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "dense matter - elementary particles - methods: numerical - radiation mechanisms: nonthermal - stars: interiors", "abstract": ["The results of the calculations of the neutrino energy-loss rates", "resulting from pair, photo-, plasma, bremsstrahlung, and recombination", "processes are summarized in the form of analytic fitting formulae and", "tables. Care has been taken in order to serve the convenience of the", "users of these results. We have tried to make the present paper as", "self-contained as possible. The contents of the present paper are", "intended to serve as useful physical input data for stellar evolution", "computations. We intend to publish the numerical data and the FORTRAN", "codes for the results of the neutrino energy-loss rates in the CD-ROM", "series of the American Astronomical Society. In the CD-ROM, we intend", "to give three options for the FORTRAN codes. The first option", "comprises the results with analytic fitting formulae only. The", "second option comprises the results with analytic fitting formulae for", "the bremsstrahlung and recombination neutrino processes, and the", "numerical tables for the pair, photo- and plasma neutrino processes", "with a standard quadratic interpolation procedure. In this option,", "the grid of log T for the pair neutrino energy-loss rate is 0.2. The", "third option is a variant of the second option, with the replacement", "of the grid of log T for the pair neutrino energy-loss rate to be", "0.05."], "description": ["The contents of the directories listed below are adequately described", "by the author-supplied documentation, and the manuscript for the paper", "accepted by the Astrophysical Journal Supplement Series. The", "following is directly from the file 'content.doc' supplied by the", "authors."], "curator": "Lee Brotzman [ADS]", "doi_pub": ["10.1086/192264"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_107_175"}} {"id": "J/ApJS/107/175", "title_cds": "Steep-spectrum radio galaxies VLA imaging", "title_create": "Rhee+, 1996", "year": "1996", "author": "Rhee G., Marvel K., Wilson T., Roland J., Bremer M., Jackson N., Webb J.", "title_pub": "VLA imaging of a sample of steep-spectrum radio galaxies.", "first_author": "Rhee G.", "ref_biblio": [""], "bibcode": ["1996ApJS..107..175R\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/192359"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_107_312"}} {"id": "J/ApJS/107/312", "title_cds": "Ordinary Cool Stars in K Band", "title_create": "Wallace+ 1996", "year": "1996", "author": "Wallace L., Hinkle K.", "title_pub": "High Resolution Spectra of Ordinary Cool Stars in the K Band", "first_author": "Wallace L.", "ref_biblio": [""], "bibcode": ["1996ApJS..107..312W"], "keyword_cds": "Stars, late-type ; Spectra, infrared ; Atlases", "keyword_pub": "atlases - infrared: stars - line: identification - stars: late-type", "abstract": ["We present an atlas of high-resolution (R>=45,000) 2.02-2.41um spectra", "of 12 representative stars, a sunspot, three Mira variables, and a", "carbon star. The star sample, MK spectral types from about early-G to", "about mid-M, with luminosity classes dwarf to supergiant. The Mira", "variables are one each of M, S, and C types. All of the spectra have", "been corrected for atmospheric absorption and have the major spectral", "features labeled with responsible absorbers. Spectra and line lists", "are also available on the AAS CD-ROM series Vol. 7. (ApJS, 106, 165)", "The 2.0-2.4 um region includes molecular vibration-rotation", "transitions from the CO first overtone, HF fundamental, and several", "bands of H2O as well as the CN red system, an electronic transition.", "The relative contribution of H2O versus CN in cool star spectra is", "discussed. Atomic features include clean measurable lines of H, C, Na,", "Mg, Al, Si, S, Ca, Sc, Ti, V, and Fe. We discuss temperature and", "luminosity spectral indicators and the effects of blending on these", "indicators at lower spectral resolution."], "doi_pub": ["10.1086/192367"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "tablea1.dat", "desc": "Atomic features ", "columns": [{"name": "Atom", "desc": "Atom designation "}, {"name": "Freq", "desc": "Frequency "}]}, {"name": "tablea2.dat", "desc": "Molecular features ", "columns": [{"name": "band", "desc": "Band designation "}, {"name": "Freq", "desc": "Frequency "}, {"name": "Trans", "desc": "Rotational transition "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_120_335"}} {"id": "J/ApJS/120/335", "title_cds": "Gamma-ray source catalog", "title_create": "Macomb+, 1999", "year": "1999", "author": "Macomb D.J., Gehrels N.", "title_pub": "A general gamma-ray source catalog.", "first_author": "Macomb D.J.", "ref_biblio": [""], "bibcode": ["1999ApJS..120..335M"], "see_also": ["J/ApJS/101/259 : The second EGRET catalog (Thompson+ 1995)", "J/ApJS/107/227 : Supplement to Second EGRET Catalog (Thompson+ 1996)", "J/ApJS/123/79 : Third EGRET catalog (3EG) (Hartman+, 1999)"], "keyword_cds": "Gamma rays", "keyword_pub": "catalog - gamma rays: observations", "abstract": ["The past several years have seen unprecedented growth in the field of", "gamma-ray astronomy. Highly successful missions such as the Compton", "Gamma-Ray Observatory (CGRO) have led to both a great increase in the", "number of detected gamma-ray sources and a more fundamental", "understanding of the basic physical processes involved for those", "sources. New ground-based observatories, the Rossi X-Ray Timing", "Explorer (RXTE), and the SIGMA instrument aboard the GRANAT spacecraft", "have all contributed to this explosion. Detailed observations of", "active galaxies, pulsars, accreting binaries, and diffuse emission", "have had a tremendous impact on our view of the universe. Given that", "new experiments that will provide a similar increase in source numbers", "are several years away, it is a good time to take inventory of the", "state of gamma-ray astronomy. To this end, we have developed a general", "gamma-ray point-source catalog containing 309 objects that summarize", "the field. Gamma-ray astronomy, as we define it, includes photon", "energies from 50 keV to about 1 TeV. While many catalogs concentrate", "on a single type of astronomical object and/or a very restricted", "energy range, the nature of this catalog is somewhat different. The", "large variety of objects and the many orders of magnitude in energy", "space covered by gamma-ray astronomy presents an organizational", "challenge. We focus on two main types of information: a general", "listing of the basic characteristics of each source, and detailed", "tables of a representative sample of high-energy observations. We also", "summarize the gamma-ray instruments whose observations are included in", "the catalog."], "doi_pub": ["10.1086/313182"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1a.dat", "desc": "Gamma-Ray Source Summary ", "columns": [{"name": "Name", "desc": "Source Name "}, {"name": "Type", "desc": "Source type "}, {"name": "GLON", "desc": "Galactic position "}, {"name": "GLAT", "desc": "Galactic position "}, {"name": "RAdeg", "desc": "Celestial position (2000) "}, {"name": "DEdeg", "desc": "Celestial position (2000) "}, {"name": "Dist1", "desc": "? Lower range in distance (galactic sources) "}, {"name": "n_Dist1", "desc": "[-] Indicates an interval of distances "}, {"name": "Dist2", "desc": "? Upper range in distance (galactic sources) "}, {"name": "z", "desc": "? Redshift (extragalactic sources) "}, {"name": "Energy", "desc": "Energy ranges "}, {"name": "Names", "desc": "Alternate Names "}]}, {"name": "table1b.dat", "desc": "Gamma-Ray Source, General informations ", "columns": [{"name": "Name", "desc": "Source name "}, {"name": "Com", "desc": "Comments "}]}, {"name": "table2.dat", "desc": "Source observations ", "columns": [{"name": "Type", "desc": "[A-G] Type of source (G1) "}, {"name": "Name", "desc": "Most common name for the source in the gamma-ray literature"}, {"name": "n_Name", "desc": "[*] when 2 entries for the same observation "}, {"name": "Inst", "desc": "Name of the experiment whose results are described by the current row"}, {"name": "E1", "desc": "Lower energy limit (1) "}, {"name": "E2", "desc": "? Upper energy limit (1) "}, {"name": "l_E2", "desc": "[L] for the observation of a line "}, {"name": "l_Flux", "desc": "limit flag on Flux "}, {"name": "Flux", "desc": "? Flux , over the energy range E1 - E2 (2) "}, {"name": "e_Flux", "desc": "? rms uncertainty on Flux "}, {"name": "f_Flux", "desc": "[)] When fluxes within (...) "}, {"name": "n_Flux", "desc": "Various notes on Flux (units, range,...) (3) "}, {"name": "Norm", "desc": "? Normalisation constant in spectral fit "}, {"name": "e_Norm", "desc": "? rms uncertainty on Normalisation "}, {"name": "f_Norm", "desc": "[)] When Norm within (...) "}, {"name": "n_Norm", "desc": "Various notes on Normalisation "}, {"name": "l_Index", "desc": "Limit flag on Index "}, {"name": "Index", "desc": "? spectral form (4) "}, {"name": "e_Index", "desc": "? rms uncertainty on Index "}, {"name": "f_Index", "desc": "[)] When Index within (...) "}, {"name": "n2_Index", "desc": "[o] when Index is the temperature in keV "}, {"name": "n_Index", "desc": "Notes about the spectral form "}, {"name": "E0", "desc": "? Energy at which the normalization is evaluated"}, {"name": "n_E0", "desc": "Second value of E0 "}, {"name": "Date", "desc": "Calendar dates for the observations. (5) "}, {"name": "r_Name", "desc": "At least, one reference for the observation in question (see \"refs.dat\" file)"}]}, {"name": "refs.dat", "desc": "References to table2.dat ", "columns": [{"name": "Ref", "desc": "Reference number "}, {"name": "Bibcode", "desc": "Simbad bibcode "}, {"name": "Aut", "desc": "Author's names "}, {"name": "Com", "desc": "Comments "}]}, {"name": "table3.dat", "desc": "Observation notes ", "columns": [{"name": "Type", "desc": "[A-G] Type (G1) "}, {"name": "Name", "desc": "Source name "}, {"name": "Inst", "desc": "Name of the experiment "}, {"name": "Notes", "desc": "Text of the note "}]}, {"name": "table4.dat", "desc": "Gamma-ray instruments ", "columns": [{"name": "Inst", "desc": "Name of the experiment "}, {"name": "n_Inst", "desc": "Note on Inst "}, {"name": "TypeInst", "desc": "A brief description of the instrument type, based upon the nature of the photon detection mechanism"}, {"name": "Energy", "desc": "Usually the stated energy range of the experiment in question, independent of the stated energy ranges of the catalog"}, {"name": "Refs", "desc": "One or several pointers to appropriate information"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_121_417"}} {"id": "J/ApJS/121/417", "title_cds": "Compact nuclei in galaxies. I.", "title_create": "Sarajedini+ 1999", "year": "1999", "author": "Sarajedini V.L., Green R.F., Griffiths R.E., Ratnatunga K.", "title_pub": "Compact nuclei in galaxies at moderate redshift. I. Imaging and spectroscopy.", "first_author": "Sarajedini V.L.", "ref_biblio": [""], "bibcode": ["1999ApJS..121..417S"], "see_also": ["http://archive.stsci.edu/mds/mds.cgi : MDS website"], "keyword_cds": "Galaxy catalogs ; Redshifts ; Magnitudes", "keyword_pub": "galaxies: active - galaxies: nuclei - galaxies: starburst - surveys", "mission": "HST", "description": ["In this paper, the first of two for this study, we present the", "selected Hubble Space Telescope imaged galaxies having unresolved", "nuclei and discuss the selection procedure. We also present the", "ground-based spectroscopy for these galaxies as well as the", "photometric redshift predictions for those galaxies without spectra."], "doi_pub": ["10.1086/313199"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "MDS fields ", "columns": [{"name": "MDS", "desc": "Field name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "o_Vmag", "desc": "Number of V exposures "}, {"name": "Vexp", "desc": "Total V exposure time "}, {"name": "o_Imag", "desc": "Number of I exposures "}, {"name": "Iexp", "desc": "Total I exposure time "}, {"name": "Vmag", "desc": "Limiting V integrated galaxy magnitude for fitting galaxies with a three-component model"}, {"name": "Imag", "desc": "Limiting I integrated galaxy magnitude for fitting galaxies with a three-component model"}, {"name": "Ngal", "desc": "Number of galaxies in the I image above this limiting magnitude"}, {"name": "Note", "desc": "[a] Note "}]}, {"name": "table2.dat", "desc": "Model parameters for galaxies containing unresolved nuclei", "columns": [{"name": "ID", "desc": "Identification number "}, {"name": "Name", "desc": "Object name "}, {"name": "Imag", "desc": "I magnitude of the galaxy model "}, {"name": "e_Imag", "desc": "rms uncertainty on Imag "}, {"name": "log(hlr)", "desc": "log of the I filter half-light radius "}, {"name": "e_log(hlr)", "desc": "rms uncertainty on log(hlr) "}, {"name": "V-I", "desc": "V-I galaxy colour index "}, {"name": "e_V-I", "desc": "rms uncertainty on V-I "}, {"name": "B/TI", "desc": "I bulge-to-total measurement "}, {"name": "P/TI", "desc": "I point-source-to-total measurement "}, {"name": "P/TV", "desc": "V point-source-to-total measurement "}, {"name": "V-Ip", "desc": "? V-I colour index of the point source "}, {"name": "e_V-Ip", "desc": "? rms uncertainty on V-Ip "}]}, {"name": "table4.dat", "desc": "Redshift list ", "columns": [{"name": "ID", "desc": "Identification number "}, {"name": "Name", "desc": "Object name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "z", "desc": "Redshift "}, {"name": "u_z", "desc": "[? ] Uncertainty flag on z "}, {"name": "e_z", "desc": "? rms uncertainty on z "}, {"name": "Note", "desc": "[*12] Notes (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_125_35"}} {"id": "J/ApJS/125/35", "title_cds": "ACO clusters redshifts and velocity dispersions", "title_create": "Struble+ 1999", "year": "1999", "author": "Struble M.F., Rood H.J.", "title_pub": "A compilation of redshifts and velocity dispersions for ACO clusters.", "first_author": "Struble M.F.", "ref_biblio": [""], "bibcode": ["1999ApJS..125...35S"], "see_also": ["VII/4 : Abell and Zwicky Clusters of Galaxies (Abell+ 1974)", "VII/110 : Rich Clusters of Galaxies (Abell+ 1989)", "VII/56 : Redshifts for Abell Clusters (Sarazin+ 1982)", "VII/177 : Redshifts and Vel Dispersions for Abell Clusters (Struble+, 1991)"], "keyword_cds": "Clusters, galaxy ; Redshifts ; Velocity dispersion", "keyword_pub": "galaxies: clusters: general - galaxies: distances and redshifts", "abstract": ["We present a compilation of redshifts for 1572 Abell, Corwin, & Olowin", "(ACO, 1989, Cat. ) clusters, referenced to both the", "heliocentric and cosmic background radiation reference frames, and 395", "velocity dispersions corrected to the reference frame of the cluster,", "available from the literature as of 1998 December. We present an", "additional list of 81 ACO clusters with published redshifts which are", "probably those of galaxies or groups superimposed on, or near, the ACO", "cluster position."], "doi_pub": ["10.1086/313274"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Redshifts and velocity dispersions for ACO clusters", "columns": [{"name": "ACO", "desc": "ACO number "}, {"name": "n_ACO", "desc": "[*] *: membership in Abell's (1958, See Cat. ) nonstatistical sample"}, {"name": "zh", "desc": "Adopted heliocentric redshift "}, {"name": "u_zh", "desc": "Uncertainty flag on zh "}, {"name": "a", "desc": "? [2-3] Flag indicating the accuracy of z_h_ in the original references (1)"}, {"name": "zC", "desc": "Redshift with respect to the cosmic background radiation (2)"}, {"name": "l_Nz", "desc": "Limit flag on Nz "}, {"name": "Nz", "desc": "Number of cluster members with published redshift (3)"}, {"name": "sigma", "desc": "? Adopted velocity dispersion in the rest frame of the cluster"}, {"name": "Ref", "desc": "References for redshift and radial velocity (4) "}, {"name": "Note", "desc": "[0nN] Note on comments (5) "}]}, {"name": "table2.dat", "desc": "New and Revised Notes to Table 1 ", "columns": [{"name": "ACO", "desc": "Cluster number "}, {"name": "Note", "desc": "Text of the note (1) "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference number "}, {"name": "BibCode", "desc": "BibCode "}, {"name": "Aut", "desc": "Author's name "}, {"name": "Com", "desc": "Comments "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_130_37"}} {"id": "J/ApJS/130/37", "title_cds": "Analysis of the Ly{alpha} forest at z=0-5. I.", "title_create": "Scott+ 2000", "year": "2000", "author": "Scott J., Bechtold J., Dobrzycki A.", "title_pub": "A uniform analysis of the Ly{alpha} forest at z=0-5. I. The sample and distribution of clouds at z>1.7.", "first_author": "Scott J.", "ref_biblio": [""], "bibcode": ["2000ApJS..130...37S\t(SIMBAD/NED"], "see_also": ["http://lithops.as.arizona.edu/~jill/QuasarSpectra/"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/317339"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_139_199"}} {"id": "J/ApJS/139/199", "title_cds": "Catalog of distances of planetary nebulae", "title_create": "Phillips, 2002", "year": "2002", "author": "Phillips J.P.", "title_pub": "The distances of planetary nebulae: a scale based upon nearby sources.", "first_author": "Phillips J.P.", "ref_biblio": [""], "bibcode": ["2002ApJS..139..199P"], "see_also": ["V/84 : Strasbourg-ESO Catalogue of Galactic Planetary Nebulae (Acker+, 1992)", "IV/24 : Catalogue of Galactic Planetary Nebulae (Kohoutek, 2001)"], "keyword_cds": "Planetary nebulae ; Stars, distances", "keyword_pub": "catalogs - planetary nebulae: general", "description": ["We present a database of standard sources that is as complete as", "possible, and that samples the broadest possible range of nebular", "surface brightnesses and radii.", "We have therefore, in order to achieve this, compiled a list of", "sources having distances D <=1.0 sec b kpc, where b is Galactic", "latitude; that is, of sources located within a cylinder of radius", "R_C_=1kpc, centered upon the Sun. This list is presented in", "table1.dat", "A table of standards having well-defined distances, D>1.0 sec b kpc,", "is given in table2.dat", "We have compared the distances obtained here, and summarized in", "table3.dat, with those of Zhang (1995, Cat. ),", "Cahn et al. (1992A&AS...94..399C), van de Steene & Zijlstra", "(1995A&A...293..541V), and Daub (1982ApJ...260..612D)"], "doi_pub": ["10.1086/338028"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Distances and Emission Characteristics of Nearby Reference Nebulae", "columns": [{"name": "Name", "desc": "Planetary nebula name "}, {"name": "n_Name", "desc": "[*] Note on Name (1) "}, {"name": "GC", "desc": "Galactic coordinates (2) "}, {"name": "Dist", "desc": "Distance "}, {"name": "Rad", "desc": "? Radius "}, {"name": "Tb", "desc": "? 5GHz brightness temperature "}, {"name": "r_Dist", "desc": "Reference code for distance, separated by comma in refs.dat file"}, {"name": "Method", "desc": "Method used "}]}, {"name": "table2.dat", "desc": "Distances and Emission Characteristics of Distant Reference Nebulae", "columns": [{"name": "Name", "desc": "Planetary nebula name "}, {"name": "n_Name", "desc": "[*] Note on Name (1) "}, {"name": "GC", "desc": "Galactic coordinates (2) "}, {"name": "Dist", "desc": "Distance "}, {"name": "Rad", "desc": "? Radius "}, {"name": "Tb", "desc": "? 5GHz brightness temperature "}, {"name": "r_Dist", "desc": "Reference code for distance, separated by comma in refs.dat file"}, {"name": "Method", "desc": "Method used "}]}, {"name": "refs.dat", "desc": "References for tables 1 and 2 ", "columns": [{"name": "Ref", "desc": "Reference code "}, {"name": "BibCode", "desc": "BibCode "}, {"name": "Aut", "desc": "Author's name "}, {"name": "Com", "desc": "Comments "}]}, {"name": "table3.dat", "desc": "Statistical Distances to Planetary Nebula ", "columns": [{"name": "Name", "desc": "Planetary nebula name "}, {"name": "n_Name", "desc": "[*W] Note on Name "}, {"name": "PK", "desc": "PK designation (1) "}, {"name": "n_PK", "desc": "[*] Note on PK (2) "}, {"name": "theta", "desc": "Angular radius of the source "}, {"name": "Tb", "desc": "5GHz brightness temperature "}, {"name": "Dist", "desc": "Distance "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_181_o129"}} {"id": "J/ApJS/181/129", "title_cds": "QUEST1 variability survey (QVS). III.", "title_create": "Rengstorf+, 2009", "year": "2009", "author": "Rengstorf A.W., Thompson D.L., Mufson S.L., Andrews P., Honeycutt R.K., Vivas A.K., Abad C., Adams B., Bailyn C., Baltay C., Bongiovanni A., Briceno C., Bruzual G., Coppi P., Della Prugna F., Emmet W., Ferrin I., Fuenmayor F., Gebhard M., Hernandez J., Magris G., Musser J., Naranjo O., Oemler A., Rosenzweig P., Sabbey C.N., Sanchez Ge., Sanchez Gu., Schaefer B., Schenner H., Sinnott J., Snyder J.A., Sofia S., Stock J., Van Altena W.", "title_pub": "QUEST1 Variability Survey. III: Light Curve Catalog Update", "first_author": "Rengstorf A.W.", "ref_biblio": [""], "bibcode": ["2009ApJS..181..129R"], "see_also": ["II/266 : QUEST1 200k light curve catalog (Rengstorf+, 2004)", "J/AJ/127/1158 : QUEST RR Lyrae Survey first catalog (Vivas+, 2004)", "J/AJ/131/1923 : Known quasars in QUEST Variability Survey (Rengstorf+, 2006)", "J/AJ/132/714 : QUEST RR Lyrae survey. II. Halo overdensities (Vivas+, 2006)"], "keyword_cds": "Surveys ; Photometry ; Stars, variable", "keyword_pub": "catalogs - methods: data analysis - surveys", "abstract": ["This paper reports an update to the QUEST1 (QUasar Equatorial Survey", "Team, Phase 1) Variability Survey (QVS) light curve catalog, which", "links QVS instrumental Light curve magnitude at jdlight curves to", "Sloan Digital Sky Survey (SDSS) objects and photometry. In the time", "since the original QVS catalog release, the overlap between publicly", "available SDSS data and QVS data has increased by 8% in sky coverage", "and 16728 in number of matched objects. The astrometric matching and", "the treatment of SDSS masks have been refined for the updated catalog.", "We report on these improvements and present multiple bandpass light", "curves, global variability information, and matched SDSS photometry", "for 214941 QUEST1 objects."], "description": ["QUEST1 constructed a 16-chip CCD camera to be used on the 1m Schmidt", "telescope at the Llano del Hato National Astronomical Observatory in", "Venezuela. Normally operated in the drift-scan mode, an equatorial", "scan will expose any point on the sky for 143s and result in limiting", "magnitudes of B=18.5, V=19.2, and R=19.5 at S/N=10. These data were", "collected between 1999 February and 2001 April."], "date_update": "14-Jan-2010", "tables": [{"name": "catalog.dat", "desc": "QVS Light Curve Catalog, version 2: Main Table ", "columns": [{"name": "QVS2", "desc": "[1/214941] Unique Running Identifier "}, {"name": "QUEST", "desc": "QUEST Identifier (JHHMMSS.s+DDMMSS.s) "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "GCL", "desc": "Global confidence level (GCL) for variability "}, {"name": "N1", "desc": "Number of data points in r1 light curve "}, {"name": "N2", "desc": "Number of data points in b light curve "}, {"name": "N3", "desc": "Number of data points in r3 light curve "}, {"name": "N4", "desc": "Number of data points in v light curve "}, {"name": "ObjID", "desc": "SDSS DR6 Object ID String "}, {"name": "umag", "desc": "?=00.0 SDSS DR6 u band model magnitude "}, {"name": "gmag", "desc": "?=00.0 SDSS DR6 g band model magnitude "}, {"name": "rmag", "desc": "?=00.0 SDSS DR6 r band model magnitude "}, {"name": "imag", "desc": "?=00.0 SDSS DR6 i band model magnitude "}, {"name": "zmag", "desc": "?=00.0 SDSS DR6 z band model magnitude "}]}, {"name": "bmaglc.dat", "desc": "b band light curves ", "columns": [{"name": "QVS2", "desc": "Unique Running Identifier "}, {"name": "JD01", "desc": "Date of observation 1; JD-2451224.0 "}, {"name": "mag1", "desc": "Light curve magnitude at JD1 "}, {"name": "e_mag1", "desc": "rms uncertainty on mag1 "}, {"name": "JD2", "desc": "Date of observation 2; JD-2451224.0 "}, {"name": "mag2", "desc": "Light curve magnitude at JD2 "}, {"name": "e_mag2", "desc": "rms uncertainty on mag2 "}, {"name": "JD3", "desc": "Date of observation 3; JD-2451224.0 "}, {"name": "mag3", "desc": "Light curve magnitude at JD3 "}, {"name": "e_mag3", "desc": "rms uncertainty on mag3 "}, {"name": "JD4", "desc": "? Date of observation 4; JD-2451224.0 "}, {"name": "mag4", "desc": "? Light curve magnitude at JD4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "JD5", "desc": "? Date of observation 5; JD-2451224.0 "}, {"name": "mag5", "desc": "? Light curve magnitude at JD5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "JD6", "desc": "? Date of observation 6; JD-2451224.0 "}, {"name": "mag6", "desc": "? Light curve magnitude at JD6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "JD7", "desc": "? Date of observation 7; JD-2451224.0 "}, {"name": "mag7", "desc": "? Light curve magnitude at JD7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "JD8", "desc": "? Date of observation 8; JD-2451224.0 "}, {"name": "mag8", "desc": "? Light curve magnitude at JD8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "JD9", "desc": "? Date of observation 9; JD-2451224.0 "}, {"name": "mag9", "desc": "? Light curve magnitude at JD9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "JD10", "desc": "? Date of observation 10; JD-2451224.0 "}, {"name": "mag10", "desc": "? Light curve magnitude at JD10 "}, {"name": "e_mag10", "desc": "? rms uncertainty on mag10 "}, {"name": "JD11", "desc": "? Date of observation 11; JD-2451224.0 "}, {"name": "mag11", "desc": "? Light curve magnitude at JD11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}, {"name": "JD12", "desc": "? Date of observation 12; JD-2451224.0 "}, {"name": "mag12", "desc": "? Light curve magnitude at JD12 "}, {"name": "e_mag12", "desc": "? rms uncertainty on mag12 "}, {"name": "JD13", "desc": "? Date of observation 13; JD-2451224.0 "}, {"name": "mag13", "desc": "? Light curve magnitude at JD13 "}, {"name": "e_mag13", "desc": "? rms uncertainty on mag13 "}, {"name": "JD14", "desc": "? Date of observation 14; JD-2451224.0 "}, {"name": "mag14", "desc": "? Light curve magnitude at JD14 "}, {"name": "e_mag14", "desc": "? rms uncertainty on mag14 "}, {"name": "JD15", "desc": "? Date of observation 15; JD-2451224.0 "}, {"name": "mag15", "desc": "? Light curve magnitude at JD15 "}, {"name": "e_mag15", "desc": "? rms uncertainty on mag15 "}, {"name": "JD16", "desc": "? Date of observation 16; JD-2451224.0 "}, {"name": "mag16", "desc": "? Light curve magnitude at JD16 "}, {"name": "e_mag16", "desc": "? rms uncertainty on mag16 "}, {"name": "JD17", "desc": "? Date of observation 17; JD-2451224.0 "}, {"name": "mag17", "desc": "? Light curve magnitude at JD17 "}, {"name": "e_mag17", "desc": "? rms uncertainty on mag17 "}, {"name": "JD18", "desc": "? Date of observation 18; JD-2451224.0 "}, {"name": "mag18", "desc": "? Light curve magnitude at JD18 "}, {"name": "e_mag18", "desc": "? rms uncertainty on mag18 "}, {"name": "JD19", "desc": "? Date of observation 19; JD-2451224.0 "}, {"name": "mag19", "desc": "? Light curve magnitude at JD19 "}, {"name": "e_mag19", "desc": "? rms uncertainty on mag19 "}, {"name": "JD20", "desc": "? Date of observation 20; JD-2451224.0 "}, {"name": "mag20", "desc": "? Light curve magnitude at JD20 "}, {"name": "e_mag20", "desc": "? rms uncertainty on mag20 "}, {"name": "JD21", "desc": "? Date of observation 21; JD-2451224.0 "}, {"name": "mag21", "desc": "? Light curve magnitude at JD21 "}, {"name": "e_mag21", "desc": "? rms uncertainty on mag21 "}, {"name": "JD22", "desc": "? Date of observation 22; JD-2451224.0 "}, {"name": "mag22", "desc": "? Light curve magnitude at JD22 "}, {"name": "e_mag22", "desc": "? rms uncertainty on mag22 "}, {"name": "JD23", "desc": "? Date of observation 23; JD-2451224.0 "}, {"name": "mag23", "desc": "? Light curve magnitude at JD23 "}, {"name": "e_mag23", "desc": "? rms uncertainty on mag23 "}, {"name": "JD24", "desc": "? Date of observation 24; JD-2451224.0 "}, {"name": "mag24", "desc": "? Light curve magnitude at JD24 "}, {"name": "e_mag24", "desc": "? rms uncertainty on mag24 "}, {"name": "JD25", "desc": "? Date of observation 25; JD-2451224.0 "}, {"name": "mag25", "desc": "? Light curve magnitude at JD25 "}, {"name": "e_mag25", "desc": "? rms uncertainty on mag25 "}, {"name": "JD26", "desc": "? Date of observation 26; JD-2451224.0 "}, {"name": "mag26", "desc": "? Light curve magnitude at JD26 "}, {"name": "e_mag26", "desc": "? rms uncertainty on mag26 "}, {"name": "JD27", "desc": "? Date of observation 27; JD-2451224.0 "}, {"name": "mag27", "desc": "? Light curve magnitude at JD27 "}, {"name": "e_mag27", "desc": "? rms uncertainty on mag27 "}, {"name": "JD28", "desc": "? Date of observation 28; JD-2451224.0 "}, {"name": "mag28", "desc": "? Light curve magnitude at JD28 "}, {"name": "e_mag28", "desc": "? rms uncertainty on mag28 "}, {"name": "JD29", "desc": "? Date of observation 29; JD-2451224.0 "}, {"name": "mag29", "desc": "? Light curve magnitude at JD29 "}, {"name": "e_mag29", "desc": "? rms uncertainty on mag29 "}, {"name": "JD30", "desc": "? Date of observation 30; JD-2451224.0 "}, {"name": "mag30", "desc": "? Light curve magnitude at JD30 "}, {"name": "e_mag30", "desc": "? rms uncertainty on mag30 "}, {"name": "JD31", "desc": "? Date of observation 31; JD-2451224.0 "}, {"name": "mag31", "desc": "? Light curve magnitude at JD31 "}, {"name": "e_mag31", "desc": "? rms uncertainty on mag31 "}, {"name": "JD32", "desc": "? Date of observation 32; JD-2451224.0 "}, {"name": "mag32", "desc": "? Light curve magnitude at JD32 "}, {"name": "e_mag32", "desc": "? rms uncertainty on mag32 "}, {"name": "JD33", "desc": "? Date of observation 33; JD-2451224.0 "}, {"name": "mag33", "desc": "? Light curve magnitude at JD33 "}, {"name": "e_mag33", "desc": "? rms uncertainty on mag33 "}, {"name": "JD34", "desc": "? Date of observation 34; JD-2451224.0 "}, {"name": "mag34", "desc": "? Light curve magnitude at JD34 "}, {"name": "e_mag34", "desc": "? rms uncertainty on mag34 "}, {"name": "JD35", "desc": "? Date of observation 35; JD-2451224.0 "}, {"name": "mag35", "desc": "? Light curve magnitude at JD35 "}, {"name": "e_mag35", "desc": "? rms uncertainty on mag35 "}, {"name": "JD36", "desc": "? Date of observation 36; JD-2451224.0 "}, {"name": "mag36", "desc": "? Light curve magnitude at JD36 "}, {"name": "e_mag36", "desc": "? rms uncertainty on mag36 "}, {"name": "JD37", "desc": "? Date of observation 37; JD-2451224.0 "}, {"name": "mag37", "desc": "? Light curve magnitude at JD37 "}, {"name": "e_mag37", "desc": "? rms uncertainty on mag37 "}, {"name": "JD38", "desc": "? Date of observation 38; JD-2451224.0 "}, {"name": "mag38", "desc": "? Light curve magnitude at JD38 "}, {"name": "e_mag38", "desc": "? rms uncertainty on mag38 "}, {"name": "JD39", "desc": "? Date of observation 39; JD-2451224.0 "}, {"name": "mag39", "desc": "? Light curve magnitude at JD39 "}, {"name": "e_mag39", "desc": "? rms uncertainty on mag39 "}, {"name": "JD40", "desc": "? Date of observation 40; JD-2451224.0 "}, {"name": "mag40", "desc": "? Light curve magnitude at JD40 "}, {"name": "e_mag40", "desc": "? rms uncertainty on mag40 "}, {"name": "JD41", "desc": "? Date of observation 41; JD-2451224.0 "}, {"name": "mag41", "desc": "? Light curve magnitude at JD41 "}, {"name": "e_mag41", "desc": "? rms uncertainty on mag41 "}, {"name": "JD42", "desc": "? Date of observation 42; JD-2451224.0 "}, {"name": "mag42", "desc": "? Light curve magnitude at JD42 "}, {"name": "e_mag42", "desc": "? rms uncertainty on mag42 "}, {"name": "JD43", "desc": "? Date of observation 43; JD-2451224.0 "}, {"name": "mag43", "desc": "? Light curve magnitude at JD43 "}, {"name": "e_mag43", "desc": "? rms uncertainty on mag43 "}]}, {"name": "r1maglc.dat", "desc": "r1 band light curves ", "columns": [{"name": "QVS2", "desc": "Unique Running Identifier "}, {"name": "JD01", "desc": "Date of observation 1; JD-2451224.0 "}, {"name": "mag1", "desc": "Light curve magnitude at JD1 "}, {"name": "e_mag1", "desc": "rms uncertainty on mag1 "}, {"name": "JD2", "desc": "Date of observation 2; JD-2451224.0 "}, {"name": "mag2", "desc": "Light curve magnitude at JD2 "}, {"name": "e_mag2", "desc": "rms uncertainty on mag2 "}, {"name": "JD3", "desc": "Date of observation 3; JD-2451224.0 "}, {"name": "mag3", "desc": "Light curve magnitude at JD3 "}, {"name": "e_mag3", "desc": "rms uncertainty on mag3 "}, {"name": "JD4", "desc": "? Date of observation 4; JD-2451224.0 "}, {"name": "mag4", "desc": "? Light curve magnitude at JD4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "JD5", "desc": "? Date of observation 5; JD-2451224.0 "}, {"name": "mag5", "desc": "? Light curve magnitude at JD5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "JD6", "desc": "? Date of observation 6; JD-2451224.0 "}, {"name": "mag6", "desc": "? Light curve magnitude at JD6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "JD7", "desc": "? Date of observation 7; JD-2451224.0 "}, {"name": "mag7", "desc": "? Light curve magnitude at JD7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "JD8", "desc": "? Date of observation 8; JD-2451224.0 "}, {"name": "mag8", "desc": "? Light curve magnitude at JD8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "JD9", "desc": "? Date of observation 9; JD-2451224.0 "}, {"name": "mag9", "desc": "? Light curve magnitude at JD9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "JD10", "desc": "? Date of observation 10; JD-2451224.0 "}, {"name": "mag10", "desc": "? Light curve magnitude at JD10 "}, {"name": "e_mag10", "desc": "? rms uncertainty on mag10 "}, {"name": "JD11", "desc": "? Date of observation 11; JD-2451224.0 "}, {"name": "mag11", "desc": "? Light curve magnitude at JD11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}, {"name": "JD12", "desc": "? Date of observation 12; JD-2451224.0 "}, {"name": "mag12", "desc": "? Light curve magnitude at JD12 "}, {"name": "e_mag12", "desc": "? rms uncertainty on mag12 "}, {"name": "JD13", "desc": "? Date of observation 13; JD-2451224.0 "}, {"name": "mag13", "desc": "? Light curve magnitude at JD13 "}, {"name": "e_mag13", "desc": "? rms uncertainty on mag13 "}, {"name": "JD14", "desc": "? Date of observation 14; JD-2451224.0 "}, {"name": "mag14", "desc": "? Light curve magnitude at JD14 "}, {"name": "e_mag14", "desc": "? rms uncertainty on mag14 "}, {"name": "JD15", "desc": "? Date of observation 15; JD-2451224.0 "}, {"name": "mag15", "desc": "? Light curve magnitude at JD15 "}, {"name": "e_mag15", "desc": "? rms uncertainty on mag15 "}, {"name": "JD16", "desc": "? Date of observation 16; JD-2451224.0 "}, {"name": "mag16", "desc": "? Light curve magnitude at JD16 "}, {"name": "e_mag16", "desc": "? rms uncertainty on mag16 "}, {"name": "JD17", "desc": "? Date of observation 17; JD-2451224.0 "}, {"name": "mag17", "desc": "? Light curve magnitude at JD17 "}, {"name": "e_mag17", "desc": "? rms uncertainty on mag17 "}, {"name": "JD18", "desc": "? Date of observation 18; JD-2451224.0 "}, {"name": "mag18", "desc": "? Light curve magnitude at JD18 "}, {"name": "e_mag18", "desc": "? rms uncertainty on mag18 "}, {"name": "JD19", "desc": "? Date of observation 19; JD-2451224.0 "}, {"name": "mag19", "desc": "? Light curve magnitude at JD19 "}, {"name": "e_mag19", "desc": "? rms uncertainty on mag19 "}, {"name": "JD20", "desc": "? Date of observation 20; JD-2451224.0 "}, {"name": "mag20", "desc": "? Light curve magnitude at JD20 "}, {"name": "e_mag20", "desc": "? rms uncertainty on mag20 "}, {"name": "JD21", "desc": "? Date of observation 21; JD-2451224.0 "}, {"name": "mag21", "desc": "? Light curve magnitude at JD21 "}, {"name": "e_mag21", "desc": "? rms uncertainty on mag21 "}, {"name": "JD22", "desc": "? Date of observation 22; JD-2451224.0 "}, {"name": "mag22", "desc": "? Light curve magnitude at JD22 "}, {"name": "e_mag22", "desc": "? rms uncertainty on mag22 "}, {"name": "JD23", "desc": "? Date of observation 23; JD-2451224.0 "}, {"name": "mag23", "desc": "? Light curve magnitude at JD23 "}, {"name": "e_mag23", "desc": "? rms uncertainty on mag23 "}, {"name": "JD24", "desc": "? Date of observation 24; JD-2451224.0 "}, {"name": "mag24", "desc": "? Light curve magnitude at JD24 "}, {"name": "e_mag24", "desc": "? rms uncertainty on mag24 "}, {"name": "JD25", "desc": "? Date of observation 25; JD-2451224.0 "}, {"name": "mag25", "desc": "? Light curve magnitude at JD25 "}, {"name": "e_mag25", "desc": "? rms uncertainty on mag25 "}, {"name": "JD26", "desc": "? Date of observation 26; JD-2451224.0 "}, {"name": "mag26", "desc": "? Light curve magnitude at JD26 "}, {"name": "e_mag26", "desc": "? rms uncertainty on mag26 "}, {"name": "JD27", "desc": "? Date of observation 27; JD-2451224.0 "}, {"name": "mag27", "desc": "? Light curve magnitude at JD27 "}, {"name": "e_mag27", "desc": "? rms uncertainty on mag27 "}, {"name": "JD28", "desc": "? Date of observation 28; JD-2451224.0 "}, {"name": "mag28", "desc": "? Light curve magnitude at JD28 "}, {"name": "e_mag28", "desc": "? rms uncertainty on mag28 "}, {"name": "JD29", "desc": "? Date of observation 29; JD-2451224.0 "}, {"name": "mag29", "desc": "? Light curve magnitude at JD29 "}, {"name": "e_mag29", "desc": "? rms uncertainty on mag29 "}, {"name": "JD30", "desc": "? Date of observation 30; JD-2451224.0 "}, {"name": "mag30", "desc": "? Light curve magnitude at JD30 "}, {"name": "e_mag30", "desc": "? rms uncertainty on mag30 "}, {"name": "JD31", "desc": "? Date of observation 31; JD-2451224.0 "}, {"name": "mag31", "desc": "? Light curve magnitude at JD31 "}, {"name": "e_mag31", "desc": "? rms uncertainty on mag31 "}, {"name": "JD32", "desc": "? Date of observation 32; JD-2451224.0 "}, {"name": "mag32", "desc": "? Light curve magnitude at JD32 "}, {"name": "e_mag32", "desc": "? rms uncertainty on mag32 "}, {"name": "JD33", "desc": "? Date of observation 33; JD-2451224.0 "}, {"name": "mag33", "desc": "? Light curve magnitude at JD33 "}, {"name": "e_mag33", "desc": "? rms uncertainty on mag33 "}, {"name": "JD34", "desc": "? Date of observation 34; JD-2451224.0 "}, {"name": "mag34", "desc": "? Light curve magnitude at JD34 "}, {"name": "e_mag34", "desc": "? rms uncertainty on mag34 "}, {"name": "JD35", "desc": "? Date of observation 35; JD-2451224.0 "}, {"name": "mag35", "desc": "? Light curve magnitude at JD35 "}, {"name": "e_mag35", "desc": "? rms uncertainty on mag35 "}, {"name": "JD36", "desc": "? Date of observation 36; JD-2451224.0 "}, {"name": "mag36", "desc": "? Light curve magnitude at JD36 "}, {"name": "e_mag36", "desc": "? rms uncertainty on mag36 "}, {"name": "JD37", "desc": "? Date of observation 37; JD-2451224.0 "}, {"name": "mag37", "desc": "? Light curve magnitude at JD37 "}, {"name": "e_mag37", "desc": "? rms uncertainty on mag37 "}, {"name": "JD38", "desc": "? Date of observation 38; JD-2451224.0 "}, {"name": "mag38", "desc": "? Light curve magnitude at JD38 "}, {"name": "e_mag38", "desc": "? rms uncertainty on mag38 "}, {"name": "JD39", "desc": "? Date of observation 39; JD-2451224.0 "}, {"name": "mag39", "desc": "? Light curve magnitude at JD39 "}, {"name": "e_mag39", "desc": "? rms uncertainty on mag39 "}, {"name": "JD40", "desc": "? Date of observation 40; JD-2451224.0 "}, {"name": "mag40", "desc": "? Light curve magnitude at JD40 "}, {"name": "e_mag40", "desc": "? rms uncertainty on mag40 "}, {"name": "JD41", "desc": "? Date of observation 41; JD-2451224.0 "}, {"name": "mag41", "desc": "? Light curve magnitude at JD41 "}, {"name": "e_mag41", "desc": "? rms uncertainty on mag41 "}, {"name": "JD42", "desc": "? Date of observation 42; JD-2451224.0 "}, {"name": "mag42", "desc": "? Light curve magnitude at JD42 "}, {"name": "e_mag42", "desc": "? rms uncertainty on mag42 "}, {"name": "JD43", "desc": "? Date of observation 43; JD-2451224.0 "}, {"name": "mag43", "desc": "? Light curve magnitude at JD43 "}, {"name": "e_mag43", "desc": "? rms uncertainty on mag43 "}]}, {"name": "r3maglc.dat", "desc": "r3 band light curves ", "columns": [{"name": "QVS2", "desc": "Unique Running Identifier "}, {"name": "JD01", "desc": "Date of observation 1; JD-2451224.0 "}, {"name": "mag1", "desc": "Light curve magnitude at JD1 "}, {"name": "e_mag1", "desc": "rms uncertainty on mag1 "}, {"name": "JD2", "desc": "Date of observation 2; JD-2451224.0 "}, {"name": "mag2", "desc": "Light curve magnitude at JD2 "}, {"name": "e_mag2", "desc": "rms uncertainty on mag2 "}, {"name": "JD3", "desc": "Date of observation 3; JD-2451224.0 "}, {"name": "mag3", "desc": "Light curve magnitude at JD3 "}, {"name": "e_mag3", "desc": "rms uncertainty on mag3 "}, {"name": "JD4", "desc": "? Date of observation 4; JD-2451224.0 "}, {"name": "mag4", "desc": "? Light curve magnitude at JD4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "JD5", "desc": "? Date of observation 5; JD-2451224.0 "}, {"name": "mag5", "desc": "? Light curve magnitude at JD5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "JD6", "desc": "? Date of observation 6; JD-2451224.0 "}, {"name": "mag6", "desc": "? Light curve magnitude at JD6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "JD7", "desc": "? Date of observation 7; JD-2451224.0 "}, {"name": "mag7", "desc": "? Light curve magnitude at JD7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "JD8", "desc": "? Date of observation 8; JD-2451224.0 "}, {"name": "mag8", "desc": "? Light curve magnitude at JD8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "JD9", "desc": "? Date of observation 9; JD-2451224.0 "}, {"name": "mag9", "desc": "? Light curve magnitude at JD9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "JD10", "desc": "? Date of observation 10; JD-2451224.0 "}, {"name": "mag10", "desc": "? Light curve magnitude at JD10 "}, {"name": "e_mag10", "desc": "? rms uncertainty on mag10 "}, {"name": "JD11", "desc": "? Date of observation 11; JD-2451224.0 "}, {"name": "mag11", "desc": "? Light curve magnitude at JD11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}, {"name": "JD12", "desc": "? Date of observation 12; JD-2451224.0 "}, {"name": "mag12", "desc": "? Light curve magnitude at JD12 "}, {"name": "e_mag12", "desc": "? rms uncertainty on mag12 "}, {"name": "JD13", "desc": "? Date of observation 13; JD-2451224.0 "}, {"name": "mag13", "desc": "? Light curve magnitude at JD13 "}, {"name": "e_mag13", "desc": "? rms uncertainty on mag13 "}, {"name": "JD14", "desc": "? Date of observation 14; JD-2451224.0 "}, {"name": "mag14", "desc": "? Light curve magnitude at JD14 "}, {"name": "e_mag14", "desc": "? rms uncertainty on mag14 "}, {"name": "JD15", "desc": "? Date of observation 15; JD-2451224.0 "}, {"name": "mag15", "desc": "? Light curve magnitude at JD15 "}, {"name": "e_mag15", "desc": "? rms uncertainty on mag15 "}, {"name": "JD16", "desc": "? Date of observation 16; JD-2451224.0 "}, {"name": "mag16", "desc": "? Light curve magnitude at JD16 "}, {"name": "e_mag16", "desc": "? rms uncertainty on mag16 "}, {"name": "JD17", "desc": "? Date of observation 17; JD-2451224.0 "}, {"name": "mag17", "desc": "? Light curve magnitude at JD17 "}, {"name": "e_mag17", "desc": "? rms uncertainty on mag17 "}, {"name": "JD18", "desc": "? Date of observation 18; JD-2451224.0 "}, {"name": "mag18", "desc": "? Light curve magnitude at JD18 "}, {"name": "e_mag18", "desc": "? rms uncertainty on mag18 "}, {"name": "JD19", "desc": "? Date of observation 19; JD-2451224.0 "}, {"name": "mag19", "desc": "? Light curve magnitude at JD19 "}, {"name": "e_mag19", "desc": "? rms uncertainty on mag19 "}, {"name": "JD20", "desc": "? Date of observation 20; JD-2451224.0 "}, {"name": "mag20", "desc": "? Light curve magnitude at JD20 "}, {"name": "e_mag20", "desc": "? rms uncertainty on mag20 "}, {"name": "JD21", "desc": "? Date of observation 21; JD-2451224.0 "}, {"name": "mag21", "desc": "? Light curve magnitude at JD21 "}, {"name": "e_mag21", "desc": "? rms uncertainty on mag21 "}, {"name": "JD22", "desc": "? Date of observation 22; JD-2451224.0 "}, {"name": "mag22", "desc": "? Light curve magnitude at JD22 "}, {"name": "e_mag22", "desc": "? rms uncertainty on mag22 "}, {"name": "JD23", "desc": "? Date of observation 23; JD-2451224.0 "}, {"name": "mag23", "desc": "? Light curve magnitude at JD23 "}, {"name": "e_mag23", "desc": "? rms uncertainty on mag23 "}, {"name": "JD24", "desc": "? Date of observation 24; JD-2451224.0 "}, {"name": "mag24", "desc": "? Light curve magnitude at JD24 "}, {"name": "e_mag24", "desc": "? rms uncertainty on mag24 "}, {"name": "JD25", "desc": "? Date of observation 25; JD-2451224.0 "}, {"name": "mag25", "desc": "? Light curve magnitude at JD25 "}, {"name": "e_mag25", "desc": "? rms uncertainty on mag25 "}, {"name": "JD26", "desc": "? Date of observation 26; JD-2451224.0 "}, {"name": "mag26", "desc": "? Light curve magnitude at JD26 "}, {"name": "e_mag26", "desc": "? rms uncertainty on mag26 "}, {"name": "JD27", "desc": "? Date of observation 27; JD-2451224.0 "}, {"name": "mag27", "desc": "? Light curve magnitude at JD27 "}, {"name": "e_mag27", "desc": "? rms uncertainty on mag27 "}, {"name": "JD28", "desc": "? Date of observation 28; JD-2451224.0 "}, {"name": "mag28", "desc": "? Light curve magnitude at JD28 "}, {"name": "e_mag28", "desc": "? rms uncertainty on mag28 "}, {"name": "JD29", "desc": "? Date of observation 29; JD-2451224.0 "}, {"name": "mag29", "desc": "? Light curve magnitude at JD29 "}, {"name": "e_mag29", "desc": "? rms uncertainty on mag29 "}, {"name": "JD30", "desc": "? Date of observation 30; JD-2451224.0 "}, {"name": "mag30", "desc": "? Light curve magnitude at JD30 "}, {"name": "e_mag30", "desc": "? rms uncertainty on mag30 "}, {"name": "JD31", "desc": "? Date of observation 31; JD-2451224.0 "}, {"name": "mag31", "desc": "? Light curve magnitude at JD31 "}, {"name": "e_mag31", "desc": "? rms uncertainty on mag31 "}, {"name": "JD32", "desc": "? Date of observation 32; JD-2451224.0 "}, {"name": "mag32", "desc": "? Light curve magnitude at JD32 "}, {"name": "e_mag32", "desc": "? rms uncertainty on mag32 "}, {"name": "JD33", "desc": "? Date of observation 33; JD-2451224.0 "}, {"name": "mag33", "desc": "? Light curve magnitude at JD33 "}, {"name": "e_mag33", "desc": "? rms uncertainty on mag33 "}, {"name": "JD34", "desc": "? Date of observation 34; JD-2451224.0 "}, {"name": "mag34", "desc": "? Light curve magnitude at JD34 "}, {"name": "e_mag34", "desc": "? rms uncertainty on mag34 "}, {"name": "JD35", "desc": "? Date of observation 35; JD-2451224.0 "}, {"name": "mag35", "desc": "? Light curve magnitude at JD35 "}, {"name": "e_mag35", "desc": "? rms uncertainty on mag35 "}, {"name": "JD36", "desc": "? Date of observation 36; JD-2451224.0 "}, {"name": "mag36", "desc": "? Light curve magnitude at JD36 "}, {"name": "e_mag36", "desc": "? rms uncertainty on mag36 "}, {"name": "JD37", "desc": "? Date of observation 37; JD-2451224.0 "}, {"name": "mag37", "desc": "? Light curve magnitude at JD37 "}, {"name": "e_mag37", "desc": "? rms uncertainty on mag37 "}, {"name": "JD38", "desc": "? Date of observation 38; JD-2451224.0 "}, {"name": "mag38", "desc": "? Light curve magnitude at JD38 "}, {"name": "e_mag38", "desc": "? rms uncertainty on mag38 "}, {"name": "JD39", "desc": "? Date of observation 39; JD-2451224.0 "}, {"name": "mag39", "desc": "? Light curve magnitude at JD39 "}, {"name": "e_mag39", "desc": "? rms uncertainty on mag39 "}, {"name": "JD40", "desc": "? Date of observation 40; JD-2451224.0 "}, {"name": "mag40", "desc": "? Light curve magnitude at JD40 "}, {"name": "e_mag40", "desc": "? rms uncertainty on mag40 "}, {"name": "JD41", "desc": "? Date of observation 41; JD-2451224.0 "}, {"name": "mag41", "desc": "? Light curve magnitude at JD41 "}, {"name": "e_mag41", "desc": "? rms uncertainty on mag41 "}, {"name": "JD42", "desc": "? Date of observation 42; JD-2451224.0 "}, {"name": "mag42", "desc": "? Light curve magnitude at JD42 "}, {"name": "e_mag42", "desc": "? rms uncertainty on mag42 "}, {"name": "JD43", "desc": "? Date of observation 43; JD-2451224.0 "}, {"name": "mag43", "desc": "? Light curve magnitude at JD43 "}, {"name": "e_mag43", "desc": "? rms uncertainty on mag43 "}]}, {"name": "vmaglc.dat", "desc": "v band light curves ", "columns": [{"name": "QVS2", "desc": "Unique Running Identifier "}, {"name": "JD01", "desc": "Date of observation 1; JD-2451224.0 "}, {"name": "mag1", "desc": "Light curve magnitude at JD1 "}, {"name": "e_mag1", "desc": "rms uncertainty on mag1 "}, {"name": "JD2", "desc": "Date of observation 2; JD-2451224.0 "}, {"name": "mag2", "desc": "Light curve magnitude at JD2 "}, {"name": "e_mag2", "desc": "rms uncertainty on mag2 "}, {"name": "JD3", "desc": "Date of observation 3; JD-2451224.0 "}, {"name": "mag3", "desc": "Light curve magnitude at JD3 "}, {"name": "e_mag3", "desc": "rms uncertainty on mag3 "}, {"name": "JD4", "desc": "? Date of observation 4; JD-2451224.0 "}, {"name": "mag4", "desc": "? Light curve magnitude at JD4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "JD5", "desc": "? Date of observation 5; JD-2451224.0 "}, {"name": "mag5", "desc": "? Light curve magnitude at JD5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "JD6", "desc": "? Date of observation 6; JD-2451224.0 "}, {"name": "mag6", "desc": "? Light curve magnitude at JD6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "JD7", "desc": "? Date of observation 7; JD-2451224.0 "}, {"name": "mag7", "desc": "? Light curve magnitude at JD7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "JD8", "desc": "? Date of observation 8; JD-2451224.0 "}, {"name": "mag8", "desc": "? Light curve magnitude at JD8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "JD9", "desc": "? Date of observation 9; JD-2451224.0 "}, {"name": "mag9", "desc": "? Light curve magnitude at JD9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "JD10", "desc": "? Date of observation 10; JD-2451224.0 "}, {"name": "mag10", "desc": "? Light curve magnitude at JD10 "}, {"name": "e_mag10", "desc": "? rms uncertainty on mag10 "}, {"name": "JD11", "desc": "? Date of observation 11; JD-2451224.0 "}, {"name": "mag11", "desc": "? Light curve magnitude at JD11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}, {"name": "JD12", "desc": "? Date of observation 12; JD-2451224.0 "}, {"name": "mag12", "desc": "? Light curve magnitude at JD12 "}, {"name": "e_mag12", "desc": "? rms uncertainty on mag12 "}, {"name": "JD13", "desc": "? Date of observation 13; JD-2451224.0 "}, {"name": "mag13", "desc": "? Light curve magnitude at JD13 "}, {"name": "e_mag13", "desc": "? rms uncertainty on mag13 "}, {"name": "JD14", "desc": "? Date of observation 14; JD-2451224.0 "}, {"name": "mag14", "desc": "? Light curve magnitude at JD14 "}, {"name": "e_mag14", "desc": "? rms uncertainty on mag14 "}, {"name": "JD15", "desc": "? Date of observation 15; JD-2451224.0 "}, {"name": "mag15", "desc": "? Light curve magnitude at JD15 "}, {"name": "e_mag15", "desc": "? rms uncertainty on mag15 "}, {"name": "JD16", "desc": "? Date of observation 16; JD-2451224.0 "}, {"name": "mag16", "desc": "? Light curve magnitude at JD16 "}, {"name": "e_mag16", "desc": "? rms uncertainty on mag16 "}, {"name": "JD17", "desc": "? Date of observation 17; JD-2451224.0 "}, {"name": "mag17", "desc": "? Light curve magnitude at JD17 "}, {"name": "e_mag17", "desc": "? rms uncertainty on mag17 "}, {"name": "JD18", "desc": "? Date of observation 18; JD-2451224.0 "}, {"name": "mag18", "desc": "? Light curve magnitude at JD18 "}, {"name": "e_mag18", "desc": "? rms uncertainty on mag18 "}, {"name": "JD19", "desc": "? Date of observation 19; JD-2451224.0 "}, {"name": "mag19", "desc": "? Light curve magnitude at JD19 "}, {"name": "e_mag19", "desc": "? rms uncertainty on mag19 "}, {"name": "JD20", "desc": "? Date of observation 20; JD-2451224.0 "}, {"name": "mag20", "desc": "? Light curve magnitude at JD20 "}, {"name": "e_mag20", "desc": "? rms uncertainty on mag20 "}, {"name": "JD21", "desc": "? Date of observation 21; JD-2451224.0 "}, {"name": "mag21", "desc": "? Light curve magnitude at JD21 "}, {"name": "e_mag21", "desc": "? rms uncertainty on mag21 "}, {"name": "JD22", "desc": "? Date of observation 22; JD-2451224.0 "}, {"name": "mag22", "desc": "? Light curve magnitude at JD22 "}, {"name": "e_mag22", "desc": "? rms uncertainty on mag22 "}, {"name": "JD23", "desc": "? Date of observation 23; JD-2451224.0 "}, {"name": "mag23", "desc": "? Light curve magnitude at JD23 "}, {"name": "e_mag23", "desc": "? rms uncertainty on mag23 "}, {"name": "JD24", "desc": "? Date of observation 24; JD-2451224.0 "}, {"name": "mag24", "desc": "? Light curve magnitude at JD24 "}, {"name": "e_mag24", "desc": "? rms uncertainty on mag24 "}, {"name": "JD25", "desc": "? Date of observation 25; JD-2451224.0 "}, {"name": "mag25", "desc": "? Light curve magnitude at JD25 "}, {"name": "e_mag25", "desc": "? rms uncertainty on mag25 "}, {"name": "JD26", "desc": "? Date of observation 26; JD-2451224.0 "}, {"name": "mag26", "desc": "? Light curve magnitude at JD26 "}, {"name": "e_mag26", "desc": "? rms uncertainty on mag26 "}, {"name": "JD27", "desc": "? Date of observation 27; JD-2451224.0 "}, {"name": "mag27", "desc": "? Light curve magnitude at JD27 "}, {"name": "e_mag27", "desc": "? rms uncertainty on mag27 "}, {"name": "JD28", "desc": "? Date of observation 28; JD-2451224.0 "}, {"name": "mag28", "desc": "? Light curve magnitude at JD28 "}, {"name": "e_mag28", "desc": "? rms uncertainty on mag28 "}, {"name": "JD29", "desc": "? Date of observation 29; JD-2451224.0 "}, {"name": "mag29", "desc": "? Light curve magnitude at JD29 "}, {"name": "e_mag29", "desc": "? rms uncertainty on mag29 "}, {"name": "JD30", "desc": "? Date of observation 30; JD-2451224.0 "}, {"name": "mag30", "desc": "? Light curve magnitude at JD30 "}, {"name": "e_mag30", "desc": "? rms uncertainty on mag30 "}, {"name": "JD31", "desc": "? Date of observation 31; JD-2451224.0 "}, {"name": "mag31", "desc": "? Light curve magnitude at JD31 "}, {"name": "e_mag31", "desc": "? rms uncertainty on mag31 "}, {"name": "JD32", "desc": "? Date of observation 32; JD-2451224.0 "}, {"name": "mag32", "desc": "? Light curve magnitude at JD32 "}, {"name": "e_mag32", "desc": "? rms uncertainty on mag32 "}, {"name": "JD33", "desc": "? Date of observation 33; JD-2451224.0 "}, {"name": "mag33", "desc": "? Light curve magnitude at JD33 "}, {"name": "e_mag33", "desc": "? rms uncertainty on mag33 "}, {"name": "JD34", "desc": "? Date of observation 34; JD-2451224.0 "}, {"name": "mag34", "desc": "? Light curve magnitude at JD34 "}, {"name": "e_mag34", "desc": "? rms uncertainty on mag34 "}, {"name": "JD35", "desc": "? Date of observation 35; JD-2451224.0 "}, {"name": "mag35", "desc": "? Light curve magnitude at JD35 "}, {"name": "e_mag35", "desc": "? rms uncertainty on mag35 "}, {"name": "JD36", "desc": "? Date of observation 36; JD-2451224.0 "}, {"name": "mag36", "desc": "? Light curve magnitude at JD36 "}, {"name": "e_mag36", "desc": "? rms uncertainty on mag36 "}, {"name": "JD37", "desc": "? Date of observation 37; JD-2451224.0 "}, {"name": "mag37", "desc": "? Light curve magnitude at JD37 "}, {"name": "e_mag37", "desc": "? rms uncertainty on mag37 "}, {"name": "JD38", "desc": "? Date of observation 38; JD-2451224.0 "}, {"name": "mag38", "desc": "? Light curve magnitude at JD38 "}, {"name": "e_mag38", "desc": "? rms uncertainty on mag38 "}, {"name": "JD39", "desc": "? Date of observation 39; JD-2451224.0 "}, {"name": "mag39", "desc": "? Light curve magnitude at JD39 "}, {"name": "e_mag39", "desc": "? rms uncertainty on mag39 "}, {"name": "JD40", "desc": "? Date of observation 40; JD-2451224.0 "}, {"name": "mag40", "desc": "? Light curve magnitude at JD40 "}, {"name": "e_mag40", "desc": "? rms uncertainty on mag40 "}, {"name": "JD41", "desc": "? Date of observation 41; JD-2451224.0 "}, {"name": "mag41", "desc": "? Light curve magnitude at JD41 "}, {"name": "e_mag41", "desc": "? rms uncertainty on mag41 "}, {"name": "JD42", "desc": "? Date of observation 42; JD-2451224.0 "}, {"name": "mag42", "desc": "? Light curve magnitude at JD42 "}, {"name": "e_mag42", "desc": "? rms uncertainty on mag42 "}, {"name": "JD43", "desc": "? Date of observation 43; JD-2451224.0 "}, {"name": "mag43", "desc": "? Light curve magnitude at JD43 "}, {"name": "e_mag43", "desc": "? rms uncertainty on mag43 "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_2_315"}} {"id": "J/ApJS/2/315", "title_cds": "H{alpha} emission stars and nebulae", "title_create": "Henize, 1956", "year": "1956", "author": "Henize K.G.", "title_pub": "Catalogues of H-alpha emission stars and nebulae in the Magellanic Clouds.", "first_author": "Henize K.G.", "ref_biblio": [""], "bibcode": ["1956ApJS....2..315H\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "description": ["H{alpha} emission stars and emission nebulae were discovered on", "objective-prism photographs of the Magellanic Clouds made at the", "Lamount-Hussay Observatory of the University of Michigan.", "The original catalog was divided in 5 tables containing the emission", "stars of the Large Cloud (LHA 120-S), the emission nebulae in the", "Large Cloud (LHA 120-N), the exciting stars in the Large Cloud, the", "emission stars of the Small Cloud (LHA 115-S), and the emission", "nebulae in the Small Cloud (LHA 115-N).", "The accurate positions of these stars were found by Brian Skiff."], "object": [], "curator": "Brian Skiff [Lowell Obs.], Francois Ochsenbein [CDS]", "alias": ["LHA"], "type": ["OC"], "doi_pub": ["10.1086/190025"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_207_6"}} {"id": "J/ApJS/207/6", "title_cds": "YNOGK code for null geodesics in Kerr spacetime", "title_create": "Yang+, 2013", "year": "2013", "author": "Yang X., Wang J.", "title_pub": "YNOGK: a new public code for calculating null geodesics in the Kerr spacetime.", "first_author": "Yang X.", "ref_biblio": [""], "bibcode": ["2013ApJS..207....6Y"], "see_also": ["http://www1.ynao.ac.cn/~yangxl/yxl.html : autho's repository", "J/A+A/561/A127 : YNOGKM code for calculating time-like geodesics (Yang+, 2014)"], "keyword_cds": "Models ; Accretion", "keyword_pub": "accretion, accretion disks; black hole physics; radiative transfer relativistic processes", "abstract": ["Following the work of Dexter & Agol, we present a new public code for", "the fast calculation of null geodesics in the Kerr spacetime. Using", "Weierstrass's and Jacobi's elliptic functions, we express all", "coordinates and affine parameters as analytical and numerical", "functions of a parameter p, which is an integral value along the", "geodesic. This is the main difference between our code and previous", "similar ones. The advantage of this treatment is that the information", "about the turning points does not need to be specified in advance by", "the user, and many applications such as imaging, the calculation of", "line profiles, and the observer-emitter problem, become root-finding", "problems. All elliptic integrations are computed by Carlson's elliptic", "integral method as in Dexter & Agol, which guarantees the fast", "computational speed of our code. The formulae to compute the constants", "of motion given by Cunningham & Bardeen have been extended, which", "allow one to readily handle situations in which the emitter or the", "observer has an arbitrary distance from, and motion state with respect", "to, the central compact object. The validation of the code has been", "extensively tested through applications to toy problems from the", "literature. The source FORTRAN code is freely available for download", "on our Web site http://www1.ynao.ac.cn/~yangxl/yxl.html."], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1088/0067-0049/207/1/6"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_213_12"}} {"id": "J/ApJS/213/12", "title_cds": "SDSS Stripe 82 co-added runs", "title_create": "Jiang+, 2014", "year": "2014", "author": "Jiang L., Fan X., Bian F., McGreer I.D., Strauss M.A., Annis J., Buck Z., Green R., Hodge J.A., Myers A.D., Rafiee A., Richards G.", "title_pub": "The Sloan Digital Sky Survey Stripe 82 imaging data: depth-optimized co-adds over 300 deg^2^ in five filters.", "first_author": "Jiang L.", "ref_biblio": [""], "bibcode": ["2014ApJS..213...12J"], "see_also": ["V/139 : The SDSS Photometric Catalog, Release 9 (Adelman-McCarthy+, 2012)", "V/141 : Light-Motion Curve Catalogue (LMCC) in Stripe 82 (Bramich+ 2008)", "J/MNRAS/436/3581 : X-ray observations of Stripe 82 (LaMassa+, 2013)", "http://www.sdss.org/ : The SDSS home page", "http://classic.sdss.org/legacy/stripe82.html : Stripe 82 home page"], "keyword_cds": "Atlases ; Surveys ; Observatory log", "keyword_pub": "atlases; catalogs; surveys", "abstract": ["We present and release co-added images of the Sloan Digital Sky Survey", "(SDSS) Stripe 82. Stripe 82 covers an area of ~300deg^2^ on the", "celestial equator, and has been repeatedly scanned 70-90 times in the", "ugriz bands by the SDSS imaging survey. By making use of all available", "data in the SDSS archive, our co-added images are optimized for depth.", "Input single-epoch frames were properly processed and weighted based", "on seeing, sky transparency, and background noise before co-addition.", "The resultant products are co-added science images and their", "associated weight images that record relative weights at individual", "pixels. The depths of the co-adds, measured as the 5{sigma} detection", "limits of the aperture (3.2\" diameter) magnitudes for point sources,", "are roughly 23.9, 25.1, 24.6, 24.1, and 22.8 AB magnitudes in the five", "bands, respectively. They are 1.9-2.2mag deeper than the best SDSS", "single-epoch data. The co-added images have good image quality, with", "an average point-spread function FWHM of ~1\" in the r, i, and z bands.", "We also release object catalogs that were made with SExtractor. These", "co-added products have many potential uses for studies of galaxies,", "quasars, and Galactic structure. We further present and release", "near-IR J-band images that cover ~90deg^2^ of Stripe 82. These images", "were obtained using the NEWFIRM camera on the NOAO 4m Mayall", "telescope, and have a depth of about 20.0-20.5 Vega magnitudes (also", "5{sigma} detection limits for point sources)."], "description": ["Stripe 82 covers 300deg^2^, and was repeatedly scanned 70-90 times", "over roughly 10 years. These Stripe 82 images, when co-added, reach a", "much greater depth than do SDSS single-run data.", "All our data products, including 24060 co-added science images and", "their associated weight images and object catalogs, are released on", "this Web site: http://das.sdss.org/ge/sample/stripe82/."], "type": ["OC"], "doi_pub": ["10.1088/0067-0049/213/1/12"], "orcid_pub": ["0000-0003-4176-6486"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table3.dat", "desc": "SDSS runs used for our co-adds ", "columns": [{"name": "Run", "desc": "[125/7202] SDSS run number "}, {"name": "MJD", "desc": "[51081/54433] Modified Julian Date of observation "}, {"name": "Fst", "desc": "[11/702] Starting field number "}, {"name": "Fend", "desc": "[50/1000] Ending field number "}, {"name": "RAst", "desc": "[-70/54] Starting Right Ascension in decimal degrees"}, {"name": "RAend", "desc": "[-55/87] Ending Right Ascension in decimal degrees "}, {"name": "ID", "desc": "Stripe 82 identifier (N=North or S=South) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_219_26"}} {"id": "J/ApJS/219/26", "title_cds": "OGLE atlas of classical novae. I. Galactic bulge", "title_create": "Mroz+, 2015", "year": "2015", "author": "Mroz P., Udalski A., Poleski R., Soszynski I., Szymanski M.K., Pietrzynski G., Wyrzykowski L., Ulaczyk K., Kozlowski S., Pietrukowicz P., Skowron J.", "title_pub": "OGLE atlas of classical novae. I. Galactic bulge objects.", "first_author": "Mroz P.", "ref_biblio": [""], "bibcode": ["2015ApJS..219...26M"], "see_also": ["B/vsx : AAVSO International Variable Star Index VSX (Watson+, 2006-2014)", "B/gcvs : General Catalogue of Variable Stars (Samus+ 2007-2013)", "V/123 : Catalog of Cataclysmic Variables (Downes+ 2001-2006)", "II/213 : OGLE Galactic Bulge periodic variables (Udalski+ 1996)", "J/AcA/64/197 : OGLE-IV 2012-2014 transients (Wyrzykowski+, 2014)", "J/AcA/63/135 : New OGLEIII dwarf novae in Galactic disk (Mroz+, 2013)", "J/A+A/554/A123 : Near-IR catalog of novae in VVV survey area (Saito+, 2013)", "J/ApJ/721/L28 : Red clump stars in Bulge from OGLE-III (Nataf+, 2010)", "J/AJ/140/34 : Classification of nova light curves (Strope+, 2010)", "J/ApJS/187/275 : Photometric histories of recurrent novae (Schaefer, 2010)", "J/MNRAS/387/344 : BVRcIC photometry of V2615 Oph (Munari+, 2008)", "J/PAZh/34/270 : Photometric parameters of Galactic novae (Burlak+, 2008)", "J/AcA/52/217 : OGLE II. VI photometry of Galactic Bulge (Udalski+, 2002)", "J/AJ/99/1079 : Nova rate in NGC 5128 (Ciardullo+, 1990)", "http://ogle.astrouw.edu.pl/ : OGLE home page", "http://ogle.astrouw.edu.pl/ogle4/transients/ : OGLE-IV transients", "http://www.cbat.eps.harvard.edu/nova_list.html : IAU CBAT list of MW novae", "http://asd.gsfc.nasa.gov/Koji.Mukai/novae/novae.html : Koji's list of recent"], "keyword_cds": "Novae ; Stars, variable ; Photometry, VRI", "keyword_pub": "novae, cataclysmic variables; stars: statistics", "abstract": ["Eruptions of classical novae are possible sources of lithium formation", "and gamma-ray emission. Nova remnants can also become Type Ia", "supernovae (SNe Ia). The contribution of novae to these phenomena", "depends on nova rates, which are not well established for the Galaxy.", "Here, we directly measure a Galactic bulge nova rate of", "13.8+/-2.6yr^-1^. This measurement is much more accurate than any", "previous measurement of this kind thanks to many years' monitoring of", "the bulge by the Optical Gravitational Lensing Experiment (OGLE)", "survey. Our sample consists of 39 novae eruptions, ~1/3 of which are", "OGLE-based discoveries. This long-term monitoring allows us to not", "only measure the nova rate but also to study in detail the light", "curves of 39 eruptions and more than 80 post-nova candidates. We", "measured orbital periods for 9 post-novae and 9 novae, and in 14 cases", "we procured the first estimates. The OGLE survey is very sensitive to", "the frequently erupting recurrent novae. We did not find any object", "similar to M31 2008-12a, which erupts once a year. The lack of", "detection indicates that there is only a small number of them in the", "Galactic bulge."], "description": ["All of the data presented in this paper were collected in the course", "of OGLE. The OGLE sky survey began operation in 1992. In the first", "phase, OGLE-I, conducted from 1992 to 1995 with the 1.0 m Swope", "telescope at Las Campanas Observatory (LCO), Chile, 16 Galactic bulge", "fields with a total field of view of about 1 sq. degree were observed.", "In its second phase, OGLE-II, from 1997 to 2000, approximately 30", "million stars from 11 sq. degrees of the Galactic bulge were monitored", "with the dedicated 1.3m Warsaw Telescope (located at LCO). In the", "OGLE-III phase (2001 to 2009), 92 sq. degrees around the Galactic", "center were regularly observed. Currently, the project is in its", "fourth phase, OGLE-IV (since 2010). The OGLE-IV observations analyzed", "here cover 140 sq. degrees of the Galactic bulge. The majority of", "measurements were taken through the I-band filter, closely resembling", "that of the standard Johnson-Cousins system."], "type": ["OC"], "doi_pub": ["10.1088/0067-0049/219/2/26"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "List of nova eruptions recorded by the OGLE survey ", "columns": [{"name": "Name", "desc": "Designation "}, {"name": "f_Name", "desc": "Flag on Name (1) "}, {"name": "OName", "desc": "Other nova name "}, {"name": "RAh", "desc": "[17/18] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Arcminute of right ascension (J2000) "}, {"name": "RAs", "desc": "Arcsecond of right ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[20/36] Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "Field", "desc": "OGLE field "}, {"name": "OGLE", "desc": "OGLE database number "}, {"name": "Date", "desc": "UT date of the eruption "}]}, {"name": "table2.dat", "desc": "Properties of novae recorded by the OGLE survey ", "columns": [{"name": "Name", "desc": "Designation "}, {"name": "Type", "desc": "Light curve type (1) "}, {"name": "Per", "desc": "[0.1/1.6]? Orbital period "}, {"name": "e_Per", "desc": "[/0.0001]? Per uncertainty "}, {"name": "l_ImagPre", "desc": "Limit flag on ImagPre "}, {"name": "ImagPre", "desc": "[13.7/21.5]? OGLE I-band brightness of pre-nova (G1)"}, {"name": "V-IPre", "desc": "[0.6/5]? (V-I) color index of pre-nova "}, {"name": "ImagPst", "desc": "[13.7/21.5]? OGLE I-band brightness of post-nova (G1)"}, {"name": "f_ImagPst", "desc": "[b] b = During decline "}, {"name": "V-IPst", "desc": "[-1.2/3.1]? (V-I) color index of post-nova "}]}, {"name": "table3.dat", "desc": "Likely post-novae: stars showing eclipse-like variability", "columns": [{"name": "Star", "desc": "GCVS identifier "}, {"name": "Name", "desc": "Nova name (Nova XXX YYYYZ) "}, {"name": "RAh", "desc": "[17/18] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Arcminute of right ascension (J2000) "}, {"name": "RAs", "desc": "Arcsecond of right ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[17/39] Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "sep", "desc": "[0.03/7] Distance from SIMBAD position "}, {"name": "Field", "desc": "OGLE field "}, {"name": "OGLE", "desc": "OGLE database number "}, {"name": "Imag", "desc": "[12.4/21.4] OGLE mean I-band brightness (G1) "}, {"name": "Vmag", "desc": "[14.2/22.1]? OGLE mean V-band brightness "}, {"name": "V-I", "desc": "[0.5/5.6]? OGLE mean (V-I) color index "}, {"name": "Type", "desc": "Type of the secondary (MS=main sequence; RG=red giant)"}, {"name": "Per", "desc": "[0.1/0.9]? Orbital period (only for table 3) "}, {"name": "e_Per", "desc": "? Per uncertainty "}]}, {"name": "table4.dat", "desc": "Possible post-novae: old novae counterparts ", "columns": [{"name": "Star", "desc": "GCVS identifier "}, {"name": "Name", "desc": "Nova name (Nova XXX YYYYZ) "}, {"name": "RAh", "desc": "[17/18] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Arcminute of right ascension (J2000) "}, {"name": "RAs", "desc": "Arcsecond of right ascension (J2000) "}, {"name": "DE-", "desc": "[-] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[17/39] Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "sep", "desc": "[0.03/7] Distance from SIMBAD position "}, {"name": "Field", "desc": "OGLE field "}, {"name": "OGLE", "desc": "OGLE database number "}, {"name": "Imag", "desc": "[12.4/21.4] OGLE mean I-band brightness (G1) "}, {"name": "Vmag", "desc": "[14.2/22.1]? OGLE mean V-band brightness "}, {"name": "V-I", "desc": "[0.5/5.6]? OGLE mean (V-I) color index "}, {"name": "Type", "desc": "Type of the secondary (MS=main sequence; RG=red giant)"}, {"name": "Per", "desc": "[0.1/0.9]? Orbital period (only for table 3) "}, {"name": "e_Per", "desc": "? Per uncertainty "}]}, {"name": "phot/*", "desc": "I-band photometry of individual objects ", "columns": [{"name": "HJD", "desc": "Heliocentric Julian Date; JD-2450000 "}, {"name": "Imag", "desc": "?=99.999 OGLE I-band magnitude "}, {"name": "e_Imag", "desc": "?=9.999 Imag uncertainty "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_220_5"}} {"id": "J/ApJS/220/5", "title_cds": "Chandra survey of 3CR extragalactic sources", "title_create": "Massaro+, 2015", "year": "2015", "author": "Massaro F., Harris D.E., Liuzzo E., Orienti M., Paladino R., Paggi A., Tremblay G.R., Wilkes B.J., Kuraszkiewicz J., Baum S.A., O'Dea C.P.", "title_pub": "The Chandra survey of extragalactic sources in the 3CR catalog: X-ray emission from nuclei, jets, and hotspots in the Chandra archival observations.", "first_author": "Massaro F.", "ref_biblio": [""], "bibcode": ["2015ApJS..220....5M"], "see_also": ["B/chandra : The Chandra Archive Log (CXC, 1999-2014)", "VIII/1 : The 3C and 3CR Catalogues (Edge+ 1959-1962)", "J/A+A/575/A80 : FIR photometry of 3CR galaxies (Podigachoski+, 2015)", "J/ApJS/206/12 : Blazars with {gamma}-ray counterparts. I. (D'Abrusco+, 2013)", "J/ApJS/197/24 : Chandra large-scale extragalactic jets. I. (Massaro+, 2011)", "J/ApJ/726/20 : X-ray emission from quasars (Miller+, 2011)", "J/ApJ/704/1586 : BCGs with radio AGN (Sun, 2009)", "J/MNRAS/392/1509 : Distribution of AGNs in galaxy clusters (Gilmour+, 2009)", "J/ApJS/164/307 : NICMOS observations of 3CR radio sources (Madrid+, 2006)", "J/ApJS/177/148 : HST survey of 3CR radio source counterparts II. (Floyd+, 2008)", "J/AJ/130/23 : Spectrophotometry of 3CR lobe-dominated quasars (Aars+, 2005)", "J/A+A/396/397 : Deep cluster survey in Chandra archival data (Boschin+, 2002)", "J/ApJS/122/81 : HST snapshot survey of 3CR radio sources (Martel+, 1999)", "J/PASP/97/932 : 3CR Source Identifications (Spinrad+, 1985)", "http://hea-www.cfa.harvard.edu/XJET/ : XJET home page", "http://www.jb.man.ac.uk/atlas/ : Online atlas of DRAGNs"], "keyword_cds": "Active gal. nuclei ; Radio sources ; X-ray sources ; Redshifts", "keyword_pub": "galaxies: active; radio continuum: galaxies; X-rays: general", "abstract": ["As part of our program to build a complete radio and X-ray database of", "all Third Cambridge catalog extragalactic radio sources, we present an", "analysis of 93 sources for which Chandra archival data are available.", "Most of these sources have already been published. Here we provide a", "uniform re-analysis and present nuclear X-ray fluxes and X-ray", "emission associated with radio jet knots and hotspots using both", "publicly available radio images and new radio images that have been", "constructed from data available in the Very Large Array archive. For", "about 1/3 of the sources in the selected sample, a comparison between", "the Chandra and radio observations was not reported in the literature:", "we find X-ray detections of 2 new radio jet knots and 17 hotspots. We", "also report the X-ray detection of extended emission from the", "intergalactic medium for 15 galaxy clusters."], "description": ["In the present paper, we uniformly analyzed 93 3CR sources observed by", "Chandra that were not reported in our previous investigations (see", "table 2)."], "type": ["OC"], "doi_pub": ["10.1088/0067-0049/220/1/5"], "orcid_pub": ["0000-0002-1704-9850"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "Source list of the archival Chandra 3CR radio sources", "columns": [{"name": "3CR", "desc": "3CR name (NNN.N) "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) (1) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) (1) "}, {"name": "DEd", "desc": "Degree of declination (J2000) (1) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "z", "desc": "[0.01/2] Redshift (G1) "}, {"name": "Scale", "desc": "[0.3/8.5] Angular to linear scale factor (G2) "}, {"name": "Dist", "desc": "[72/15097] Luminosity distance D_L_ (G2) "}, {"name": "ObsID", "desc": "[326/15656] Chandra observation ID "}, {"name": "PropID", "desc": "[1600145/14700660] Chandra proposal ID "}, {"name": "Date", "desc": "UT date of Chandra observation "}, {"name": "Mode", "desc": "Data mode (2) "}, {"name": "Time", "desc": "[2/72.1] Live time of Chandra observation "}, {"name": "Ref", "desc": "Reference(s) for the Chandra observation "}]}, {"name": "table4.dat", "desc": "X-Ray emission from radio cores ", "columns": [{"name": "3CR", "desc": "3CR name (NNN.N) "}, {"name": "f_3CR", "desc": "[b] Flag on 3CR (1) "}, {"name": "Ncts", "desc": "[6/20856] net counts "}, {"name": "e_Ncts", "desc": "[2/144] Ncts uncertainty (2) "}, {"name": "ExtR", "desc": "[0.05/1.1] Ext. ratio (3) "}, {"name": "e_ExtR", "desc": "[0.004/0.5]? ExtR uncertainty (2) "}, {"name": "F0.5-1keV", "desc": "[0/699] 0.5-1keV flux in 10^-15^erg/cm^2^/s "}, {"name": "e_F0.5-1keV", "desc": "[0/20] F0.5-1keV uncertainty (4) "}, {"name": "E_F0.5-1keV", "desc": "[0.03]? Second uncertainty on F0.5-1keV (4) "}, {"name": "F1-2keV", "desc": "[0.2/822] 1-2keV flux in 10^-15^erg/cm^2^/s "}, {"name": "e_F1-2keV", "desc": "[0.2/26] F1-2keV uncertainty (4) "}, {"name": "F2-7keV", "desc": "[0.7/2364] Measured X-ray flux between 2 and 7keV in 10^-15^erg/cm^2^/s"}, {"name": "e_F2-7keV", "desc": "[1/97] F2-7keV uncertainty (4) "}, {"name": "F0.5-7keV", "desc": "[4/3022] 0.5-7keV flux in 10^-15^erg/cm^2^/s"}, {"name": "e_F0.5-7keV", "desc": "[1/102] F0.5-7keV uncertainty (4) "}, {"name": "LX", "desc": "[/425] 0.5-7keV X-ray luminosity "}, {"name": "e_LX", "desc": "[/7] LX 1{sigma} uncertainty "}]}, {"name": "table8.dat", "desc": "The current status of the 3CR Chandra observations ", "columns": [{"name": "3CR", "desc": "3CR name (NNN.N) "}, {"name": "m_3CR", "desc": "3CR component letter "}, {"name": "Class", "desc": "Radio-to-optical classification (1) "}, {"name": "z", "desc": "? Redshift (G1) "}, {"name": "f_z", "desc": "[?] ?=Undetermined redshift (2) "}, {"name": "Dist", "desc": "[2.9/21341]? Luminosity distance D_L_ (G2) "}, {"name": "Flag", "desc": "[yes/no ] Cluster flag (3) "}, {"name": "XDet", "desc": "X-ray detection flag(s) (4) "}, {"name": "CFlag", "desc": "[yes/no ] Chandra flag (5) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_221_6"}} {"id": "J/ApJS/221/6", "title_cds": "H2O & CH3OH maser survey of class II methanol masers", "title_create": "Kang+, 2015", "year": "2015", "author": "Kang H., Kim K.-T., Byun D.-Y., Lee S., Park Y.-S.", "title_pub": "Simultaneous observation of water and class I methanol masers toward class II methanol maser sources.", "first_author": "Kang H.", "ref_biblio": [""], "bibcode": ["2015ApJS..221....6K"], "see_also": ["J/other/IJAA/4.571 : Methanol masers in HII regions (Farmer, 2014)", "J/MNRAS/439/2584 : Southern methanol masers at 36 and 44GHz (Voronkov+, 2014)", "J/ApJS/209/25 : H2O + CH_3_OH maser survey of Orion protostars (Kang+, 2013)", "J/ApJ/763/2 : 95GHz methanol masers in molecular outflows (Gan+, 2013)", "J/AZh/89/611 : Class I methanol maser catalog (Bayandina+, 2012)", "J/ApJ/753/50 : 6.7GHz methanol masers. I. NH_3_ lines (Pandian+, 2012)", "J/ApJS/200/5 : 95GHz class I methanol maser survey (Chen+, 2012)", "J/MNRAS/418/1689 : Red MSX water maser and ammonia emissions (Urquhart+, 2011)", "J/ApJS/196/9 : 95GHz methanol maser survey toward GLIMPSE EGOs (Chen+, 2011)", "J/ApJ/702/1615 : CH_3_OH maser survey of EGOs (Cyganowski+, 2009)", "J/ApJ/656/255 : Arecibo methanol maser Galactic Plane Survey (Pandian+, 2007)", "J/MNRAS/359/1498 : Class I and class II methanol masers (Ellingsen+, 2005)", "J/A+A/434/613 : Water maser survey of methanol maser sources (Szymczak+, 2005)", "J/A+A/417/615 : Maser and outflows in UC HII region (Codella+, 2004)", "J/A+A/403/1095 : 6.7GHz methanol masers survey of low-mass YSO (Minier+, 2003)", "J/A+AS/137/43 : OH/H2O masers database (Forster+, 1999)", "J/MNRAS/301/640 : Ultracompact H II regions studies. II. (Walsh+, 1998)"], "keyword_cds": "Masers ; Radio lines ; Millimetric/submm sources ; Surveys", "keyword_pub": "ISM: abundances; ISM: molecules; masers; stars: formation", "abstract": ["We present a simultaneous single-dish survey of 22GHz water masers and", "44 and 95GHz class I methanol masers toward 77 6.7GHz class II", "methanol maser sources, which were selected from the Arecibo methanol", "maser Galactic plane survey catalog. Water maser emission is detected", "in 39 (51%) sources, 15 of which are new detections. Methanol maser", "emission at 44 and 95GHz is found in 25 (32%) and 19 (25%) sources, 21", "and 13 of which, respectively, are newly detected. We find four", "high-velocity (>30km/s) water maser sources, including three dominant", "blue- or redshifted outflows. The 95GHz masers always appear with", "44GHz maser emission. They are strongly correlated with 44GHz masers", "in velocity, flux density, and luminosity, yet they are not correlated", "with either water or 6.7GHz class II methanol masers. The average peak", "flux density ratio of 95GHz masers to 44GHz masers is close to unity,", "which is two times higher than previous estimates. The flux densities", "of class I methanol masers are more closely correlated with the", "associated Bolocam Galactic Plane Survey core mass than those of water", "masers or class II methanol masers. Using the large velocity gradient", "model and assuming unsaturated class I methanol maser emission, we", "derive the fractional abundance of methanol to be in the range", "4.2x10^-8^-2.3x10^-6^, with a median value of 3.3+/-2.7x10^-7^."], "description": ["We selected 77 sources from the Arecibo methanol maser Galactic plane", "survey (AMGPS) catalog of 6.7GHz methanol maser sources (Pandian+,", "2007, J/ApJ/656/255).", "Using the Korean VLBI Network (KVN) 21m telescopes, we performed", "simultaneous surveys of the H_2_O 6_16_-5_23_ (22.23508GHz),", "CH_3_OH 7_0_-6_1_ A^+^ (44.06943GHz), and CH_3_OH 8_0_-7_1_ A^+^", "(95.169463GHz) masers toward the 77 class II methanol maser sources.", "The observations took a total of 18 days to complete and were", "undertaken between 2011 November and 2012 March: 15 days for the", "survey and 3 days for the grid mapping.", "We also observed four sources in the ^13^CO (J=1-0) (110.201353GHz)", "line and one of them in the HCO+ (J=1-0) (89.188523GHz) line using the", "Taeduk Radio Astronomy Observatory (TRAO) 14m telescope on 2014 March 17."], "type": ["OC"], "doi_pub": ["10.1088/0067-0049/221/1/6"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Source summary with detection results ", "columns": [{"name": "Name", "desc": "Source designation (GLL.ll+B.bb) (1) "}, {"name": "f_Name", "desc": "[d] Flag on Name (2) "}, {"name": "RAh", "desc": "[18/19] Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "[+] Sign of declination (J2000) "}, {"name": "DEd", "desc": "[1/18] Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "Fpos", "desc": "[c] Flag on J2000 coordinates (2) "}, {"name": "Vsys", "desc": "[-44.4/94.6] Systemic velocity from the NH3 observation (Pandian+ 2012, J/ApJ/753/50)"}, {"name": "f_Vsys", "desc": "[ef] Flag on Vsys (2) "}, {"name": "Date", "desc": "UT date "}, {"name": "22GHz", "desc": "New 22GHz water maser "}, {"name": "r_22GHz", "desc": "22GHz water maser reference(s) (3) "}, {"name": "44GHz", "desc": "44GHz class I maser reference(s) (3) "}, {"name": "95GHz", "desc": "New 95GHz ClassI maser "}, {"name": "r_95GHz", "desc": "[11/13]? 95GHz ClassI maser reference (3) "}, {"name": "Fig", "desc": "[2/6]? Figure number "}]}, {"name": "table3.dat", "desc": "Line parameters of detected masers ", "columns": [{"name": "Name", "desc": "Source designation (GLL.ll+B.bb) "}, {"name": "Freq", "desc": "[22/95] Frequency "}, {"name": "Sint", "desc": "[0.7/494] Integrated flux density (Gaussian fit)"}, {"name": "e_Sint", "desc": "[0.1/13.2] Sint uncertainty "}, {"name": "Vpk", "desc": "[-16.9/137] Peak velocity "}, {"name": "e_Vpk", "desc": "[0/0.7] Vpk uncertainty "}, {"name": "FWHM", "desc": "[0.2/6.8] Full-width at half-maximum "}, {"name": "e_FWHM", "desc": "[0/2.3] FWHM uncertainty "}, {"name": "Spk", "desc": "[0.8/716.9] Peak flux density (Gaussian fit) "}, {"name": "e_Spk", "desc": "[0.3/4.9] Spk uncertainty "}, {"name": "SintI", "desc": "[0.8/608] Integrated flux density (Integrated fit)"}, {"name": "Vmin", "desc": "[-18.2/135.3] Minimum velocity "}, {"name": "Vmax", "desc": "[-16.6/139.1] Maximum velocity "}, {"name": "SpkI", "desc": "[1.2/714.2] Peak flux density (Integrated fit) "}, {"name": "VpkI", "desc": "[-16.8/137.2] Peak velocity (Integrated fit) "}]}, {"name": "table4.dat", "desc": "Maser luminosities and associated BGPS sources ", "columns": [{"name": "Name", "desc": "Source designation (GLL.ll+B.bb) "}, {"name": "L6.7", "desc": "6.7GHz luminosity (1) "}, {"name": "L22", "desc": "[/0.003]? 22GHz luminosity "}, {"name": "L44", "desc": "[/0.0002]? 44GHz luminosity "}, {"name": "L95", "desc": "[/0.0004]? 95GHz luminosity "}, {"name": "Tkin", "desc": "[14/67.3]? Kinetic temperature (2) "}, {"name": "BGPS", "desc": "BGPS name (GLLL.lll+BB.bbb) "}, {"name": "Sint", "desc": "[0.1/9.6]? Integrated flux density "}, {"name": "NH2", "desc": "[0.5/12.1]? H_2_ column density (T=20K) "}, {"name": "Mgas", "desc": "[41/5800]? M_gas_ value (T_kin_) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_223_29"}} {"id": "J/ApJS/223/29", "title_cds": "The VLT LEGA-C spectroscopic survey", "title_create": "van der Wel+, 2016", "year": "2016", "author": "van der Wel A., Noeske K., Bezanson R., Pacifici C., Gallazzi A., Franx M., Munoz-mateos J.C., Bell E.F., Brammer G., Charlot S., Chauke P., Labbe I., Maseda M.V., Muzzin A., Rix H.-W., Sobral D., van de Sande J., van Dokkum P.G., Wild V., Wolf C.", "title_pub": "The VLT LEGA-C spectroscopic survey: the physics of galaxies at a lookback time of 7 Gyr.", "first_author": "van der Wel A.", "ref_biblio": [""], "bibcode": ["2016ApJS..223...29V"], "see_also": ["J/ApJS/94/687 : Old stellar populations. V. (Worthey+, 1994)", "J/ApJS/111/377 : H{gamma} & H{delta} absorption features (Worthey+ 1997)", "J/ApJ/706/1364 : SINS survey of high-redshift gal. (Forster Schreiber+, 2009)", "J/MNRAS/396/818 : Blue early-type galaxies in Galaxy Zoo (Schawinski+, 2009)", "J/ApJ/724/714 : Velocity dispersions of MS1054-03 & Coma gal. (Holden+, 2010)", "J/ApJ/741/115 : Deep spectroscopy in the GOODS fields (Miller+, 2011)", "J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012)", "J/ApJS/203/24 : Structural param. of galaxies in CANDELS (van der Wel+, 2012)", "J/AJ/145/77 : Imaging & spectrosc. in 3 galaxy clusters (Jorgensen+, 2013)", "J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013)", "J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)", "J/ApJ/788/72 : Observed sample of z~0.7 massive galaxies (Gallazzi+, 2014)", "J/ApJ/799/148 : DEIMOS galaxy sample at z~0.7 (Bezanson+, 2015)", "http://www.mpia.de/home/legac/index.html : LEGA-C survey home page", "http://www.eso.org/rm/api/v1/public/releaseDescriptions/83 : Description of"], "keyword_cds": "Galaxies, spectra ; Redshifts ; Surveys", "keyword_pub": "galaxies: evolution; galaxies: fundamental parameters; galaxies: general; galaxies: stellar content; surveys", "abstract": ["The Large Early Galaxy Census (LEGA-C) is an ESO Public Spectroscopic", "Survey of ~3200K-band selected galaxies at redshifts z=0.6-1.0 with", "stellar masses M*>10^10^M_{sun}_, conducted with VIMOS on ESO's Very", "Large Telescope. The survey is embedded in the COSMOS field", "(RA=10h00,DEC=+2{deg}). The 20hr long integrations produce", "high-signal-to-noise ratio continuum spectra that reveal ages,", "metallicities and velocity dispersions of the stellar populations.", "LEGA-C's unique combination of sample size and depth will enable us", "for the first time to map the stellar content at large lookback time,", "across galaxies of different types and star formation activity.", "Observations started in 2014 December and are planned to be completed", "by mid 2018, with early data releases of the spectra and value-added", "products. In this paper we present the science case, the observing", "strategy, an overview of the data reduction process and data products,", "and a first look at the relationship between galaxy structure and", "spectral properties, as it existed 7Gyr ago."], "description": ["This catalog is the first data release (DR1) from the LEGA-C (Large", "Early Galaxy Census) survey. The VIMOS high-resolution red grating is", "used in combination with the GG475 order separation filter, which", "results in a typical wavelength range of ~6300-8800{AA} at a", "resolution of R=2500 and a dispersion of 0.6{AA}/pix.", "In this release, we provide the data resulting from our first year of", "observations, totaling 892 galaxy spectra for 865 unique galaxies as", "well as a catalog that provides survey IDs, coordinates, and redshifts", "for this first subsample. The data presented here were taken during", "the ESO observing periods 94 and 95, during the runs 194.A-2005(A) to", "194.A-2005(F), with the respective date windows:", "22 Dec 2014 - 27 Dec 2014, 15 Jan 2015 - 25 Jan 2015, 14 Feb 2015 -", "24 Feb 2014, 15 Mar 2015 - 26 Mar 2015, 13 Apr 2015 -", "23 Apr 2015, 12 May 2015 - 22 May 2015.", "The parent sample is the photometric sample from Muzzin+ (2013,", "J/ApJS/206/8). Their UltraVISTA K-band selected catalog is 90%", "complete down to K=23.4 and contains 160070 sources across 1.62deg^2^", "in the COSMOS field (RA=10:00,DE=+2:12; J2000)."], "type": ["OC"], "doi_pub": ["10.3847/0067-0049/223/2/29"], "orcid_pub": ["0000-0002-5027-0135"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "legac_v1.dat", "desc": "Large Early Galaxy Census (LEGA-C) spectroscopic survey, DR1", "columns": [{"name": "[MMS2013]", "desc": "[73754/241460] ID from UltraVISTA (Muzzin+ 2013, J/ApJS/206/8)"}, {"name": "SpID", "desc": "Spectrum unique identifier (mask number+ objID) "}, {"name": "RAdeg", "desc": "[149.7/150.5] Right ascension (J2000) "}, {"name": "DEdeg", "desc": "[2/2.6] Declination (J2000) "}, {"name": "z", "desc": "[0.3/1.4]? Spectroscopic redshift "}, {"name": "FileName", "desc": "FITS file name of the original spectrum "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_228_13"}} {"id": "J/ApJS/228/13", "title_cds": "Short Title", "title_create": "Roming+, 2017", "year": "2017", "author": "Roming P.W.A., Koch T.S., Oates S.R., Porterfield B.L., Bayless A.J., Breeveld A.A., Gronwall C., Kuin N.P.M., Page M.J., De Pasquale M., Siegel M.H., Swenson C.A., Tobler J.M.", "title_pub": "A large catalog of homogeneous ultra-violet/optical GRB afterglows: temporal and spectral evolution.", "first_author": "Roming P.W.A.", "ref_biblio": [""], "bibcode": ["2017ApJS..228...13R"], "keyword_cds": "", "keyword_pub": "catalogs; gamma-ray burst: general", "abstract": ["We present the second Swift Ultra-Violet/Optical Telescope (UVOT)", "gamma-ray burst (GRB) afterglow catalog, greatly expanding on the", "first Swift UVOT GRB afterglow catalog. The second catalog is", "constructed from a database containing over 120,000 independent UVOT", "observations of 538 GRBs first detected by Swift, the High Energy", "Transient Explorer 2 (HETE2), the INTErnational Gamma-Ray Astrophysics", "Laboratory (INTEGRAL), the Interplanetary Network (IPN), Fermi, and", "Astro-rivelatore Gamma a Immagini Leggero (AGILE). The catalog covers", "GRBs discovered from 2005 January 17 to 2010 December 25. Using", "photometric information in three UV bands, three optical bands, and a", "\"white\" or open filter, the data are optimally coadded to maximize the", "number of detections and normalized to one band to provide a detailed", "light curve. The catalog provides positional, temporal, and", "photometric information for each burst, as well as Swift Burst Alert", "Telescope and X-ray Telescope (XRT) GRB parameters. Temporal slopes", "are provided for each UVOT filter. The temporal slope per filter of", "almost half the GRBs are fit with a single power law, but one to three", "breaks are required in the remaining bursts. Morphological comparisons", "with the X-ray reveal that \\sim 75 \\% of the UVOT light curves are", "similar to one of the four morphologies identified by Evans et al.", "(2009). The remaining \\sim 25 \\% have a newly identified morphology.", "For many bursts, redshift- and extinction-corrected UV/optical", "spectral slopes are also provided at 2 x 10^3^, 2 x 10^4^, and 2 x", "10^5^ s."], "doi_pub": ["10.3847/1538-4365/228/2/13"], "orcid_pub": ["0000-0002-5499-953X"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table5.dat", "desc": "Normalized Optimally Coadded (NOC) table ", "columns": [{"name": "Name", "desc": "GRB name (OBJECT) "}, {"name": "Filt", "desc": "UVOT filter used for exposure (uvw2, uvm2, uvwu, b, v, and white) (FILTER)"}, {"name": "Time", "desc": "[63/13649310] Weighted time of the detection as described in M08 (TIME)"}, {"name": "Tstart", "desc": "[58/] MET start time of the data used in the optimal coaddition (TSTART)"}, {"name": "Tstop", "desc": "[68/] MET stop time of the data used in the optimal coaddition (TSTOP)"}, {"name": "Exp", "desc": "[1.5/52183] Total exposure time for the optimally coadded data (EXPOSURE) (1)"}, {"name": "Cts", "desc": "[4/40343] Computed source counts in a coadded image as described in M08 (CSRC)"}, {"name": "e_Cts", "desc": "[2/294] Cts uncertainty (CERR) "}, {"name": "Rate", "desc": "[0/404] Computed coadded source rate calculated using (Cts*Scale)/Exp"}, {"name": "e_Rate", "desc": "[0/29] Source rate error calculated using (e_Cts*Scale)/Exp (RATE_ERR)"}, {"name": "mag", "desc": "[11.3/28.4] Magnitude of the source in the UVOT system computed from RATE (MAG)"}, {"name": "e_mag", "desc": "[0.006/0.6] mag uncertainty (MAG_ERR) "}, {"name": "Flux", "desc": "Flux density based on an average GRB spectrum, in erg/cm^2^/s/{AA} (FLUX)"}, {"name": "e_Flux", "desc": "1{sigma} error in Flux (FLUX_ERR) "}, {"name": "S/N", "desc": "[2/193] Signal-to-noise of the coadded weighted image as described in M08"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_228_14"}} {"id": "J/ApJS/228/14", "title_cds": "Short Title", "title_create": "Chilingarian+, 2017", "year": "2017", "author": "Chilingarian I.V., Zolotukhin I.Y., Katkov I.Y., Melchior A.-L., Rubtsov E.V., Grishin K.A.", "title_pub": "RCSED - A value-added Reference Catalog of Spectral Energy Distributions of 800299 galaxies in 11 ultraviolet, optical, and near-infrared bands: morphologies, colors, ionized gas, and stellar population properties.", "first_author": "Chilingarian I.V.", "keyword_cds": "", "keyword_pub": "catalogs; galaxies: fundamental parameters; galaxies: photometry galaxies: stellar content", "abstract": ["We present RCSED, the value-added Reference Catalog of Spectral Energy", "Distributions of galaxies, which contains homogenized", "spectrophotometric data for 800299 low- and intermediate-redshift", "galaxies (0.007"], "bibcode": ["2017ApJS..230...24B"], "keyword_cds": "", "keyword_pub": "catalogs; Galaxy: stellar content; stars: AGB and post-AGB; stars: early-type; surveys; ultraviolet: general", "abstract": ["The Galaxy Evolution Explorer (GALEX) imaged the sky in two", "ultraviolet (UV) bands, far-UV (FUV, {lambda}_eff_~1528{AA}), and", "near-UV (NUV, {lambda}_eff_~2310{AA}), delivering the first", "comprehensive sky surveys at these wavelengths. The GALEX database", "contains FUV and NUV images, ~500 million source measurements and over", "100000 low-resolution UV spectra. The UV surveys are a unique resource", "for statistical studies of hot stellar objects, z<~2 QSOs,", "star-forming galaxies, nebulae and the interstellar medium, and", "provide a roadmap for planning future UV instrumentation and follow-up", "observing programs. We present science-enhanced, \"clean\" catalogs of", "GALEX UV sources, with useful tags to facilitate scientific", "investigations. The catalogs are an improved and expanded version of", "our previous catalogs of UV sources (BCScat). With respect to BCScat,", "we have patched 640 fields for which the pipeline had improperly", "coadded non-overlapping observations, and we provide a version with a", "larger sky coverage (about 10%) by relaxing the restriction to the", "central area of the GALEX field to 1.1{deg} diameter", "(GUVcat_AIS_fov055), as well as the cleaner, more restrictive version", "using only the 1{deg} central portion of each field as in BCScat", "(GUVcat_AIS_fov050). We added new tags to facilitate selection and", "cleaning of statistical samples for science applications: we flag", "sources within the footprint of extended objects (nearby galaxies,", "stellar clusters) so that these regions can be excluded for estimating", "source density. As in our previous catalogs, in GUVcat duplicate", "measurements of the same source are removed, so that each", "astrophysical object has only one entry. Such a unique-source catalog", "is needed to study the density and distributions of sources, and to", "match UV sources with catalogs at other wavelengths. The catalog", "includes all observations from the All-Sky Imaging Survey (AIS), the", "survey with the largest area coverage, with both FUV and NUV detectors", "exposed: over 28700 fields, made up of a total of 57000 observations", "(\"visits\"). The total area covered, when overlaps are removed and gaps", "are accounted for, is 24790 square degrees for GUVcat_AIS_fov055", "(GUVcat_AIS_fov055) and 22125 square degrees for (GUVcat_AIS_fov050).", "The total numbers of \"unique\" AIS sources (eliminating duplicate", "measurements) are 82,992,086 (GUVcat\\_AIS\\_fov055) and 69,772,677", "(GUVcat\\_AIS\\_fov050). The typical depth of the GUVcat_AIS catalog is", "FUV=19.9, NUV=20.8 AB mag."], "doi_pub": ["10.3847/1538-4365/aa7053"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "List of clusters included in the GUVcat footprint ", "columns": [{"name": "ID", "desc": "Source identifier (1) "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "GLON", "desc": "Galactic longitude in decimal degrees (J2000) "}, {"name": "GLAT", "desc": "Galactic latitude in decimal degrees (J2000) "}, {"name": "R1", "desc": "Angular radius of central part of cluster "}, {"name": "o_R1", "desc": "Number of optical cluster stars (most probable) inside R1"}, {"name": "R0", "desc": "Angular radius of core of cluster "}, {"name": "o_R0", "desc": "Number of optical cluster stars (most probable) inside R0"}, {"name": "Class", "desc": "Cluster classification (2) "}, {"name": "Bd", "desc": "Broad type (3) "}, {"name": "St", "desc": "Cluster status (4) "}, {"name": "Type", "desc": "Cluster type (5) "}]}, {"name": "table3.dat", "desc": "List of galaxies larger than 1' included in the GUVcat footprint", "columns": [{"name": "ID", "desc": "Source identifier "}, {"name": "Type", "desc": "Source type (1) "}, {"name": "RAdeg", "desc": "Right Ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "v3k", "desc": "Radial velocity (cz) with respect to CMB radiation (2)"}, {"name": "vlg", "desc": "Radial velocity (cz) with respect to Local Group (2)"}, {"name": "PosAng", "desc": "Position angle (2) "}, {"name": "Inc", "desc": "Inclination "}, {"name": "D25", "desc": "D_25_ diameter in units of arcmin "}, {"name": "e_D25", "desc": "Uncertainty in D25 "}, {"name": "R25", "desc": "Axis ratio (major axis / minor axis) "}, {"name": "e_R25", "desc": "Uncertainty in R25 "}]}, {"name": "table4.dat", "desc": "List of AIS GALEX fields used to construct the GUVcat AIS catalog", "columns": [{"name": "ID", "desc": "Field identifier "}, {"name": "RAdeg", "desc": "Center Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Center Declination (J2000) "}, {"name": "GLON", "desc": "Center Galactic longitude "}, {"name": "GLAT", "desc": "Center Galactic latitude "}, {"name": "FUVexp", "desc": "FUV exposure time "}, {"name": "NUVexp", "desc": "NUV exposure time "}, {"name": "CorV", "desc": "Observation type (1) "}]}, {"name": "table5.dat", "desc": "List of AIS eliminated bad coadds, and their associated visits", "columns": [{"name": "C-ID", "desc": "Coadd identifier (1) "}, {"name": "RAdeg", "desc": "Coadd center Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "Coadd center Declination (J2000) "}, {"name": "C-GLON", "desc": "Coadd center Galactic longitude "}, {"name": "C-GLAT", "desc": "Coadd center Galactic latitude "}, {"name": "C-FUVexp", "desc": "Coadd FUV exposure time "}, {"name": "C-NUVexp", "desc": "Coadd NUV exposure time "}, {"name": "V-ID", "desc": "Visit identifier "}, {"name": "RAVdeg", "desc": "Visit center Right Ascension (J2000) "}, {"name": "DEVdeg", "desc": "Visit center Declination (J2000) "}, {"name": "V-FUVexp", "desc": "Visit FUV exposure time "}, {"name": "V-NUVexp", "desc": "Visit NUV exposure time "}, {"name": "Dist", "desc": "Angular distance between Coadd and Visit observations"}, {"name": "GUVcat", "desc": "In GUVcat; G=Yes,N=No "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_231_7"}} {"id": "J/ApJS/231/7", "title_cds": "The VISTA-CFHT Stripe 82 NIR survey (VICS82)", "title_create": "Geach+, 2017", "year": "2017", "author": "Geach J.E., Lin Y.-T., Makler M., Kneib J.-P., Ross N.P., Wang W.-H., Hsieh B.-C., Leauthaud A., Bundy K., McCracken H.J., Comparat J., Caminha G.B., Hudelot P., Lin L., Van Waerbeke L., Pereira M.E.S., Mast D.", "title_pub": "VICS82: the VISTA-CFHT Stripe 82 near-infrared survey.", "first_author": "Geach J.E.", "ref_biblio": [""], "bibcode": ["2017ApJS..231....7G"], "keyword_cds": "Surveys; Photometry, infrared", "keyword_pub": "catalogs; infrared: general; surveys", "abstract": ["We present the VISTA-CFHT Stripe 82 (VICS82) survey: a near-infrared", "(J+K_s_) survey covering 150 square degrees of the Sloan Digital Sky", "Survey (SDSS) equatorial Stripe 82 to an average depth of J=21.9 AB", "mag and K_s_=21.4 AB mag (80% completeness limits; 5{sigma}", "point-source depths are approximately 0.5mag brighter). VICS82", "contributes to the growing legacy of multiwavelength data in the", "Stripe 82 footprint. The addition of near-infrared photometry to the", "existing SDSS Stripe 82 coadd ugriz photometry reduces the scatter in", "stellar mass estimates to {delta}log(M_*_)~0.3dex for galaxies with", "M_*_>10^9^M_{sun}_ at z~0.5, and offers improvement compared to", "optical-only estimates out to z~1, with stellar masses constrained", "within a factor of approximately 2.5. When combined with other", "multiwavelength imaging of the Stripe, including moderate-to-deep", "ultraviolet (GALEX), optical and mid-infrared (Spitzer-IRAC) coverage,", "as well as tens of thousands of spectroscopic redshifts, VICS82 gives", "access to approximately 0.5Gpc^3^ of comoving volume. Some of the main", "science drivers of VICS82 include (a) measuring the stellar mass", "function of L^*^ galaxies out to z~1; (b) detecting", "intermediate-redshift quasars at 2<~z<~3.5; (c) measuring the stellar", "mass function and baryon census of clusters of galaxies, and (d)", "performing cross-correlation experiments of cosmic microwave", "background lensing in the optical/near-infrared that link stellar mass", "to large-scale dark matter structure. Here we define and describe the", "survey, highlight some early science results, and present the first", "public data release, which includes an SDSS-matched catalog as well as", "the calibrated pixel data themselves."], "description": ["The VISTA-CFHT Stripe 82 (VICS82) (VICS82) survey is conducted with", "the CFHT WIRCam instrument and with the Visible Infrared Survey", "Telescope for Astronomy (VISTA) VIRCAM instrument in J- and Ks", "broadband filters.", "The VICS82 coverage of Stripe 82 is a near-contiguous ~150deg^2^", "region defined by the boundaries 3hr and 22.2hr in RA and", "-1<{delta}<1deg in DEC."], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/aa74b6"], "data": "", "date_update": "12-Mar-2020", "tables": [{"name": "vics82.dat", "desc": "*Full VICS82 catalogue limited to Ks<22 AB mag ", "columns": [{"name": "---", "desc": "[VICS82/blah ] 313,883 sources are identified as \"blah\""}, {"name": "VICS82", "desc": "? VICS82 identifier (JHHMMSS.ss+DDMMSS.s)"}, {"name": "RAdeg", "desc": "[4.3e-7/360] Right ascension (J2000) (ALPHA_J2000)"}, {"name": "DEdeg", "desc": "[-1.3/1.3] Declination (J2000) (DELTA_J2000) "}, {"name": "Img", "desc": "Image file name (IMAGE) "}, {"name": "SNR", "desc": "[-164.5/1e+30] Signal to noise ratio (SNR_WIN)"}, {"name": "mag", "desc": "[5.7/36]?=- Total magnitude (MAG_AUTO) "}, {"name": "magAp1", "desc": "[13.2/37]?=- 1\" aperture magnitude (MAG_APER1)"}, {"name": "magAp1.5", "desc": "[12.3/38.5]?=- 1.5\" aperture magnitude (MAG_APER2)"}, {"name": "magAp2", "desc": "[11.7/41.6]?=- 2\" aperture magnitude (MAG_APER3)"}, {"name": "magAp2.5", "desc": "[11.3/40.8]?=- 2.5\" aperture magnitude (MAG_APER4)"}, {"name": "magAp3", "desc": "[11/39.3]?=- 3\" aperture magnitude (MAG_APER5)"}, {"name": "S/G", "desc": "[2e-5/1] S/G classifier output (1=star) (CLASS_STAR)"}, {"name": "Jmag", "desc": "[7/99]?=- J-band total magnitude (JMAG_AUTO) "}, {"name": "JmagAp1", "desc": "[13.5/99]?=- 1\" aperture J-band magnitude (JMAG_APER1)"}, {"name": "JmagAp1.5", "desc": "[12.6/99]?=- 1.5\" aperture J-band magnitude (JMAG_APER2)"}, {"name": "JmagAp2", "desc": "[12/99]?=- 2\" aperture J-band magnitude (JMAG_APER3)"}, {"name": "JmagAp2.5", "desc": "[11.6/99]?=- 2.5\" aperture J-band magnitude (JMAG_APER4)"}, {"name": "JmagAp3", "desc": "[11.2/99]?=- 3\" aperture J-band magnitude (JMAG_APER5)"}, {"name": "JSNR", "desc": "[-689.5/1e+30]?=- Signal to noise ratio in J (JSNR_WIN)"}, {"name": "objID", "desc": "[8647474690320302162/8647475122531011475]?=- VICS82 objID?? (objID)"}, {"name": "RASdeg", "desc": "? SDSS-DR9 right ascension (J2000) (ra) "}, {"name": "DESdeg", "desc": "? SDSS-DR9 declination (J2000) (dec) "}, {"name": "umag0", "desc": "[11.7/38.5]? Dereddened u-band magnitude (dered_u)"}, {"name": "gmag0", "desc": "[9.9/38.8]? Dereddened g-band magnitude (dered_g)"}, {"name": "rmag0", "desc": "[10.7/38]? Dereddened r-band magnitude (dered_r)"}, {"name": "imag0", "desc": "[10.4/42.7]?=- Dereddened i-band magnitude (dered_i)"}, {"name": "zmag0", "desc": "[11/36.7]?=- Dereddened z-band magnitude (dered_z)"}, {"name": "e_umag", "desc": "[0.002/166]? Model magnitude in u filter, AB scale, uncertainty (modelMagErr_u)"}, {"name": "e_gmag", "desc": "[0.001/192]? Model magnitude in g filter, AB scale, uncertainty (modelMagErr_g)"}, {"name": "e_rmag", "desc": "[0.001/254]? Model magnitude in r filter, AB scale, uncertainty (modelMagErr_r)"}, {"name": "e_imag", "desc": "[0.001/66]?=- Model magnitude in i filter, AB scale, uncertainty (modelMagErr_i)"}, {"name": "e_zmag", "desc": "[0.001/181]?=- Model magnitude in z filter, AB scale, uncertainty (modelMagErr_z)"}, {"name": "SDSS9", "desc": "SDSS DR9 IAU name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "DESdeg2", "desc": "? SDSS DR9 declination (J2000) (DEdeg) "}, {"name": "cl", "desc": "[0/6]?=- Class (1) "}, {"name": "q_mode", "desc": "[0/1] 1 (ou 0??) SDSS clean photometry flag "}, {"name": "flags", "desc": "Flags "}, {"name": "Q", "desc": "[3]?=- Quality of the observation: 3=good (Always \"3\" or blank)"}, {"name": "ObsDate", "desc": "[1998.72/2009.71]? Observing date in decimal years"}, {"name": "pmRA", "desc": "[-727/823]?=- SDSS proper motion in RA "}, {"name": "e_pmRA", "desc": "[2/183]?=- pmRA uncertainty "}, {"name": "pmDE", "desc": "[-1163/920]?=- SDSS proper motion in DEC "}, {"name": "e_pmDE", "desc": "[2/183]?=- pmDE uncertainty "}, {"name": "SpObjID", "desc": "[0/4920432000009434112]?=- SDSS-DR9 SpObjID "}, {"name": "zsp", "desc": "[-0.011/7.1]? SDSS spectroscopic redshift "}, {"name": "e_zsp", "desc": "[-6/10]? Redshift uncertainty "}, {"name": "f_zsp", "desc": "[0/134]?=- Flag on zsp (2) "}, {"name": "spType", "desc": "SDSS source type (3) "}, {"name": "spCl", "desc": "SDSS spectroscopic class (class): GALAXY (69,016 sources),"}, {"name": "sources)", "desc": "or "}, {"name": "sources)", "desc": " "}, {"name": "subClass", "desc": "SDSS spectroscopic subclass (subClass) (4) "}, {"name": "Sep", "desc": "[0.00014/2]? Separation between VICS82 and SDSS DR9 source (angDist)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_234_26"}} {"id": "J/ApJS/234/26", "title_cds": "Short Title", "title_create": "Li+, 2018", "year": "2018", "author": "Li L., Wang Y., Shao L., Wu X.-F., Huang Y.-F., Zhang B., Ryde F., Yu H.-F.", "title_pub": "A large catalog of multiwavelength GRB afterglows. I. Color evolution and its physical implication.", "first_author": "Li L.", "ref_biblio": [""], "bibcode": ["2018ApJS..234...26L"], "see_also": ["J/ApJ/672/449 : GRB 061126 light curves (Perley+, 2008)", "J/ApJ/691/723 : BVIJHKs observations of GRB 080319B (Bloom+, 2009)", "J/ApJ/693/1484 : Early optical afterglow catalog (Cenko+, 2009)", "J/AJ/137/4517 : UVOT light curves of supernovae (Brown+, 2009)", "J/ApJ/702/226 : Swift/UVOT panchromatic obs. of SN 2008D (Modjaz+, 2009)", "J/ApJ/702/489 : ROTSE obs. of gamma-ray burst afterglows (Rykoff+, 2009)", "J/A+A/508/593 : GRB 080710 bright optical/NIR afterglow (Kruehler+, 2009)", "J/MNRAS/406/2473 : Photometry of GRB 071025 (Perley+, 2010)", "J/ApJ/720/862 : Afterglow light curve of GRB 090926A (Rau+, 2010)", "J/ApJ/720/1513 : The afterglows of Swift-era GRBs. I. (Kann+, 2010)", "J/AJ/141/36 : GRB 080607 multi-band light curves (Perley+, 2011)", "J/AJ/141/163 : Ultimate LC of SN 1998bw/GRB 980425 (Clocchiatti+, 2011)", "J/A+A/531/A39 : g'r'i'z'JHKs light curves of GRB 081029 (Nardini+, 2011)", "J/A+A/535/A57 : g'r'i'z'JH light curves of GRB 091127 (Filgas+, 2011)", "J/ApJ/743/154 : Multi-band photom. of GRB 110205A + 110213A (Cucchiara+, 2011)", "J/MNRAS/421/2692 : Optical/near-IR obs. of GRB 080310 (Littlejohns+, 2012)", "J/MNRAS/426/2 : GRB 091018 Optical/NIR photometry (Wiersema+, 2012)", "J/A+A/557/A18 : GRB 120815A afterglow spectra (Kruehler+, 2013)", "J/A+A/560/A70 : GRB 100621A unusual afterglow (Greiner+, 2013)", "J/ApJ/781/37 : Multi-band photometry of GRB 130427A (Perley+, 2014)", "J/A+A/562/A29 : GRB 100814A GROND and UVOT light curves (Nardini+, 2014)", "J/A+A/568/A19 : Photometry of 3 {gamma}-ray burst supernovae (Cano+, 2014)", "J/A+A/568/A75 : GRB 130925A GROND light curves (Greiner+, 2014)", "J/A+A/607/A29 : GRB 120327A afterglow colour variations (Melandri+, 2017)", "http://gcn.gsfc.nasa.gov/ : GCN: The Gamma-ray Coordinates Network home page"], "keyword_cds": "GRB ; Colors ; Optical ; Infrared", "keyword_pub": "methods: statistical; stars: gamma-ray burst; ISM: dust, extinction", "abstract": ["The spectrum of gamma-ray burst (GRB) afterglows can be studied with", "color indices. Here, we present a large comprehensive catalog of 70", "GRBs with multiwavelength optical transient data on which we perform a", "systematic study to find the temporal evolution of color indices. We", "categorize them into two samples based on how well the color indices", "are evaluated. The Golden sample includes 25 bursts mostly observed by", "GROND, and the Silver sample includes 45 bursts observed by other", "telescopes. For the Golden sample, we find that 96% of the color", "indices do not vary over time. However, the color indices do vary", "during short periods in most bursts. The observed variations are", "consistent with effects of (i) the cooling frequency crossing the", "studied energy bands in a wind medium (43%) and in a constant-density", "medium (30%), (ii) early dust extinction (12%), (iii) transition from", "reverse-shock to forward-shock emission (5%), or (iv) an emergent SN", "emission (10%). We also study the evolutionary properties of the mean", "color indices for different emission episodes. We find that 86% of the", "color indices in the 70 bursts show constancy between consecutive", "ones. The color index variations occur mainly during the late GRB-SN", "bump, the flare, and early reverse-shock emission components. We", "further perform a statistical analysis of various observational", "properties and model parameters (spectral index {beta}_o_^CI^,", "electron spectral indices p^CI^, etc.) using color indices. Overall,", "we conclude that ~90% of colors are constant in time and can be", "accounted for by the simplest external forward-shock model, while the", "varying color indices call for more detailed modeling."], "description": ["We extensively compiled as many optical/near-IR (NIR) photometric data", "as possible, detected by ground-based telescopes from both pre-Swift-", "and Swift-era afterglows. We collected observational data from", "published papers and the Gamma-ray Burst Coordinates Networks Circular", "Service (GCN). A total of 70 bursts satisfy our selection criteria", "(from 1997 February 28 to 2015 December)."], "doi_pub": ["10.3847/1538-4365/aaa02a"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Properties of the GRB sample with multicolor light curves", "columns": [{"name": "GRB", "desc": "GRB name (YYMMDDA) "}, {"name": "Filt", "desc": "Filters "}, {"name": "E(B-V)", "desc": "[0.008/1] Galaxy color excess "}, {"name": "beta0", "desc": "[0.1/1.4]? Spectral index {beta}_0_ "}, {"name": "e_beta0", "desc": "[0/0.5]? beta0 uncertainty "}, {"name": "l_Av", "desc": "Limit flag on Av "}, {"name": "Av", "desc": "[0/5]? Host galaxy extinction "}, {"name": "e_Av", "desc": "[0.01/20.6]? Av uncertainty "}, {"name": "f_Av", "desc": "[a] a: Range 0.3-1.5 for 111209A "}, {"name": "r_Av", "desc": "Reference for Av (see refs.dat file) "}, {"name": "z", "desc": "[0.007/5.2]? Redshift "}, {"name": "r_z", "desc": "Reference for z (see refs.dat file) "}, {"name": "Ref", "desc": "References for data sources (see refs.dat file) "}]}, {"name": "table2.dat", "desc": "Color indices of the Golden sample ", "columns": [{"name": "GRB", "desc": "GRB name (YYMMDDA) "}, {"name": "m_GRB", "desc": "[0/4] Components within time sequence (1) "}, {"name": "Comp", "desc": "Component (2) "}, {"name": "Epoch", "desc": "The time intervals for each component in the observer frame"}, {"name": "Model", "desc": "Model of the light-curve fits for each component"}, {"name": "g-r", "desc": "[-0.2/1.4]? g-r color index "}, {"name": "e_g-r", "desc": "[0.01/0.5]? g-r uncertainty "}, {"name": "r-i", "desc": "[-1.1/0.5]? r-i color index "}, {"name": "e_r-i", "desc": "[0.01/2.3]? r-i uncertainty "}, {"name": "i-z", "desc": "[-0.8/0.6]? i-z color index "}, {"name": "e_i-z", "desc": "[0.01/1.9]? i-z uncertainty "}, {"name": "J-H", "desc": "[-0.4/0.7]? J-H color index "}, {"name": "e_J-H", "desc": "[0.02/2]? J-H uncertainty "}, {"name": "H-Ks", "desc": "[-0.04/0.9]? H-Ks color index "}, {"name": "e_H-Ks", "desc": "[0.02/0.8]? H-Ks uncertainty "}]}, {"name": "table3.dat", "desc": "Color indices of the Silver sample ", "columns": [{"name": "GRB", "desc": "GRB name (YYMMDDA) "}, {"name": "m_GRB", "desc": "[0/3] Components within time sequence (1) "}, {"name": "Comp", "desc": "Component (2) "}, {"name": "Epoch", "desc": "The time intervals for each component in the observer frame"}, {"name": "Model", "desc": "Model of the light-curve fits for each component"}, {"name": "W2-M2", "desc": "[-0.6/1.5]? UVW2-UVM2 color index "}, {"name": "e_W2-M2", "desc": "[0.1/1.2]? W2-M2 uncertainty "}, {"name": "M2-W1", "desc": "[-1.1/0.6]? UVM2-UVW1 color index "}, {"name": "e_M2-W1", "desc": "[0.1/3]? M2-W1 uncertainty "}, {"name": "W1-U", "desc": "[0.1/2]? UVW1-U color index "}, {"name": "e_W1-U", "desc": "[0.1/3]? W1-U uncertainty "}, {"name": "U-B", "desc": "[-1.6/2.4]? U-B color index "}, {"name": "e_U-B", "desc": "[0.07/1.1]? U-B uncertainty "}, {"name": "B-V", "desc": "[-0.8/1.5]? B-V color index "}, {"name": "e_B-V", "desc": "[0.06/0.6]? B-V uncertainty "}, {"name": "V-R", "desc": "[-0.7/1.4]? V-R color index "}, {"name": "e_V-R", "desc": "[0.08/0.5]? V-R uncertainty "}, {"name": "R-I", "desc": "[-0.6/1.4]? R-I color index "}, {"name": "e_R-I", "desc": "[0.08/0.8]? R-I uncertainty "}, {"name": "I-J", "desc": "[-0.9/3.1]? I-J color index "}, {"name": "e_I-J", "desc": "[0.05/0.5]? I-J uncertainty "}, {"name": "J-H", "desc": "[-0.4/0.7]? J-H color index "}, {"name": "e_J-H", "desc": "[0.09/0.3]? J-H uncertainty "}, {"name": "H-K", "desc": "[-0.4/1.6]? H-K color index "}, {"name": "e_H-K", "desc": "[0.09/0.4]? H-K uncertainty "}]}, {"name": "table7.dat", "desc": "Color indices and their relation spectral indices for the Golden samples", "columns": [{"name": "GRB", "desc": "Gamma-ray burst identifier (YYMMDDA) "}, {"name": "Time(g-r)", "desc": "[0.1/29200]? The (g-r) color time window (1) "}, {"name": "g-r", "desc": "[-0.3/1.7]? The (g-r) color index "}, {"name": "e_g-r", "desc": "[0.01/0.8]? Uncertainty in g-r "}, {"name": "beta(g-r)", "desc": "[-0.7/5.6]? Spectral index of (g-r) color "}, {"name": "e_beta(g-r)", "desc": "[0.02/2.6]? Uncertainty in beta(g-r) "}, {"name": "Time(r-i)", "desc": "[0.1/29200]? The (r-i) color time window (1) "}, {"name": "r-i", "desc": "[-1.1/1.3]? The (r-i) color index "}, {"name": "e_r-i", "desc": "[0.01/2.3]? Uncertainty in r-i "}, {"name": "beta(r-i)", "desc": "[-5/6.2]? Spectral index of (r-i) color "}, {"name": "e_beta(r-i)", "desc": "[0.03/11]? Uncertainty in beta(r-i) "}, {"name": "Time(i-z)", "desc": "[0.1/29200]? The (i-z) color time window (1) "}, {"name": "i-z", "desc": "[-0.8/1.3]? The (i-z) color index "}, {"name": "e_i-z", "desc": "[0.01/2]? Uncertainty in i-z "}, {"name": "beta(i-z)", "desc": "[-4.3/7]? Spectral index of (i-z) color "}, {"name": "e_beta(i-z)", "desc": "[0.03/9.6]? Uncertainty in beta(i-z) "}, {"name": "Time(J-H)", "desc": "[0.1/2400]? The (J-H) color time window (1) "}, {"name": "J-H", "desc": "[-0.7/1.4]? The (J-H) color index "}, {"name": "e_J-H", "desc": "[0.03/3]? Uncertainty in J-H "}, {"name": "beta(J-H)", "desc": "[-2.3/4.5]? Spectral index of (J-H) color "}, {"name": "e_beta(J-H)", "desc": "[0.1/9.8]? Uncertainty in beta(J-H) "}, {"name": "Time(H-Ks)", "desc": "[0.1/1880]? The (H-K_s_) color time window (1) "}, {"name": "H-Ks", "desc": "[-0.5/2]? The (H-K_s_) color index "}, {"name": "e_H-Ks", "desc": "[0.04/1.1]? Uncertainty in H-Ks "}, {"name": "beta(H-Ks)", "desc": "[-1.4/5.7]? Spectral index of (H-Ks) color "}, {"name": "e_beta(H-Ks)", "desc": "[0.1/3.2]? Uncertainty in beta(H-Ks) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_236_31"}} {"id": "J/ApJS/236/31", "title_cds": "H2O & class I CH3OH masers toward red MSX sources", "title_create": "Kim+, 2018", "year": "2018", "author": "Kim C.-H., Kim K.-T., Park Y.-S.", "title_pub": "Simultaneous survey of water and class I methanol masers toward red MSX sources.", "first_author": "Kim C.-H.", "ref_biblio": [""], "bibcode": ["2018ApJS..236...31K"], "see_also": ["V/114 : MSX6C Infrared Point Source Catalog (Egan+ 2003)", "J/other/PPMtO/14.185 : Purple Mountain H_2_O maser atlas (Han+ 1995)", "J/AZh/72/22 : A 95 GHz Survey of Methanol Masers (Valtts+, 1995)", "J/A+AS/127/181 : H2O maser sources new detections (Han+ 1998)", "J/A+A/368/845 : Arcetri updated cat. of H2O masers (Valdettaro+, 2001)", "J/ApJ/581/325 : NGC 2071 water masers (Seth+, 2002)", "J/A+A/417/615 : Maser and outflows in UC HII region (Codella+, 2004)", "J/ApJS/155/149 : CH_3_OH 7_0_-6_1_ A^+^ maser sources (Kurtz+, 2004)", "J/A+A/428/1019 : Rest frequencies of methanol maser lines (Mueller+, 2004)", "J/MNRAS/359/1498 : Class I and class II methanol masers (Ellingsen+, 2005)", "J/A+A/434/613 : Water maser survey of methanol masers (Szymczak+, 2005)", "J/ApJ/641/389 : Millimetric observations of IRDC cores (Rathborne+, 2006)", "J/ApJ/651/L125 : H2O masers associated with IR dark cloud cores (Wang+, 2006)", "J/PASJ/59/1185 : Water maser in galactic IRAS sources (Sunada+, 2007)", "J/AZh/84/579 : Catalog of Class I methanol masers (Val'tts+, 2007)", "J/A+A/487/993 : MAMBO Mapping of c2d Clouds and Cores (Kauffmann+, 2008)", "J/other/PASA/26.454 : Precise positions of methanol masers (Caswell, 2009)", "J/ApJ/702/1615 : CH_3_OH maser survey of EGOs (Cyganowski+, 2009)", "J/A+A/501/539 : RMS survey. 6cm observations of YSOs (Urquhart+, 2009)", "J/ApJ/706/83 : Embedded YSO candidates in W51 (Kang+, 2009)", "J/MNRAS/416/178 : 1.2-mm dust clumps with luminous water masers (Breen+, 2011)", "J/ApJS/196/9 : Methanol maser survey toward GLIMPSE EGOs (Chen+, 2011)", "J/MNRAS/418/1689 : Red MSX water maser and ammonia emissions (Urquhart+, 2011)", "J/AZh/89/611 : Class I methanol maser catalog (Bayandina+, 2012)", "J/ApJS/200/5 : 95GHz class I methanol maser survey (Chen+, 2012)", "J/ApJS/206/9 : New EGOs from Spitzer GLIMPSE II survey. I. (Chen+, 2013)", "J/A+A/552/A40 : MSX high-contrast IRDCs with NH_3_ (Chira+, 2013)", "J/A+A/549/A45 : ATLASGAL Compact Source Catalog: 33030km/s) features in 27 H_2_O maser sources. The 95GHz", "maser emission is detected only in 44GHz maser sources. The two", "transitions show strong correlations in the peak velocity, peak flux", "density, and isotropic maser luminosity, indicating that they are", "likely generated in the same sites by the same mechanisms. The 44GHz", "masers have much narrower distributions than 22GHz masers in the", "relative peak velocity and velocity range, while 6.7GHz class II", "CH_3_OH masers have distributions intermediate between the two. The", "maser luminosity significantly correlates with the parental clump", "mass, while it correlates well with the bolometric luminosity of the", "central protostar only when data of the low-mass regime from the", "literature are added. Comparison with the results of previous maser", "surveys toward massive star-forming regions suggests that the", "detection rates of 22 and 44GHz masers tend to increase as the central", "objects evolve. This is contrary to the trends found in low- and", "intermediate-mass star-forming regions. Thus, the occurrence of both", "masers might depend on the surrounding environments as well as on the", "evolution of the central object."], "description": ["We surveyed 299 Red MSX Source (RMS; see Lumsden+, 2002MNRAS.336..621L", "2013, J/ApJS/208/11 and Urquhart+, 2014, J/MNRAS/437/1791) high-mass", "protostellar object (HMPO) candidates in three maser transitions:", "H_2_O 616-523 (22.235080GHz), CH_3_OH 70-61 A+ (44.069430GHz), and", "80-71 A+ (95.169463GHz). The observations were undertaken using the", "Korean VLBI Network (KVN) 21m telescopes from 2011 April to 2014 May.", "The FWHMs of the telescopes were about 130\" at 22GHz, 65\" at 44GHz,", "and 32\" at 95GHz. The pointing accuracy was better than 5\".", "We also surveyed 10 sources in our sample in the ^13^CO J=1-0 and", "HCO^+^ J=1-0 lines in 2013 June. The 13CO line observations were", "conducted with the Taeduk Radio Astronomy Observatory (TRAO) 14m", "telescope, while the HCO^+^ line observations were made with the KVN", "telescope at the Tamna station."], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/aab88f"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Summary of target sources ", "columns": [{"name": "ID", "desc": "[4/4954] Red MSX source identifier "}, {"name": "f_ID", "desc": "Flag on ID (1) "}, {"name": "MSX", "desc": "MSX identifier (GLLL.llll+BB.bbbbA) "}, {"name": "RAh", "desc": "Hour of Right Ascension (J2000) "}, {"name": "RAm", "desc": "Minute of Right Ascension (J2000) "}, {"name": "RAs", "desc": "Second of Right Ascension (J2000) "}, {"name": "DE-", "desc": "Sign of the Declination (J2000) "}, {"name": "DEd", "desc": "Degree of Declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of Declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of Declination (J2000) "}, {"name": "Dist", "desc": "Distance "}, {"name": "Lbol", "desc": "[132/310000]? Bolometric luminosity "}, {"name": "Vsys", "desc": "[-88.6/113.6]? RMS archive systemic velocity "}, {"name": "Det22?", "desc": "Detection at 22 GHz? (2) "}, {"name": "f_Det22?", "desc": "Flag(s) on Det22? (3) "}, {"name": "Det44?", "desc": "Detection at 44 GHz? (2) "}, {"name": "f_Det44?", "desc": "Flag(s) on Det22? (3) "}, {"name": "Det95?", "desc": "Detection at 95 GHz? (2) "}, {"name": "f_Det95?", "desc": "Flag on Det22? (3) "}, {"name": "MMB", "desc": "MMB coverage? (y)es "}]}, {"name": "table4.dat", "desc": "Detected maser line parameters ", "columns": [{"name": "ID", "desc": "[4/4941] Red MSX source identifier "}, {"name": "Freq", "desc": "[6.7/95] Frequency of maser detection "}, {"name": "Date", "desc": "Date of the observation "}, {"name": "YS", "desc": "Station code (1) "}, {"name": "Vp", "desc": "[-96.4/125.8]? Velocity peak "}, {"name": "Sp", "desc": "[0.8/4552.1]? Peak flux density in Freq "}, {"name": "IntSnudv", "desc": "[0.2/14832.7] Integrated flux density "}, {"name": "Vmin", "desc": "[-109.5/122.4]? Minimum velocity of maser line "}, {"name": "Vmax", "desc": "[-91.8/150.8]? Maximum velocity of maser line "}, {"name": "Vrange", "desc": "[0.2/230.7]? Velocity range of maser line "}, {"name": "Lmaser", "desc": "[9.3e-09/0.01] Isotropic maser luminosity "}, {"name": "Notes", "desc": "Additional notes (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_239_14"}} {"id": "J/ApJS/239/14", "title_cds": "", "title_create": "Johns+, 2018", "year": "2018", "author": "Johns D., Marti C., Huff M., McCann J., Wittenmyer R.A., Horner J., Wright D.J.", "title_pub": "Revised exoplanet radii and habitability using Gaia Data Release 2.", "first_author": "Johns D.", "ref_biblio": [""], "bibcode": ["2018ApJS..239...14J"], "see_also": ["I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "J/A+A/375/L27 : HD 80606b, planet on an very elongated orbit (Naef+ 2001)", "J/A+A/491/889 : CoRoT-Exo-3b observations (Deleuil+, 2008)", "J/A+A/480/L33 : Radial velocities of HD 4113 and HD 156846 (Tamuz+, 2008)", "J/A+A/507/487 : GJ 581 radial velocity curve (Mayor+, 2009)", "J/A+A/523/A15 : HARPS XXIII: RV data for the 8 targets (Naef+, 2010)", "J/ApJ/761/123 : KELT-1 photometry and spectroscopy follow-up (Siverd+, 2012)", "J/ApJ/761/123 : KELT-1 photometry and spectroscopy follow-up (Siverd+, 2012)", "J/AJ/145/5 : Follow-up photometry of HATS-1 (Penev+, 2013)", "J/A+A/562/L3 : WASP-103b radial velocities and light curves (Gillon+, 2014)", "J/ApJS/210/20 : Small Kepler planets radial velocities (Marcy+, 2014)", "J/MNRAS/452/2127 : Fundamental param. of Kepler stars (Silva Aguirre+, 2015)", "J/AJ/152/105 : Kepler-80 transit timing observations (MacDonald+, 2016)", "J/AJ/153/211 : Differential photometry of F-subgiant HAT-P-67 (Zhou+, 2017)", "J/A+A/613/A25 : Radial velocity for Ross 128 (Bonfils+, 2018)"], "keyword_cds": "", "keyword_pub": "astrobiology ; planets and satellites: fundamental parameters ; planets and satellites: general ; catalogs ; surveys ; planets and satellites: fundamental parameters", "abstract": ["Accurate stellar properties are crucial for determining exoplanet", "characteristics. Gaia DR2 presents revised distances, luminosities,", "and radii for 1.6 billion stars. Here, we report the calculation of", "revised radii and densities for 320 non-Kepler exoplanets using this", "data and present updated calculations of the incident flux received by", "690 known exoplanets. This allows us to reassess the likelihood that", "those planets orbit in the habitable zone of their host stars. As a", "result of this analysis, three planets can be added to the catalog of", "potentially habitable worlds: HIP 67537b, HD 148156b, and HD 106720b.", "In addition, the changed parameterization of BD +49 898 means that its", "planet, BD +49 898b, now receives an incident flux that places it", "outside the optimistic habitable zone region, as defined by Kopparapu", "et al. We find that use of the new Gaia data results in a mean", "increase in the calculated exoplanet radius of 3.76%. Previously,", "CoRoT-3 b had been reported as having the highest density of all known", "exoplanets. Here, we use updated information to revise the calculated", "density of CoRoT-3 b from 26.4 to 16.1+/-3.98g/cm^3^. We also report", "the densest exoplanet in our data set, KELT-1 b, with a density of", "22.1_-9.16_^+5.62^g/cm^3^. Overall, our results highlight the", "importance of ensuring the parameterizations of known exoplanets are", "revisited whenever significant improvements are made to the precision", "of the stellar parameters upon which they are based."], "doi_pub": ["10.3847/1538-4365/aae5fb"], "orcid_pub": ["0000-0001-6311-8629"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "Host star properties; all parameters are taken from Gaia DR2", "columns": [{"name": "Host", "desc": "Host name "}, {"name": "Lum", "desc": "[0.04/1244.2]? Host luminosity, solar units "}, {"name": "E_Lum", "desc": "[0/97.2]? Upper uncertainty in Lum "}, {"name": "e_Lum", "desc": "[-97.2/0]? Lower uncertainty in Lum "}, {"name": "Rad", "desc": "[0.5/78.2]? Host radius, solar units "}, {"name": "E_Rad", "desc": "[0.003/8.5]? Upper uncertainty in Rad "}, {"name": "e_Rad", "desc": "[-13.2/-0.003]? Lower uncertainty in Rad "}, {"name": "Teff", "desc": "[3382/9435] Host effective temperature "}]}, {"name": "table3.dat", "desc": "Revised properties of exoplanets ", "columns": [{"name": "Planet", "desc": "Planet Name "}, {"name": "Rad", "desc": "[0.1/2.9]? Planet Radius "}, {"name": "E_Rad", "desc": "[0.01/1.8]? Upper uncertainty in Rad "}, {"name": "e_Rad", "desc": "[-1.8/-0.01]? Lower uncertainty in Rad "}, {"name": "Mass", "desc": "[0.01/55.6]? Planet Mass (1) "}, {"name": "E_Mass", "desc": "[0/78.6]? Upper uncertainty in Mass "}, {"name": "e_Mass", "desc": "[-78.6/0]? Lower uncertainty in Mass "}, {"name": "rho", "desc": "[0.04/26]? Planet Density "}, {"name": "E_rho", "desc": "[0.01/27.1]? Upper uncertainty in rho "}, {"name": "e_rho", "desc": "[-27/-0.01]? Lower uncertainty in rho "}, {"name": "a", "desc": "[0.01/773]? Semi-major axis (1) "}, {"name": "E_a", "desc": "[0/30]? Upper uncertainty in a "}, {"name": "e_a", "desc": "[-30/0]? Lower uncertainty in a "}, {"name": "Sinc", "desc": "[0/19317]? Planet Incident Flux "}, {"name": "E_Sinc", "desc": "[0/3395]? Upper uncertainty in Sinc "}, {"name": "e_Sinc", "desc": "[-3388/0]? Lower uncertainty in Sinc "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_239_29"}} {"id": "J/ApJS/239/29", "title_cds": "Short Title", "title_create": "Peralta+, 2018", "year": "2018", "author": "Peralta J., Muto K., Hueso R., Horinouchi T., Sanchez-lavega A., Murakami S.-Y., Machado P., Young E.F., Lee Y.J., Kouyama T., Sagawa H., Mcgouldrick K., Satoh T., Imamura T., Limaye S.S., Sato T.M., Ogohara K., Nakamura M., Luz D.", "title_pub": "Nightside winds at the lower clouds of Venus with Akatsuki/IR2: longitudinal, local time, and decadal variations from comparison with previous measurements.", "first_author": "Peralta J.", "ref_biblio": [""], "bibcode": ["2018ApJS..239...29P"], "keyword_cds": "", "keyword_pub": "planets and satellites: atmospheres planets and satellites: terrestrial planets", "mission": "", "abstract": ["We present measurements of the wind speeds at the nightside lower clouds of Venus from observations by JAXA's mission Akatsuki during 2016, complemented by new wind measurements from ground-based observations acquired with the TNG/Near Infrared Camera Spectrometer (NICS) in 2012 and IRTF/SpeX in 2015 and 2017. The zonal and meridional components of the winds were measured via cloud tracking on a total of 466 Akatsuki images of Venus acquired by the camera IR2 using the 2.26 {mu}m filter, with spatial resolutions ranging from 10 to 80 km per pixel and covering 2016 March 22 to October 31. More than 149,000 wind vectors were obtained using an automatic template-matching technique, and 2947 wind vectors were inferred using a manual procedure. The meridional profiles for both components of the winds are found to be consistent with results from the Venus Express mission during 2006-2008, although stronger wind variability is found for the zonal component at equatorial latitudes where Akatsuki observations have better viewing geometry than Venus Express. The zonal winds at low latitudes also suggest a zonal variability that could be associated with solar tides or vertically propagating orographic waves. Finally, the combination of our wind measurements from TNG/NICS, IRTF/SpeX, and Akatsuki images with previously published data from 1978 to 2017 suggests variations of up to 30 m s^-1^ in the winds at the nightside lower clouds of Venus."], "object": [], "curator": "Emmanuelle Perret [CDS]", "doi_pub": ["10.3847/1538-4365/aae844"], "orcid_pub": ["0000-0002-6823-1695"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_239_33"}} {"id": "J/ApJS/239/33", "title_cds": "Radio-loud AGNs sample from literature", "title_create": "Yuan+, 2018", "year": "2018", "author": "Yuan Z., Wang J., Worrall D.M., Zhang B.-B., Mao J.", "title_pub": "Determining the core radio luminosity function of radio AGNs via copula.", "first_author": "Yuan Z.", "ref_biblio": [""], "bibcode": ["2018ApJS..239...33Y"], "see_also": ["VIII/36 : The Second Bologna Survey (Colla+ 1970-1974)", "VIII/2 : Molonglo Reference Catalog of Radio Sources (Large+ 1981)", "VIII/37 : The Third Bologna Survey (B3) (Ficarra+ 1985)", "VIII/22 : 6C Survey of Radio Sources - III. (Hales+ 1990)", "VIII/16 : Molonglo Reference Catalogue of Radio Sources (Large+ 1991)", "VIII/17 : The North 20cm Survey (White+ 1992)", "VIII/42 : Texas Survey of radio sources at 365MHz (Douglas+ 1996)", "VIII/38 : The Parkes-MIT-NRAO 4.85GHz (PMN) Surveys (Griffith+ 1993-1996)", "VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)", "J/MNRAS/268/602 : Compact radio cores in radio galaxies. (Jones+, 1994)", "J/A+A/298/375 : Jet-disk symbiosis II (Falcke+ 1995)", "J/ApJ/448/521 : Radio powers in radio galaxies (Zirbel+, 1995)", "J/A+AS/132/31 : Kinematical models for double radio sources (Nilsson 1998)", "J/ApJS/124/285 : VLA Images of Extragalactic Objects (Reid+, 1999)", "J/A+A/381/757 : List of extra-galactic radio jets (Liu+, 2002)", "J/MNRAS/371/898 : Extragalactic radio sources selected at 20GHz (Sadler+, 2006)", "J/AJ/138/1874 : MOJAVE. VI. Kinematic analysis of blazar jets (Lister+, 2009)", "J/MNRAS/402/2403 : Australia Telescope 20GHz Survey Cat. AT20G (Murphy+, 2010)", "J/MNRAS/416/1900 : CENSORS + other 1.4GHz sources (Rigby+, 2011)", "J/ApJ/744/84 : Combined sample of radio-loud AGNs at 408MHz (Yuan+, 2012)", "J/MNRAS/429/2080 : Lockman Hole 10C radio spectral indices (Whittam+ 2013)", "J/ApJ/780/73 : Redshifts of BL Lac objects from Fermi (Ajello+, 2014)", "J/MNRAS/445/955 : Radio-AGN feedback for 0.5"], "bibcode": ["2019ApJS..240...34M"], "see_also": ["II/294 : The SDSS Photometric Catalog, Release 7 (Adelman-McCarthy+, 2009)", "VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)", "J/MNRAS/362/9 : Radio-loud AGN in SDSS (Best+, 2005)", "J/AJ/133/2097 : FIRST \"Winged\" & X-shaped radio source cand. (Cheung, 2007)", "J/MNRAS/390/819 : Combined NVSS-FIRST Galaxies (CoNFIG) sample (Gendre+, 2008)", "J/MNRAS/404/1719 : CoNFIG sample. II (Gendre+, 2010)", "J/ApJ/723/1119 : Optical properties of radio galaxies at z<0.3 (Lin+, 2010)", "J/ApJS/194/31 : Morphology for groups in the FIRST database (Proctor, 2011)", "J/AJ/141/88 : Galaxy cluster environments of radio sources (Wing+, 2011)", "J/MNRAS/421/1569 : Properties of 18286 SDSS radio galaxies (Best+, 2012)", "J/ApJS/230/20 : Machine learning technique to classify CoNFIG gal.", "J/A+A/601/A81 : FIRST catalog of FR II radio galaxies (Capetti+, 2017)", "J/A+A/598/A49 : FRICAT FIRST catalog of FRI radio galaxies (Capetti+, 2017)", "J/A+A/608/A39 : X-ATLAS X-ray sources photom. redshifts (Mountrichas+, 2017)", "J/A+A/609/A1 : FR0CAT. a FIRST catalog of FR0 radio galaxies (Baldi+, 2018)", "http://sundog.stsci.edu/ : The VLA FIRST survey home page"], "keyword_cds": "Active gal. nuclei; Morphology; Radio sources; Galaxy catalogs", "keyword_pub": "catalogs ; galaxies: statistics ; methods: data analysis ; radio continuum: galaxies ; techniques: miscellaneous", "abstract": ["We present a morphological classification of 14245 radio active", "galactic nuclei (AGNs) into six types, i.e., typical Fanaroff-Riley", "Class I/II (FRI/II), FRI/II-like bent-tailed, X-shaped radio galaxy,", "and ringlike radio galaxy, by designing a convolutional neural network", "based autoencoder, namely MCRGNet, and applying it to a labeled radio", "galaxy (LRG) sample containing 1442 AGNs and an unlabeled radio galaxy", "(unLRG) sample containing 14245 unlabeled AGNs selected from the", "Best-Heckman sample (2012, J/MNRAS/421/1569). We train MCRGNet and", "implement the classification task by a three-step strategy, i.e.,", "pre-training, fine-tuning, and classification, which combines both", "unsupervised and supervised learnings. A four-layer dichotomous tree", "is designed to classify the radio AGNs, which leads to a significantly", "better performance than the direct six-type classification. On the LRG", "sample, our MCRGNet achieves a total precision of ~93% and an averaged", "sensitivity of ~87%, which are better than those obtained in previous", "works. On the unLRG sample, whose labels have been human-inspected,", "the neural network achieves a total precision of ~80%. Also, using", "Sloan Digital Sky Survey Data Release 7 to calculate the r-band", "absolute magnitude (Mopt) and using the flux densities to calculate", "the radio luminosity (Lradio), we find that the distributions of the", "unLRG sources on the Lradio-Mopt plane do not show an apparent", "redshift evolution and could confirm with a sufficiently large sample", "that there could not exist an abrupt separation between FRIs and FRIIs", "as reported in some previous works."], "description": ["All the images of the radio AGNs included in both the unlabeled sample", "(unlabeled radio galaxy sample or unLRG sample) and the labeled sample", "(LRG sample) are drawn from the Very Large Array (VLA) FIRST survey", "archive at http://sundog.stsci.edu/"], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/aaf9a2"], "orcid_pub": ["0000-0003-1263-9453"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table3.dat", "desc": "1442 labeled radio galaxies (LRGs) in the LRG sample ", "columns": [{"name": "Name", "desc": "Source name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "RAh", "desc": "Right ascension in decimal hours (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "z", "desc": "[0.006/3.9]? Spectroscopic redshift "}, {"name": "S1.4", "desc": "[6/14903]? NVSS 1.4GHz integrated flux density "}, {"name": "r_Name", "desc": "Original catalog of the source (1) "}, {"name": "BH12", "desc": "[0/1] Flag of source in the BH12 (Best & Heckman, 2012, J/MNRAS/421/1569) samples"}, {"name": "Type-Lit", "desc": "Morphology type labeled in literature (G1) "}, {"name": "Type-CNN", "desc": "Morphology type labeled by MCRGNet (G1) "}, {"name": "BT-Type", "desc": "Subtype label for BT sample (G2) "}, {"name": "Prob", "desc": "[0.77/1] Probability of classification by MCRGNet"}]}, {"name": "table4.dat", "desc": "14245 unlabeled radio AGNs (unLRG) in the unLRG sample", "columns": [{"name": "Name", "desc": "Source name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "RAh", "desc": "Right ascension in decimal hours (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "z", "desc": "[0.015/0.7] Spectroscopic redshift "}, {"name": "S1.4", "desc": "[5/22721] NVSS 1.4GHz integrated flux density "}, {"name": "rMag", "desc": "[-26.2/-10.4]? SDSS r band absolute magnitude "}, {"name": "Type-CNN", "desc": "Morphology type labeled by MCRGNet (G1) "}, {"name": "BT-CNN", "desc": "Subtype label for BT sample by the MCRGNet "}, {"name": "Type-MAN", "desc": "Morphology type labeled by human inspection (G1) "}, {"name": "BT-MAN", "desc": "Subtype label for BT sample by human inspection (G2)"}, {"name": "Prob", "desc": "[0.76/1] Probability of classification by MCRGNet "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_240_5"}} {"id": "J/ApJS/240/5", "title_cds": "SHELA. II. DECam and IRAC multiwavelength catalog", "title_create": "Wold+, 2019", "year": "2019", "author": "Wold I.G.B., Kawinwanichakij L., Stevans M.L., Finkelstein S.L., Papovich C., Devarakonda Y., Ciardullo R., Feldmeier J., Florez J., Gawiser E., Gronwall C., Jogee S., Marshall J.L., Sherman S., Shipley H.V., Somerville R.S., Valdes F., Zeimann G.R.", "title_pub": "The Spitzer-HETDEX Exploratory Large Area survey. II. The Dark Energy Camera and Spitzer/IRAC multiwavelength catalog.", "first_author": "Wold I.G.B.", "ref_biblio": [""], "bibcode": ["2019ApJS..240....5W"], "see_also": ["J/ApJS/162/1 : MUSYC: optical source catalog (Gawiser+, 2006)", "J/ApJS/206/8 : COSMOS/UltraVISTA Ks-selected catalogs v4.1 (Muzzin+, 2013)"], "keyword_cds": "Galaxies, photometry; Photometry, ugriz; Photometry, infrared ; Redshifts; Surveys", "keyword_pub": "catalogs; cosmology: observations; galaxies: photometry; surveys", "abstract": ["We present the ugriz-band Dark Energy Camera (DECam) plus 3.6 and", "4.5{mu}m IRAC catalogs for the Spitzer/HETDEX Exploratory Large-Area", "(SHELA) survey. SHELA covers ~24deg^2^ of the Sloan Digital Sky Survey", "(SDSS) \"Stripe 82\" region, with seven bandpasses spanning a wavelength", "range of 0.35 to 4.5{mu}m. SHELA falls within the footprint of the", "Hobby-Eberly Telescope Dark Energy Experiment (HETDEX), which will", "provide spectroscopic redshifts for ~200000 Ly{alpha} emitters at", "1.9=0.33 SDSS spectroscopic redshifts with a", "1{sigma} scatter in {Delta}z/(1+z) of 0.04."], "description": ["We observed with the Blanco 4m telescope at CTIO using the 3deg^2^", "DECam imager and the u-, g-, r-, i-, and z-band filters. Data were", "obtained over 5 nights in the 2013B semester (PI: Papovich; NOAO PID:", "2013B-0438). As shown in Figure 1, we observed six slightly", "overlapping pointings covering a total area of 17.5deg^2^."], "alias": ["SHELA"], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/aaee85"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table6.dat", "desc": "Spitzer/HETDEX Exploratory Large-Area (SHELA) Dark Energy Camera (DECam) catalog", "columns": [{"name": "ID", "desc": "Unique object ID number (B3_ to B6_ tiles plus 000001 to 684409 numbers)"}, {"name": "RAdeg", "desc": "[14/24.6] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-1.4/1.4] Declination (J2000) "}, {"name": "amaj", "desc": "[0.1/3048] Semimajor axis (1) "}, {"name": "ell", "desc": "[0/1] Ellipticity (1) "}, {"name": "PA", "desc": "[-90/90] Postion angle (1) "}, {"name": "rKron", "desc": "[0/877] Sextractor Kron radius, AUTO photometry (1)"}, {"name": "r0.5", "desc": "[0/15905] PSF half-light radius "}, {"name": "FuPSF", "desc": "[-4/993] DECam u-band PSF fitting flux (2)"}, {"name": "e_FuPSF", "desc": "[0.001/46] Uncertainty in FuPSF (5) "}, {"name": "Fu", "desc": "[-132/46824] DECam u-band AUTO aperture flux (3)"}, {"name": "e_Fu", "desc": "[0.001/2942] Uncertainty in Fu (5) "}, {"name": "uflagI", "desc": "[0/153] DECam u-band internal flag (4) "}, {"name": "uflagE", "desc": "[0/1] DECam u-band external flag (4) "}, {"name": "FgPSF", "desc": "[-4/34050] DECam g-band PSF fitting flux (2)"}, {"name": "e_FgPSF", "desc": "[0.001/1570] Uncertainty in FgPSF (5) "}, {"name": "Fg", "desc": "[-21/521598] DECam g-band AUTO aperture flux (3)"}, {"name": "e_Fg", "desc": "[0.001/24346] Uncertainty in Fg (5) "}, {"name": "gflagI", "desc": "[0/153] DECam g-band internal flag (4) "}, {"name": "gflagE", "desc": "[0/1] DECam g-band external flag (4) "}, {"name": "FrPSF", "desc": "[-6/19361] DECam r-band PSF fitting flux (2)"}, {"name": "e_FrPSF", "desc": "[0.001/892] Uncertainty in FrPSF (5) "}, {"name": "Fr", "desc": "[-54/366386] DECam r-band AUTO aperture flux (3)"}, {"name": "e_Fr", "desc": "[0.001/29114] Uncertainty in Fr (5) "}, {"name": "rflagI", "desc": "[0/157] DECam r-band internal flag (4) "}, {"name": "rflagE", "desc": "[0/1] DECam r-band external flag (4) "}, {"name": "FiPSF", "desc": "[-7/16418] DECam i-band PSF fitting flux (2)"}, {"name": "e_FiPSF", "desc": "[0.001/758] Uncertainty in FiPSF (5) "}, {"name": "Fi", "desc": "[-1135/743848] DECam i-band AUTO aperture flux (3)"}, {"name": "e_Fi", "desc": "[0.001/220928] Uncertainty in Fi (5) "}, {"name": "iflagI", "desc": "[0/157] DECam i-band internal flag (4) "}, {"name": "iflagE", "desc": "[0/1] DECam i-band external flag (4) "}, {"name": "FzPSF", "desc": "[-5/47832] DECam z-band PSF fitting flux (2)"}, {"name": "e_FzPSF", "desc": "[0.001/2216] Uncertainty in FzPSF (5) "}, {"name": "Fz", "desc": "[-322/568888] DECam z-band AUTO aperture flux (3)"}, {"name": "e_Fz", "desc": "[0.001/161580] Uncertainty in Fz (5) "}, {"name": "zflagI", "desc": "[0/157] DECam z-band internal flag (4) "}, {"name": "zflagE", "desc": "[0/1] DECam z-band external flag (4) "}, {"name": "---", "desc": "[VICS82] "}, {"name": "VICS82", "desc": "JK object ID number (JHHMMSS.ss+DDMMSS.s), Geach+ (2017ApJS..231....7G) => a faire."}, {"name": "FJ", "desc": "[0.01/948492]?=-99 J band AUTO aperture flux (6)"}, {"name": "e_FJ", "desc": "[0/4153]?=-99 Uncertainty in FJ (6) "}, {"name": "FK", "desc": "[0/921168]?=-99 K band AUTO aperture flux (6)"}, {"name": "e_FK", "desc": "[0/37964]?=-99 Uncertainty in FK (6) "}, {"name": "F3.6um", "desc": "[-5e+6/2.1e+6]?=-99 IRAC 3.6um Tractor total flux"}, {"name": "e_F3.6um", "desc": "[0.01/5e+12]?=-99 Uncertainty in F3.6um "}, {"name": "Mod3.6", "desc": "[0/4] IRAC Tractor model profile, 3.6um (7)"}, {"name": "logP3.6", "desc": "[-7e+10/0] IRAC Tractor log-probability, 3.6um"}, {"name": "Tflag3.6um", "desc": "[0/2] Tractor flag, 3.6um observation (8) "}, {"name": "F4.5um", "desc": "[-1e+6/1.3e+6]?=-99 IRAC 4.5um Tractor total flux"}, {"name": "e_F4.5um", "desc": "[0.01/3e+12]?=-99 Uncertainty in F4.5um "}, {"name": "Mod4.5um", "desc": "[0/4] IRAC Tractor model profile, 4.5um (7)"}, {"name": "logP4.5um", "desc": "[-3e+10/0] IRAC Tractor log-probability, 4.5um"}, {"name": "Tflag4.5um", "desc": "[0/2] Tractor flag, 4.5um observation (8) "}, {"name": "zspec", "desc": "[0/1.7]?=-99 SDSS spectroscopic redshift "}, {"name": "zpeak", "desc": "[0.01/10.5]?=-99 EAZY peak photometric redshift"}, {"name": "za", "desc": "[0.01/11]?=-99 EAZY {chi}^2^ minimum photometric redshift"}, {"name": "chi2a", "desc": "[0/2664]?=-99 EAZY {chi}^2 minimum value "}, {"name": "Nfilt", "desc": "[5/9]?=-99 EAZY number of filters "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_240_6"}} {"id": "J/ApJS/240/6", "title_cds": "", "title_create": "Yao+, 2019", "year": "2019", "author": "Yao Su, Wu X.-B., Ai Y.L., Yang J., Yang Q., Dong X., Joshi R., Wang F., Feng X., Fu Y., Hou W., Luo A.-L., Kong X., Liu Y., Zhao Y.-H., Zhang Y.-X., Yuan H.-L., Shen S.", "title_pub": "The Large Sky Area Multi-object Fiber Spectroscopic Telescope (LAMOST) Quasar Survey: The Fourth and Fifth Data Releases.", "first_author": "Yao Su", "bibcode": [""], "bibcode": ["1974ApJS...28....1J"], "keyword_cds": "Stars, M-type", "keyword_pub": "late-type stars ; luminosities ; spectral classification", "description": ["Spectral types are given for 426 M dwarf stars on a uniform system", "based on the TiO bands. Most of the stars where discovered by their", "large proper motions except for the McCormick (Vyssotkey) stars. The", "observations were made with the Mount Wilson telescopes at dispersions", "of 100{AA}/mm or higher."], "curator": "Brian Skiff [Lowell Obs.], Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190307"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_30_491"}} {"id": "J/ApJS/30/491", "title_cds": "Hen-3 list of southern emission-line stars", "title_create": "Henize+, 1976", "year": "1976", "author": "Henize K.G.", "title_pub": "Observations of southern emission-line stars.", "first_author": "Henize K.G.", "ref_biblio": [""], "bibcode": ["1976ApJS...30..491H"], "keyword_cds": "Stars, emission ; Spectral types", "keyword_pub": "clusters: associations ; stars: Be \u2014 stars: stellar statistics", "abstract": ["A catalog is presented of 1929 stars showing emission at H{alpha} on", "plates taken with the Mount Wilson 10inch (25cm) camera at the", "Lamont-Hussey Observatory in 1949\u20141951. The survey covers the entire", "southern sky south of declination -25{deg} to a red limiting magnitude", "of about 11.0. A region of the northern Milky Way approximately 600", "square degrees in area is also included in order to allow comparison", "with northern surveys. Emission-line stars of all spectral classes are", "listed including 16 M stars, 25 S stars, and 37 carbon stars, as well", "as 40 con\ufb01rmed or suspected T Tauri stars. This survey has resulted", "in the discovery of two new T associations, one in Lupus and one in", "Chamaeleon.", "Variations in the intensity of the continuous spectrum have been", "observed in 53 stars, of which 32 are newly discovered variable stars.", "Variations in Ha intensity only are observed in an addi- tional 32", "stars.", "Of the 1232 stars having spectral classi\ufb01cations (mostly HD types),", "the peak frequency (17%) occurs at spectral class B8. However,", "frequency of emission per 100 stars of a given spectral class", "increases gradually from 0.2 for A0\u2014A4 stars to a maximum of 18.5 at", "B2.", "The sky distribution of the emission-line stars shows signi\ufb01cant", "concentrations in the region of the small Sagittarius cloud and in the", "Carina region. The emission-line stars in the Carina region appear to", "be predominantly B8\u2014B9 stars. The B8\u2014B9 stars form a relatively", "compact group centered at a distance of 1200 pc and are probably a", "part of the concentration of B8\u2014A0 stars seen in the Carina", "direction."], "description": ["Accurate positions of this list were dervied by Brian Skiff", "(Lowell Obs.)"], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190369"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_35_111"}} {"id": "J/ApJS/35/111", "title_cds": "MK classification of OB stars", "title_create": "Garrison+, 1977", "year": "1977", "author": "Garrison R.F., Hiltner W.A., Schild R.E.", "title_pub": "MK spectral classifications for southern OB stars.", "first_author": "Garrison R.F.", "ref_biblio": [""], "bibcode": ["1977ApJS...35..111G"], "keyword_cds": "MK spectral classification", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190468"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_4_73"}} {"id": "J/ApJS/4/73", "title_cds": "The LF2 survey in infra-red", "title_create": "Westerlund, 1959", "year": "1959", "author": "Westerlund B.", "title_pub": "An infrared survey of a region in Cygnus.", "first_author": "Westerlund B.", "ref_biblio": [""], "bibcode": ["1959ApJS....4...73W"], "see_also": ["II/221 : The LF Survey (McCuskey+ 1949-1959)"], "keyword_cds": "", "description": ["Spectral classes on the Case infrared system and infrared photographic", "magnitudes are given in the LF2 region (see Cat. II/221). The data are", "complete down to 12.25mag for the early M stars, and 12.75mag for the", "late M and Carbon stars. The search for M and S stars was carried out", "also in 3 other regions of the same galactic longitude (32.5deg), and", "the search for Carbon stars was extended to all observations covering", "a surface of 50 sq.deg."], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190045"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_43_379"}} {"id": "J/ApJS/43/379", "title_cds": "MK Types of S and SC stars", "title_create": "Keenan+ 1980", "year": "1980", "author": "Keenan P.C., Boeshaar P.C.", "title_pub": "Spectral types of S and SC stars on the revised MK system.", "first_author": "Keenan P.C.", "ref_biblio": [""], "bibcode": ["1980ApJS...43..379K"], "see_also": ["http://www.astronomy.ohio-state.edu/MKCool/ : The Revised Catalog of"], "keyword_cds": "Stars, S ; MK spectral classification", "keyword_pub": "", "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/190673"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_58_439"}} {"id": "J/ApJS/58/439", "title_cds": "Observations of double stars. XII.", "title_create": "Heintz, 1985", "year": "1985", "author": "Heintz W.D.", "title_pub": "Micrometer observations of double stars and new pairs. XII.", "first_author": "Heintz W.D.", "ref_biblio": [""], "bibcode": ["1985ApJS...58..439H"], "see_also": ["J/ApJS/74/275 : Observations of double stars. XIV. (Heintz 1990)", "J/ApJS/83/351 : Observations of double stars. XV. (Heintz, 1992)", "J/ApJS/99/693 : Observations of double stars. XVI. (Heintz 1995)", "J/ApJS/105/475 : Observations of double stars. XVII. (Heintz 1996)", "J/ApJS/117/587 : Observations of double stars. XVIII. (Heintz 1998)"], "keyword_cds": "Stars, double and multiple", "keyword_pub": "stars: visual multiples", "abstract": ["Measures of 2235 pairs, including 103 new doubles, obtained at", "Swarthmore and at Cerro Tololo in the time 1982.4 to 1984.8 are", "listed."], "doi_pub": ["10.1086/191048"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Observations with the 61cm refractor ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "RAh", "desc": "? Right ascension (1900.0) "}, {"name": "RAdm", "desc": "? Right ascension (1900.0) (deci-minutes) "}, {"name": "DE-", "desc": "Declination sign (1900.0) "}, {"name": "DEd", "desc": "? Declination (1900.0) "}, {"name": "DEm", "desc": "? Declination (1900.0) "}, {"name": "Date-1980", "desc": "Observing date (minus 1980) "}, {"name": "PA", "desc": "? Position angle "}, {"name": "n_PA", "desc": "[r:?] r: round "}, {"name": "Sep", "desc": "? Separation "}, {"name": "u_Sep", "desc": "Uncertainnty flag on Sep "}, {"name": "Nnights", "desc": "Number of nights "}, {"name": "m_Name", "desc": "[ABCD -] Components for multiple systems "}, {"name": "m1/dm", "desc": "? Magnitude of brightest component or difference of magnitude (1)"}, {"name": "n_m2", "desc": "[-] '-' when m1 = magnitude of the primary "}, {"name": "m2", "desc": "? Magnitude of second brightest component "}, {"name": "Rem", "desc": "Remarks "}]}, {"name": "table2.dat", "desc": "Observations with the 100 and 91cm reflectors ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "RAh", "desc": "? Right ascension (1900.0) "}, {"name": "RAdm", "desc": "? Right ascension (1900.0) (deci-minutes) "}, {"name": "DE-", "desc": "Declination sign (1900.0) "}, {"name": "DEd", "desc": "? Declination (1900.0) "}, {"name": "DEm", "desc": "? Declination (1900.0) "}, {"name": "Date-1980", "desc": "Observing date (minus 1980) "}, {"name": "PA", "desc": "? Position angle "}, {"name": "n_PA", "desc": "[r:?] r: round "}, {"name": "Sep", "desc": "? Separation "}, {"name": "u_Sep", "desc": "Uncertainnty flag on Sep "}, {"name": "Nnights", "desc": "Number of nights "}, {"name": "m_Name", "desc": "[ABCD -] Components for multiple systems "}, {"name": "m1/dm", "desc": "? Magnitude of brightest component or difference of magnitude (1)"}, {"name": "n_m2", "desc": "[-] '-' when m1 = magnitude of the primary "}, {"name": "m2", "desc": "? Magnitude of second brightest component "}, {"name": "Rem", "desc": "Remarks "}]}, {"name": "table3a.dat", "desc": "Stars of table3 ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "m_Name", "desc": "[ABC] Multiplicity index on name "}, {"name": "IDS", "desc": "IDS designation "}, {"name": "m1", "desc": "? Magnitude of the primary "}, {"name": "---", "desc": "[-] "}, {"name": "m2", "desc": "? Magnitude of the secondary "}, {"name": "n_m2", "desc": "[v] v: variable "}, {"name": "Rem", "desc": "Remarks "}]}, {"name": "table3b.dat", "desc": "Measures of astrometric plates ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "m_Name", "desc": "[ABC] Multiplicity index on name "}, {"name": "Obs-1900", "desc": "Observation date (minus 1900) "}, {"name": "PA", "desc": "Position angle "}, {"name": "Sep", "desc": "Separation "}, {"name": "Nnights", "desc": "? Number of nights "}, {"name": "Nexp", "desc": "Number of exposures "}]}, {"name": "table4.dat", "desc": "New pairs ", "columns": [{"name": "Hei", "desc": "Hei number "}, {"name": "RAh", "desc": "Right ascension (2000.0) "}, {"name": "RA1dm", "desc": "Rigth ascension (1900.0) "}, {"name": "RAdm", "desc": "Rigth ascension (2000.0) "}, {"name": "DE-", "desc": "[NS] Declination sign (2000.0) "}, {"name": "DEd", "desc": "Declination (2000.0) "}, {"name": "DE1m", "desc": "Declination (1900.0) "}, {"name": "DEm", "desc": "[0/90] Declination (2000.0) "}, {"name": "BD/CPD", "desc": "BD (Cat. ) or CPD (Cat. ) designation"}, {"name": "Com", "desc": "Comment "}]}, {"name": "notes.dat", "desc": "Notes ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_60_507"}} {"id": "J/ApJS/60/507", "title_cds": "GRI photometry of NGC 6822", "title_create": "Hoessel+, 1986", "year": "1986", "author": "Hoessel J.G., Anderson N.", "title_pub": "Photometry of resolved galaxies. V. NGC 6822.", "first_author": "Hoessel J.G.", "ref_biblio": [""], "bibcode": ["1986ApJS...60..507H"], "see_also": ["J/ApJ/501/153 : VRB photometry of red supergiants (Massey 1998)", "J/AJ/110/2715 : UBV photometry in NGC 6822, M31 and M33 (Massey+ 1995)"], "keyword_cds": "Galaxies, photometry ; Photometry, CCD", "keyword_pub": "galaxies: individual - galaxies: Local Group - galaxies: photometry - galaxies: stellar content - luminosity function", "abstract": ["Three-color CCD frames of the local group irregular galaxy NGC 6822", "have been reduced to GRI photometry for 3475 stars using RICHFLD", "point-spread function fitting techniques. The data are compared with", "earlier work on this galaxy, particularly with Kayser (1966, Ph.D.", "Thesis, California Institute of Technology) on a star-by-star basis.", "While the general agreement between the results of photographic and", "electronic techniques is good, some differences in detail exist, which", "are attributed to a small nonlinearity in the photographic results and", "zero-point offsets of ~0.1mag. Color-magnitude diagrams are", "constructed from the data and compared with both theoretical stellar", "model tracks and the expected foreground star contamination. A", "luminosity function for the blue stars (G-R<0) is derived; comparison", "of this luminosity function with those of 10 other irregular galaxies", "indicates that NGC 6822 has a typical young star population. The", "stellar birthrate and initial mass function are estimated for this", "galaxy. The slope at the bright end of the mass function looks similar", "to recent results for the Galaxy, the Magellanic Clouds, and the", "irregular galaxy Sextans A. NGC 6822 appears to be presently forming", "stars at a slower rate for its mass than Sextans A or the Magellanic", "Clouds.", "For a description of the GRI photometric system, see e.g.", " and "], "object": ["19 44 57.8 -14 48 11 NGC 6822 = IC 4895"], "doi_pub": ["10.1086/191095"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Photometry of stars in CCD field 1 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table2.dat", "desc": "Photometry of stars in CCD field 2 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table3.dat", "desc": "Photometry of stars in CCD field 3 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table4.dat", "desc": "Photometry of stars in CCD field 4 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table5.dat", "desc": "Photometry of stars in CCD field 5 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table6.dat", "desc": "Photometry of stars in CCD field 6 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table7.dat", "desc": "Photometry of stars in CCD field 7 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table8.dat", "desc": "Photometry of stars in CCD field 8 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}, {"name": "table9.dat", "desc": "Photometry of stars in CCD field 9 ", "columns": [{"name": "[HA86]", "desc": "Sequential number, N-NNN (1) "}, {"name": "Xpos", "desc": "X position, relative to the field (2) "}, {"name": "Ypos", "desc": "Y position, relative to the field (2) "}, {"name": "Rmag", "desc": "R magnitude "}, {"name": "G-R", "desc": "? G-R colour index "}, {"name": "R-I", "desc": "? R-I colour index "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_62_751"}} {"id": "J/ApJS/62/751", "title_cds": "A catalog of Markarian galaxies", "title_create": "Mazzarella+, 1986", "year": "1986", "author": "Mazzarella J.M., Balzano V.A.", "title_pub": "A catalog of Markarian galaxies.", "first_author": "Mazzarella J.M.", "ref_biblio": [""], "bibcode": ["1986ApJS...62..751M\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191155"], "orcid_pub": ["0000-0002-8204-8619"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_69_1"}} {"id": "J/ApJS/69/1", "title_cds": "First addition to the new optical catalog of QSO", "title_create": "Hewitt+, 1989", "year": "1989", "author": "Hewitt A., Burbidge G.", "title_pub": "The first addition to the new optical catalog of quasi-stellar objects.", "first_author": "Hewitt A.", "ref_biblio": [""], "bibcode": ["1989ApJS...69....1H\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricio Ortiz [CDS]", "doi_pub": ["10.1086/191307"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_70_637"}} {"id": "J/ApJS/70/637", "title_cds": "Southern Milky Way carbon stars", "title_create": "Aaronson+, 1989", "year": "1989", "author": "Aaronson M., Blanco V.M., Cook K.H., Schechter P.L.", "title_pub": "Southern Milky Way carbon stars: new candidates, JHK photometry and radial velocities.", "first_author": "Aaronson M.", "ref_biblio": [""], "bibcode": ["1989ApJS...70..637A"], "keyword_cds": "Stars, carbon;", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191350"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_72_715"}} {"id": "J/ApJS/72/715", "title_cds": "Cluster Radial Velocity Samples", "title_create": "Teague+, 1990", "year": "1990", "author": "Teague P.F., Carter D., Gray P.M.", "title_pub": "The dynamics and structure of rich clusters of galaxies. I. Velocity data.", "first_author": "Teague P.F.", "ref_biblio": [""], "bibcode": ["1990ApJS...72..715T"], "keyword_cds": "Clusters, galaxy ; X-ray sources ; Redshifts", "keyword_pub": "galaxies: clustering - galaxies: redshifts", "abstract": ["An extensive spectroscopic study of 10 rich southern X-ray clusters of", "galaxies is presented. Between 40 and 200 redshifts have been obtained", "in the field of each of the clusters, which cover a wide range of", "morphological types and richnesses. Applying rigorous statistical", "analyses to the total data base of 1000 precise radial velocities", "provides the necessary information to undertake a thorough dynamical", "investigation of these individual clusters and of cluster systems in", "general."], "doi_pub": ["10.1086/191430"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table4.dat", "desc": "Cluster radial velocity samples ", "columns": [{"name": "TCG", "desc": "Galaxy identification number (ANNNN NNNA) (1) "}, {"name": "RA1h", "desc": "Right ascension (B1950) "}, {"name": "RA1m", "desc": "Right ascension (B1950) "}, {"name": "RA1s", "desc": "Right ascension (B1950) "}, {"name": "DE1-", "desc": "Declination sign (B1950) "}, {"name": "DE1d", "desc": "Declination (B1950) "}, {"name": "DE1m", "desc": "Declination (B1950) "}, {"name": "DE1s", "desc": "Declination (B1950) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Dist", "desc": "Projected radial distance of galaxy from cluster centre"}, {"name": "HRV", "desc": "Heliocentric radial velocity "}, {"name": "u_HRV", "desc": "Uncertainty flag on HRV "}, {"name": "e_HRV", "desc": "Error in radial velocity "}, {"name": "R(TD)", "desc": "? Tonry & Davis (1979AJ.....84.1511T) R-value "}, {"name": "Com", "desc": "Comments (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_73_841"}} {"id": "J/ApJS/73/841", "title_cds": "Carbon stars in the Northern Milky Way", "title_create": "Aaronson+, 1990", "year": "1990", "author": "Aaronson M., Blanco V.M., Cook K.H., Olszewski E.W., Schechter P.L.", "title_pub": "Northern Milky Way carbon star: new candidates, JHK photometry and radial velocities.", "first_author": "Aaronson M.", "ref_biblio": [""], "bibcode": ["1990ApJS...73..841A"], "keyword_cds": "Stars, carbon", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191491"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_82_1"}} {"id": "J/ApJS/82/1", "title_cds": "Optical identification of Texas Survey radio sources", "title_create": "Bozyan, 1992", "year": "1992", "author": "Bozyan E.P.", "title_pub": "Optical identification, radio galaxy environment and statistical properties for a homogeneous sample of 3196 radio sources from the Texas survey.", "first_author": "Bozyan E.P.", "ref_biblio": [""], "bibcode": ["1992ApJS...82....1B"], "see_also": ["VII/54 : Extragalactic Radio Source Identifications (Veron-Cetty+ 1983)", "VIII/42 : Texas Survey of Radio Sources at 365 MHz (Douglas+ 1996)"], "keyword_cds": "Radio sources ; Galaxies, radio ; QSOs ; Clusters, galaxy ; Surveys", "keyword_pub": "Galaxies: clustering - Quasars: general - Radio continuum: galaxies", "description": ["National Geographic Society Palomar Sky Survey E and O glass copy", "plates were searched for optical counterparts to a homogeneous sample", "of 3196 sources from the 365MHz Texas Survey in the region", "+31{deg}20{deg}. The search resulted in 860", "optical identifications coincident with the radio centroid within the", "4 arcsecond search radius. There were also 728 possible", "identifications at the plate limit and 1608 empty fields with no", "optical counterpart to the plate limit. Radio source data and optical", "identification data are tabulated for the entire sample. For the", "positive identifications, the optical data includes magnitudes", "estimated from the plates to 0.5mag and classifications of the", "appearance as stellar or diffuse."], "doi_pub": ["10.1086/191709"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table456.dat", "desc": "Optical identifications ", "columns": [{"name": "Name", "desc": "Texas Survey radio source name in IAU format "}, {"name": "Mflg", "desc": "Goodness of structure model fit (1) "}, {"name": "Eflg", "desc": "Influence of environment on fit (1) "}, {"name": "Lflg", "desc": "Probability the position is lobe-shifted (1) "}, {"name": "RAh", "desc": "Right Ascension (1950) "}, {"name": "RAm", "desc": "Right Ascension (1950) "}, {"name": "RAs", "desc": "Right Ascension (1950) "}, {"name": "e_RAs", "desc": "Right Ascension error "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "DEs", "desc": "Declination (1950) "}, {"name": "e_DEs", "desc": "Declination error "}, {"name": "S365MHz", "desc": "365 MHz flux density "}, {"name": "e_S365MHz", "desc": "Flux density error "}, {"name": "Sp+Index", "desc": "? 335-385 MHz spectral index, S{prop.to}nu^(-Sp+Index)^"}, {"name": "e_Sp+Index", "desc": "? Error in spectral index "}, {"name": "Chi2", "desc": "? Chi-squared per dof flux residual over 4 observing cycles"}, {"name": "Vflg", "desc": "[*]? * means source may be variable "}, {"name": "Sep", "desc": "? Component separation in double model "}, {"name": "e_Sep", "desc": "? Error in component separation "}, {"name": "Struct", "desc": "Structure model type, P: point source, D: double, AD: asymmetric double"}, {"name": "q", "desc": "? Flux asymmetry parameter for AD model (2) "}, {"name": "Xi", "desc": "[-180,180]? Position angle of double "}, {"name": "e_Xi", "desc": "? Error in position angle (99=unknown) "}, {"name": "KA2", "desc": "? Second most likely RA lobe "}, {"name": "KD2", "desc": "? Second most likely Dec lobe "}, {"name": "IDE", "desc": "Identification on E plate (3) "}, {"name": "AppE", "desc": "[SD]? Appearance on E plate S: stellar, D: diffuse"}, {"name": "IDO", "desc": "Identification on O plate (3) "}, {"name": "AppO", "desc": "[SD]? Appearance on O plate: S: stellar, D: diffuse"}, {"name": "Color", "desc": "[BRN]? B: blue, R: red, N: neutral "}, {"name": "QualE", "desc": "? Qualifications for E identification (4) "}, {"name": "QualO", "desc": "? Qualifications for O identification (4) "}, {"name": "Comment", "desc": "? Additional identifications, close optical companions, or other comments"}, {"name": "Known", "desc": "? Previous ID, or ID within 2 arcmin of center of Abell or Zwicky cluster (5)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_83_203"}} {"id": "J/ApJS/83/203", "title_cds": "Catalog of faint A, F and G stars at SGP", "title_create": "Lu+, 1992", "year": "1992", "author": "Lu P.K., Miller J., Platt D.", "title_pub": "A catalog of faint A, F, and G stars at the South Galactic Pole.", "first_author": "Lu P.K.", "ref_biblio": [""], "bibcode": ["1992ApJS...83..203L"], "see_also": ["II/119 : Stellar Distribution near the South Galactic Pole (Bok+ 1964)", "III/74 : Faint blue stars in the region near SGP (Haro+ 1962)", "II/120 : Phot and Spectrophot Investigation, SGP (Eriksson 1978)", "I/129 : Parallaxes and Proper Motions near SGP (Murray+ 1986)", "J/AJ/112/772 : VI photometry in South Galactic Pole (Caldwell+ 1996)", "J/AJ/109/2229 : South Galactic Pole stars photometry (Eggen 1995)"], "keyword_cds": "Stars, faint ; Galactic pole, south ; MK spectral classification ; Photometry", "keyword_pub": "catalogs - stars: fundamental parameters", "abstract": ["A catalog of identifications and positions for 3155 A, F, and G stars", "at the south Galactic pole is presented. The new thin-prism spectra", "survey yields a set of uniformly selected A, F, and early G stars to", "a limiting magnitude of 16.0. The positions are based on PDS scans of", "a 6.3{deg}x6.3{deg} UK Schmidt direct film centered on the SGP.", "Objective-prism plates covering approximately 100{deg}^2^ centered on", "the SGP were obtained using the Michigan Curtis Schmidt telescope at", "CTIO with a dispersion of 1360{AA}/mm. Approximately 30% of the", "catalog stars now have 2D-Frutti MK spectral types and uvby,H{beta}", "photometry. Of 822 spectra classified with luminosities, 76 stars (9%)", "have classes III and IV-III; 21 (3%) stars are class IV, 669 stars", "(81%) are of luminosity classes V and V-IV, and 56 stars (7%) are", "classified as Vw for weak-lined or intermediate Population II objects.", "The mean spectral distribution for dwarf stars peaks at F9.3 V and", "declines sharply at G4. The mean color index for 1104 stars is", "=0.359+/-0.080, a value typical of F9 V. Correlations between", "spectral types and photometry (b-y) index are also presented. Detailed", "analyses of radial velocity determinations using cross-correlation", "techniques and direct CCD and ASCAP photometry will be reported in a", "subsequent paper. The purpose of publishing the catalog at this stage", "is to invite other investigators to collaborate in collecting the", "photometric and spectroscopic data."], "alias": ["[LMP92]"], "type": ["OC"], "doi_pub": ["10.1086/191735"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Catalog of faint F and G stars at the South Galactic Pole", "columns": [{"name": "SAx", "desc": "Frame number (pixel number in RA) "}, {"name": "SAy", "desc": "Frame number (pixel number in DE) "}, {"name": "Star", "desc": "Number of the star in the Frame SAxSAy (1) "}, {"name": "m_Star", "desc": "[AB] Multiplicity index on Star "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "[0/60] Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "[0/60] Declination (J2000) "}, {"name": "u_SpT", "desc": "[:] Uncertainty flag on SpT "}, {"name": "n_SpT", "desc": "[*] *: Multiple observations exist "}, {"name": "SpT", "desc": "Spectral type "}, {"name": "Vmag", "desc": "V or photographic magnitude "}, {"name": "b-y", "desc": "? b-y colour index "}, {"name": "n_b-y", "desc": "[*] *: Multiple observations exist "}, {"name": "2DF", "desc": "? 2D-Frutti frame number "}, {"name": "Note", "desc": "[ac*] FLAGS NOT EXPLANED "}, {"name": "CCD", "desc": "? CCD frame number "}, {"name": "HD", "desc": "? HD, Bok or CGG number (see \"n_HD\" column) "}, {"name": "n_HD", "desc": "[cb] b = Bok and Basinski, 1964, Cat. ) number; c = Corbally+Garrison SGP number"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_83_273"}} {"id": "J/ApJS/83/273", "title_cds": "High Galactic latitude stars photometry", "title_create": "Penprase+, 1992", "year": "1992", "author": "Penprase B.E.", "title_pub": "Photometric and spectroscopic analysis of high galactic latitude molecular clouds. I. Distances and extinctions of stars toward 25 selected regions.", "first_author": "Penprase B.E.", "ref_biblio": [""], "bibcode": ["1992ApJS...83..273P"], "see_also": ["III/31 : Michigan catalogue for the HD stars, vol. 1 (Houk+, 1975)"], "keyword_cds": "Molecular clouds ; Photometry, UBV ; Photometry, H-beta ; Photometry, uvby, beta ; Reddening", "keyword_pub": "ISM: clouds - ISM: molecules - stars: fundamental parameters", "abstract": ["New photoelectric photometry in the UBV, uvby, and H{beta} systems is", "presented for 320 stars at high Galactic latitudes, selected for their", "proximity to the densest portions of a variety of high Galactic", "latitude atomic and molecular clouds. Low-resolution digital spectra", "are used to classify 115 of the stars, using both stellar line", "strengths and statistical tests against a library of standard stars of", "all spectral types. Several new techniques are developed for automatic", "digital spectral classification, and for dereddening Stromgren", "uvby{beta} and Johnson UBV, H{beta} photometry. An empirical determination", "of the errors in the derived dereddened colors, and techniques for", "converting between the two photometric systems are presented, based on", "the analysis of a statistically significant sample of 1480 stars with", "complete data sets in both photometric systems and with an accurate MK", "spectral type. For several stars, spectroscopic and photometric", "observations are combined to derive distances and reddenings toward", "selected high-latitude clouds. New constraints on the distances to", "several clouds are presented: for MBM 41, 200 < d < 300pc;", "for MBM 3-4, 90 < d < 180pc; for MBM 27-31, 130 < d < 220pc;", "for MBM 15, 110 < d < 160pc; and for MBM 57, 150 < d < 210pc. Additional", "distance constraints have been obtained for over 25 cloud complexes,", "and several highly reddened sightlines have been identified which", "should offer opportunities for spectroscopic analysis of the molecular", "clouds."], "doi_pub": ["10.1086/191738"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table3.dat", "desc": "The stars observed with UBV,H{beta} photometry ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "SAO", "desc": "? SAO (Cat. ) number) "}, {"name": "RAh", "desc": "Right ascension (B1950) "}, {"name": "RAm", "desc": "Right ascension (B1950) "}, {"name": "RAs", "desc": "Right ascension (B1950) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) "}, {"name": "DEm", "desc": "Declination (B1950) "}, {"name": "DEs", "desc": "Declination (B1950) "}, {"name": "SpType", "desc": "Spectral type (from HD catalogue) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "LRS", "desc": "[yes no] Low-resolution digital spectroscopy "}, {"name": "ubvybeta", "desc": "[yes no] uvby{beta} photometry "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "U-B", "desc": "U-B colour index "}, {"name": "o_Vmag", "desc": "Number of observations in UBV "}, {"name": "e_Vmag", "desc": "rms uncertainty on UBV observations "}, {"name": "Hbeta", "desc": "H{beta} colour index "}, {"name": "o_Hbeta", "desc": "Number of observations in Hbeta "}, {"name": "e_Hbeta", "desc": "rms uncertainty on Hbeta "}, {"name": "Region", "desc": "Associated interstellar cloud (G1) "}]}, {"name": "table4.dat", "desc": "The stars observed with ubvy,{beta} photometry ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "SAO", "desc": "? SAO (Cat. ) number) "}, {"name": "RAh", "desc": "Right ascension (B1950) "}, {"name": "RAm", "desc": "Right ascension (B1950) "}, {"name": "RAs", "desc": "Right ascension (B1950) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) "}, {"name": "DEm", "desc": "Declination (B1950) "}, {"name": "DEs", "desc": "Declination (B1950) "}, {"name": "SpType", "desc": "Spectral type (HD) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "LRS", "desc": "[yes no] Low-resolution spectroscopy "}, {"name": "UBVbeta", "desc": "[yes no] UBV,H{beta} photometry "}, {"name": "vmag", "desc": "v magnitude "}, {"name": "b-y", "desc": "b-y colour index "}, {"name": "m1", "desc": "m1 colour index "}, {"name": "c1", "desc": "c1 colour index "}, {"name": "o_vmag", "desc": "Number of observations in uvby "}, {"name": "e_vmag", "desc": "rms uncertainty on uvby observations "}, {"name": "Hbeta", "desc": "H{beta} colour index "}, {"name": "o_Hbeta", "desc": "Number of observations in Hbeta "}, {"name": "e_Hbeta", "desc": "rms uncertainty on Hbeta "}, {"name": "Region", "desc": "Associated interstellar cloud (G1) "}]}, {"name": "table6.dat", "desc": "Photometric estimates of E(B-V) and distance ", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "SAO", "desc": "? SAO (Cat. ) number) "}, {"name": "Sys", "desc": "Photometric system used for the classification "}, {"name": "Hbeta", "desc": "H{beta} colour index "}, {"name": "Index", "desc": "Q (UBV) or [m1] (uvby) reddening-free index (1) "}, {"name": "sigma1", "desc": "Number of standard deviations for the star from the average relation in the H{beta},Q or H{beta},[m1] plane in the direction of H{beta}"}, {"name": "sigma2", "desc": "Number of standard deviations for the star from the average relation in the H{beta},Q or H{beta},[m1] plane in the direction of Q or [m1]"}, {"name": "(B-V)0", "desc": "? Dereddened B-V colour index "}, {"name": "VMAG", "desc": "? Absolute V magnitude "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "E(B-V)", "desc": "? Colour excess "}, {"name": "e_E(B-V)", "desc": "? rms uncertainty on E(B-V) "}, {"name": "Dist", "desc": "? Distance "}, {"name": "e_Dist", "desc": "? rms uncertainty on Dist "}, {"name": "Region", "desc": "Nearest interstellar cloud to the star (G1) "}]}, {"name": "table7b.dat", "desc": "Comparison of Michigan Spectral Catalog (MSC, ) spectral types with Digital Spectral Classification", "columns": [{"name": "HD", "desc": "HD (Cat. ) number "}, {"name": "SAO", "desc": "SAO (Cat. ) number) "}, {"name": "SpTypeM", "desc": "MSC spectral type "}, {"name": "(B-V)0M", "desc": "MSC dereddened B-V colour index "}, {"name": "(U-B)0M", "desc": "MSC dereddened U-B colour index "}, {"name": "VMAGM", "desc": "MSC absolute V magnitude "}, {"name": "SpType", "desc": "This work spectral type "}, {"name": "(B-V)0", "desc": "This work dereddened B-V colour index "}, {"name": "(U-B)0", "desc": "This work dereddened U-B colour index "}, {"name": "VMAG", "desc": "This work absolute V magnitude "}]}, {"name": "table8.dat", "desc": "Spectroscopic classification and estimates of E(B-V) and distance", "columns": [{"name": "HD", "desc": "? HD (Cat. ) number "}, {"name": "n_HD", "desc": "[#] Note on E(B-V) and distance determination (1) "}, {"name": "SAO", "desc": "? SAO (Cat. ) number) "}, {"name": "RAh", "desc": "Right ascension (B1950) "}, {"name": "RAm", "desc": "Right ascension (B1950) "}, {"name": "RAs", "desc": "Right ascension (B1950) "}, {"name": "DE-", "desc": "Declination sign (B1950) "}, {"name": "DEd", "desc": "Declination (B1950) "}, {"name": "DEm", "desc": "Declination (B1950) "}, {"name": "DEs", "desc": "Declination (B1950) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "Sys", "desc": "Photometric system used for the classification "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "(B-V)0", "desc": "Dereddened B-V colour index "}, {"name": "VMAG", "desc": "Absolute V magnitude "}, {"name": "B-V", "desc": "B-V colour index "}, {"name": "E(B-V)", "desc": "Colour excess (1) "}, {"name": "e_E(B-V)", "desc": "rms uncertainty on E(B-V) "}, {"name": "Dist", "desc": "Distance (1) "}, {"name": "e_Dist", "desc": "rms uncertainty on Dist "}, {"name": "Region", "desc": "Nearest interstellar cloud to the star (G1) "}]}, {"name": "table9.dat", "desc": "Summary of cloud distance and extinction estimates ", "columns": [{"name": "Cloud", "desc": "Cloud name "}, {"name": "Nobs", "desc": "Number of observations "}, {"name": "Dinf", "desc": "? Lower limit for distance "}, {"name": "---", "desc": "[<] "}, {"name": "---", "desc": "[d] "}, {"name": "---", "desc": "[<] "}, {"name": "Dsup", "desc": "? Upper limit for distance "}, {"name": "Av", "desc": "? Estimates of Av extinction, computed used an average value of R_V_=3.05"}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_87_197"}} {"id": "J/ApJS/87/197", "title_cds": "Carina OB2 association", "title_create": "Garcia+, 1993", "year": "1993", "author": "Garcia B.", "title_pub": "A study of Carina OB2 assciation. I. Observational data.", "first_author": "Garcia B.", "ref_biblio": [""], "bibcode": ["1993ApJS...87..197G"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191802"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_91_1"}} {"id": "J/ApJS/91/1", "title_cds": "Lyman-Alpha forest near 34 QSOs", "title_create": "Bechtold 1994", "year": "1994", "author": "Bechtold J.", "title_pub": "The Lyman-Alpha forest near 34 quasi-stellar objects with z > 2.6.", "first_author": "Bechtold J.", "ref_biblio": [""], "bibcode": ["1994ApJS...91....1B"], "see_also": ["http://lithops.as.arizona.edu/~jill/QuasarSpectra/MMT/ :"], "keyword_cds": "Spectra", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/191937"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_94_551"}} {"id": "J/ApJS/94/551", "title_cds": "The first EGRET catalog", "title_create": "Fichtel+ 1994", "year": "1994", "author": "Fichtel C.E., Bertsch D.L., Chiang J., Dingus B.L., Esposito J.A., Fierro J.M., Hartman R.C., Hunter S.D., Kanbach G., Kniffen D.A., Kwok P.W., Lin Y.C., Mattox J.R., Mayer-Hasselwander H.A., McDonald L., Michelson P.F., von Montigny C., Nolan P.L., Pinkau K., Radecke H.-D., Rothermel H., Sreekumar P., Sommer M., Schneid E.J., Thompson D.J., Willis T.", "title_pub": "The first energetic gamma-ray experiment telescope (EGRET) source catalog", "first_author": "Fichtel C.E.", "ref_biblio": [""], "bibcode": ["1994ApJS...94..551F\t(SIMBAD/NED"], "keyword_cds": "Gamma rays", "keyword_pub": "gamma rays: observations", "mission": "EGRET", "description": ["In this catalog the results related to high-energy gamma-ray sources", "obtained from the Energetic Gamma Ray Experiment Telescope (EGRET) on", "the Compton Gamma Ray Observatory are summarized for the period from", "1991 April 22 to 1992 November 17, called phase I. This phase of the", "Compton Observatory mission was devoted to an all-sky survey. Tables", "are included for the following EGRET results; solar flares with", "detected gamma radiation; pulsars; sources with |b|<10deg; gamma-ray", "bursts; normal galaxies; clusters of galaxies; positive detections of", "radio-loud quasars and BL Lac objects; marginal detections of", "radio-loud quasars and BL Lac objects; upper limits for radio-loud", "quasars and BL Lac objects; uppet limits for Seyfert galaxies and", "selected radio-quiet quasars, and other sources with |b|>+10deg in the", "Galactic Plane. There is also a table relating the dates of the", "observations to the Compton Observatory viewing period numbers to", "assist in referencing the observations."], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/192082"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_99_223"}} {"id": "J/ApJS/99/223", "title_cds": "IUE UV Observations of SN 1987A", "title_create": "Pun+ 1995", "year": "1995", "author": "Pun C.S.J., Kirshner R.P., Sonneborn G., Challis P., Nassiopoulos G., Arquilla R., Michael C.D., Shrader C., Teays T., Cassatella A., Gilmozzi R., Talavera A., Wamsteker W., Fransson C., Panagia N.", "title_pub": "Ultraviolet Observations of SN 1987A with the IUE Satellite", "first_author": "Pun C.S.J.", "ref_biblio": [""], "bibcode": ["1995ApJS...99..223P"], "keyword_cds": "Supernovae ; Spectra, ultraviolet", "keyword_pub": "ultraviolet: stars - stars: individual (SN 1987A)", "abstract": ["Ultraviolet (lambda: 1150-3300A) observations of SN 1987A with the", "IUE satellite provide a unique data set. Observations started the day", "after discovery, 1987 February 24 (day 1.6), and a total of 751", "spectra were obtained through 1992 June 9 (day 1567). The data have", "been processed to generate a complete catalog of SN 1987A ultraviolet", "spectra. The data reduction procedure includes careful line-by-line", "extraction, removing hits and hot pixels, and, most importantly, a", "scrupulous subtraction of the contribution from stars near SN 1987A", "within the IUE aperture. In addition to processing the data, we have", "also extracted light curves, and combined them with the ground-based", "optical data and HST observations (day 1278 to 2431) to extend the", "study in both wavelength and time. The data-processing procedures of", "our IUE study produce results that are consistent with the HST data", "where they overlap, but not with the IUE study by Sanz Fernandez de", "Cordoba (1993A&A...276..103S) because of its incorrect background", "subtraction. The IUE data are consistent with the ground-based", "Walraven VBLUW photometry, while we found that flux scale of the", "Soviet ASTRON satellite spectroscopic data is low by ~15%. The UV flux", "plummeted during the earliest days of observations because of the drop", "in the photospheric temperature and the increase in opacity. However,", "after reaching a minimum of 0.04% on day 44, the UV flux increased by", "175 times in its contribution to 7% of the total UVOIR bolometric", "luminosity at day 800. A revised set of bolometric data has been", "constructed which includes the contribution of UV from day 1 to day", "1352. Studies of the UV colors show that the supernova started to get", "bluer in UV around the time when dust started to form in the ejecta.", "Our results are consistent with the possibility that the dust", "condensed may be metal-rich."], "description": ["The data for this paper were supplied in five UNIX tar files", "containing the FITS images for (1) the IUE LWP background, (2) LWP", "data, (3) SWP background, (4) SWP data, and (5) optical observations.", "Tables 2(a), 2(b), 3(a), and 3(b) containing the journal of IUE", "observations were also included. The FITS files contained in the tar", "files had names such as 'lwp.18792.bgd.fits'. These names are not", "compatible with the ISO 9660 CD-ROM file system standard. The files", "were renamed first by placing each of the files from the five tar", "files into their own subdirectory, e.g. 'lwpbgd', and renaming the", "files to ISO 9660-style names, e.g. 'l18792.fit'. The tables", "containing the journals of observations include the new file names so", "that the user can correlate the FITS files to the proper observations.", "The author-supplied README file has been included to provide further", "explanations of the data."], "doi_pub": ["10.1086/192185"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "readme.dat", "desc": "Author-supplied description of data files ", "columns": []}, {"name": "table2a.dat", "desc": "Journal of observations: swpbgd FITS files ", "columns": [{"name": "File", "desc": "Name of FITS file in swpbgd directory "}, {"name": "CAM", "desc": "IUE camera, always SWP "}, {"name": "IMG", "desc": "IUE image number "}, {"name": "Date", "desc": "Date of observation "}, {"name": "Day", "desc": "Day number of SN 1987A "}, {"name": "Exp", "desc": "Exposure time. Trailing 's' for sec, 'm' for min"}]}, {"name": "table2b.dat", "desc": "Journal of observations: lwpbgd FITS files ", "columns": [{"name": "File", "desc": "Name of FITS file in lwpbgd directory "}, {"name": "CAM", "desc": "IUE camera, always LWP "}, {"name": "IMG", "desc": "IUE image number "}, {"name": "Date", "desc": "Date of observation "}, {"name": "Day", "desc": "Day number of SN 1987A "}, {"name": "Exp", "desc": "Exposure time. Trailing 's' for sec, 'm' for min"}]}, {"name": "table3a.dat", "desc": "Journal of observations: swpdata FITS files ", "columns": [{"name": "File", "desc": "*Name of FITS file in swpdata directory "}, {"name": "CAM", "desc": "IUE camera, always SWP "}, {"name": "IMG", "desc": "IUE image number "}, {"name": "n_IMG", "desc": "[*] "}, {"name": "Date", "desc": "Date of observation "}, {"name": "Day", "desc": "[]? Day number of SN 1987A "}, {"name": "Exp", "desc": "Exposure time. Trailing 's' for sec, 'm' for min"}]}, {"name": "table3b.dat", "desc": "Journal of observations: lwpdata FITS files ", "columns": [{"name": "File", "desc": "*Name of FITS file in lwpdata directory "}, {"name": "CAM", "desc": "IUE camera, always LWP "}, {"name": "IMG", "desc": "*IUE image number "}, {"name": "n_IMG", "desc": "[*] "}, {"name": "Date", "desc": "Date of observation "}, {"name": "Day", "desc": "[]? Day number of SN 1987A "}, {"name": "Exp", "desc": "Exposure time. Trailing 's' for sec, 'm' for min"}]}, {"name": "swpbgd/*", "desc": "Short wavelength spectra (1150 - 1975 A) averaged for background subtraction", "columns": []}, {"name": "lwpbgd/*", "desc": "Long wavelength spectra (1975 - 3300 A) averaged for background subtraction", "columns": []}, {"name": "swpdat/*", "desc": "IUE SWP camera (1150 - 1975 A) observations of SN 1987A", "columns": []}, {"name": "lwpdat/*", "desc": "IUE LWP camera (1975 - 3300 A) observations of SN 1987A", "columns": []}, {"name": "optfit/*", "desc": "Combined IUE and CTIO spectra of SN 1987A ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_99_693"}} {"id": "J/ApJS/99/693", "title_cds": "Observations of double stars. XVI.", "title_create": "Heintz 1995", "year": "1995", "author": "Heintz W.D.", "title_pub": "Observations of double stars and new pairs. XVI. Results in 1992-1994.", "first_author": "Heintz W.D.", "ref_biblio": [""], "bibcode": ["1995ApJS...99..693H"], "see_also": ["J/AJ/108/2338 : Photographic astrometry. VIII. (Heintz 1994)", "J/ApJS/74/275 : Observations of double stars. XIV. (Heintz 1990)", "J/ApJS/83/351 : Observations of double stars. XV. (Heintz 1992)", "J/ApJS/105/475 : Observations of double stars. XVII. (Heintz 1996)", "J/ApJS/117/587 : Observations of double stars. XVIII. (Heintz 1998)"], "keyword_cds": "Stars, double and multiple", "keyword_pub": "binaries: visual", "abstract": ["Visual and photographic measures listed for 730 pairs were obtained in", "the time 1992.2-1994.9. Tables and notes include corrections to", "catalog positions and some revised orbits."], "doi_pub": ["10.1086/192202"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1", "desc": "New pairs ", "columns": [{"name": "Hei", "desc": "Heintz number "}, {"name": "RAh1", "desc": "Right ascension (1900) "}, {"name": "RAdm1", "desc": "Right ascension (1900) "}, {"name": "DE-1", "desc": "Declination sign "}, {"name": "DEd1", "desc": "Declination (1900) "}, {"name": "DEm1", "desc": "Declination (1900) "}, {"name": "RAh2", "desc": "Right ascension (2000) "}, {"name": "RAdm2", "desc": "Right ascension (2000) "}, {"name": "DE-2", "desc": "Declination sign "}, {"name": "DEd2", "desc": "Declination (2000) "}, {"name": "DEm2", "desc": "Declination (2000) "}, {"name": "BD", "desc": "BD (Cat. ) number "}, {"name": "Com", "desc": "Comment "}]}, {"name": "table2", "desc": "Micrometer observations ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "RAh", "desc": "Right ascension (2000) "}, {"name": "RAdm", "desc": "Right ascension (2000) (deci-minutes) "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (2000) "}, {"name": "DEm", "desc": "Declination (2000) "}, {"name": "Ep-1990", "desc": "Epoch of observation 1990+ "}, {"name": "PA", "desc": "? Position angle "}, {"name": "n_PA", "desc": "[rs:] r: round; s: single; : uncertain value "}, {"name": "Sep", "desc": "? Separation between the components "}, {"name": "u_Sep", "desc": "Uncertainty flag on Sep "}, {"name": "Nobs", "desc": "? Number of nights "}, {"name": "Comp", "desc": "[ABCa -] Components for multiple systems "}, {"name": "m1", "desc": "? Magnitude of brightest component "}, {"name": "m2", "desc": "? Magnitude of second brightest component "}]}, {"name": "table3", "desc": "Measures on astronomic plates ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "m1", "desc": "? Magnitude of brightest component "}, {"name": "m2", "desc": "? Magnitude of second brightest component "}, {"name": "RAh", "desc": "Right ascension (2000) "}, {"name": "RAdm", "desc": "Right ascension (2000) (deci-minutes) "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (2000) "}, {"name": "DEm", "desc": "Declination (2000) "}, {"name": "Ep-1900", "desc": "Epoch of observation 1900+ "}, {"name": "PA", "desc": "Position angle "}, {"name": "Sep", "desc": "Separation between the components "}, {"name": "Nobs", "desc": "? Number of nights "}, {"name": "Nexp", "desc": "Measured exposures "}]}, {"name": "table4", "desc": "Orbits ", "columns": [{"name": "RAh", "desc": "Right ascension (2000) "}, {"name": "RAdm", "desc": "Right ascension (2000) "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "DEclination (2000) "}, {"name": "DEm", "desc": "DEclination (2000) "}, {"name": "ADS", "desc": "? ADS number "}, {"name": "Name", "desc": "Star name "}, {"name": "mag1", "desc": "Visual magnitude of the primary "}, {"name": "mmag2", "desc": "Visual magnitude of the secondary "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "Per", "desc": "Period "}, {"name": "n", "desc": "Yearly motion "}, {"name": "T", "desc": "Time of the perihelion passage "}, {"name": "a", "desc": "Semi-major axis "}, {"name": "e", "desc": "Eccentricity "}, {"name": "i", "desc": "Inclination angle "}, {"name": "omega", "desc": "Longitude of the perihelion "}, {"name": "OMEGA", "desc": "Longitude of the ascensing node "}, {"name": "plx", "desc": "? Dynamical parallax "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_244_18"}} {"id": "J/ApJS/244/18", "title_cds": "Kepler Smear Campaign: LCs & sp of very bright stars", "title_create": "Pope+, 2019", "year": "2019", "author": "Pope B.J.S., Davies G.R., Hawkins K., White T.R., Stokholm A., Bieryla A., Latham D.W., Lucey M., Aerts C., Aigrain S., Antoci V., Bedding T.R., Bowman D.M., Caldwell D.A., Chontos A., Esquerdo G.A., Huber D., Jofre P., Murphy S.J., van Reeth T., Silva Aguirre V., Yu J.", "title_pub": "The Kepler Smear Campaign: light curves for 102 very bright stars.", "first_author": "Pope B.J.S.", "ref_biblio": [""], "bibcode": ["2019ApJS..244...18P"], "see_also": ["I/311 : Hipparcos, the New Reduction (van Leeuwen, 2007)", "V/133 : Kepler Input Catalog (Kepler, 2009)", "I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/A+A/275/101 : Chemical evolution of the gal. disk I. (Edvardsson+ 1993)", "J/MNRAS/389/869 : Multiplicity among bright stellar systems (Eggleton+, 2008)", "J/AJ/142/112 : KIC photometric calibration (Brown+, 2011)", "J/A+A/545/A32 : Chemical abundances of 1111 FGK stars (Adibekyan+, 2012)", "J/other/Nat/486.375 : Stellar parameters of KOI stars (Buchhave+, 2012)", "J/PASP/124/1279 : Q3 Kepler's combined photometry (Christiansen+, 2012)", "J/A+A/540/A143 : Oscillations of red giants with Kepler (Mosser+, 2012)", "J/MNRAS/431/2240 : Activity in A-type stars from Kepler (Balona, 2013)", "J/ApJ/767/127 : Asteroseismic solutions for 77 Kepler stars (Huber+, 2013)", "J/MNRAS/441/3543 : Possible planets around A stars (Balona, 2014)", "J/A+A/562/A71 : Abundances of solar neighbourhood dwarfs (Bensby+, 2014)", "J/A+A/566/A98 : The Gaia Benchmark Stars - Library (Blanco-Cuaresma+, 2014)", "J/AJ/148/54 : The Hypatia Catalog ((Hinkel+, 2014)", "J/A+A/564/A133 : Gaia FGK benchmark stars: metallicity (Jofre+, 2014)", "J/A+A/571/A47 : Extensive linelist of CH in stellar atm. (Masseron+, 2014)", "J/A+A/572/L5 : Red giant evolution states from seismology (Mosser+, 2014)", "J/ApJS/215/19 : APOKASC catalog of Kepler red giants (Pinsonneault+, 2014)", "J/A+A/577/A9 : Sc, V, Mn, and Co in Milky Way stars (Battistini+, 2015)", "J/A+A/575/A26 : Properties of the Pop. II star HD 140283 (Creevey+, 2015)", "J/A+A/582/A81 : Gaia FGK benchmark stars: abundances (Jofre+, 2015)", "J/MNRAS/452/2127 : Fundamental param. of Kepler stars (Silva Aguirre+, 2015)", "J/AJ/151/101 : Kepler Mission. VIII. False positives (Abdul-Masih+, 2016)", "J/A+A/586/A49 : r- & s- process elements in MW disk (Battistini+, 2016)", "J/MNRAS/460/1970 : Kepler {delta}Sct stars amplitude modulation (Bowman+, 2016)", "J/ApJ/829/23 : Stellar flares from Q0-Q17 Kepler LCs (Davenport, 2016)", "J/A+A/592/A70 : Gaia FGK stars: low-metallicities cand. (Hawkins+, 2016)", "J/A+A/594/A43 : APOGEE/Kepler sample stars abundances (Hawkins+, 2016)", "J/MNRAS/467/1830 : Starspots on A stars (Balona, 2017)", "J/ApJ/844/102 : KIC star plx from asteroseismology vs Gaia (Huber+, 2017)", "J/ApJ/835/172 : Kepler asteroseismic LEGACY sample. I. (Lund+, 2017)", "J/MNRAS/471/770 : Parameters & IR excesses of Gaia DR1 stars (McDonald+, 2017)", "J/ApJS/233/23 : APOKASC cat. of KIC dwarfs and subgiants (Serenelli+, 2017)", "J/ApJ/835/173 : Kepler asteroseism. LEGACY sample II. (Silva Aguirre+, 2017)", "J/MNRAS/474/4322 : Orbital parameters of 341 new binaries (Murphy+, 2018)", "J/A+A/609/A116 : Low extinction TGAS HR Catalogue (Ruiz-Dern+, 2018)", "http://gaia-kepler.fun/ : Gaia and Kepler/K2 cross-matched catalogs webpage", "http://archive.stsci.edu/kepler/data_search/search.php : Kepler data on MAST"], "keyword_cds": "Asteroseismology; Stars, giant; Stars, variable; Radial velocities Abundances; Photometry; Spectra, optical; Rotational velocities Stars, masses", "keyword_pub": "asteroseismology ; stars: early-type ; stars: rotation ; stars: variables: general ; techniques: photometric", "abstract": ["We present the first data release of the Kepler Smear Campaign, using", "collateral \"smear\" data obtained in the Kepler four-year mission to", "reconstruct light curves of 102 stars too bright to have been", "otherwise targeted. We describe the pipeline developed to extract and", "calibrate these light curves and show that we attain photometric", "precision comparable to stars analyzed by the standard pipeline in the", "nominal Kepler mission. In this paper, aside from publishing the light", "curves of these stars, we focus on 66 red giants for which we detect", "solar-like oscillations, characterizing 33 of these in detail with", "spectroscopic chemical abundances and asteroseismic masses as", "benchmark stars. We also classify the whole sample, finding nearly all", "to be variable, with classical pulsations and binary effects."], "description": ["We selected all stars on silicon in Kepler with Kp<9 that were", "targeted for fewer than eight quarters. The full sample of stars is", "listed in Table 1.", "The Kepler spacecraft rotates between quarters, so that it cycles", "through four orientation \"seasons\" each rotated from the last by 90{deg}.", "When generating light curves of the Kepler smear stars, we followed", "the methods described by Pope+ (2016MNRAS.455L..36P), with some", "improvements. See section 2.2 for further explanations.", "We have obtained high-resolution spectroscopy with the Tillinghast", "Reflector Echelle Spectrograph (TRES) for 63 stars, mainly giants, in", "order to constrain stellar parameters and elemental abundances.", "Operating with a spectral resolving power of R=44000, we have obtained", "spectra with a mean S/N of ~100 per resolution element."], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/ab2c04"], "orcid_pub": ["0000-0003-2595-9114"], "data": "", "date_update": "19-Feb-2020", "tables": [{"name": "table1.dat", "desc": "Input catalog ", "columns": [{"name": "Name", "desc": "Identifier "}, {"name": "m_Name", "desc": "Component identifier for HD 189636 "}, {"name": "SpType", "desc": "SIMBAD spectral type if available "}, {"name": "[Fe/H]", "desc": "[-0.6/1.4]? Metallicity "}, {"name": "theta", "desc": "[0.226/3.429]? Estimated angular size for interferometric scheduling"}, {"name": "Obs", "desc": "Observing comment "}, {"name": "Sea", "desc": "[1/4] Season observed "}, {"name": "Teff", "desc": "[3676/9887]? Effective temperature "}, {"name": "log(g)", "desc": "[1.4/4.4]? log surface gravity "}, {"name": "E(B-V)", "desc": "[0.01/0.09]? The (B-V) color excess "}, {"name": "gmag", "desc": "[5.3/10.5] Apparent SDSS g band magnitude "}, {"name": "rmag", "desc": "[5/9] Apparent SDSS r band magnitude "}, {"name": "Jmag", "desc": "[1.8/8.3] Apparent 2MASS J band magnitude "}, {"name": "kpmag", "desc": "[5/8.7] Apparent Kepler magnitude "}, {"name": "Edge", "desc": "[0/458]? Distance from edge of Kepler chip "}, {"name": "Note", "desc": "Additional notes "}, {"name": "IF?", "desc": "Interferometry available? "}, {"name": "TRES?", "desc": "TRES data available? "}, {"name": "RAdeg", "desc": "[281.2/300.5] Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[37/51.4] Declination (J2000) "}, {"name": "KIC", "desc": "[1572070/12456737] Kepler identifier "}, {"name": "Class", "desc": "Variability classification (1) "}, {"name": "rEst", "desc": "[41/1867]? Estimated radius from KIC "}, {"name": "b_rEst", "desc": "[41/1746]? Lower boundary on rEst "}, {"name": "B_rEst", "desc": "[41/2005]? Upper boundary on rEst "}, {"name": "RAIdeg", "desc": "Input Right Ascension (J2000) "}, {"name": "DEIdeg", "desc": "Input Declination (J2000) "}, {"name": "Sep", "desc": "[3e-7/0.0007] Distance "}, {"name": "---", "desc": "[Gaia DR2] "}, {"name": "Gaia", "desc": "Gaia DR2 designation "}, {"name": "RAGdeg", "desc": "Gaia DR2 Right Ascension (J2000) "}, {"name": "DEGdeg", "desc": "Gaia DR2 Declination (J2000) "}, {"name": "GLON", "desc": "[68.8/84] Galactic longitude "}, {"name": "GLAT", "desc": "[5.9/20] Galactic latitude "}, {"name": "ELON", "desc": "[290/323.7] Ecliptic longitude "}, {"name": "ELAT", "desc": "[57.9/72] Ecliptic latitude "}, {"name": "plx", "desc": "[0.5/24.3]? Gaia parallax "}, {"name": "pmRA", "desc": "[-94.7/84.4]? Proper motion along RA "}, {"name": "pmDE", "desc": "[-104.8/120.3]? Proper motion along DE "}, {"name": "Gmag", "desc": "[4.8/8.7] Mean Gaia DR2 magnitude "}, {"name": "bpmag", "desc": "[5/9.3] Mean Gaia DR2 blue passband magnitude"}, {"name": "rpmag", "desc": "[4/8.2] Mean Gaia DR2 red passband magnitude"}, {"name": "e_RAGdeg", "desc": "[0.01/1] Uncertainty in RAGdeg "}, {"name": "e_DEGdeg", "desc": "[0.02/1] Uncertainty in DEGdeg "}, {"name": "e_plx", "desc": "[0.01/0.4]? Uncertainty in plx "}, {"name": "e_pmRA", "desc": "[0.03/0.7]? Uncertainty in pmRA "}, {"name": "e_pmDE", "desc": "[0.03/0.7]? Uncertainty in pmDE "}, {"name": "E_Gmag", "desc": "[0/1.3]? Upper percentile uncertainty in Gmag"}, {"name": "e_Gmag", "desc": "[0.07/2.5]? Lower percentile uncertainty in Gmag"}, {"name": "FileName", "desc": "Name of the FITS file in subdirectory Sp; column added by CDS"}, {"name": "m_FileName", "desc": "? Number indicating the number of spectra available in the subdirectory Sp for this star; column added by CDS"}]}, {"name": "table2.dat", "desc": "Global asteroseismic parameters for the red giant sample as discussed in Section 2.3", "columns": [{"name": "Name", "desc": "Object identifier "}, {"name": "Delnu", "desc": "[0.37/5.94] Mean large spacing {Delta}{nu} "}, {"name": "e_Delnu", "desc": "[0.004/0.06] Uncertainty in Delnu "}, {"name": "numax", "desc": "[1.5/70] Asteroseismic frequency at maximum amplitude {nu}_max_"}, {"name": "e_numax", "desc": "[0.03/1.1] Uncertainty in numax "}, {"name": "eps", "desc": "[0.6/1.1] Asteroseismic parameter {epsilon} "}, {"name": "e_eps", "desc": "[0.01/0.4] Uncertainty in epsilon "}]}, {"name": "table3.dat", "desc": "Fundamental stellar parameters for the red giant sample as determined jointly by asteroseismology and spectroscopy", "columns": [{"name": "Name", "desc": "Object identifier "}, {"name": "BJD", "desc": "Barycentric Julian Date; TDB "}, {"name": "RVel", "desc": "[-80.4/31] Radial velocity "}, {"name": "e_RVel", "desc": "[0.01/0.2] Uncertainty in RVel "}, {"name": "Teff", "desc": "[3556/5090] Effective temperature "}, {"name": "e_Teff", "desc": "[50] Uncertainty in Teff "}, {"name": "log(g)a", "desc": "[1/2.8] log surface gravity from asteroseismology"}, {"name": "e_log(g)a", "desc": "[0.1] Uncertainty in log(g)a "}, {"name": "[M/H]", "desc": "[-1.7/0.2] Metallicity "}, {"name": "e_[M/H]", "desc": "[0.08] Uncertainty in [M/H] "}, {"name": "Vsin(i)", "desc": "[3.5/11] Projected rotational velocity "}, {"name": "e_Vsin(i)", "desc": "[0.5] Uncertainty in Vsin(i) "}, {"name": "CCF", "desc": "[0.9/1.1] Unknown "}, {"name": "SNRe", "desc": "[31.7/187.2] Unknown "}, {"name": "nAps", "desc": "[3] Unknown (always = 3) "}, {"name": "Exp", "desc": "[45/360] Exposure time "}, {"name": "Spec", "desc": "Spectrograph used; always \"tres\" "}, {"name": "Res", "desc": "Spectrograph resolution "}, {"name": "Version", "desc": "Method used in reduction (always \"SPC2.9\"); the Stellar Parameter Classification code (SPC; Buchhave+ 2012, J/other/Nat/486.375)"}, {"name": "numax", "desc": "[1.5/69.8] Asteroseismic parameter {nu}_max_ (1)"}, {"name": "e_numax", "desc": "[0.03/1.1] Uncertainty in numax "}, {"name": "log(g)", "desc": "[1/2.8] log surface gravity "}, {"name": "e_log(g)", "desc": "[0.003/0.02] Uncertainty in log(g) "}, {"name": "Mass", "desc": "[0.7/3.4] Mass "}, {"name": "E_Mass", "desc": "[0.02/0.3] Upper uncertainty in Mass "}, {"name": "e_Mass", "desc": "[0.007/0.2] Lower uncertainty in Mass "}, {"name": "Rad", "desc": "[9.6/48.6] Radius "}, {"name": "E_Rad", "desc": "[0.02/2] Upper uncertainty in Rad "}, {"name": "e_Rad", "desc": "[0.03/2] Lower uncertainty in Rad "}, {"name": "log(g)s", "desc": "[1/2.8] log surface gravity from spectroscopy "}, {"name": "E_log(g)s", "desc": "[0.001/0.02] Upper uncertainty in log(g)s "}, {"name": "e_log(g)s", "desc": "[0.001/0.02] Lower uncertainty in log(g)s "}, {"name": "logAge", "desc": "[0.2/16] log age "}, {"name": "E_logAge", "desc": "[0.02/3.6] Upper uncertainty in logAge "}, {"name": "e_logAge", "desc": "[0/4] Lower uncertainty in logAge "}]}, {"name": "table4.dat", "desc": "Chemical abundances relative to iron for stars in the red giant sample as determined by BACCHUS, differential line-by-line comparison to Arcturus, as described in Section 2.4", "columns": [{"name": "Name", "desc": "Object identifier "}, {"name": "[O/Fe]", "desc": "?=-9.999 log O/Fe abundance ratio (always blank) (1)"}, {"name": "e_[O/Fe]", "desc": "?=-9.999 Uncertainty in [O/Fe] (always blank) (1)"}, {"name": "[Mg/Fe]", "desc": "[0.03/0.4]?=-9.999 log Mg/Fe abundance ratio (1) "}, {"name": "e_[Mg/Fe]", "desc": "[0.007/0.2]?=-9.999 Uncertainty in [Mg/Fe] (1) "}, {"name": "[Ca/Fe]", "desc": "[-0.3/0.1]?=-9.999 log Ca/Fe abundance ratio (1) "}, {"name": "e_[Ca/Fe]", "desc": "[0.001/0.07]?=-9.999 Uncertainty in [Ca/Fe] (1) "}, {"name": "[Si/Fe]", "desc": "[-0.0041/0.4]?=-9.999 log Si/Fe abundance ratio (1)"}, {"name": "e_[Si/Fe]", "desc": "[0.008/0.3]?=-9.999 Uncertainty in [Si/Fe] (1) "}, {"name": "[Ti/Fe]", "desc": "[-0.3/0.4]?=-9.999 log Ti/Fe abundance ratio (1) "}, {"name": "e_[Ti/Fe]", "desc": "[0.006/0.1]?=-9.999 Uncertainty in [Ti/Fe] (1) "}, {"name": "[Al/Fe]", "desc": "[0.04/0.3]?=-9.999 log Al/Fe abundance ratio (1) "}, {"name": "e_[Al/Fe]", "desc": "[0.0003/0.1]?=-9.999 Uncertainty in [Al/Fe] (1) "}, {"name": "[Ni/Fe]", "desc": "[-0.3/0.3]?=-9.999 log Ni/Fe abundance ratio (1) "}, {"name": "e_[Ni/Fe]", "desc": "[0.01/0.3]?=-9.999 Uncertainty in [Ni/Fe] (1) "}, {"name": "[Na/Fe]", "desc": "?=-9.999 log Na/Fe abundance ratio (always blank) (1)"}, {"name": "e_[Na/Fe]", "desc": "?=-9.999 Uncertainty in [Na/Fe] (always blank) (1)"}, {"name": "[Mn/Fe]", "desc": "[-0.2/0.3]?=-9.999 log Mn/Fe abundance ratio (1) "}, {"name": "e_[Mn/Fe]", "desc": "[0.02/0.1]?=-9.999 Uncertainty in [Mn/Fe] (1) "}, {"name": "[Cr/Fe]", "desc": "[-0.4/0.2]?=-9.999 log Cr/Fe abundance ratio (1) "}, {"name": "e_[Cr/Fe]", "desc": "[0.0003/0.2]?=-9.999 Uncertainty in [Cr/Fe] (1) "}, {"name": "[Co/Fe]", "desc": "[-0.3/0.2]?=-9.999 log Co/Fe abundance ratio (1) "}, {"name": "e_[Co/Fe]", "desc": "[0.007/0.2]?=-9.999 Uncertainty in [Co/Fe] (1) "}, {"name": "[V/Fe]", "desc": "[-0.2/0.4]?=-9.999 log V/Fe abundance ratio (1) "}, {"name": "e_[V/Fe]", "desc": "[0.002/0.1]?=-9.999 Uncertainty in [V/Fe] (1) "}, {"name": "[Cu/Fe]", "desc": "[-0.8/0.08]?=-9.999 log Cu/Fe abundance ratio (1) "}, {"name": "e_[Cu/Fe]", "desc": "[0.0007/0.2]?=-9.999 Uncertainty in [Cu/Fe] (1) "}]}, {"name": "table5.dat", "desc": "Chemical abundances relative to iron of neutron capture elements for stars in the red giant sample as determined by BACCHUS, without differential line-by-line comparison to Arcturus, as described in Section 2.4", "columns": [{"name": "Name", "desc": "Object identifier "}, {"name": "[Mg/Fe]", "desc": "[0.02/0.5]?=-9.999 log Mg/Fe abundance ratio (1) "}, {"name": "e_[Mg/Fe]", "desc": "[0.01/0.2]?=-9.999 Uncertainty in [Mg/Fe] (1) "}, {"name": "[Si/Fe]", "desc": "[-0.1/0.4]?=-9.999 log Si/Fe abundance ratio (1) "}, {"name": "e_[Si/Fe]", "desc": "[0.01/0.2]?=-9.999 Uncertainty in [Si/Fe] (1) "}, {"name": "[Ca/Fe]", "desc": "[-0.2/0.2]?=-9.999 log Ca/Fe abundance ratio (1) "}, {"name": "e_[Ca/Fe]", "desc": "[0/0.09]?=-9.999 Uncertainty in [Ca/Fe] (1) "}, {"name": "[Ti/Fe]", "desc": "[-0.2/0.2]?=-9.999 log Ti/Fe abundance ratio (1) "}, {"name": "e_[Ti/Fe]", "desc": "[0.001/0.2]?=-9.999 Uncertainty in [Ti/Fe] (1) "}, {"name": "[Mn/Fe]", "desc": "[-0.7/-0.05]?=-9.999 log Mn/Fe abundance ratio (1)"}, {"name": "e_[Mn/Fe]", "desc": "[0.002/0.2]?=-9.999 Uncertainty in [Mn/Fe] (1) "}, {"name": "[Co/Fe]", "desc": "[-0.3/0.2]?=-9.999 log Co/Fe abundance ratio (1) "}, {"name": "e_[Co/Fe]", "desc": "[0.01/0.2]?=-9.999 Uncertainty in [Co/Fe] (1) "}, {"name": "[O/Fe]", "desc": "[0.2/0.4]?=-9.999 log O/Fe abundance ratio (1) "}, {"name": "e_[O/Fe]", "desc": "[0.02/0.1]?=-9.999 Uncertainty in [O/Fe] (1) "}, {"name": "[Li/Fe]", "desc": "[-0.7/0.03]?=-9.999 log Li/Fe abundance ratio (1) "}, {"name": "e_[Li/Fe]", "desc": "[0.1]?=-9.999 Uncertainty in [Li/Fe] (1) "}, {"name": "[Cr/Fe]", "desc": "[-0.5/0.03]?=-9.999 log Cr/Fe abundance ratio (1) "}, {"name": "e_[Cr/Fe]", "desc": "[0.006/0.3]?=-9.999 Uncertainty in [Cr/Fe] (1) "}, {"name": "[Cu/Fe]", "desc": "[-0.4/0.4]?=-9.999 log Cu/Fe abundance ratio (1) "}, {"name": "e_[Cu/Fe]", "desc": "[0.02/0.3]?=-9.999 Uncertainty in [Cu/Fe] (1) "}, {"name": "[La/Fe]", "desc": "[-0.4/0.3]?=-9.999 log La/Fe abundance ratio (1) "}, {"name": "e_[La/Fe]", "desc": "[0.006/0.3]?=-9.999 Uncertainty in [La/Fe] (1) "}, {"name": "[Al/Fe]", "desc": "[0.1/0.4]?=-9.999 log Al/Fe abundance ratio (1) "}, {"name": "e_[Al/Fe]", "desc": "[0.004/0.2]?=-9.999 Uncertainty in [Al/Fe] (1) "}, {"name": "[Na/Fe]", "desc": "[-0.5/0.4]?=-9.999 log Na/Fe abundance ratio (1) "}, {"name": "e_[Na/Fe]", "desc": "[0.001/0.2]?=-9.999 Uncertainty in [Na/Fe] (1) "}, {"name": "[Ni/Fe]", "desc": "[-0.08/0.3]?=-9.999 log Ni/Fe abundance ratio (1) "}, {"name": "e_[Ni/Fe]", "desc": "[0.02/0.3]?=-9.999 Uncertainty in [Ni/Fe] (1) "}, {"name": "[Ba/Fe]", "desc": "[-0.05/0.6]?=-9.999 log Ba/Fe abundance ratio (1) "}, {"name": "e_[Ba/Fe]", "desc": "[0.1]?=-9.999 Uncertainty in [Ba/Fe] (1) "}, {"name": "[Sr/Fe]", "desc": "[-0.5/0.3]?=-9.999 log Sr/Fe abundance ratio (1) "}, {"name": "e_[Sr/Fe]", "desc": "[0.01/0.3]?=-9.999 Uncertainty in [Sr/Fe] (1) "}, {"name": "[Y/Fe]", "desc": "[-0.5/-0.05]?=-9.999 log Y/Fe abundance ratio (1) "}, {"name": "e_[Y/Fe]", "desc": "[0.006/0.3]?=-9.999 Uncertainty in [Y/Fe] (1) "}, {"name": "[Eu/Fe]", "desc": "[-0.09/0.3]?=-9.999 log Eu/Fe abundance ratio (1) "}, {"name": "e_[Eu/Fe]", "desc": "[0.1]?=-9.999 Uncertainty in [Eu/Fe] (1) "}, {"name": "[V/Fe]", "desc": "[-0.3/0.3]?=-9.999 log V/Fe abundance ratio (1) "}, {"name": "e_[V/Fe]", "desc": "[0.01/0.2]?=-9.999 Uncertainty in [V/Fe] (1) "}, {"name": "[Sc/Fe]", "desc": "[-0.05/0.2]?=-9.999 log Sc/Fe abundance ratio (1) "}, {"name": "e_[Sc/Fe]", "desc": "[0.03/0.2]?=-9.999 Uncertainty in [Sc/Fe] (1) "}, {"name": "[Zr/Fe]", "desc": "[-0.5/0.4]?=-9.999 log Zr/Fe abundance ratio (1) "}, {"name": "e_[Zr/Fe]", "desc": "[0.02/0.3]?=-9.999 Uncertainty in [Zr/Fe] (1) "}, {"name": "[Nd/Fe]", "desc": "[-0.7/0.2]?=-9.999 log Nd/Fe abundance ratio (1) "}, {"name": "e_[Nd/Fe]", "desc": "[0.02/0.3]?=-9.999 Uncertainty in [Nd/Fe] (1) "}]}, {"name": "lcs/*", "desc": "Individual light curves from the Kepler Smear Campaign in CSV format", "columns": []}, {"name": "sp/*", "desc": "Raw data of all spectra in FITS format ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_244_24"}} {"id": "J/ApJS/244/24", "title_cds": "A z=0 Multiwavelength Galaxy Synthesis. I.", "title_create": "Leroy+, 2019", "year": "2019", "author": "Leroy A.K., Sandstrom K.M., Lang D., Lewis A., Salim S., Behrens E.A., Chastenet J., Chiang I.-D., Gallagher M.J., Kessler S., Utomo D.", "title_pub": "A z=0 Multiwavelength Galaxy Synthesis. I. A WISE and GALEX atlas of local galaxies.", "first_author": "Leroy A.K.", "ref_biblio": [""], "bibcode": ["2019ApJS..244...24L"], "see_also": ["VII/237 : HYPERLEDA. I. Catalog of galaxies (Paturel+, 2003)", "VII/238 : HYPERLEDA. II. Homogenized HI data (Paturel+, 2003)", "VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "J/ApJS/173/185 : GALEX ultraviolet atlas of nearby galaxies (Gil de Paz+, 2007)", "J/ApJ/671/333 : Aperture photometry in NGC 5194 (Kennicutt+, 2007)", "J/ApJS/173/572 : GALEX/Spitzer photometry in NGC 7331 (Thilker+, 2007)", "J/AJ/136/2563 : HI Nearby Galaxy Survey, THINGS (Walter+, 2008)", "J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008)", "J/ApJ/703/517 : The Spitzer Local Volume Legacy: IR photometry (Dale+, 2009)", "J/ApJ/706/599 : H{alpha} and UV SFR in the local volume (Lee+, 2009)", "J/PASP/122/261 : Herschel Reference Survey Sample (Boselli+, 2010)", "J/ApJ/714/1256 : Far-IR star formation rate indicators (Calzetti+, 2010)", "J/PASP/122/1397 : Spitzer Survey of Stellar Structure in Gal. (Sheth+, 2010)", "J/PASP/123/1011 : Star Formation Reference Survey (SFRS) (Ashby+, 2011)", "J/ApJ/777/42 : Kinematic and HI data for the NFGS (Kannappan+, 2013)", "J/A+A/582/A121 : Dust properties in galaxies (Remy-Ruyer+, 2015)", "J/AJ/152/50 : Cosmicflows-3 catalog (CF3) (Tully+, 2016)", "J/ApJS/234/18 : GALEX/S4G surface brightness profiles. I. (Bouquin+, 2018)", "J/A+A/609/A37 : 875 nearby galaxies multiwavelength photometry (Clark+, 2018)", "J/A+A/622/A103 : Python Code Investigating GALaxy Emission (Boquien+, 2019)"], "keyword_cds": "Galaxy catalogs; Infrared sources; Ultraviolet", "keyword_pub": "galaxies: general; galaxies: ISM; galaxies: spiral galaxies: star formation; infrared: galaxies; ultraviolet: galaxies", "abstract": ["We present an atlas of ultraviolet and infrared images of ~15750 local", "(d<~50Mpc) galaxies, as observed by NASA's Wide-field Infrared Survey", "Explorer (WISE) and Galaxy Evolution Explorer (GALEX) missions. These", "maps have matched resolution (FWHM 7.5\" and 15\"), matched astrometry,", "and a common procedure for background removal. We demonstrate that", "they agree well with resolved intensity measurements and integrated", "photometry from previous surveys. This atlas represents the first part", "of a program (the z=0 Multiwavelength Galaxy Synthesis) to create a", "large, uniform database of resolved measurements of gas and dust in", "nearby galaxies. This atlas allows us estimate local and integrated", "star formation rates (SFRs) and stellar masses (M_*_) across the local", "galaxy population in a uniform way. In the appendix, we use the", "population synthesis fits of Salim+ (2016ApJS..227....2S and", "2018ApJ...859...11S) to calibrate integrated M_*_ and SFR estimators", "based on GALEX and WISE. Because they leverage a Sloan Digital Sky", "Survey (SDSS)-based training set of >100000 galaxies, these", "calibrations have high precision and allow us to rigorously compare", "local galaxies to SDSS results. We provide these SFR and M_*_", "estimates for all galaxies in our sample and show that our results", "yield a \"main sequence\" of star-forming galaxies comparable to", "previous work. We also show the distribution of intensities from", "resolved galaxies in NUV-to-WISE1 versus WISE1-to-WISE3 space, which", "captures much of the key physics accessed by these bands."], "description": ["Our final \"z=0 Multiwavelength Galaxy Synthesis\" (z0MGS) sample,", "extracted from LEDA, consists of ~15750 local galaxies with luminosity", "greater than the Large Magellanic Cloud (LMC) and likely to lie within", "~50Mpc.", "To create the WISE maps, we used the unWISE reprocessing (Lang", "2014AJ....147..108L) of the WISE all-sky survey (Wright+", "2010AJ....140.1868W). See Section 4.", "To create the GALEX maps, we downloaded every FUV and NUV tile", "obtained by GALEX during its mission and constructed our own cutouts.", "See Section 5."], "type": ["OC"], "doi_pub": ["10.3847/1538-4365/ab3925"], "orcid_pub": ["0000-0002-2545-1700"], "data": "", "date_update": "19-Feb-2020", "tables": [{"name": "table4.dat", "desc": "SFR and M* estimates for local galaxies ", "columns": [{"name": "PGC", "desc": "[4/5953111] PGC identifier "}, {"name": "NGC", "desc": "NGC identifer; if available "}, {"name": "UGC", "desc": "UGC identifer; if available "}, {"name": "IC", "desc": "IC identifer; if available "}, {"name": "Dist", "desc": "[0.4/335]? Adopted distance "}, {"name": "e_Dist", "desc": "[0.01/1.1]? Uncertainty in log_10_ distance "}, {"name": "logM*", "desc": "[5.9/12.2]? log stellar mass (1) "}, {"name": "e_logM*", "desc": "[0.1/1.2]? Uncertainty in logM* (2) "}, {"name": "Gamma*", "desc": "[0.2/0.5]? Adopted WISE 3.4 micron band mass-to-light ratio (3)"}, {"name": "n_Gamma*", "desc": "Method used to estimate Gamma* "}, {"name": "logSFR", "desc": "[-5.2/3.1]? log star formation rate (4) "}, {"name": "e_logSFR", "desc": "[0.2/3.3]? Uncertainty in logSFR (2) "}, {"name": "n_logSFR", "desc": "Method used to estimate logSFR "}, {"name": "DelMS", "desc": "[-1.6/2.4]? Offset from star forming main sequence (5)"}, {"name": "Flags", "desc": "[AGS] Additional flags (6) "}]}, {"name": "table5.dat", "desc": "WISE Mass-to-Light ratio and SFR calibrations in M*-sSFR space", "columns": [{"name": "logM*", "desc": "log stellar mass; X axis "}, {"name": "logSFR/M*", "desc": "log stellar mass from CIGALE; Y axis "}, {"name": "logN", "desc": "? log number of galaxies in cell "}, {"name": "Gamma*", "desc": "? Median WISE 3.4 micron band mass to light ratio"}, {"name": "logC1", "desc": "? log C for WISE 22 micron band in FUV+WISE4 (1)"}, {"name": "logC2", "desc": "? log C for WISE 22 micron band4 in NUV+WISE4 (1)"}, {"name": "logC3", "desc": "? log C for WISE 22 micron band4 in WISE4 only (1)"}, {"name": "logC4", "desc": "? log C for WISE 12 micron band3 in FUV+WISE3 (1)"}, {"name": "logC5", "desc": "? log C for WISE 12 micron band3 in NUV+WISE3 (1)"}, {"name": "logC6", "desc": "? log C for WISE 12 micron band3 in WISE3 only (1)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_244_36"}} {"id": "J/ApJS/244/36", "title_cds": "QSO properties from SDSS. II. The first two years", "title_create": "Chen+, 2019", "year": "2019", "author": "Chen Z.-F., Yi S.-X., Pang T.-T., Chen Z.-G., Gui R.-J., Wang Z.-W., Mo X.-H., Yi T.-F.", "title_pub": "Quasar properties from the Sloan Digital Sky Survey. II. The quasars obtained by the SDSS-IV in the first two years.", "first_author": "Chen Z.-F.", "ref_biblio": [""], "bibcode": ["2019ApJS..244...36C"], "see_also": ["VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)", "V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)", "VII/279 : SDSS quasar catalog: twelfth data release (Paris+, 2017)", "VII/286 : SDSS quasar catalog, fourteenth data release (Paris+, 2018)", "J/A+A/417/515 : I Zw 1 unusual emission line spectrum (Veron-Cetty+, 2004)", "J/MNRAS/366/480 : Emission-line properties of Seyfert 2 nuclei (Gu+, 2006)", "J/AJ/131/1 : Binary quasars in the SDSS (Hennawi+, 2006)", "J/AJ/131/2766 : Quasar luminosity function from SDSS-DR3 (Richards+, 2006)", "J/AJ/133/2222 : Clustering of high-redshift QSOs from SDSS (Shen+, 2007)", "J/ApJ/680/169 : SDSS DR5 virial black hole masses (Shen+, 2008)", "J/MNRAS/397/1713 : SDSS DR3 flat-spectrum radio quasars (Chen+, 2009)", "J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010)", "J/ApJ/708/427 : Type 2 AGNs with double-peaked [OIII] lines (Liu+, 2010)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/MNRAS/462/2980 : BOSS narrow CIV absorption lines. III. (Chen+, 2016)", "J/ApJ/831/7 : SDSS-RM project: peak velocities of QSOs (Shen+, 2016)", "J/ApJS/228/9 : Parameters of ~300000 SDSS-DR12 QSOs (Kozlowski, 2017)", "J/ApJS/235/11 : Absorption features in SDSS. I. MgII abs. (Chen+, 2018)", "J/ApJS/234/16 : H{alpha} & H{beta} spectral regions of QSOs (Chen+, 2018)", "J/AJ/155/189 : LAMOST Quasar Survey: QSO data from DR2&3 (Dong+, 2018)", "http://www.sdss.org/ : SDSS home page"], "keyword_cds": "QSOs; Spectra, optical; Redshifts; Equivalent widths; Surveys", "keyword_pub": "Black hole physics; Quasars; Active galaxies; Astronomy data reduction", "abstract": ["This work aims to measure the properties of continuum and emission", "lines around CIV, MgII, H{beta}, and H{alpha} for the quasars observed", "by the extended Baryon Oscillation Spectroscopic Survey (eBOSS) during", "the first two years. We determine the quasar redshifts based on narrow", "[OIII]{lambda}5007, broad MgII{lambda}2799, and/or CIV{lambda}1548", "emission lines. The comparisons between the visual inspection", "redshifts included in DR14Q and the redshifts determined by us suggest", "that the visual inspection redshifts would be robust. We also infer", "the virial black hole mass of quasars based on CIV, MgII, H{beta},", "and/or H{alpha} broad emission lines, using empirical relationships", "reported by previous studies. Systematic differences are remarkable", "among different line-based mass estimators reported by previous", "studies. Using the empirical relationship (Equation (1)), we improve", "the line-based mass estimators by recalibrating new coefficient (a,b),", "so that different line-based mass estimators are more consistent. We", "find that (a,b)=(0.96,0.5), (0.91,0.5), (0.82,0.5), and (0.77,0.5) are", "the best choices for the H{alpha}-, H{beta}-, MgII-, and CIV-based", "mass estimators, respectively. All these above properties are publicly", "available. We also find that the line and continuum luminosities are", "tightly correlated with each other. The Balmer lines show a negative", "Baldwin effect, while the metal lines display a positive Baldwin", "effect. In addition, we find that tight correlations are indwelled in", "different line luminosities."], "description": ["The SDSS dedicated wide-field 2.5m telescope is located at the Apache", "Point Observatory, New Mexico. All the quasar spectra of the", "SDSS-IV/eBOSS (Dawson+ 2016AJ....151...44D and", "Blanton+ 2017AJ....154...28B) are obtained with the BOSS spectrographs", "installed on the SDSS 2.5m telescope. The spectra have resolutions of", "1300"], "bibcode": ["2020ApJS..246....9Z"], "see_also": ["V/153 : LAMOST DR4 catalogs (Luo+, 2018)", "V/164 : LAMOST DR5 catalogs (Luo+, 2019)", "J/other/RAA/11.924 : Atmospheric parameters for 771 stars (Wu+, 2011)", "J/ApJ/808/16 : Cannon: a new approach to determine abundances (Ness+, 2015)", "J/AJ/151/144 : ASPCAP weights for APOGEE chemical elements (Garcia+, 2016)", "J/ApJ/836/5 : Abundances of LAMOST giants from APOGEE DR12 (Ho+, 2017)", "J/MNRAS/478/4513 : GALAH Survey DR2 (Buder+, 2018)", "J/ApJS/241/32 : OB stars from the LAMOST DR5 spectra (Liu+, 2019)", "J/ApJS/244/8 : M-type stars in LAMOST DR5 (Zhong+, 2019)", "http://www.sdss.org/ : SDSS home page"], "keyword_cds": "Abundances; Spectroscopy; Models; Stars, giant; Surveys", "keyword_pub": "Astronomical methods ; Astronomy data analysis ; Bayesian statistics ; Stellar abundances ; Chemical abundances ; Fundamental parameters of stars ; Catalogs ; Surveys", "abstract": ["The LAMOST survey has provided 9 million spectra in its Data Release 5", "(DR5) at R~1800. Extracting precise stellar labels is crucial for such", "a large sample. In this paper, we report the implementation of the", "Stellar LAbel Machine (SLAM), which is a data-driven method based on", "support vector regression (SVR), a robust nonlinear regression", "technique. Thanks to the capability to model highly nonlinear problems", "with SVR, SLAM can generally derive stellar labels over a wide range", "of spectral types. This gives it a unique capability compared to other", "popular data-driven methods. To illustrate this capability, we test", "the performance of SLAM on stars ranging from Teff~4000 to ~8000K", "trained on LAMOST spectra and stellar labels. At g-band", "signal-to-noise ratio (S/Ng) higher than 100, the random uncertainties", "of Teff, logg, and [Fe/H] are 50K, 0.09dex, and 0.07dex, respectively.", "We then set up another SLAM model trained by APOGEE and LAMOST common", "stars to demonstrate its capability of dealing with high dimensional", "problems. The spectra are from LAMOST DR5 and the stellar labels of", "the training set are from APOGEE DR15, including Teff, logg, [M/H],", "[{alpha}/M], [C/M], and [N/M]. The cross-validated scatters at", "S/N_g_~100 are 49K, 0.10dex, 0.037dex, 0.026dex, 0.058dex, and", "0.106dex for these parameters, respectively. This performance is at", "the same level as other up-to-date data-driven models."], "type": ["MC"], "data": "", "date_update": "03-Apr-2020", "tables": [{"name": "catalog.dat", "desc": "The Catalog of the 5 million converged LAMOST DR5 K giant stars with SLAM-derived stellar labels", "columns": [{"name": "ObsID", "desc": "[101008/585216248]?=- LAMOST identifier "}, {"name": "RAdeg", "desc": "Right ascension (J2000) (ra) "}, {"name": "DEdeg", "desc": "Declination (J2000) (dec) "}, {"name": "snrg", "desc": "[0/998]?=- g-band signal-to-noise ratio of the spectra"}, {"name": "Teff", "desc": "[-7492/15227] SLAM-predicted effective temperature (teff_slam)"}, {"name": "logg", "desc": "[-41.7/31.3] SLAM-predicted log of surface gravity (logg_slam)"}, {"name": "[M/H]", "desc": "[-21.6/12] SLAM-predicted metallicity (mh_slam) "}, {"name": "[a/M]", "desc": "[-4.2/7.1] SLAM-predicted [{alpha}/M] (am_slam) "}, {"name": "[C/M]", "desc": "[-9/7.5] SLAM-predicted [C/M] (cm_slam) "}, {"name": "[N/M]", "desc": "[-9.5/15.5] SLAM-predicted [N/M] (nm_slam) "}, {"name": "e_Teff", "desc": "[38.8/241.3] Teff uncertainty (teff_err_slam) "}, {"name": "e_logg", "desc": "[0.06/0.7] logg uncertainty (logg_err_slam) "}, {"name": "e_[M/H]", "desc": "[0.02/0.5] Uncertainty in [M/H] (mh_err_slam) "}, {"name": "e_[a/M]", "desc": "[0.01/0.2] Uncertainty in [a/M] (am_err_slam) "}, {"name": "e_[C/M]", "desc": "[0.04/0.2] Uncertainty in [C/M] (cm_err_slam) "}, {"name": "e_[N/M]", "desc": "[0.07/0.3] Uncertainty in [N/M] (nm_err_slam) "}, {"name": "O-C", "desc": "[0.005/243963] rms deviation between the observed and fitted spectra (rmseppix_slam)"}, {"name": "K", "desc": "[0/1] K giant star selected (1=yes) (ind_kgiant) "}, {"name": "D", "desc": "[0.0005/16038]? Distance D (DHo17) (1) "}, {"name": "Fl", "desc": "[0/1] APOGEE observation flag (1:observed by APOGEE) (ind_common)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_247_50"}} {"id": "J/ApJS/247/50", "title_cds": "Late-type contact binaries in CSS DR1", "title_create": "Sun+, 2020", "year": "2020", "author": "Sun W., Chen X., Deng L., de Grijs R.", "title_pub": "Physical parameters of late-type contact binaries in the northern Catalina Sky Survey.", "first_author": "Sun W.", "ref_biblio": [""], "bibcode": ["2020ApJS..247...50S"], "see_also": ["I/347 : Distances to 1.33 billion stars in Gaia DR2 (Bailer-Jones+, 2018)", "I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "V/119 : Catalogue of field contact binary stars (Pribulla+, 2003)", "V/146 : LAMOST DR1 catalogs (Luo+, 2015)", "J/AJ/106/2096 : Limb-darkening coefficients in binaries (Van Hamme 1993)", "J/A+A/311/523 : Photometry of W UMa (Maceroni+, 1996)", "J/A+A/426/1001 : Catalog of contact binary stars (Csizmadia+, 2004)", "J/ApJ/629/1055 : Evolution of close binary systems (Yakut+, 2005)", "J/MNRAS/373/1483 : W UMa type and CAB stars dynamical evolution (Eker+, 2006)", "J/AJ/131/621 : Catalog of 1022 bright contact binary stars (Gettel+, 2006)", "J/A+A/528/A90 : SuperWASP short period eclipsing binaries (Norton+, 2011)", "J/ApJ/763/32 : Galactic halo RRab stars from CSS (Drake+, 2013)", "J/AJ/146/101 : LINEAR. III. Periodic variables (Palaversa+, 2013)", "J/ApJS/208/9 : Intrinsic colors & temperatures of PMS stars (Pecaut+, 2013)", "J/MNRAS/430/2029 : Initial masses of W UMa contact binaries (Yildiz+, 2013)", "J/ApJS/213/9 : Catalina Surveys periodic variable stars (Drake+, 2014)", "J/AJ/148/81 : APASS BVgri photometry of RAVE stars. I. (Munari+, 2014)", "J/MNRAS/446/2251 : Southern Catalina Survey type-ab RR Lyrae (Torrealba+, 2015)", "J/AJ/152/129 : VR photometry for 914 stars in NGC 188 (Chen+, 2016)", "J/MNRAS/465/4678 : 9380 contact binaries from CRTS VSC (Marsh+, 2017)", "J/ApJ/859/140 : Multi-band magnitudes for W UMa EB* candidates (Chen+, 2018)", "J/ApJS/237/28 : WISE catalog of periodic variable stars (Chen+, 2018)", "J/AJ/156/241 : A first cat. of var. stars measured by ATLAS (Heinze+, 2018)"], "keyword_cds": "Binaries, eclipsing; Stars, masses ; Effective temperatures ; Stars, diameters; Optical", "keyword_pub": "Astronomy data analysis ; contact binary stars ; fundamental parameters of stars", "abstract": ["We present the physical parameters of 2335 late-type contact binary", "(CB) systems extracted from the Catalina Sky Survey (CSS). Our sample", "was selected from the CSS Data Release 1 by strictly limiting the", "prevailing temperature uncertainties and light-curve fitting", "residuals, allowing us to almost eliminate any possible contaminants.", "We developed an automatic Wilson-Devinney-type code to derive the", "relative properties of CBs based on their light-curve morphology. By", "adopting the distances derived from CB (orbital) period-luminosity", "relations (PLRs), combined with the well-defined mass-luminosity", "relation for the systems' primary stars and assuming solar", "metallicity, we calculated the objects' masses, radii, and", "luminosities. Our sample of fully eclipsing CBs contains 1530 W-, 710", "A-, and 95 B-type CBs. A comparison with literature data and with the", "results from different surveys confirms the accuracy and coherence of", "our measurements. The period distributions of the various CB subtypes", "are different, hinting at a possible evolutionary sequence. W-type CBs", "are clearly located in a strip in the total mass versus mass-ratio", "plane, while A-type CBs may exhibit a slightly different dependence.", "There are no significant differences among the PLRs of A- and W-type", "CBs, but the PLR zero-points are affected by their mass ratios and", "fill-out factors. Determination of zero-point differences for", "different types of CBs may help us improve the accuracy of the", "resulting PLRs. We demonstrate that automated approaches to deriving", "CB properties could be a powerful tool for application to the much", "larger CB samples expected to result from future surveys."], "description": ["We used contact binary (CB) data from the Catalina Sky Survey (CSS)", "Data Release 1 (CSDR1; Drake+ 2014, J/ApJS/213/9). The survey used", "three telescopes to cover the sky between declinations DEC=-75{deg}", "and +70{deg} at Galactic latitudes |b|>15{deg}."], "type": ["CCC"], "doi_pub": ["10.3847/1538-4365/ab7894"], "orcid_pub": ["0000-0002-3279-0233"], "data": "f-v", "date_creation": "20-Jul-2020", "xmatch": "J/ApJS/247/50/table1", "last_update": "20-Jul-2020", "catid": "22470050", "date_update": "20-Jul-2020", "tables": [{"name": "table1.dat", "desc": "Total-eclipsing contact binary (CB) catalog ", "columns": [{"name": "---", "desc": "[CSS_] "}, {"name": "CRTS", "desc": "Catalina Sky Survey (CSS) identifier (JHHMMSS.s+DDMMSS)"}, {"name": "RAdeg", "desc": "Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-19.7/70.1] Declination (J2000) "}, {"name": "Period", "desc": "[0.196/0.56] Orbital period "}, {"name": "Teff1", "desc": "[3436/15530] Primary effective temperature (1) "}, {"name": "Teff2", "desc": "[3520/11079] Secondary effective temperature (1)"}, {"name": "e_Teff1", "desc": "[8/4226]? Uncertainty in Teff1 (1) "}, {"name": "e_Teff2", "desc": "[13/3290]? Uncertainty in Teff2 (1) "}, {"name": "inc", "desc": "[70/90] Inclination angle "}, {"name": "e_inc", "desc": "[0.1/22.2] Uncertainty in inc "}, {"name": "Omega", "desc": "[1.8/15] Surface potential ({Omega}={Omega}_1_={Omega}_2_)"}, {"name": "e_Omega", "desc": "[0/0.8] Uncertainty in Omega "}, {"name": "q", "desc": "[0.07/0.8] Mass ratio; M2/M1 "}, {"name": "e_q", "desc": "[0.09] Uncertainty in q "}, {"name": "f", "desc": "[-1/1] Fill-out factor (2) "}, {"name": "e_f", "desc": "[0.01/4.1] Uncertainty in f "}, {"name": "LFrac", "desc": "[0.4/1] Primary to total V band luminosity ratio"}, {"name": "e_LFrac", "desc": "[0/0.4] Uncertainty in LFrac "}, {"name": "OT", "desc": "CB classification (1530 W-, 710 A-, and 95 B-type CBs)"}, {"name": "M1", "desc": "[0.8/2.5] Primary mass "}, {"name": "M2", "desc": "[0.08/1.4] Secondary mass "}, {"name": "e_M1", "desc": "[0.02/0.1] Uncertainty in M1 "}, {"name": "e_M2", "desc": "[0.07/0.3] Uncertainty in M2 "}, {"name": "r1", "desc": "[0.7/2.2] Primary radius "}, {"name": "r2", "desc": "[0.3/1.5] Secondary radius "}, {"name": "e_r1", "desc": "[0.02/0.07] Uncertainty in r1 "}, {"name": "e_r2", "desc": "[0.01/0.03] Uncertainty in r2 "}, {"name": "L1", "desc": "[0.3/26.8] Primary luminosity "}, {"name": "L2", "desc": "[0.05/9.2] Secondary luminosity "}, {"name": "e_L1", "desc": "[0.08/6.4] Uncertainty in L1 "}, {"name": "e_L2", "desc": "[0.02/4.6] Uncertainty in L2 "}, {"name": "a", "desc": "[1.5/4.2] Semi-major axis "}, {"name": "e_a", "desc": "[0.03/0.1] Uncertainty in a "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_248_25"}} {"id": "J/ApJS/248/25", "title_cds": "The SFRS: 3-33GHz VLA obs. of star-forming regions", "title_create": "Linden+, 2020", "year": "2020", "author": "Linden S.T., Murphy E.J., Dong D., Momjian E., Kennicutt R.C., Meier D.S., Schinnerer E., Turner J.L.", "title_pub": "The Star Formation in Radio Survey: 3-33GHz imaging of nearby galaxy Nuclei and extranuclear star-forming regions.", "first_author": "Linden S.T.", "ref_biblio": [""], "bibcode": ["2020ApJS..248...25L"], "see_also": ["VII/155 : Third Reference Cat. of Bright Galaxies (RC3) (de Vaucouleurs+ 1991)", "J/ApJ/577/31 : PNe in six galaxies (Ciardullo+, 2002)", "J/ApJ/586/794 : Multiwavelength luminosities of galaxies (Bell, 2003)", "J/ApJ/703/517 : The Spitzer Local Volume Legacy: IR photometry (Dale+, 2009)", "J/ApJS/190/233 : Spectroscopy & abundances of SINGS galaxies (Moustakas+, 2010)", "J/ApJ/745/95 : Herschel FIR & submm photom. of KINGFISH sample (Dale+, 2012)", "J/ApJ/761/97 : Star Formation in Radio Survey (SFRS): 33GHz (Murphy+, 2012)", "J/A+A/576/A33 : KINGFISH galaxy sample radial profile SED (Hunt+, 2015)", "J/ApJ/836/185 : SEDs of radio continuum from KINGFISHER (Tabatabaei+, 2017)", "J/ApJS/234/24 : VLA 33GHz obs. of star-forming regions (Murphy+, 2018)"], "keyword_cds": "Active gal. nuclei; Star Forming Region; Radio sources; Galaxies, nearby; Galaxies, IR; Photometry, H-alpha; Ultraviolet", "keyword_pub": "Star formation ; H II regions ; Radio continuum emission ; Star- forming regions ; Radio interferometry ; Radio astronomy ; Galaxies ; Galaxy evolution ; Spiral galaxies ; Extragalactic radio sources", "abstract": ["We present 3, 15, and 33GHz imaging toward galaxy nuclei and", "extranuclear star-forming regions using the Karl G. Jansky Very Large", "Array as part of the Star Formation in Radio Survey (SFRS). With", "3-33GHz radio spectra, we measured the spectral indices and", "corresponding thermal (free-free) emission fractions for a sample of", "335 discrete regions having significant detections in at least two", "radio bands. After removing 14 likely background galaxies, we find", "that the median thermal fraction at 33 GHz is 92%+/-0.8% with a median", "absolute deviation of 11%, when a two-component power-law model is", "adopted to fit the radio spectrum. Limiting the sample to 238 sources", "that are confidently identified as star-forming regions and not", "affected by potential AGN contamination (i.e., having galactocentric", "radii r_G_>=250pc) results in a median thermal fraction of 93%+/-0.8%", "with a median absolute deviation of 10%. We further measure the", "thermal fraction at 33GHz for 163 regions identified at 7\" resolution", "to be 94%+/-0.8% with a median absolute deviation of 8%. Together,", "these results confirm that free-free emission dominates the radio", "spectra of star-forming regions on scales up to ~500pc in normal", "star-forming galaxies. We additionally find a factor of ~1.6 increase", "in the scatter of the measured spectral index and thermal fraction", "distributions as a function of decreasing galactocentric radius. This", "trend is likely reflective of the continuous star formation activity", "occurring in the galaxy centers, resulting in a larger contribution of", "diffuse nonthermal emission relative to star-forming regions in the", "disk."], "description": ["The Star Formation in Radio Survey (SFRS) sample includes targeted", "observations from 56 nearby galaxies (d_L_<30Mpc) in the Spitzer", "Infrared Nearby Galaxies Survey (SINGS; Kennicutt+ 2003PASP..115..928K)", "and Key Insights on Nearby Galaxies: a Far-Infrared Survey (KINGFISH;", "Kennicutt+ 2011PASP..123.1347K) legacy programs (Table 1).", "The full sample over the entire sky consists of 118 star-forming", "complexes (56 nuclei and 62 extranuclear regions), 112 of which (50", "nuclei and 62 extranuclear regions; see Tables 2 and 3, respectively)", "are observable with the VLA (i.e., having {delta}>-35{deg}).", "The observational setup and reduction procedure for the Ka-band", "(29-37GHz) data (11B-032,13A-129) is described in detail in M18a", "(Murphy+, 2018, J/ApJS/234/24). Observations in the S band (2-4GHz)", "were taken during the 2013 VLA B-configuration cycle (13B-215) and", "utilized the 8-bit sampler. Observations in the Ku band (12-18GHz)", "were taken in 2014 November in the C configuration (13B-215) using the", "3-bit samplers. Both sets of observations utilized the full available", "bandwidth of the respective receivers."], "type": ["OC"], "data": "", "date_update": "22-Jul-2020", "tables": [{"name": "table1.dat", "desc": "Galaxy properties ", "columns": [{"name": "Name", "desc": "Galaxy name "}, {"name": "Type", "desc": "Morphological type from RC3 (VII/155) "}, {"name": "Dist", "desc": "[3.05/30.6] Redshift-independent distance (1) "}, {"name": "Nuc", "desc": "Nuclear type (2) "}, {"name": "f_Nuc", "desc": "[*] Flag on Nuc (3) "}, {"name": "D25", "desc": "Diameter from RC3 (VII/155) "}, {"name": "inc", "desc": "[21/83] Inclination "}, {"name": "PA", "desc": "[10/173] Position angle from RC3 (VII/155) "}, {"name": "f_PA", "desc": "[d] d: PA from Jarrett+ (2003AJ....125..525J) "}]}, {"name": "table2.dat", "desc": "*Nuclear source positions and imaging characteristics ", "columns": [{"name": "Name", "desc": "Galaxy name "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "Beam3GHz", "desc": "FWHM of the synthesized beam at 3GHz "}, {"name": "Sig3GHz", "desc": "[12.8/45] 3GHZ point source sensitivity {sigma}"}, {"name": "Tb3GHz", "desc": "[239/1431] 3GHz brightness temperature sensitivity {sigma}_Tb_"}, {"name": "Beam15GHz", "desc": "FWHM of the synthesized beam at 15GHz "}, {"name": "Sig15GHz", "desc": "[7.8/51] 15GHZ point source sensitivity {sigma}"}, {"name": "Tb15GHz", "desc": "[10/133] 15GHz brightness temperature sensitivity {sigma}_Tb_"}]}, {"name": "enuc.dat", "desc": "Extranuclear source positions and imaging characteristics (Table 3)", "columns": [{"name": "Name", "desc": "Extranuclear source name "}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "Beam3GHz", "desc": "FWHM of the synthesized beam at 3GHz "}, {"name": "Sig3GHz", "desc": "[12.8/45] 3GHZ point source sensitivity {sigma}"}, {"name": "Tb3GHz", "desc": "[239/1431] 3GHz brightness temperature sensitivity {sigma}_Tb_"}, {"name": "Beam15GHz", "desc": "FWHM of the synthesized beam at 15GHz "}, {"name": "Sig15GHz", "desc": "[7.8/51] 15GHZ point source sensitivity {sigma}"}, {"name": "Tb15GHz", "desc": "[9.8/133] 15GHz brightness temperature sensitivity {sigma}_Tb_"}]}, {"name": "table4.dat", "desc": "Region photometry and derived parameters ", "columns": [{"name": "OT", "desc": "Source type (G1) "}]}, {"name": "table5.dat", "desc": "Region photometry and derived parameters at 7\" angular resolution", "columns": [{"name": "OT", "desc": "Source type (G1) "}]}, {"name": "tablea1.dat", "desc": "Ancillary source photometry at 7\" angular resolution ", "columns": [{"name": "OT", "desc": "Source type (G1) "}, {"name": "Name", "desc": "Field identifier (galaxy nuclei or extranuclear HII regions)"}, {"name": "m_Name", "desc": "Source identifier (blank if only one source in the field)"}, {"name": "l_F1528", "desc": "Limit flag on F1528 "}, {"name": "F1528", "desc": "[0.2/1733]? GALEX FUV (1528{AA}) flux (f_{nu}_)"}, {"name": "e_F1528", "desc": "[0.4/260]? F1528 uncertainty "}, {"name": "l_F2271", "desc": "Limit flag on F2271 "}, {"name": "F2271", "desc": "[0.4/2033]? GALEX NUV (2271{AA}) flux (f_{nu}_)"}, {"name": "e_F2271", "desc": "[1/305]? F2271 uncertainty "}, {"name": "l_FHa", "desc": "Limit flag on FHa "}, {"name": "FHa", "desc": "[0.01/8.2]? H{alpha} flux in 10^-13^erg/s/cm^2^ units (1)"}, {"name": "e_FHa", "desc": "[0.003/1.7]? FHa uncertainty "}, {"name": "F24", "desc": "[0.3/2076]? Spitzer/MIPS 24um flux (f_{nu}_) "}, {"name": "e_F24", "desc": "[0.02/104]? F24 uncertainty "}, {"name": "f_F24", "desc": "[a] Flag on F24 (2) "}]}, {"name": "tablea2.dat", "desc": "Local background measurements ", "columns": [{"name": "OT", "desc": "Source type (G1) "}, {"name": "Name", "desc": "Field identifier (galaxy nuclei or extranuclear HII regions)"}, {"name": "m_Name", "desc": "Source identifier (blank if only one source in the field)"}, {"name": "f_Name", "desc": "[a] Flag on Name (G2) "}, {"name": "bg3GHz", "desc": "[-0.14/16.8]? 3GHz local background value "}, {"name": "bg15GHz", "desc": "[-0.06/1.5]? 15GHz local background value "}, {"name": "bg33GHz", "desc": "[-0.2/1.4]? 33GHz local background value "}, {"name": "f3GHzbg", "desc": "[0/0.37]? 3GHz fractional contribution (1) "}, {"name": "f15GHzbg", "desc": "[0/0.33]? 15GHz fractional contribution (1) "}, {"name": "f33GHzbg", "desc": "[0/0.26]? 33GHz fractional contribution (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_249_7"}} {"id": "J/ApJS/249/7", "title_cds": "Stellar ages & masses of main-sequence and giant stars", "title_create": "Bu+, 2020", "year": "2020", "author": "Bu Y., Kumar Y.B., Xie J., Pan J., Zhao G., Wu Y.", "title_pub": "Estimation of stellar ages and masses using Gaussian process regression.", "first_author": "Bu Y.", "ref_biblio": [""], "bibcode": ["2020ApJS..249....7B"], "see_also": ["V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)", "J/AcA/41/167 : UBV photometry in Berkeley 32 (Kaluzny+, 1991)", "J/A+A/348/897 : Ages of main-sequence stars (Lachaume+, 1999)", "J/A+AS/141/371 : Low-mass stars evolutionary tracks (Girardi+, 2000)", "J/ApJ/562/528 : Teff and log(g) of low-metallicity stars (Snider+, 2001)", "J/AJ/127/1513 : Lick indices on M67 members (Schiavon+, 2004)", "J/A+A/530/A115 : Rotating massive MS stars evolutionary models (Brott+, 2011)", "J/A+A/537/A146 : Stellar models with rotation. 0.8"], "bibcode": ["2020ApJS..250...32L"], "see_also": ["II/363 : The band-merged unWISE Catalog (Schlafly+, 2019)", "VIII/51 : the FIRST Survey, version 1998Feb (White+ 1998)", "VIII/90 : The FIRST Survey Catalog, Version 12Feb16 (Becker+ 2012)", "J/MNRAS/356/568 : Deep Chandra survey of the Groth Strip (Nandra+, 2005)", "J/A+A/497/635 : XMM-Newton wide-field survey in COSMOS (Cappelluti+, 2009)", "J/ApJ/692/758 : BAL QSOs in SDSS-DR5 (Gibson+, 2009)", "J/ApJS/180/102 : AEGIS-X: Chandra deep survey (Laird+, 2009)", "J/A+A/493/339 : XMM-Newton serendipitous Survey. V. (Watson+, 2009)", "J/ApJS/202/6 : XDEEP2 survey catalog (Goulding+, 2012)", "J/ApJS/199/34 : Clusters of galaxies in SDSS-III (Wen+, 2012)", "J/ApJ/766/60 : GALEX Time Domain Survey I. UV variables (Gezari+, 2013)", "J/ApJS/220/10 : AEGIS-X Deep survey of EGS (AEGIS-XD) (Nandra+, 2015)", "J/A+A/577/A121 : The XMM-ATLAS catalogues (Ranalli+, 2015)", "J/ApJS/216/4 : SDSS-RM project: technical overview (Shen+, 2015)", "J/ApJ/819/62 : The COSMOS-Legacy Survey (CLS) catalog (Civano+, 2016)", "J/A+A/594/A116 : HI4PI spectra and column density maps (HI4PI team+, 2016)", "J/ApJ/817/172 : X-ray Observations of Stripe 82 (LaMassa+, 2016)", "J/ApJS/228/2 : Chandra Deep Field-South survey: 7Ms sources (Luo+, 2017)", "J/MNRAS/473/4937 : AllWISE ctp to ROSAT/2RXS & XMMSLEW2 cat. (Salvato+, 2018)", "http://www.mpe.mpg.de/XraySurveys/XMM-RM/ : XMM-RM project home page", "http://www.legacysurvey.org/ : Legacy Survey home page"], "keyword_cds": "X-ray sources; Cross identifications; Photometry, ugriz", "keyword_pub": "Astronomy data analysis ; Supermassive black holes ; Active galactic nuclei ; X-ray active galactic nuclei ; Quasars ; X-ray point sources", "abstract": ["The XMM-RM project was designed to provide X-ray coverage of the Sloan", "Digital Sky Survey Reverberation Mapping (SDSS-RM) field. Forty-one", "XMM-Newton exposures, placed surrounding the Chandra AEGIS field, were", "taken, covering an area of 6.13deg^2^ and reaching a nominal exposure", "depth of ~15ks. We present an X-ray catalog of 3553 sources detected", "in these data, using a PSF-fitting algorithm and a sample selection", "threshold that produces a ~5% fraction of spurious sources. In", "addition to the PSF-fitting likelihood, we calculate a second source", "reliability measure based on Poisson theory using source and", "background counts within an aperture. Using the Poissonian likelihood,", "we select a subsample with a high purity and find that it has number", "count profiles similar to previous X-ray surveys. The Bayesian method", "\"NWAY\" was employed to identify counterparts of the X-ray sources from", "the optical Legacy and the IR unWISE catalogs, using a two-dimensional", "unWISE magnitude-color prior created from optical/IR counterparts of", "Chandra X-ray sources. A significant number of the optical/IR", "counterparts correspond to sources with low detection likelihoods,", "proving the value of retaining the low-likelihood detections in the", "catalog. A total of 932 of the XMM-RM sources are covered by SDSS", "spectroscopic observations, where 89% of them are classified as active", "galactic nuclei, and 71% of these active galactic nuclei are in the", "SDSS-RM quasar catalog. Among the SDSS-RM quasars, 80% are detectable", "at the depth of the XMM observations."], "description": ["The XMM-Newton observations cover a total sky area of ~6.13deg^2^", "within the 7deg^2^ Sloan Digital Sky Survey Reverberation Mapping (RM)", "field. The main data set is formed by 41 XMM observations with", "individual exposure times of ~15ks, with 13 pointings obtained in AO15", "(PI P. Green) and 28 in AO16 (PI A. Merloni). All observations were", "taken in full-frame mode of the EPIC-PN/MOS cameras.", "In addition to these XMM-RM dedicated observations, we also reanalyze", "seven archival XMM observations in the RM field (see Figure 1),", "including five Groth-Westphal Strip observations (PI R. Griffiths) and", "two object-targeted observations (0503960101, PI M. Agueros;", "0723860101, PI D. Lin).", "We identify multiband counterparts of the XMM-RM sources from the", "optical Legacy (Dey+ 2019AJ....157..168D) and the infrared unWISE", "(Schlafly+ 2019, II/363) catalogs. The Legacy catalog presents g-, r-,", "and z-band magnitudes for each source. The unWISE catalog provides the", "W1 (3.4um) and W2 (4.6um) magnitudes, although some sources are", "detected in only one of the two bands. Considering that the typical", "XMM positional uncertainty (~2\", half-pixel size) is much larger than", "that of the optical/IR positions, we first combine the Legacy and", "unWISE catalogs and then match the XMM sources to the combined", "catalog. See Section 5 for further details.", "In order to efficiently identify optical/IR counterparts of the XMM-RM", "sources using the Bayesian method NWAY (Salvato+ 2018, J/MNRAS/473/4937),", "we create optical/IR color and magnitude priors on the basis of the", "Chandra catalogs of C-COSMOS (Marchesi+ 2016ApJ...830..100M) and", "Stripe 82 (LaMassa+ 2016, J/ApJ/817/172). See Section 5.2."], "data": "", "date_update": "18-Nov-2020", "tables": [{"name": "maincat.dat", "desc": "XMM-RM main X-ray source catalog ", "columns": [{"name": "RACdeg", "desc": "[211.3/216.3] Combined Legacy-unWISE catalog right ascension (J2000) (UWLS_RA) (1)"}, {"name": "DECdeg", "desc": "[51.6/54.6] Combined Legacy-unWISE catalog declination (J2000) (UWLS_DEC) (1)"}, {"name": "eCPos", "desc": "[0.3/8] Error on position (UWLS_POSERR) (1) "}, {"name": "Distbf", "desc": "[-124.5/11.4] Log of ratio between prior and posterior from distance matching"}]}, {"name": "xid.dat", "desc": "Optical-IR counterpart catalog ", "columns": [{"name": "ID", "desc": "[1/3560] Identifier (ID) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) (RA) "}, {"name": "DEdeg", "desc": "Declination (J2000) (DEC) "}, {"name": "ePos", "desc": "[0.08/16] Positional uncertainty from PSF fitting (RADEC_ERR)"}, {"name": "eSys", "desc": "[0.28/1.6] Additional systematic positional uncertainty (SYSERRCC) (1)"}, {"name": "Band", "desc": "[FHS] The detection band that has the highest detection likelihood and in which"}]}, {"name": "phot.dat", "desc": "X-ray photometry of the SDSS-RM catalog ", "columns": [{"name": "RMID", "desc": "SDSS-RM catalog ID (RMID) (G2) "}, {"name": "RAdeg", "desc": "Right ascension in decimal degrees (J2000) (RA)"}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) (DEC) "}, {"name": "CRlimF", "desc": "2{sigma} count rate upper limit in full band (0.5-10keV) on the background-subtracted"}]}, {"name": "table1.dat", "desc": "XMM-RM observations ", "columns": [{"name": "obsID", "desc": "[127921001/804272801] XMM observation ID "}, {"name": "RAdeg", "desc": "[211.7/216] Aim point right ascension (J2000) "}, {"name": "DEdeg", "desc": "[51.8/54.4] Aim point declination (J2000) "}, {"name": "Date", "desc": "Date of observation (UT) "}, {"name": "ModePN", "desc": "Observation mode and filter for PN camera (1) "}, {"name": "ExpPN", "desc": "[2.8/45]? Cleaned exposure time (\"ONTIME\") after removal of background flares for PN"}, {"name": "RatioPN", "desc": "[18/99]? Clean to raw exposure time ratio for PN"}, {"name": "ModeMOS", "desc": "Observation mode and filter for MOS camera (1) "}, {"name": "ExpMOS", "desc": "[4.1/53.1] Cleaned exposure time (\"ONTIME\") after removal of background flares for MOS"}, {"name": "RatioMOS", "desc": "[34/100] Clean to raw exposure time ratio for MOS"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_252_1"}} {"id": "J/ApJS/252/1", "title_cds": "OH and HI data in molecular clouds", "title_create": "Tang+, 2021", "year": "2021", "author": "Tang N., Li Di, Yue N., Zuo P., Liu T., Luo G., Chen L., Qin S.-L., Wu Y., Heiles C.", "title_pub": "OH evolution in molecular clouds.", "first_author": "Tang N.", "ref_biblio": [""], "bibcode": ["2021ApJS..252....1T"], "see_also": ["J/A+A/383/631 : Catalogue of dust clouds in the Galaxy (Dutra+, 2002)", "J/A+A/414/235 : OH maser emission from star forming regions (Szymczak+, 2004)", "J/A+A/505/405 : A catalogue of Spitzer dark clouds (Peretto+, 2009)", "J/ApJ/756/76 : Planck cold dust clumps CO survey (Wu+, 2012)", "J/ApJS/209/37 : Planck cold clumps in ^12^CO, ^13^CO and C^18^O (Meng+, 2013)", "J/A+A/580/A112 : THOR. The HI, OH, Recombination Line Survey (Bihr+, 2015)", "J/A+A/590/A72 : Herschel counterparts of SDC (Peretto+, 2016)", "J/A+A/594/A28 : Planck Catalogue of Galactic cold clumps (PGCC) (Planck+, 2016)", "J/ApJS/224/43 : Planck cold clumps and cores in the 2nd quadrant (Zhang+, 2016)", "J/ApJS/234/2 : The GALFA-HI survey data release 2 (Peek+, 2018)", "J/ApJ/883/158 : Dark molecular gas in the Galaxy II. Perseus arm (Busch+, 2019)"], "keyword_cds": "Molecular clouds; H I data; Molecular data", "keyword_pub": "Hydroxyl sources ; Molecular gas ; Diffuse molecular clouds", "abstract": ["We have conducted a OH 18cm survey toward 141 molecular clouds in", "various environments, including 33 optical dark clouds, 98 Planck", "Galactic cold clumps (PGCCs), and 10 Spitzer dark clouds with the", "Arecibo telescope. The deviations from local thermal equilibrium are", "common for intensity ratios of both OH main lines and satellite lines.", "Line intensity of OH 1667MHz is found to correlate linearly with", "visual extinction A_V_ when A_V_ is less than 3mag. It was converted", "into OH column density by adopting the excitation temperature derived", "from Monte Carlo simulations with 1{sigma} uncertainty. The", "relationship between OH abundance X(OH) relative to H_2_ and", "A_V_ is found to follow an empirical formula,", "X(OH)/10^-7^=1.3_-0.4_^+0.4^+6.3_-0.5_^+0.5^*exp(-A_V_/2.9_-0.6_^+0.6^).", "Linear correlation is found between OH and ^13^CO intensity. Besides,", "nonthermal velocity dispersions of OH and ^13^CO are closely", "correlated. These results imply tight chemical evolution and spatial", "occupation between OH and ^13^CO. No obvious correlation is found", "between column density and nonthermal velocity dispersion of OH and HI", "narrow self-absorption (HINSA), indicating different chemical", "evolution and spatial volume occupation between OH and HINSA. Using", "the age information of HINSA analysis, OH abundance X(OH) is found to", "increase linearly with cloud age, which is consistent with previous", "simulations. Fourteen OH components without corresponding CO emission", "were detected, implying the effectiveness of OH in tracing the", "\"CO-dark\" molecular gas."], "description": ["Observations of the OH 18cm transitions were carried out with the", "Arecibo 300m telescope, whose beam size is 3.5' at 1.6GHz.", "ODC (optical dark clouds from Dutra & Bica, 2002, J/A+A/383/631):", "Three transitions of OH, 1612.2310, 1665.4018, and 1667.3590MHz, were", "obtained during 2018 September and October.", "PGCC (Planck Galactic cold clump from Planck+, 2016, J/A+A/594/A28).", "Four transitions of OH, 1612.2310, 1665.4018, 1667.3590, and", "1720.5300MHz, were obtained between 2013 November and 2015 November.", "SDC (Spitzer dark cloud from Peretto & Fuller, 2009, J/A+A/505/405).", "The observations were taken in 2013 November with same settings as for", "PGCCs. See Section 2.2.", "^12^CO(1-0) and its isotopes (^13^CO(1-0) and C^18^O(1-0))", "observations toward 33 ODCs, 11 PGCCs, and 10 SDCs were made with", "Delingha 13.7m during 2020 May and June. CO data of the rest of the 87", "PGCCs were obtained from a CO survey with Delingha 13.7m in 2011", "(Wu+ 2012, J/ApJ/756/76). See Section 2.3.", "HI spectra toward ODCs were obtained simultaneously with the OH data.", "HI data for the rest of the sources were extracted from the Galactic", "Arecibo L-band Feed Array HI (GALFA-HI; Peek+ 2018, J/ApJS/234/2)."], "type": ["OC"], "data": "", "date_update": "21-Apr-2021", "tables": [{"name": "table2.dat", "desc": "Gaussian fitting parameters of OH data ", "columns": [{"name": "Seq", "desc": "[1/141] Source index identifier "}, {"name": "m_Seq", "desc": "[0/4] Component number "}, {"name": "Name", "desc": "Common identifier "}, {"name": "GLON", "desc": "[33.10/201.85] Galactic longitude "}, {"name": "GLAT", "desc": "[-24.9/11.4] Galactic latitude "}, {"name": "Tp1665", "desc": "[-1.5/2.6]? OH 1665MHz line peak temperature "}, {"name": "e_Tp1665", "desc": "[0.01/1.1]? Uncertainty in Tp1665 "}, {"name": "Vc1665", "desc": "[-20.5/110.2]? OH 1665MHz line center velocity"}, {"name": "e_Vc1665", "desc": "[0.01/1.1]? Uncertainty in Vc1665 "}, {"name": "DV1665", "desc": "[0.2/9.1]? OH 1665MHz line width "}, {"name": "e_DV1665", "desc": "[0.01/2.5]? Uncertainty in DV1665 "}, {"name": "Tp1667", "desc": "[-1.6/4.4]? OH 1667MHz line peak temperature "}, {"name": "e_Tp1667", "desc": "[0.01/0.3]? Uncertainty in Tp1667 "}, {"name": "Vc1667", "desc": "[-22.7/106.3]? OH 1667MHz line center velocity"}, {"name": "e_Vc1667", "desc": "[0/0.9]? Uncertainty in Vc1667 "}, {"name": "DV1667", "desc": "[0.3/12.7]? OH 1667MHz line width "}, {"name": "e_DV1667", "desc": "[0.01/2.1]? Uncertainty in DV1667 "}, {"name": "N(OH)", "desc": "[0.2/76.2]? OH column density "}, {"name": "e_N(OH)", "desc": "[0.1/5.4]? Uncertainty in N(OH) "}, {"name": "Tk", "desc": "[3.7/20.3]? Kinetic temperature "}, {"name": "e_Tk", "desc": "[0.06/1.2]? Uncertainty in Tk "}, {"name": "N(13CO)", "desc": "[0/102.3]? ^13^CO column density "}, {"name": "e_N(13CO)", "desc": "[0/14]? Uncertainty in N(13CO) "}, {"name": "N(H2)", "desc": "[0.18/54]? H_2_ column density "}, {"name": "e_N(H2)", "desc": "[0.02/17.2]? Uncertainty in N(H2) "}]}, {"name": "table3.dat", "desc": "Gaussian fitting parameters of HI narrow self-absorption (HINSA) data", "columns": [{"name": "Seq", "desc": "[2/141] Source index identifier "}, {"name": "Name", "desc": "Common identifier "}, {"name": "GLON", "desc": "[33.10/201.85] Galactic longitude "}, {"name": "GLAT", "desc": "[-21.9/9.2] Galactic latitude "}, {"name": "N(OH)", "desc": "[1.1/42.2] OH column density "}, {"name": "e_N(OH)", "desc": "[0.14/5.4] Uncertainty in N(OH) "}, {"name": "N(HINSA)", "desc": "[0.2/14.8] H I Narrow Self-Absorption column density"}, {"name": "e_N(HINSA)", "desc": "[0.07/9.2] Uncertainty in N(HINSA) "}, {"name": "p", "desc": "[0.38/0.98] Fraction of background "}, {"name": "Den", "desc": "[0.2/18.5]? Density "}, {"name": "e_Den", "desc": "[0.1/17.1]? Uncertainty in Den "}, {"name": "N(H2)", "desc": "[0.3/18.7] H_2_ column density "}, {"name": "e_N(H2)", "desc": "[0.04/17.2] Uncertainty in N(H2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_252_15"}} {"id": "J/ApJS/252/15", "title_cds": "The GNRIS-Distant Quasar Survey (GNRIS-DQS)", "title_create": "Matthews+, 2021", "year": "2021", "author": "Matthews B.M., Shemmer O., Dix C., Brotherton M.S., Myers A.D., Andruchow I., Brandt W.N., Ferrero G.A., Gallagher S.C., Green R., Lira P., Plotkin R.M., Richards G.T., Runnoe J.C., Schneider D.P., Shen Y., Strauss M.A., Wills B.J.", "title_pub": "Placing high-redshift quasars in perspective: a catalog of spectroscopic properties from the Gemini Near InfRared Spectrograph-Distant Quasar Survey.", "first_author": "Matthews B.M.", "ref_biblio": [""], "bibcode": ["2021ApJS..252...15M"], "see_also": ["VII/279 : SDSS quasar catalog: twelfth data release (Paris+, 2017)", "VII/286 : SDSS quasar catalog, fourteenth data release (Paris+, 2018)", "VII/289 : SDSS quasar catalog, sixteenth data release (DR16Q) (Lyke+, 2020)", "J/A+A/333/231 : O-M stars model atmospheres (Bessell+ 1998)", "J/AJ/131/2766 : Quasar luminosity function from SDSS-DR3 (Richards+, 2006)", "J/MNRAS/405/2302 : Improved redshifts for SDSS quasar spectra (Hewett+, 2010)", "J/ApJ/708/137 : Broad-line AGNs in zCOSMOS survey (Merloni+, 2010)", "J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)", "J/ApJ/753/125 : NIR spectroscopy follow-up of 60 SDSS-DR7 QSOs (Shen+, 2012)", "J/ApJ/813/82 : z<0.06 broad-line AGN emission-line measures (Reines+, 2015)", "J/ApJ/817/55 : NIR spectroscopy of 1.5"], "bibcode": ["2021ApJS..252...20L"], "see_also": ["VII/20 : Catalogue of HII Regions (Sharpless 1959)", "J/A+AS/103/541 : Arcetri Catalogue of H2O Maser Sources (Brand+ 1994)", "J/A+AS/132/211 : Interstellar SiO sources (Harju+ 1998)", "J/PASJ/56/313 : 13CO survey of Mon & CMa molecular clouds (Kim+, 2004)", "J/ApJ/665/1194 : Dense cores in the Orion A cloud survey (Ikeda+, 2007)", "J/ApJ/684/1240 : Prestellar cores in Perseus, Serpens & Oph (Enoch+, 2008)", "J/MNRAS/418/2121 : CO 3-2 observations of outflows in W5 (Ginsburg+, 2011)", "J/ApJ/756/76 : Planck cold dust clumps CO survey (Wu+, 2012)", "J/ApJ/772/45 : Hi-GAL: star formation in the 3rd quadrant (Elia+, 2013)", "J/MNRAS/431/1752 : ATLASGAL 6.7GHz methanol masers (Urquhart+, 2013)", "J/A+A/564/A68 : Orion A GMC 13CO and C18O maps (Shimajiri+, 2014)", "J/AJ/147/46 : Properties of clumps in the NAN complex (Zhang+, 2014)", "J/ApJS/219/20 : Outflows and bubbles in Taurus (Li+, 2015)", "J/ApJ/798/L27 : CO obs. of molecular clouds in the 2nd quadrant (Sun+, 2015)", "J/A+A/594/A58 : Hi-GAL l=224deg region CO(1-0) data cubes (Olmi+, 2016)", "J/ApJS/224/7 : CO obs. of the outer arm in the 2nd quadrant (Du+, 2016)", "J/ApJS/230/17 : CO of MCs in the Extreme Outer Galaxy region (Sun+, 2017)", "J/ApJS/235/3 : Outflows associated with ATLASGAL clumps (Yang+, 2018)", "J/ApJS/242/19 : CO outflow candidates toward W3/4/5 complex (Li+, 2019)", "J/ApJS/240/26 : YSO cand. in Canis Major OB1 association (Sewilo+, 2019)", "J/A+A/633/A147 : FQS. Galactic Plane CO survey (Benedettini+, 2020)"], "keyword_cds": "Molecular clouds; Carbon monoxide; Interstellar medium; Velocity dispersion; Surveys", "keyword_pub": "Jets ; Star formation ; Interstellar molecules", "abstract": ["Using the Purple Mountain Observatory 13.7m millimeter telescope at", "Delingha in China, we have conducted a large-scale simultaneous survey", "of ^12^CO, ^13^CO, and C^18^O (J=1-0) toward the CMa OB1 complex with", "a sky coverage of 16.5deg^2^ (221.5{deg}<=l<=227{deg},", "-2.5{deg}<=b<=0.5{deg}). Emission from the CMa OB1 complex is found in", "the range 7km/s<=V_LSR_<=25km/s. The large-scale structure, physical", "properties, and chemical abundances of the molecular clouds are", "presented. A total of 83 C^18^O molecular clumps are identified with", "the GaussClumps algorithm within the mapped region. We find that 94%", "of these C18O molecular clumps are gravitationally bound. The", "relationship between their size and mass indicates that none of the", "C^18^O clumps has the potential to form high-mass stars. Using a", "semiautomatic IDL algorithm, we newly discover 85 CO outflow", "candidates in the mapped area, including 23 bipolar outflow", "candidates. Additionally, a comparative study reveals evidence for a", "significant variety of physical properties, evolutionary stages, and", "levels of star formation activity in different subregions of the CMa", "OB1 complex."], "description": ["In this paper, we present a new J=1-0 ^12^CO/^13^CO/C^18^O survey", "toward the CMa OB1 complex with a sky coverage of 16.5deg^2^", "(221.5{deg}<=l<=227{deg}, -2.5{deg}<=b<=0.5{deg}), which is part of", "the ongoing Milky Way Imaging Scroll Painting project (MWISP,", "Su+ 2019ApJS..240....9S).", "The observations used in this study were conducted during", "2017 September - 2018 April using the 13.7m millimeter-wavelength", "telescope of the Purple Mountain Observatory in Delingha, China."], "type": ["OC"], "data": "", "date_update": "22-Apr-2021", "tables": [{"name": "tablea1.dat", "desc": "The physical properties of C^18^O clumps ", "columns": [{"name": "Name", "desc": "Name of each clump, as defined by its central Galactic Coordinates, GLLL.lll+/-BB.bbb"}, {"name": "VLSR", "desc": "[9.9/20.7] Central velocity "}, {"name": "dv", "desc": "[0.17/0.8] Clump velocity dispersion "}, {"name": "TC18O", "desc": "[1.2/3.7] Peak main beam temperature of the C^18^O emission peak fitted by GaussClumps"}, {"name": "T12CO", "desc": "[3.9/22] Main beam temperature of ^12^CO peak within the same area of clumps in ^12^CO data"}, {"name": "Area", "desc": "[3.4/44] Angular area of each clump, estimated by GaussClumps"}, {"name": "Tex", "desc": "[7.2/25.4] Excitation temperature "}, {"name": "tau", "desc": "[0.07/0.6] Optical depth "}, {"name": "sigma-T", "desc": "[0.16/0.3] Thermal velocity dispersion "}, {"name": "sigma-NT", "desc": "[0.16/0.8] Non-thermal velocity dispersion "}, {"name": "Reff", "desc": "[0.3/1.3] Effective radius "}, {"name": "MLTE", "desc": "[22/979] LTE mass "}, {"name": "Mvir", "desc": "[16/540] Virial mass "}, {"name": "aVir", "desc": "[0.3/3.7] Virial parameter "}, {"name": "Seq", "desc": "Index of associated outflow candidate "}]}, {"name": "tableb1.dat", "desc": "Outflow candidates ", "columns": [{"name": "Seq", "desc": "[1/85] Outflow index "}, {"name": "GLON", "desc": "[222.4/226.6] Central Galactic longitude of outflow"}, {"name": "GLAT", "desc": "[-2.4/-0.2] Central Galactic latitude of outflow "}, {"name": "bw0", "desc": "[5.8/15.1]? Velocity range, min, of the blue line wing"}, {"name": "bw1", "desc": "[7.6/16.8]? Velocity range, max, of the blue line wing"}, {"name": "rw0", "desc": "[11.4/22.1]? Velocity range, min, of the red line wing"}, {"name": "rw1", "desc": "[14/26.7]? Velocity range, max, of the red line wing"}, {"name": "Type", "desc": "[BDR] Outflow Type (1) "}]}, {"name": "tablec1.dat", "desc": "Physical properties of the outflow candidates ", "columns": [{"name": "Seq", "desc": "[1/85] Index of outflow candidate "}, {"name": "Lobe", "desc": "[BR] Type of lobe candidate, B=Blue; R=Red "}, {"name": "GLON", "desc": "[222.4/226.6] Central Galactic longitude of lobe"}, {"name": "GLAT", "desc": "[-2.4/-0.2] Central Galactic latitude of lobe"}, {"name": "Vpk", "desc": "[8.3/21] Velocity of 12CO peak emission "}, {"name": "psi", "desc": "[0.5/0.95] Lowest contour boundary of each lobe (1)"}, {"name": "Area", "desc": "[1.2/9.5] Angular area of each lobe, defined by the lowest contour level of each lobe"}, {"name": "dv-lobe", "desc": "[-7.1/7.3] Velocity, outflow lobe candidate (2)"}, {"name": "l-lobe", "desc": "[0.6/1.9] Length, outflow lobe candidate, parsecs (2)"}, {"name": "M-lobe", "desc": "[0.03/1.2] Mass, outflow lobe candidate, solar units (2)"}, {"name": "Pmom", "desc": "[0.05/5.3] Momentum, outflow lobe candidate (2)"}, {"name": "E", "desc": "[1e+40/3.2e+44] Kinetic energy (2) "}, {"name": "t", "desc": "[78900/576000] Dynamical timescale (2) "}, {"name": "Lum", "desc": "[8.8e+28/8.6e+31] Luminosity (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_252_21"}} {"id": "J/ApJS/252/21", "title_cds": "Multiwavelength survey of WR stars in LMC", "title_create": "Hung+, 2021", "year": "2021", "author": "Hung C.S., Ou P.-S., Chu Y.-H., Gruendl R.A., Li C.-J.", "title_pub": "A multiwavelength survey of Wolf-Rayet nebulae in the Large Magellanic Cloud.", "first_author": "Hung C.S.", "ref_biblio": [""], "bibcode": ["2021ApJS..252...21H"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "VII/232 : Nebulae in the Magellanic Clouds (Davies+ 1976)", "J/ApJ/448/179 : HST photometry in R136 (Hunter+ 1995)", "J/AJ/132/2268 : SAGE calibration stars (Meixner+, 2006)", "J/A+A/585/A162 : X-ray supernova remnants in LMC (Maggi+, 2016)", "J/ApJ/863/181 : The fifth catalog of LMC Wolf-Rayet stars (Neugent+, 2018)"], "keyword_cds": "Stars, Wolf-Rayet; Interstellar medium; Magellanic Clouds; Cross identifications; H I data", "keyword_pub": "Wolf-Rayet stars ; Stellar wind bubbles ; Interstellar medium ; Large Magellanic Cloud", "abstract": ["Surveys of Wolf-Rayet (WR) stars in the Large Magellanic Cloud (LMC)", "have yielded a fairly complete catalog of 154 known stars. We have", "conducted a comprehensive, multiwavelength study of the", "interstellar/circumstellar environments of WR stars, using the", "Magellanic Cloud Emission Line Survey images in the H{alpha}, [OIII],", "and [SII] lines; Spitzer Space Telescope 8 and 24{mu}m images; Blanco", "4m Telescope H{alpha} CCD images; and Australian Telescope Compact", "Array + Parkes Telescope HI data cube of the LMC. We have also", "examined whether the WR stars are in OB associations, classified the", "HII environments of WR stars, and used this information to", "qualitatively assess the WR stars' evolutionary stages. The 30 Dor", "giant HII region has active star formation and hosts young massive", "clusters, thus we have made statistical analyses for 30 Dor and the", "rest of the LMC both separately and altogether. Due to the presence of", "massive young clusters, the WR population in 30 Dor is quite different", "from that from elsewhere in the LMC. We find small bubbles (<50pc", "diameter) around ~12% of WR stars in the LMC, most of which are WN", "stars and not in OB associations. The scarcity of small WR bubbles is", "discussed. Spectroscopic analyses of abundances are needed to", "determine whether the small WR bubbles contain interstellar medium or", "circumstellar medium. Implications of the statistics of interstellar", "environments and OB associations around WR stars are discussed.", "Multiwavelength images of each LMC WR star are presented."], "description": ["We have used multiwavelength images to examine the ionized and neutral", "gaseous environments of the LMC Wolf-Rayet (WR) stars.", "The UM/CTIO Magellanic Cloud Emission-line Survey (MCELS) is an", "emission-line survey of the Magellanic Clouds (Smith & MCELS Team", "1999IAUS..190...28S). The survey used the Curtis Schmidt Telescope at", "Cerro Tololo Inter-American Observatory (CTIO) and a CCD camera to", "take images in the H{alpha}, [OIII]5007, and [SII]6716,6731 bands, as", "well as two continuum bands centered at {lambda}6850 and {lambda}5130.", "In this paper, we only used the emission-line images without continuum", "subtraction.", "A higher-resolution H{alpha} survey of the Magellanic Clouds has been", "conducted with the MOSAIC II camera on the Blanco 4m Telescope at", "CTIO; this survey has been called MCELS2 (PI: You-Hua Chu).", "In celebration of the 30yr anniversary of the Hubble Space Telescope", "(HST), a public release of an HST H{alpha} image of NGC 2020 became", "available, and this image is used for WR 71.", "The HI 21cm data cube was constructed by Kim+ (2003ApJS..148..473K)", "using the ATCA survey data in conjunction with single-dish observations", "from the Parkes Telescope.", "The Spitzer Space Telescope Infrared Array Camera (IRAC) 8um images", "are used to identify polycyclic aromatic hydrocarbons associated with", "partially dissociated regions, and the Multiband Imaging Photometer", "for Spitzer (MIPS) 24um images to reveal emission from heated dust.", "The Spitzer images of the LMC were from the Legacy Program Surveying", "the Agents of a Galaxy's Evolution (SAGE; Meixner+ 2006, J/AJ/132/2268)."], "type": ["CCC"], "data": "", "date_update": "22-Apr-2021", "tables": [{"name": "table1.dat", "desc": "LMC WR stars and their stellar and interstellar environments", "columns": [{"name": "Seq", "desc": "[1/154] Running sequence number of the WR star in Neugent+ 2018, J/ApJ/863/181"}, {"name": "RAh", "desc": "Hour of right ascension (J2000) "}, {"name": "RAm", "desc": "Minute of right ascension (J2000) "}, {"name": "RAs", "desc": "Second of right ascension (J2000) "}, {"name": "DE-", "desc": "Sign of declination (J2000) "}, {"name": "DEd", "desc": "Degree of declination (J2000) "}, {"name": "DEm", "desc": "Arcminute of declination (J2000) "}, {"name": "DEs", "desc": "Arcsecond of declination (J2000) "}, {"name": "BAT99", "desc": "ID from Breysacher+ (1999A&AS..137..117B) "}, {"name": "Brey", "desc": "ID from Breysacher (1981A&AS...43..203B) "}, {"name": "SpT", "desc": "Spectral type from Neugent+ 2018, J/ApJ/863/181 "}, {"name": "LH", "desc": "Host OB association from Lucke & Hodge (1970AJ.....75..171L) (1)"}, {"name": "LHA", "desc": "Associated HII regions from Henize (1956ApJS....2..315H ; in Simbad)"}, {"name": "DEML", "desc": "Associated HII regions from Davies+ (1976MmRAS..81...89D)"}, {"name": "Morph", "desc": "HII morphology classification "}, {"name": "u_Morph", "desc": "Uncertainty flag on Morph "}, {"name": "Buble", "desc": "Dimensions of any bubble associated with the WR star"}, {"name": "u_Buble", "desc": "Uncertainty flag on Buble "}, {"name": "SBuble", "desc": "Dimensions of any superbubble associated with the WR star"}, {"name": "u_SBuble", "desc": "Uncertainty flag on Buble "}, {"name": "LMC", "desc": "HII supergiant shells from Meaburn (1980MNRAS.192..365M ; in Simbad)"}, {"name": "[KDS99]", "desc": "HI giant and supergiant shells from Kim+ (1999AJ....118.2797K ; GS= giant shell, SGS = supergiant shell)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_252_23"}} {"id": "J/ApJS/252/23", "title_cds": "E(V-I) reddening map of MCs from OGLE-IV RC stars", "title_create": "Skowron+, 2021", "year": "2021", "author": "Skowron D.M., Skowron J., Udalski A., Szymanski M.K., Soszynski I., Wyrzykowski L., Ulaczyk K., Poleski R., Kozlowski S., Pietrukowicz P., Mroz P., Rybicki K., Iwanek P., Wrona M., Gromadzki M.", "title_pub": "OGLE-ing the Magellanic System: optical reddening maps of the Large and Small Magellanic Clouds from Red Clump stars.", "first_author": "Skowron D.M.", "ref_biblio": [""], "bibcode": ["2021ApJS..252...23S"], "see_also": ["J/A+AS/121/95 : Giant stars abundances in 24 clusters (Carretta+ 1997)", "J/AJ/116/723 : LMC star clusters ages and metallicity (Bica+ 1998)", "J/AcA/49/223 : BVI photometry of OGLE LMC Cepheids (Udalski+, 1999)", "J/AcA/49/437 : BVI photometry of OGLE SMC Cepheids (Udalski+, 1999)", "J/AJ/123/855 : Magellanic Clouds Photometric Survey: the SMC (Zaritsky+, 2002)", "J/AJ/128/1606 : Magellanic Clouds Photometric Survey: the LMC (Zaritsky+, 2004)", "J/A+A/430/421 : Reddening in LMC bar region (Subramaniam, 2005)", "J/AJ/132/1630 : CaII spectroscopy in MC clusters (Grocholski+, 2006)", "J/MNRAS/377/300 : CT1 photometry in 6 SMC star clusters (Piatti+, 2007)", "J/MNRAS/389/678 : Extended objects in Magellanic Clouds (Bica+, 2008)", "J/AJ/136/1703 : Ridgelines of six intermediate-age SMC clusters (Glatt+, 2008)", "J/AJ/138/517 : CaII spectroscopy of SMC red giants (Parisi+, 2009)", "J/A+A/554/A33 : VMC Survey. VII. 30 Doradus reddening map (Tatton+, 2013)", "J/MNRAS/442/1680 : Red giants in SMC. Abundances (Dobbie+, 2014)", "J/ApJ/780/59 : Araucaria project: eclipsing binaries in SMC (Graczyk+, 2014)", "J/ApJ/795/108 : Stellar populations in the Magellanic bridge (Skowron+, 2014)", "J/A+A/591/A11 : SMC BV photometry of 9 star cluster fields (Dias+, 2016)", "J/AJ/151/144 : ASPCAP weights for APOGEE chemical elements (Garcia+, 2016)", "J/ApJ/832/176 : Classical Cepheids in MCs. I. LMC disk (Inno+, 2016)", "J/AJ/152/58 : CaII spectroscopy of SMC red giants. IV. (Parisi+, 2016)", "J/AcA/66/131 : VI light curves of SMC and LMC RR Lyrae (Soszynski+, 2016)", "J/A+A/605/A89 : Abund. of microlensed Bulge dwarf stars. VI. (Bensby+, 2017)", "J/AJ/154/199 : Survey of the MAgellanic Stellar History (Nidever+, 2017)", "J/AcA/67/363 : New star clusters in the Magellanic system (Sitek+, 2017)", "J/ApJ/860/1 : Radial velocity measurements of 20 EBs in LMC (Graczyk+, 2018)", "J/A+A/628/A51 : Magellanic Clouds reddening map (Joshi+, 2019)", "http://ogle.astrouw.edu.pl/cgi-ogle/get_ms_ext.py : E(V-I) Reddening Map in"], "keyword_cds": "Magellanic Clouds; Extinction; Reddening; Colors; Surveys", "keyword_pub": "Interstellar dust extinction ; Magellanic Clouds ; Red giant clump", "abstract": ["We present the most extensive and detailed reddening maps of the", "Magellanic Clouds (MCs) derived from the color properties of Red Clump", "(RC) stars. The analysis is based on the deep photometric maps from", "the fourth phase of the Optical Gravitational Lensing Experiment", "(OGLE-IV), covering approximately 670deg^2^ of the sky in the", "Magellanic System region. The resulting maps provide reddening", "information for 180deg^2^ in the Large Magellanic Cloud (LMC) and", "75deg^2^ in the Small Magellanic Cloud (SMC), with a resolution of", "1.7'x1.7' in the central parts of the MCs, decreasing to approximately", "27'x27' in the outskirts. The mean reddening is E(V-I)=0.100+/-0.043mag", "in the LMC and E(V-I)=0.047+/-0.025mag in the SMC. We refine methods", "of calculating the RC color to obtain the highest possible accuracy of", "reddening maps based on RC stars. Using spectroscopy of red giants, we", "find the metallicity gradient in both MCs, which causes a slight", "decrease of the intrinsic RC color with distance from the galaxy", "center of ~0.002mag/deg in the LMC and between 0.003 and 0.009mag/deg", "in the SMC. The central values of the intrinsic RC color are 0.886 and", "0.877mag in the LMC and SMC, respectively."], "description": ["The 1.3m telescope of the OGLE survey is located at the Las Campanas", "Observatory in Chile and has been observing the southern sky since", "1996 on a nightly basis. The fourth phase of the project started in", "2010, when a new 32 chip mosaic CCD camera with a 1.4deg^2^ total field", "of view was installed on the telescope. Since then, OGLE-IV has been", "observing the Magellanic System in the I and V bands with a cadence of", "1-4 days, later reduced to about 10 days in the sparsely populated", "regions of the Magellanic Bridge and the outskirts of the Magellanic", "Clouds (MCs).", "For technical details on the OGLE-IV survey, please refer to Udalski+", "(2015AcA....65....1U)."], "type": ["OC"], "data": "", "date_update": "23-Apr-2021", "tables": [{"name": "table1.dat", "desc": "E(V-I) reddening map based on Red Clump (RC) stars color from the OGLE-IV survey", "columns": [{"name": "Box", "desc": "[3.4/27.5] Box size "}, {"name": "RAh", "desc": "[-0.03/6.74] Right Ascension in decimal hour (J2000)"}, {"name": "DEdeg", "desc": "[-77.53/-60.62] Declination in decimal degrees (J2000)"}, {"name": "E(V-I)", "desc": "[0/0.7] Median (V-I) color excess "}, {"name": "e_E(V-I)", "desc": "[0.015/0.5] Lower 34% sigma uncertainty "}, {"name": "E_E(V-I)", "desc": "[0.014/0.6] Upper 34% sigma uncertainty "}, {"name": "(V-I)RC", "desc": "[0.8/1.6] Red clump (V-I) color index "}, {"name": "(V-I)0", "desc": "[0.8/0.9] Intrinsic (V-I) color index "}, {"name": "E(V-I)p", "desc": "[0/0.76] Peak (V-I) color excess "}, {"name": "E(V-I)SFD", "desc": "[0.02/36.3] E(V-I) based on dust infrared emission"}]}, {"name": "fig15/*", "desc": "FITS images of E(V-I), e_E(V-I), E_(V-I), Median (V-I), Intrinsic (V-I), E(V-I) mode and box size", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_252_27"}} {"id": "J/ApJS/252/27", "title_cds": "WWFI g'-band obs. of bright galaxy clusters", "title_create": "Kluge+, 2021", "year": "2021", "author": "Kluge M., Bender R., Riffeser A., Goessl C., Hopp U., Schmidt M., Ries C.", "title_pub": "Photometric dissection of intracluster light and its correlations with host cluster properties.", "first_author": "Kluge M.", "ref_biblio": [""], "bibcode": ["2021ApJS..252...27K"], "see_also": ["I/259 : The Tycho-2 Catalogue (Hog+ 2000)", "VII/110 : Rich Clusters of Galaxies (Abell+ 1989)", "J/ApJ/664/226 : Nuker law parameters of early-type galaxies (Lauer+, 2007)", "J/MNRAS/379/867 : BCG C4 cluster catalog (von der Linden+, 2007)", "J/ApJS/182/216 : Surface photometry of Virgo ellipticals (Kormendy+, 2009)", "J/ApJS/195/15 : Luminosity profiles of BCGs (Donzelli+, 2011)", "J/ApJ/797/82 : Brightest cluster galaxies in Abell clusters (Lauer+, 2014)", "J/A+A/609/A78 : MUSE combined data cubes for NGC 3311 (Barbosa+, 2018)", "J/ApJS/247/43 : WWFI g'-band obs. of bright cluster galaxies (Kluge+, 2020)"], "keyword_cds": "Clusters, galaxy; Velocity dispersion; Optical", "keyword_pub": "Brightest cluster galaxies ; Galaxy clusters ; Galaxy stellar halos ; Surface photometry ; Scaling relations", "abstract": ["We explore several ways to dissect brightest cluster galaxies (BCGs)", "and their surrounding intracluster light (ICL) using a surface", "brightness (SB) cut, a luminosity cut, excess light above a de", "Vaucouleurs profile, or a double Sersic decomposition. Assuming that", "all light above M{<}-21.85g'mag is attributable to the ICL, we find", "that an average fraction of f_ICL_^MT^=71+/-22% of all diffuse light", "centered on the BCG belongs to the ICL. Likewise, if we assume that", "all light fainter than SB>27g'mag/arcsec^2^ belongs to the ICL, the", "average ICL fraction is f_ICL_^SB27^=34+/-19% . After fitting a de", "Vaucouleurs profile to the inner parts of the SB profile, we detect", "excess light at large radii, corresponding to an average ICL fraction", "of f_ICL_^DV^=48+/-20% . Finally, by decomposing the SB profile into", "two Sersic functions, we find an average ICL fraction of", "f_ICL_^Sx^=52+/-21% associated with the outer Sersic component. Our", "measured ICL and BCG+ICL luminosities agree well with predictions from", "high-resolution simulations where the outer Sersic component traces", "the unrelaxed, accreted stellar material. BCG and ICL properties", "defined in this way are correlated with cluster parameters to study", "the coevolution of BCGs, ICL, and their host clusters. We find", "positive correlations between BCG+ICL brightness and cluster mass,", "cluster velocity dispersion, cluster radius, and integrated satellite", "brightness, confirming that BCG/ICL growth is indeed coupled with", "cluster growth. On average, the ICL is better aligned than the BCG", "with the host cluster in terms of position angle, ellipticity, and", "centering. That makes it a potential dark-matter tracer."], "description": ["Our full observational data set and data reduction pipeline are", "detailed in Kluge+ (2020, J/ApJS/247/43).", "In brief, we have observed 170 low-redshift (z>~0.08) galaxy clusters", "in the northern hemisphere (DEC>~5{deg}) with the 2m Fraunhofer", "telescope at the Wendelstein Observatory, Germany. The observations", "were taken in the g' band with the Wendelstein Wide Field Imager (WWFI)."], "type": ["OC"], "data": "", "date_update": "23-Apr-2021", "tables": [{"name": "table2.dat", "desc": "Host cluster parameters ", "columns": [{"name": "Name", "desc": "Cluster name (1) "}, {"name": "sigmac", "desc": "[123/1506]? Cluster velocity dispersion"}, {"name": "e_sigmac", "desc": "[21/1758]? Error of cluster velocity dispersion"}, {"name": "S", "desc": "[59/714]? Richness, number of galaxies in cluster"}, {"name": "Radg", "desc": "[474/1651]? Gravitational cluster radius"}, {"name": "e_Radg", "desc": "[100/467]? Error on Radg "}, {"name": "Msat", "desc": "[-27.4/-22.2]? Satellite galaxies brightness"}, {"name": "e_Msat", "desc": "[0.4/4]? Error on Msat "}, {"name": "logMg", "desc": "[13.9/15.4]? Gravitational cluster mass"}, {"name": "e_logMg", "desc": "[0.03/0.4]? Error on logMg "}, {"name": "Vsyst", "desc": "[0/1317]? BCG vs mean cluster systemic velocity offset from Lauer+2014"}, {"name": "e_Vsyst", "desc": "[30/273]? Error on Vsyst "}, {"name": "Rsyst", "desc": "[0/2065]? Radial offset between BCG and X-ray cluster center from Lauer+2014"}, {"name": "logrho", "desc": "[4.4/5.9]? log of mass density "}, {"name": "e_logrho", "desc": "[0.03/0.4]? Error on logrho "}, {"name": "logs", "desc": "[-7.7/-5.5]? Satellite galaxy number density"}, {"name": "e_logs", "desc": "[0.09/0.4]? Error on logs "}, {"name": "logfM", "desc": "[-4.2/-2.9]? Mass phase space density"}, {"name": "e_logfM", "desc": "[0.03/0.4]? Error on logfM "}, {"name": "logfs", "desc": "[-16.4/-14.2]? Number phase space density"}, {"name": "e_logfs", "desc": "[0.09/0.4]? Error on logfs "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_252_29"}} {"id": "J/ApJS/252/29", "title_cds": "BAT AGN Spectroscopic Survey. XX. Molecular gas", "title_create": "Koss+, 2021", "year": "2021", "author": "Koss M.J., Strittmatter B., Lamperti I., Shimizu T., Trakhtenbrot B., Saintonge A., Treister E., Cicone C., Mushotzky R., Oh K., Ricci C., Stern D., Ananna T.T., Bauer F.E., Privon G.C., Bar R.E., De Breuck C., Harrison F., Ichikawa K., Powell M.C., Rosario D., Sanders D.B., Schawinski K., Shao Li, Megan Urry C., Veilleux S.", "title_pub": "BAT AGN Spectroscopic Survey. XX. Molecular gas in nearby hard-X-ray-selected AGN galaxies.", "first_author": "Koss M.J.", "ref_biblio": [""], "bibcode": ["2021ApJS..252...29K"], "see_also": ["VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)", "J/ApJS/146/353 : Circumnuclear dust in galaxies (Martini+, 2003)", "J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008)", "J/ApJ/701/587 : HST H-band imaging survey. II. QUEST QSOs (Veilleux+, 2009)", "J/MNRAS/413/813 : ATLAS3D project. I. (Cappellari+, 2011)", "J/ApJ/739/57 : Ultra hard X-ray AGNs in the Swift/BAT survey (Koss+, 2011)", "J/MNRAS/415/32 : COLD GASS survey (Saintonge+, 2011)", "J/MNRAS/414/940 : ATLAS3D project. IV. (Young+, 2011)", "J/MNRAS/421/1569 : Properties of 18286 SDSS radio galaxies (Best+, 2012)", "J/ApJ/746/L22 : Dual AGNs in the nearby Universe (Koss+, 2012)", "J/MNRAS/426/2601 : CO lines in luminous IR galaxies (Papadopoulos+, 2012)", "J/A+A/541/A118 : AGN-Host Galaxy Connection (Povic+, 2012)", "J/ApJS/207/19 : Hard X-ray survey from Swift-BAT 6yrs (Baumgartner+, 2013)", "J/ApJ/765/L26 : Swift/BAT X-ray data from GOALS LIRGs (Koss+, 2013)", "J/A+A/564/A65 : Cold gas data of Herschel Reference Survey (Boselli+, 2014)", "J/ApJ/794/152 : PACS observations of Herschel-BAT sample (Melendez+, 2014)", "J/ApJS/219/1 : Catalog of Type-1 AGNs from SDSS-DR7 (Oh+, 2015)", "J/ApJ/815/L13 : Compton-thick AGNs from 70-month Swift/BAT (Ricci+, 2015)", "J/MNRAS/458/2221 : ATLAS3D Project. XXXI (Nyland+, 2016)", "J/MNRAS/457/2703 : Local SDSS galaxies in Herschel Stripe 82 (Rosario+, 2016)", "J/MNRAS/456/3335 : SPIRE observations of Herschel-BAT sample (Shimizu+, 2016)", "J/A+A/604/A53 : ALLSMOG final DR. A new APEX CO survey (Cicone+, 2017)", "J/ApJ/835/74 : IR phot. of AGNs in Swift/BAT 70 month (Ichikawa+, 2017)", "J/ApJ/850/74 : Swift/BAT AGN Spectroscopic Survey. I. (Koss+, 2017)", "J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray (Ricci+, 2017)", "J/ApJS/233/22 : xCOLD GASS catalog (Saintonge+, 2017)", "J/MNRAS/466/3161 : AGN global star-forming properties (Shimizu+, 2017)", "J/A+A/609/A9 : Local Swift-BAT AGN observed with Herschel (Lutz+, 2018)", "J/ApJ/870/31 : BAT AGN spectroscopic survey. XI. IR phot. (Ichikawa+, 2019)", "J/ApJ/881/154 : BAT AGN spectroscopic survey. XVI. Blazars (Paliya+, 2019)"], "keyword_cds": "Active gal. nuclei; Carbon monoxide; Redshifts; Molecular data; Surveys; Galaxies, Seyfert", "keyword_pub": "Active galactic nuclei ; AGN host galaxies ; Molecular gas ; Surveys ; X-ray active galactic nuclei ; Survival analysis ; Submillimeter astronomy ; High energy astrophysics ; Seyfert galaxies ; Catalogs", "abstract": ["We present the host-galaxy molecular gas properties of a sample of 213", "nearby (0.0110.5) tend to have more molecular gas and higher", "gas fractions than inactive galaxies matched in stellar mass. When", "matched in star formation, we find AGN galaxies show no difference", "from inactive galaxies, with no evidence that AGN feedback affects the", "molecular gas. The higher molecular gas content is related to AGN", "galaxies hosting a population of gas-rich early types with an order of", "magnitude more molecular gas and a smaller fraction of quenched,", "passive galaxies (~5% versus 49%) compared to inactive galaxies. The", "likelihood of a given galaxy hosting an AGN (L_bol_>10^44^erg/s)", "increases by ~10-100 between a molecular gas mass of 10^8.7^M_{sun}_", "and 10^10.2^M_{sun}_. AGN galaxies with a higher Eddington ratio", "(log(L/L_Edd_)>-1.3) tend to have higher molecular gas masses and gas", "fractions. The log(NH/cm^-2^)>23.4) of AGN galaxies with higher column", "densities are associated with lower depletion timescales and may", "prefer hosts with more gas centrally concentrated in the bulge that", "may be more prone to quenching than galaxy-wide molecular gas. The", "significant average link of host-galaxy molecular gas supply to", "supermassive black hole (SMBH) growth may naturally lead to the", "general correlations found between SMBHs and their host galaxies, such", "as the correlations between SMBH mass and bulge properties, and the", "redshift evolution of star formation and SMBH growth."], "description": ["Our AGN parent sample consists of 836 ultrahard-X-ray-selected", "(14-195keV) AGN included in the 70-month Swift-BAT all-sky catalog", "(Baumgartner+ 2013, J/ApJS/207/19).", "In total, 200 AGN galaxies were newly observed: 165 with the Atacama", "Pathfinder Experiment (APEX) and 35 with the James Clerk Maxwell", "Telescope (JCMT), while 13 were obtained from the literature", "(see col. Tel in table 2 and Section 2.1.3).", "The APEX 12m antenna observations totalled 254hr with 2288 400s long", "scans, taken over 67 days between 2016 March and 2017 September. The", "observing programs involved were mainly an ESO Large program", "(PI M. Koss, ~150hr), a follow-up ESO program (PI B. Trakthenbrot,", "~50hr), and Chilean time (PI E. Treister, ~75hr). In addition to our", "own programs, we also reduced data from archival programs for six BAT", "AGN galaxies.", "We observed the CO(2-1) transition (v_rest_=230.538GHz) using the", "Swedish Heterodyne Facility Instrument (SHFI) with the eXtended Fast", "Fourier Transform Spectrometer (XFFTS) backend (213-275GHz).", "JCMT observations of the CO(2-1) molecular line were taken between", "2011 February and 2013 April. Archival data for one additional galaxy", "were also reduced (NGC 6240). We used the A3 (211-279GHz) receiver", "with the ACSIS spectrometer with a beam size of 20.4\" HPBW.", "The results for the complementary sample of z<0.01 BAT AGN galaxies", "are presented in Rosario+ (2018MNRAS.473.5658R)."], "type": ["OC"], "data": "", "date_update": "23-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Multiwavelength properties of the BAT AGN galaxy sample", "columns": [{"name": "BAT", "desc": "[1/1413] Catalog ID in the BAT survey "}, {"name": "Name", "desc": "Galaxy Name, optical/IR counterpart to AGN "}, {"name": "RAdeg", "desc": "[0.2/352.3] Counterpart Right Ascension (J2000) "}, {"name": "DEdeg", "desc": "[-78.9/63.7] Counterpart declination (J2000) "}, {"name": "Type", "desc": "AGN type "}, {"name": "zspec", "desc": "[0.01/0.05] Redshift (1) "}, {"name": "rk20fe", "desc": "[5/82] Isophotal radius (2) "}, {"name": "Incl", "desc": "[18/89] Inclination angle (3) "}, {"name": "Morph", "desc": "Morphological classification (4) "}, {"name": "logM*", "desc": "[9.4/11.4] log of stellar masses of the BAT AGN host galaxies (5)"}, {"name": "l_SFR", "desc": "Limit flag on SFR "}, {"name": "SFR", "desc": "[0/132]? Star formation rate (6) "}, {"name": "l_D(MS)", "desc": "Limit flag on DMS "}, {"name": "D(MS)", "desc": "[-10.3/2.2]? Offset from the Main Sequence of star-formation (7)"}]}, {"name": "table2.dat", "desc": "Catalog of CO(2-1) measurements ", "columns": [{"name": "BAT", "desc": "[1/1413] Catalog ID in the BAT survey"}, {"name": "Name", "desc": "Galaxy Name, optical/IR counterpart to AGN"}, {"name": "Tel", "desc": "Telescope used for the CO observation (1)"}, {"name": "HPBW", "desc": "[20/32] Associated beam size "}, {"name": "FlagCO21", "desc": "[0/1] Detection flag for the CO(2-1) line (1=detection) (2)"}, {"name": "sigma-CO21", "desc": "[0.4/17.1]? RMS noise achieved around the CO(1-0) line (3)"}, {"name": "C-aper", "desc": "[1.0/8.71] Beam correction factor (4)"}, {"name": "SN-inte", "desc": "[-3/39.5] Signal-to-noise, integrated line"}, {"name": "L-inte", "desc": "[0.2/105.5] Total CO(2-1) line luminosity from integrated"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_252_32"}} {"id": "J/ApJS/252/32", "title_cds": "MIR outbursts in nearby SDSS gal. (MIRONG). I.", "title_create": "Jiang+, 2021", "year": "2021", "author": "Jiang N., Wang T., Dou L., Shu X., Hu X., Liu H., Wang Y., Yan L., Sheng Z., Yang C., Sun L., Zhou H.", "title_pub": "Mid-infrared outbursts in nearby galaxies (MIRONG). I. Sample selection and characterization.", "first_author": "Jiang N.", "ref_biblio": [""], "bibcode": ["2021ApJS..252...32J"], "see_also": ["II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)", "II/328 : AllWISE Data Release (Cutri+ 2013)", "V/147 : The SDSS Photometric Catalogue, Release 12 (Alam+, 2015)", "J/ApJ/670/92 : New sample of low-mass black holes in AGN (Greene+, 2007)", "J/ApJ/696/870 : Catalina Real-time Transient Survey (CRTS) (Drake+, 2009)", "J/ApJ/793/38 : Palomar Transient Factory photometric obs. (Arcavi+, 2014)", "J/ApJ/788/159 : 17 Seyfert 1 galaxies light curves (Koshida+, 2014)", "J/ApJ/792/30 : NEOWISE magnitudes for near-Earth objects (Mainzer+, 2014)", "J/ApJ/788/45 : Luminosity & redshift of galaxies from WISE/SDSS (Toba+, 2014)", "J/ApJ/788/48 : X-ray through NIR photometry of NGC 2617 (Shappee+, 2014)", "J/ApJS/219/8 : SFR for WISE + SDSS spectroscopic galaxies (Chang+, 2015)", "J/ApJ/813/82 : z<0.06 broad-line AGN emission-line measures (Reines+, 2015)", "J/ApJ/831/168 : 6GHz JVLA obs. of low-z SDSS quasars (Kellermann+, 2016)", "J/ApJ/844/46 : Phot. of the transient event iPTF16fnl (Blagorodnova+, 2017)", "J/ApJ/839/88 : 14 unusual IR transients with Spitzer (Kasliwal+, 2017)", "J/MNRAS/481/307 : Gaia Nuclear Transients (GNTs) (Kostrzewa-Rutkowska+, 2018)", "J/ApJ/866/44 : WISE/DEIMOS Redshift Catalog DR2 & extended data (Lake+, 2018)", "J/ApJ/852/72 : Luminosities tidal disruption flares (van Velzen, 2018)", "J/ApJS/243/21 : A complete sample of broad-line AGN from SDSS-DR7 (Liu+, 2019)"], "keyword_cds": "Active gal. nuclei; Photometry, infrared; Magnitudes, absolute; Velocity dispersion; Black holes; Stars, masses", "keyword_pub": "Time domain astronomy ; Tidal disruption ; Active galactic nuclei ; Infrared astronomy", "abstract": ["Optical time-domain astronomy has grown rapidly in the past decade,", "but the dynamic infrared sky is rarely explored. Aiming to construct a", "sample of mid-infrared outbursts in nearby galaxies (MIRONG), we have", "conducted a systematical search of low-redshift (z<0.35) Sloan Digital", "Sky Survey spectroscopic galaxies that have experienced recent", "mid-infrared (MIR) flares using their Wide-field Infrared Survey", "Explorer (WISE) light curves. A total of 137 galaxies have been", "selected by requiring a brightening amplitude of 0.5mag in at least", "one WISE band with respect to their quiescent phases. Only a small", "fraction (10.9%) has corresponding optical flares. Except for the four", "supernovae (SNe) in our sample, the MIR luminosities of the remaining", "sources (L_4.6{mu}m_>10^42^erg/s) are markedly brighter than known", "SNe, and their physical locations are very close to the galactic", "center (median <0.1\"). Only four galaxies are radio-loud, indicating", "that synchrotron radiation from relativistic jets could contribute to", "MIR variability. We propose that these MIR outbursts are dominated by", "the dust echoes of transient accretion onto supermassive black holes,", "such as tidal disruption events (TDEs) and turn-on (changing-look)", "active galactic nuclei. Moreover, the inferred peak MIR luminosity", "function is generally consistent with the X-ray and optical TDEs at", "the high end, albeit with large uncertainties. Our results suggest", "that a large population of transients has been overlooked by optical", "surveys, probably due to dust obscuration or intrinsically optical", "weakness. Thus, a search in the infrared band is crucial for us to", "obtain a panoramic picture of nuclear outburst. The multiwavelength", "follow-up observations of the MIRONG sample are in progress and will", "be presented in a series of subsequent papers."], "description": ["MIR outbursts in nearby galaxies (MIRONG) uses both the public WISE", "and NEOWISE databases to search for more recent outburst events in", "galaxies.", "WISE performed a full-sky imaging survey in four broad bandpasses", "centered at 3.4, 4.6, 12, and 22um (labeled W1-W4) from 2010 January", "to August. WISE continued surveying the sky in its bluest three bands", "during 2010 August and September. After that, NEOWISE hunted asteroids", "until 2011 February, with only the W1 and W2 channels. Following a 33", "month hibernation period, the WISE instrument recommenced survey", "operations in 2013 December (Mainzer+ 2014, J/ApJ/792/30). This", "posthibernation mission is referred to as NEOWISE-Reactivation (NEOWISE-R).", "Our sample selection is based on the WISE and NEOWISE-R data from 2010", "to the end of 2018."], "type": ["CCC"], "data": "", "date_update": "23-Apr-2021", "tables": [{"name": "table1.dat", "desc": "The properties of MIR flares ", "columns": [{"name": "---", "desc": "[SDSS] "}, {"name": "SDSS", "desc": "SDSS name (JHHMMSS.ss+DDMMSS.s) "}, {"name": "RAdeg", "desc": "Right ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "z", "desc": "[0.0079/0.4] SDSS redshift "}, {"name": "DelW1", "desc": "[0.1/3] Amplitude of variability in W1 (3.4um) "}, {"name": "e_DelW1", "desc": "[0.01/0.2] DelW1 uncertainty "}, {"name": "DelW2", "desc": "[0.5/3.6] Amplitude of variability in W2 (4.6um) "}, {"name": "e_DelW2", "desc": "[0.01/0.3] DelW2 uncertainty "}, {"name": "W1Mag", "desc": "[-27.4/-17.6] Peak absolute magnitude in W1 "}, {"name": "e_W1Mag", "desc": "[0.01/0.6] Uncertainty on the W1Mag "}, {"name": "W2Mag", "desc": "[-28.3/-18.4] Peak absolute magnitude in W2 "}, {"name": "e_W2Mag", "desc": "[0.01/0.3] Uncertainty on the W2Mag "}, {"name": "W1Lum", "desc": "[40.5/44.5] Peak monochromatic luminosity of W1 "}, {"name": "e_W1Lum", "desc": "[0/0.3] W1Lum uncertainty "}, {"name": "W2Lum", "desc": "[40.5/44.5] Peak monochromatic luminosity of W2 "}, {"name": "e_W2Lum", "desc": "[0/0.2] W2Lum uncertainty "}, {"name": "Deld", "desc": "[0.01/1.5] Offset distance between the maximum outburst epoch and the quiescent state"}]}, {"name": "table3.dat", "desc": "The fitted dust parameters ", "columns": [{"name": "---", "desc": "[SDSS] "}, {"name": "AName", "desc": "SDSS abbreviated name (JHHMM+DDMM) "}, {"name": "Tbb", "desc": "[560/2541] Dust temperature fitted with the blackbody model at the epoch of W2 luminosity maximum"}, {"name": "e_Tbb", "desc": "[5/476] Tbb uncertainty "}, {"name": "logLbb", "desc": "[40.6/44.6] Luminosity fitted with the blackbody model at the epoch of W2 luminosity maximum"}, {"name": "e_logLbb", "desc": "[0.02/0.5] LogLbb uncertainty "}, {"name": "logMbb", "desc": "[-5.9/-1.1] Mass fitted with the blackbody model at the epoch of W2 luminosity maximum"}, {"name": "e_logMbb", "desc": "[0.02/0.6] LogMbb uncertainty "}, {"name": "logRbb", "desc": "[-3.1/-0.6] Distance of the dust to the central heating source (1)"}, {"name": "e_logRbb", "desc": "[0.01/0.4] LogRbb uncertainty "}, {"name": "Td", "desc": "[516/1657] Dust temperature fitted with the dust absorption coefficient"}, {"name": "e_Td", "desc": "[4/179] Td uncertainty "}, {"name": "logLd", "desc": "[40.6/44.6] Luminosity fitted with the dust absorption coefficient"}, {"name": "e_logLd", "desc": "[0.01/0.5] LogLd uncertainty "}, {"name": "logMd", "desc": "[-4.9/-0.3] Mass fitted with the dust absorption coefficient"}, {"name": "e_logMd", "desc": "[0.02/0.6] LodMd uncertainty "}, {"name": "logRd", "desc": "[-2.6/-0.2] Distance of the dust to the central heating source (1)"}, {"name": "e_logRd", "desc": "[0.02/0.6] LogRd uncertainty "}]}, {"name": "table5.dat", "desc": "The properties of the host galaxies and BH ", "columns": [{"name": "---", "desc": "[SDSS] "}, {"name": "AName", "desc": "SDSS abbreviated name (JHHMM+DDMM) "}, {"name": "rMag", "desc": "[-22.9/-15.9] SDSS absolute r-band magnitude after k-correction to 0.1"}, {"name": "g-r", "desc": "[0.3/1.3] SDSS g-r color index after k-correction to 0.1"}, {"name": "sigma", "desc": "? Stellar velocity dispersion "}, {"name": "logM*", "desc": "[7.9/11.6] Stellar mass "}, {"name": "logSFR", "desc": "[-4.5/1.9] Log of stellar formation rate "}, {"name": "logMBH", "desc": "[4.3/9] Estimated BH mass "}, {"name": "Type", "desc": "Classification in the BPT diagram "}, {"name": "n_Type", "desc": "[b] b: robust broad H{alpha} detection "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_ApJS_253_3"}} {"id": "J/ApJS/253/3", "title_cds": "Sunyaev-Zel'dovich galaxy clusters surveyed by ACT", "title_create": "Hilton+, 2021", "year": "2021", "author": "Hilton M., Sifon C., Naess S., Madhavacheril M., Oguri M., Rozo E., Rykoff E., Abbott T.M.C., Adhikari S., Aguena M., Aiola S., Allam S., Amodeo S., Amon A., Annis J., Ansarinejad B., Aros-Bunster C., Austermann J.E., Avila S., Bacon D., Battaglia N., Beall J.A., Becker D.T., Bernstein G.M., Bertin E., Bhandarkar T., Bhargava S., Bond J.R., Brooks D., Burke D.L., Calabrese E., Carrasco Kind M., Carretero J., Choi S.K., Choi A., Conselice C., da Costa L.N., Costanzi M., Crichton D., Crowley K.T., Dunner R., Denison E.V., Devlin M.J., Dicker S.R., Diehl H.T., Dietrich J.P., Doel P., Duff S.M., Duivenvoorden A.J., Dunkley J., Everett S., Ferraro S., Ferrero I., Ferte A., Flaugher B., Frieman J., Gallardo P.A., Garcia-Bellido J., Gaztanaga E., Gerdes D.W., Giles P., Golec J.E., Gralla M.B., Grandis S., Gruen D., Gruendl R.A., Gschwend J., Gutierrez G., Han D., Hartley W.G., Hasselfield M., Hill J.C., Hilton G.C., Hincks A.D., Hinton S.R., Ho S.-P.P., Honscheid K., Hoyle B., Hubmayr J., Huffenberger K.M., Hughes J.P., Jaelani A.T., Jain B., James D.J., Jeltema T., Kent S., Knowles K., Koopman B.J., Kuehn K., Lahav O., Lima M., Lin Y.-T., Lokken M., Loubser S.I., MacCrann N., Maia M.A.G., Marriage T.A., Martin J., McMahon J., Melchior P., Menanteau F., Miquel R., Miyatake H., Moodley K., Morgan R., Mroczkowski T., Nati F., Newburgh L.B., Niemack M.D., Nishizawa A.J., Ogando R.L.C., Orlowski-Scherer J., Page L.A., Palmese A., Partridge B., Paz-Chinchon F., Phakathi P., Plazas A.A., Robertson N.C., Romer A.K., Carnero Rosell A., Salatino M., Sanchez E., Schaan E., Schillaci A., Sehgal N., Serrano S., Shin T., Simon S.M., Smith M., Soares-Santos M., Spergel D.N., Staggs S.T., Storer E.R., Suchyta E., Swanson M.E.C., Tarle G., Thomas D., To C., Trac H., Ullom J.N., Vale L.R., Van Lanen J., Vavagiakis E.M., De Vicente J., Wilkinson R.D., Wollack E.J., Xu Z., Zhang Y.", "title_pub": "The Atacama Cosmology Telescope: a catalog of >4000 Sunyaev-Zel'dovich galaxy clusters.", "first_author": "Hilton M.", "ref_biblio": [""], "bibcode": ["2021ApJS..253....3H"], "see_also": ["II/329 : VIKING catalogue data release 1 (Edge+, 2013)", "II/343 : VIKING catalogue data release 2 (Edge+, 2016)", "II/357 : The Dark Energy Survey (DES): Data Release 1 (Abbott+, 2018)", "VII/110 : Rich Clusters of Galaxies (Abell+ 1989)", "VII/177 : Redshifts and Velocity Dispersions for Abell Clusters (Struble+ 1991)", "VII/203 : Las Campanas Redshift Survey (Shectman+ 1996)", "VIII/91 : Planck Catalog of Compact Sources Release 1 (Planck, 2013)", "J/MNRAS/269/151 : APM cluster redshift survey (Dalton+, 1994)", "J/MNRAS/274/75 : Redshifts of ROSAT X-ray brightest clusters (Crawford+, 1995)", "J/ApJ/502/558 : Catalog of ROSAT galaxy clusters (Vikhlinin+ 1998)", "J/ApJ/514/148 : ROSAT survey of bright galaxies clusters (De Grandi+, 1999)", "J/ApJS/129/435 : NORAS galaxy cluster survey. I. (Bohringer+, 2000)", "J/ApJS/126/209 : Bright SHARC survey cluster catalog (Romer+, 2000)", "J/ApJS/140/239 : RASS: clusters of galaxies around SGP (Cruddace+, 2002)", "J/MNRAS/329/87 : 2dF Galaxy Redshift Survey: clusters (de Propris+, 2002)", "J/AJ/123/1807 : SDSS galaxy clusters redshifts (Goto+, 2002)", "J/ApJ/594/154 : 160 square degree ROSAT survey (Mullis+, 2003)", "J/A+A/425/367 : REFLEX Galaxy Cluster Survey catalogue (Boehringer+, 2004)", "J/AJ/128/1558 : NOAO Fundamental Plane Survey (Smith+, 2004)", "J/AJ/128/1017 : Northern Optical Cluster Survey. IV. (Lopes+, 2005)", "J/ApJ/645/955 : ChaMP serendipitous galaxy cluster survey (Barkhouse+, 2006)", "J/MNRAS/366/645 : LARCS. 11 X-ray luminous clusters (Pimbblet+, 2006)", "J/ApJ/638/725 : Fundamental manifold of spheroids (Zaritsky+, 2006)", "J/ApJS/172/561 : The 400d cluster Survey (Burenin+, 2007)", "J/ApJ/682/821 : Spectral fits of galaxy clusters in X-ray (Cavagnolo+, 2008)", "J/AJ/137/4795 : Dynamical state of brightest cluster galaxies (Coziol+, 2009)", "J/AJ/137/2981 : Northern Optical Cluster Survey. III. (Gal+, 2009)", "J/ApJ/690/1236 : COSMOS photometric redshift catalog (Ilbert+, 2009)", "J/A+A/535/A65 : Galaxy clusters in the 4 CFHTLS Wide fields (Durret+, 2011)", "J/MNRAS/413/3059 : 4098 galaxy clusters in SDSS Stripe 82 (Geach+, 2011)", "J/ApJ/742/61 : Phot. redshift of AGNs from XMM- & C-COSMOS (Salvato+ 2011)", "J/MNRAS/423/1024 : XCS-DR1 Cluster Catalogue (Mehrtens+, 2012)", "J/ApJ/761/22 : NIR galaxy cluster candidates in the SPT survey (Song+, 2012)", "J/ApJS/199/34 : Clusters of galaxies in SDSS-III (Wen+, 2012)", "J/ApJ/763/127 : Galaxy clusters in the SPT survey (Reichardt+, 2013)", "J/ApJ/792/76 : Lensed z~6-8 galaxies behind CLASH clusters (Bradley+, 2014)", "J/ApJ/797/82 : Brightest cluster galaxies in Abell clusters (Lauer+, 2014)", "J/MNRAS/444/147 : Richness of galaxy clusters (Oguri, 2014)", "J/ApJ/785/104 : redMaPPer. I. Algorithm applied to SDSS DR8 (Rykoff+, 2014)", "J/ApJS/213/25 : WISE Massive & Distant Clusters. II. (Stanford+, 2014)", "J/ApJS/216/20 : Blanco Cosmology Survey (BCS) new reduction (Bleem+, 2015)", "J/ApJS/216/27 : Galaxy clusters in the SPT-SZ survey (Bleem+, 2015)", "J/MNRAS/446/2709 : X-ray bright AGN in massive galaxy clusters (Ehlert+, 2015)", "J/MNRAS/452/3304 : AC114 galaxy cluster dynamical analysis (Proust+, 2015)", "J/MNRAS/450/3665 : CoMaLit. III. LC2 catalog (Sereno+, 2015)", "J/ApJ/807/178 : Newly rich galaxy clusters in SDSS-DR12 (Wen+, 2015)", "J/A+A/594/A27 : Planck Sunyaev-Zeldovich sources (PSZ2) (Planck+, 2016)", "J/ApJS/224/1 : redMaPPer cluster catalog from DES data (Rykoff+, 2016)", "J/MNRAS/461/248 : 44 SZ-selected galaxy clusters ACT obs. (Sifon+, 2016)", "J/MNRAS/472/273 : OzDES DR1 (Childress+, 2017)", "J/ApJS/232/15 : Candidate strong lens systems from DES obs. (Diehl+, 2017)", "J/ApJ/878/55 : SPT-SZ clusters with optical & X-ray data (Bocquet+, 2019)", "J/ApJ/878/66 : Spec. redshifts of gal. in SPT-CLJ0615-5746 (Connor+, 2019)", "J/ApJS/240/33 : MaDCoWS. I. Catalog of z~1 galaxy clusters (Gonzalez+, 2019)", "J/ApJS/243/17 : Strong DES lens cand. from neural networks (Jacobs+, 2019)", "J/MNRAS/488/739 : MARD-Y3 catalog (Klein+, 2019)", "J/A+A/632/A34 : KiDS+VIKING-450 opt+NIR dataset (Wright+, 2019)", "J/ApJS/247/25 : The SPTpol Extended Cluster Survey (Bleem+, 2020)"], "keyword_cds": "Clusters, galaxy;", "keyword_pub": "Galaxy clusters ; Cosmology ; Large-scale structure of the universe", "abstract": ["We present a catalog of 4195 optically confirmed Sunyaev-Zel'dovich", "(SZ) selected galaxy clusters detected with signal-to-noise ratio >4", "in 13211deg^2^ of sky surveyed by the Atacama Cosmology Telescope", "(ACT). Cluster candidates were selected by applying a multifrequency", "matched filter to 98 and 150GHz maps constructed from ACT observations", "obtained from 2008 to 2018 and confirmed using deep, wide-area optical", "surveys. The clusters span the redshift range 0.041 clusters, and a total of 868", "systems are new discoveries. Assuming an SZ signal versus mass-scaling", "relation calibrated from X-ray observations, the sample has a 90%", "completeness mass limit of M_500c_>3.8x10^14^M_{sun}_, evaluated at", "z=0.5, for clusters detected at signal-to-noise ratio >5 in maps", "filtered at an angular scale of 2.4'. The survey has a large overlap", "with deep optical weak-lensing surveys that are being used to", "calibrate the SZ signal mass-scaling relation, such as the Dark Energy", "Survey (4566deg^2^), the Hyper Suprime-Cam Subaru Strategic Program", "(469deg^2^), and the Kilo Degree Survey (825deg^2^). We highlight some", "noteworthy objects in the sample, including potentially projected", "systems, clusters with strong lensing features, clusters with active", "central galaxies or star formation, and systems of multiple clusters", "that may be physically associated. The cluster catalog will be a", "useful resource for future cosmological analyses and studying the", "evolution of the intracluster medium and galaxies in massive clusters", "over the past 10Gyr."], "description": ["For this work, we use data from only the 98 and 150GHz channels of the", "Advanced ACTPol on Atacama Cosmology Telescope (ACT), which have", "approximate beam FWHM 2.2' and 1.4', respectively. The cluster search", "was performed on coadded maps containing ACT data obtained between", "2008 and 2018."], "curator": "Emmanuelle Perret [CDS]", "data": "", "date_update": "23-Apr-2021"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_BaltA_16_349"}} {"id": "J/BaltA/16/349", "title_cds": "Vilnius photometry in Collinder 428 area", "title_create": "Laugalys+, 2007", "year": "2007", "author": "Laugalys V., Straizys V., Vrba F.J., Cernis K., Kazlauskas A., Boyle R.P., Davis P.A.G.", "title_pub": "CCD photometry and classification of stars in the North America and Pelican Nebulae region. IV. The region of a supposed cluster Collinder 428.", "first_author": "Laugalys V.", "ref_biblio": [""], "bibcode": ["2007BaltA..16..349L"], "keyword_cds": "", "keyword_pub": "stars: fundamental parameters, classification - ISM: dust, extinction, clouds - ISM: individual: LDN 935 - open clusters: individual (Collinder 428, NGC6997)", "mission": "", "abstract": ["Magnitudes and color indices of 860 stars down to V=16.7mag in the", "seven-color Vilnius photometric system were obtained in the area of", "the suspected open cluster Collinder 428 in the North America Nebula.", "Spectral types, interstellar color excesses, extinctions and distances", "of stars were determined for 290 stars from the photometric data. The", "plot of extinction vs. distance gives the front edge of the dust cloud", "at 540 pc. We conclude that Collinder 428 is not a real star cluster."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "08-Oct-2016"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_BaltA_17_161"}} {"id": "J/BaltA/17/161", "title_cds": "NGC 7023 photometry", "title_create": "Zdanavicius+, 2008", "year": "2008", "author": "Zdanavicius K., Zdanavicius J., Straizys V., Kotovas A.", "title_pub": "Photometry and classification of stars around the reflection nebula NGC 7023 in Cepheus. I. A catalog of magnitudes, indices and spectral types of 1240 stars.", "first_author": "Zdanavicius K.", "ref_biblio": [""], "bibcode": ["2008BaltA..17..161Z"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Alexandra Bauer, Patricia Vannier [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_BaltA_24_157"}} {"id": "J/BaltA/24/157", "title_cds": "Visual binaries", "title_create": "Isaeva+, 2015", "year": "2015", "author": "Isaeva A.A., Kovaleva D.A., Malkov O.Y.", "title_pub": "Visual binaries: cross-matching and compiling of a comprehensive list.", "first_author": "Isaeva A.A.", "ref_biblio": [""], "bibcode": ["2015BaltA..24..157I"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1515/astro-2017-0215"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_121_337"}} {"id": "J/MNRAS/121/337", "title_cds": "Radcliffe Catalog of stars in Magellanic Clouds", "title_create": "Feast+ 1960", "year": "1960", "author": "Feast M.W., Thackeray A.D., Wesselink A.J.", "title_pub": "The brightest stars in the Magellanic Clouds.", "first_author": "Feast M.W.", "ref_biblio": [""], "bibcode": ["1960MNRAS.121..337F"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["RMC"], "type": ["OC"], "doi_pub": ["10.1093/mnras/121.4.337"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_130_45"}} {"id": "J/MNRAS/130/45", "title_cds": "Infrared survey of the region of SA 193", "title_create": "Westerlund+, 1965", "year": "1965", "author": "Westerlund B.E.", "title_pub": "An infrared survey of the region of SA 193.", "first_author": "Westerlund B.E.", "ref_biblio": [""], "bibcode": ["1965MNRAS.130...45W"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1093/mnras/130.1.45"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_202_761"}} {"id": "J/MNRAS/202/761", "title_cds": "Southern close visual double stars", "title_create": "Hurly+, 1983", "year": "1983", "author": "Hurly P.R., Warner B.", "title_pub": "Area scanner observations of close visual double stars. II. Results for 153 southern stars.", "first_author": "Hurly P.R.", "ref_biblio": [""], "bibcode": ["1983MNRAS.202..761H"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1093/mnras/202.3.761"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_267_431"}} {"id": "J/MNRAS/267/431", "title_cds": "Photographic study of A3558", "title_create": "Metcalfe+, 1994", "year": "1994", "author": "Metcalfe N., Godwin J.G., Peach J.V.", "title_pub": "Multicolour photometry of the Shapley 8 cluster of galaxies.", "first_author": "Metcalfe N.", "ref_biblio": [""], "bibcode": ["1994MNRAS.267..431M"], "see_also": ["VII/42 : GMP catalogue: galaxies in the Coma cluster (Godwin+ 1983)", "J/MNRAS/239/459 : The clusters of galaxies A2197 and A2199 (Dixon+ 1989)", "J/ApJ/485/447 : Evidence of substructure in A3558 (Dantas+ 1997)", "J/MNRAS/296/599 : A3558 complex redshifts (Bardelli+, 1998)", "J/A+A/419/71 : 1.4GHz obs. and optical ident. in A3558 (Giacintucci+, 2004)", "J/AJ/130/2541 : Core of the Shapley supercluster at 1.4GHz (Miller+, 2005)", "http://users.ox.ac.uk/~jgodwin/clusters.htm"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1093/mnras/267.2.431"], "orcid_pub": ["0000-0001-9034-4402"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_284_477"}} {"id": "J/MNRAS/284/477", "title_cds": "The old open cluster NGC 6253", "title_create": "Bragaglia+, 1997", "year": "1997", "author": "Bragaglia A., Tessicini G., Tosi M., Marconi G., Munari U.", "title_pub": "UBVRI CCD photometry of the old open cluster NGC 6253.", "first_author": "Bragaglia A.", "ref_biblio": [""], "bibcode": ["1997MNRAS.284..477B"], "see_also": ["J/AJ/125/1383 : Stromgren photometry of NGC 6253 (Anthony-Twarog+, 2003)", "J/A+A/465/185 : Element abundances of 7 stars of NGC 6253 (Sestito+, 2007)", "J/A+A/505/1129 : BVRIJHK and proper motions in NGC 6253 (Montalto+, 2009)", "J/A+A/509/A17 : R light curves of NGC 6253 variables (De Marchi+, 2010)", "J/MNRAS/327/23 : CCD UBVRI photometry of 7 open star clusters (Sagar+, 2001)", "J/A+A/535/A39 : Radial velocity survey toward NGC 6253 (Montalto+, 2011)", "J/AJ/139/2034 : NGC 6253 stars equivalent widths (Anthony-Twarog+, 2010)"], "keyword_cds": "Clusters, open ; Photometry, CCD", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1093/mnras/284.2.477"], "orcid_pub": ["0000-0002-0338-7883"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_301_1019"}} {"id": "J/MNRAS/301/1019", "title_cds": "Seyfert galaxies/radio-quiet QSO correlation", "title_create": "Roy+, 1998", "year": "1998", "author": "Roy A.L., Norris R.P., Kesteven M.J., Troup E.R., Reynolds J.E.", "title_pub": "Seyfert galaxies and the radio-far-infrared correlation.", "first_author": "Roy A.L.", "ref_biblio": [""], "bibcode": ["1998MNRAS.301.1019R\t(SIMBAD/NED"], "keyword_cds": "Galaxies, Seyfert ; Redshifts ; Radio sources", "keyword_pub": "galaxies: active - galaxies: nuclei - galaxies: Seyfert - galaxies: starburst - infrared: galaxies - radio continuum: galaxies", "abstract": ["We have observed a sample of 149 Seyfert galaxies and radio-quiet", "quasars at 13 cm with both a 275-km radio interferometer and the 6-km", "compact array of the Australia Telescope. The high-resolution", "observations searched for the presence of compact,", "high-brightness-temperature radio emission from the active nucleus.", "The low-resolution observations measured the total radio emission from", "the galaxy disc and Seyfert core and lobes. From these we draw the", "following conclusions. (i) Seyfert galaxies that lack compact radio", "cores display a correlation between radio and far-infrared (FIR)", "emission similar to the correlation displayed by normal spirals,", "albeit with greater scatter. The correlation is found to be intrinsic", "and is not an artefact of the richness effect. (ii) A very different", "radio-FIR correlation is displayed by those Seyferts that harbour", "compact radio cores. These tend to be more radio-loud than either", "normal spirals or the Seyferts that lack compact cores. The compact", "core emission thus seems to be responsible for the generally poor", "radio-FIR correlation displayed by Seyfert galaxies. (iii) The", "radio-FIR correlation is not significantly improved by subtracting off", "the 0.1arcsec (20 to 200pc) compact radio emission from the total", "radio emission. This suggests that the emission from the active", "galactic nucleus has significant structure on scales larger than", "0.1arcsec. Perhaps these structures are the `linear' radio features", "that have been seen previously in Seyfert nuclei."], "doi_pub": ["10.1046/j.1365-8711.1998.02060.x"], "orcid_pub": ["0000-0002-1931-0135"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": " ", "columns": [{"name": "Name", "desc": "IRAS or IRAS-like name (B1950) "}, {"name": "NoteFlag", "desc": "[*] Note flag (1) "}, {"name": "Alias", "desc": "Name "}, {"name": "z", "desc": "Redshift (2) "}, {"name": "Class", "desc": "Seyfert classification (3) "}, {"name": "Smpl", "desc": "Sample in which the galaxy appears (4) "}, {"name": "l_S2.4GHz", "desc": "Limit flag on S2.4GHz "}, {"name": "S2.4GHz", "desc": "? Total flux density at 2.4GHz "}, {"name": "r_S2.4GHz", "desc": "Reference for S2.4GHz "}, {"name": "l_S2.3c", "desc": "Limit flag on S2.3c "}, {"name": "S2.3c", "desc": "? Core flux density at 2.3GHz "}, {"name": "n_S2.3c", "desc": "[*] Note on S2.3c "}, {"name": "l_HI", "desc": "Limit flag on HI "}, {"name": "HI", "desc": "? HI flux "}, {"name": "l_lgLFIR", "desc": "Limit flag on lgLFIR "}, {"name": "lgLFIR", "desc": "? FIR luminosity "}, {"name": "l_lgL2.4GHz", "desc": "Limit flag on lgL2.4GHz "}, {"name": "lgL2.4GHz", "desc": "? Total 2.4GHz luminosity "}, {"name": "l_lgMHI", "desc": "Limit flag on lgMHI "}, {"name": "lgMHI", "desc": "? HI mass "}, {"name": "lgD25", "desc": "? Major isophotal diameter "}, {"name": "lgLB", "desc": "? Total face-on magnitude corrected for "}, {"name": "internal", "desc": "extinction and "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_310_585"}} {"id": "J/MNRAS/310/585", "title_cds": "Scorpius OB2 parallaxes", "title_create": "de Bruijne+, 1999", "year": "1999", "author": "de Bruijne J.H.J.", "title_pub": "Structure and colour-magnitude diagrams of Scorpius OB2 based on kinematic modelling of Hipparcos data.", "first_author": "de Bruijne J.H.J.", "ref_biblio": [""], "bibcode": ["1999MNRAS.310..585D"], "see_also": ["I/239 : The Hipparcos and Tycho Catalogues (ESA 1997)", "J/AJ/117/354 : OB associations from Hipparcos (de Zeeuw+, 1999)"], "keyword_cds": "Associations, stellar ; Parallaxes, trigonometric ; Photometry, UBV", "keyword_pub": "astrometry - stars: distances - stars: kinematics - open clusters and associations: general - open clusters and associations: individual: Hyades - open clusters and associations: individual: Scorpius OB2", "description": ["ll stars in a `moving group' share the same space motion. The", "presence of such a coherent structure in velocity space can be", "used to derive (improved) estimates of the stellar parallaxes", "from the observed positions and proper motions. A Lund Observatory", "group (Dravins et al., 1999A&A...348.1040D) describes an elegant", "and sophisticated maximum likelihood procedure to do so using", "Hipparcos data.", "We implement the Lund procedure, and test it extensively", "using Monte Carlo simulations.", "We present an application to the nearby association Scorpius", "OB2, which consists of the three subgroups Upper Scorpius", "(mean distance 145 pc), Upper Centaurus Lupus (140 pc), and", "Lower Centaurus Crux (118 pc). Membership of these groups has recently", "been established by de Zeeuw et al. using", "Hipparcos data."], "doi_pub": ["10.1046/j.1365-8711.1999.02953.x"], "orcid_pub": ["0000-0001-6459-8599"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "tablea1.dat", "desc": "*Upper Scorpius Z99 members ", "columns": [{"name": "HIP", "desc": "Hipparcos (Cat. ) number "}, {"name": "plx", "desc": "Hipparcos (Cat. ) trigonometric parallax "}, {"name": "e_plx", "desc": "rms uncertainty on plx "}, {"name": "plxs", "desc": "Secular parallax (g_lim_=Y) ??? "}, {"name": "plx9", "desc": "? Secular parallax (g_lim_=9) "}, {"name": "e_plxs", "desc": "Secular parallax error (equations 16 and 17; s_v_=1km/s)"}, {"name": "gi", "desc": "Goodness-of-fit parameter (g_lim_=Y) ??? (1) "}, {"name": "gi9", "desc": "Goodness-of-fit parameter (g_lim_=9) (1) "}, {"name": "Vmag", "desc": "Hipparcos (Cat. ) V magnitude "}, {"name": "B-V", "desc": "Hipparcos (Cat. ) B-V colour index "}, {"name": "Ext", "desc": "? Visual extinction A_V_R_V_xE(B-V) "}, {"name": "E(B-V)", "desc": "? Colour excess "}, {"name": "Mult.", "desc": "? Multiplicity label (multiple star if M=1) "}, {"name": "Label", "desc": "Peculiarity label (2) "}, {"name": "Note", "desc": "[*] *: individual note "}, {"name": "SpType", "desc": "Hipporcos (Cat. ) spectral type "}]}, {"name": "tablea2.dat", "desc": "Upper Centaurus Lupus Z99 members ", "columns": [{"name": "HIP", "desc": "Hipparcos (Cat. ) number "}, {"name": "plx", "desc": "Hipparcos (Cat. ) trigonometric parallax "}, {"name": "e_plx", "desc": "rms uncertainty on plx "}, {"name": "plxs", "desc": "Secular parallax (g_lim_=Y) ??? "}, {"name": "plx9", "desc": "? Secular parallax (g_lim_=9) "}, {"name": "e_plxs", "desc": "Secular parallax error (equations 16 and 17; s_v_=1km/s)"}, {"name": "gi", "desc": "Goodness-of-fit parameter (g_lim_=Y) ??? (1) "}, {"name": "gi9", "desc": "Goodness-of-fit parameter (g_lim_=9) (1) "}, {"name": "Vmag", "desc": "Hipparcos (Cat. ) V magnitude "}, {"name": "B-V", "desc": "Hipparcos (Cat. ) B-V colour index "}, {"name": "Ext", "desc": "? Visual extinction A_V_R_V_xE(B-V) "}, {"name": "E(B-V)", "desc": "? Colour excess "}, {"name": "Mult.", "desc": "? Multiplicity label (multiple star if M=1) "}, {"name": "Label", "desc": "Peculiarity label (2) "}, {"name": "Note", "desc": "[*] *: individual note "}, {"name": "SpType", "desc": "Hipporcos (Cat. ) spectral type "}]}, {"name": "tablea3.dat", "desc": "Lower Centaurus Crux Z99 members ", "columns": [{"name": "HIP", "desc": "Hipparcos (Cat. ) number "}, {"name": "plx", "desc": "Hipparcos (Cat. ) trigonometric parallax "}, {"name": "e_plx", "desc": "rms uncertainty on plx "}, {"name": "plxs", "desc": "Secular parallax (g_lim_=Y) ??? "}, {"name": "plx9", "desc": "? Secular parallax (g_lim_=9) "}, {"name": "e_plxs", "desc": "Secular parallax error (equations 16 and 17; s_v_=1km/s)"}, {"name": "gi", "desc": "Goodness-of-fit parameter (g_lim_=Y) ??? (1) "}, {"name": "gi9", "desc": "Goodness-of-fit parameter (g_lim_=9) (1) "}, {"name": "Vmag", "desc": "Hipparcos (Cat. ) V magnitude "}, {"name": "B-V", "desc": "Hipparcos (Cat. ) B-V colour index "}, {"name": "Ext", "desc": "? Visual extinction A_V_R_V_xE(B-V) "}, {"name": "E(B-V)", "desc": "? Colour excess "}, {"name": "Mult.", "desc": "? Multiplicity label (multiple star if M=1) "}, {"name": "Label", "desc": "Peculiarity label (2) "}, {"name": "Note", "desc": "[*] *: individual note "}, {"name": "SpType", "desc": "Hipporcos (Cat. ) spectral type "}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "HIP", "desc": "Hipparcous number "}, {"name": "Note", "desc": "Text of the note (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_357_945"}} {"id": "J/MNRAS/357/945", "title_cds": "Evolutionary stellar pop. synthesis", "title_create": "Gonzalez-Delgado+, 2005", "year": "2005", "author": "Gonzalez-Delgado R.M., Cervino M., Martins L.P., Leitherer C., Hauschildt P.H.", "title_pub": "Evolutionary stellar population synthesis at high spectral resolution: optical wavelengths.", "first_author": "Gonzalez-Delgado R.M.", "ref_biblio": [""], "bibcode": ["2005MNRAS.357..945G"], "keyword_cds": "", "keyword_pub": "", "mission": "", "abstract": ["We present the single stellar population (SSP) synthesis results of", "our new synthetic stellar atmosphere models library with a spectral", "sampling of 0.3{AA}, covering the wavelength range from 3000 to 7000{AA}", "for a wide range of metallicities (twice solar, solar, half solar and", "1/10 solar). The stellar library is composed of 1650 spectra computed", "with the latest improvements in stellar atmospheres. In particular, it", "incorporates non-local thermodynamic equilibrium (LTE) line-blanketed", "models for hot (Teff>=27500K), and LTE line-blanketed models", "(Phoenix) for cool (3000<=Teff<=4500K) stars. Because of the high", "spectral resolution of this library, evolutionary synthesis models can", "be used to predict the strength of numerous weak absorption lines and", "the evolution of the profiles of the strongest lines over a wide range", "of ages. The SSP results have been calculated for ages from 1Myr to", "17Gyr using the stellar evolutionary tracks provided by the Geneva", "and Padova groups. For young stellar populations, our results have a", "very detailed coverage of high-temperature stars with similar results", "for the Padova and Geneva isochrones. For intermediate and old stellar", "populations, our results, once degraded to a lower resolution, are", "similar to the ones obtained by other groups (limitations imposed by", "the stellar evolutionary physics notwidthstanding). The limitations", "and advantages of our models for the analysis of integrated", "populations are described.", "The full set of the stellar library and the evolutionary models are", "available for retrieval at the websites http://www.iaa.csic.es/~rosa", "and http://www.iaa.csic.es/~mcs/sed@ ."], "description": ["The library contains 415, 409, 416 and 411 spectra for Z= 0.002, 0.010,", "0.020 (solar) and 0.040, respectively."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2005.08692.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_358_1290"}} {"id": "J/MNRAS/358/1290", "title_cds": "NGC 663 and 654 stellar contents", "title_create": "Pandey+, 2005", "year": "2005", "author": "Pandey A.K., Upadhyay K., Ogura K., Sagar R., Mohan V., Mito H., Bhatt H.C., Bhatt B.C.", "title_pub": "Stellar contents of two young open clusters: NGC 663 and 654.", "first_author": "Pandey A.K.", "ref_biblio": [""], "bibcode": ["2005MNRAS.358.1290P"], "keyword_cds": "", "keyword_pub": "stars: formation - stars: luminosity function, mass function - dust, extinction - galaxies: star clusters", "mission": "", "abstract": ["UBVRI CCD photometry in a wide field around two young open clusters,", "NGC 663 and 654, has been carried out. H{alpha} and polarimetric", "observations for the cluster NGC 654 have also been obtained. We use", "the photometric data to construct colour-colour and colour-magnitude", "diagrams, from which we can investigate the reddening, age, mass and", "evolutionary states of the stellar contents of the these clusters."], "description": ["For NGC 663, the CCD UBVIC data were acquired in 1999 November using", "the 2048x2048pixel^2^ CCD camera mounted on the 105-cm Schmidt", "telescope of the Kiso Observatory.", "For NGC 654, the CCD BVIC and H observations were carried out in 1993", "October-November and in 1998 December, respectively, using the", "1024x1024pixel^2^ CCD camera mounted on the f/13 Cassegrain focus of", "the 104-cm Sampurnanand telescope of the State Observatory, Naini Tal."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2005.08784.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_361_607"}} {"id": "J/MNRAS/361/607", "title_cds": "K_s_-selected galaxies", "title_create": "Caputi+, 2005", "year": "2005", "author": "Caputi K.I., Dunlop J.S., Mclure R.J., Roche N.D.", "title_pub": "The evolution of K_s_-selected galaxies in the GOODS/CDFS deep ISAAC field.", "first_author": "Caputi K.I.", "ref_biblio": [""], "bibcode": ["2005MNRAS.361..607C"], "keyword_cds": "", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: high-redshift - galaxies: luminosity function, mass function", "mission": "", "abstract": ["We present estimated redshifts and derived properties of a sample of", "1663 galaxies with Ks<=22 (Vega), selected from 50.4-arcmin^2^ of the", "Great Observatories Origins Deep Survey/Chandra Deep Field South", "(GOODS/CDFS) field with deep Infrared Spectrometer and Array Camera", "(ISAAC) imaging, and make an extensive comparison of their properties", "with those of the extremely red galaxies (ERGs) selected in the same", "field. We study in detail the evolution of Ks-selected galaxies up to", "redshifts z~4, and clarify the role of ERGs within the total Ks-band", "galaxy population. We compute the total Ks-band luminosity function", "(LF) and compare its evolution with the ERG LF."], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2005.09222.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_362_689"}} {"id": "J/MNRAS/362/689", "title_cds": "AAO/UKST SuperCOSMOS H{alpha} survey", "title_create": "Parker+, 2005", "year": "2005", "author": "Parker Q.A., Phillipps S., Pierce M.J., Hartley M., Hambly N.C., Read M.A., Macgillivray H.T., Tritton S.B., Cass C.P., Cannon R.D., Cohen M., Drew J.E., Frew D.J., Hopewell E., Mader S., Malin D.F., Masheder M.R.W., Morgan D.H., Morris R.A.H., Russeil D., Russell K.S., Walker R.N.F.", "title_pub": "The AAO/UKST SuperCOSMOS H{alpha} survey.", "first_author": "Parker Q.A.", "ref_biblio": [""], "bibcode": ["2005MNRAS.362..689P"], "keyword_cds": "", "keyword_pub": "astronomical data bases: miscellaneous - catalogues - surveys - stars: emission line - photometry", "abstract": ["The UK Schmidt Telescope (UKST) of the Anglo-Australian Observatory", "completed a narrow-band H{alpha} plus [N II] 6548, 6584{AA} survey of", "the Southern Galactic Plane and Magellanic Clouds in late 2003. The", "survey, which was the last UKST wide-field photographic survey and the", "only one undertaken in a narrow-band, is now an online digital data", "product of the Wide-Field Astronomy Unit of the Royal Observatory", "Edinburgh (ROE). The survey utilized a high specification, monolithic", "H{alpha} interference bandpass filter of exceptional quality. In", "conjunction with the fine-grained Tech-Pan film as a detector it has", "produced a survey with a powerful combination of area coverage (4000", "square degrees), resolution (~1 arcsec) and sensitivity (5 Rayleighs),", "reaching a depth for continuum point sources of R=~20.5. The main", "survey consists of 233 individual fields on a grid of centres", "separated by 4{deg} at declinations below +2{deg} and covers a swathe", "approximately 20{deg} wide about the Southern Galactic Plane. The", "original survey films were scanned by the SuperCOSMOS measuring", "machine at the Royal Observatory, Edinburgh, to provide the online", "digital atlas called the SuperCOSMOS H{alpha} Survey (SHS). We present", "the background of the survey, the key survey characteristics, details", "and examples of the data product, calibration process, comparison with", "other surveys and a brief description of its potential for scientific", "exploitation."], "doi_pub": ["10.1111/j.1365-2966.2005.09350.x"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "fields.dat", "desc": "H-alpha (HA) and matching Short-red (SR) fields currently available online", "columns": [{"name": "Field", "desc": "Field number "}, {"name": "RAh", "desc": "Centre Right ascnesion (B1950) "}, {"name": "RAm", "desc": "Centre Right ascnesion (B1950) "}, {"name": "DE-", "desc": "Centre Declination sign (B1950) "}, {"name": "DEd", "desc": "Centre Declination (B1950) "}, {"name": "HaFITS", "desc": "Halpha.FITS file name (HANNNN.fits.gz) "}, {"name": "HablFITS", "desc": "Halpha-block.FITS file name (halNNNNblock.fits.gz) "}, {"name": "HaGIF", "desc": "Halpha.GIF file name (HANNNN.gif) "}, {"name": "HablGIF", "desc": "Halpha-block.GIF file name (halNNNNblock.gif) "}, {"name": "SRFITS", "desc": "Short-red FITS file name (SRNNNN.fits.gz) "}, {"name": "SRblFITS", "desc": "Short-red-block FITS file (harNNNNblock.fits.gz) "}, {"name": "SRGIF", "desc": "Short-red.GIF file name (SRNNNN.gif) "}, {"name": "SRblGIF", "desc": "Short-red-block.GIF file name (harNNNNblock.gif) "}]}, {"name": "table3.dat", "desc": "Content of the fits files ", "columns": []}, {"name": "HAL0067block.fits", "desc": "Example of file : Field 0067 ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_380_1064"}} {"id": "J/MNRAS/380/1064", "title_cds": "New spectroscopic orbits of Am stars", "title_create": "Carquillat+, 2007", "year": "2007", "author": "Carquillat J.-M., Prieur J.-L.", "title_pub": "Contribution to the search for binaries among Am stars. VIII. New spectroscopic orbits of eight systems and statistical study of a sample of 91 Am stars.", "first_author": "Carquillat J.-M.", "ref_biblio": [""], "bibcode": ["2007MNRAS.380.1064C"], "keyword_cds": "", "keyword_pub": "binaries: spectroscopic - stars: fundamental parameters - stars: luminosity function, mass function", "mission": "", "abstract": ["This paper is the last of a series devoted to the study of Am stars,", "with the monitoring of radial velocities of a sample of 91 objects", "during more than 20yr. The purpose was to determine which stars were", "members of spectroscopic binaries (SBs) and study in detail those", "systems in order to obtain observational constraints on the origin of", "the Am phenomenon.", "We then present some statistical properties of the orbital parameters", "of the SBs whose primary is an Am star, on an extended sample obtained", "by adding 29 Am SB orbits published by other authors."], "description": ["Most of the observations concerning the eight objects were performed", "at OHP, but additional observations were also carried out by R.F.", "Griffin who kindly observed some stars of our programme with his own", "CORAVEL in Cambridge."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2007.12143.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_397_405"}} {"id": "J/MNRAS/397/405", "title_cds": "Variable stars in h Per", "title_create": "Saunders+, 2009", "year": "2009", "author": "Saunders E.S., Naylor T., Mayne N., Littlefair S.P.", "title_pub": "Pre-main-sequence variability across the radiative-convective gap.", "first_author": "Saunders E.S.", "ref_biblio": [""], "bibcode": ["2009MNRAS.397..405S"], "keyword_cds": "", "keyword_pub": "stars: fundamental parameters ; Hertzsprung\u2013Russell (HR) diagram ; stars: magnetic fields ; stars: pre-main-sequence ; stars: spots ; stars: variables: other", "abstract": ["We use I-band imaging to perform a variability survey of the 13Myr old", "cluster h Per. We find a significant fraction of the cluster members", "to be variable. Most importantly, we find that variable members lie", "almost entirely on the convective side of the gap in the cluster", "sequence between fully convective stars and those which have a", "radiative core. This result is consistent with a scenario in which the", "magnetic field changes topology when the star changes from being fully", "convective to one containing a radiative core. When the star is", "convective, the magnetic field appears dominated by large-scale", "structures, resulting in global-size spots that drive the observed", "variability. For those stars with radiative cores, we observe a marked", "absence of variability due to spots, which suggests a switch to a", "magnetic field dominated by smaller-scale structures, resulting in", "many smaller spots and thus less apparent variability. This implies", "that wide field variability surveys may only be sensitive to fully", "convective stars. On the one hand, this reduces the chances of picking", "out young groups (since the convective stars are the lower mass and", "therefore fainter objects), but conversely the absolute magnitude of", "the head of the convective sequence provides a straightforward measure", "of age for those groups which are discovered."], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1111/j.1365-2966.2009.14936.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_399_o.683"}} {"id": "J/MNRAS/399/683", "title_cds": "6dF galaxy survey final redshift release (6dFGS)", "title_create": "Jones+, 2009", "year": "2009", "author": "Jones D.H., Read M.A., Saunders W., Colless M., Jarrett T., Parker Q.A., Fairall A.P., Mauch T., Sadler E.M., Watson F.G., Burton D., Campbell L.A., Cass P., Croom S.M., Dawe J., Fiegert K., Frankcombe L., Hartley M., Huchra J., James D., Kirby E., Lahav O., Lucey J., Mamon G.A., Moore L., Peterson B.A., Prior S., Proust D., Russell K., Safouris V., Wakamatsu K.-I., Westra E., Williams M.", "title_pub": "The 6dF galaxy survey: final redshift release (DR3) and southern large-scale structures.", "first_author": "Jones D.H.", "ref_biblio": [""], "bibcode": ["2009MNRAS.399..683J"], "see_also": ["VII/193 : The CfA Redshift Catalogue, Version June 1995 (Huchra+ 1995)", "VII/250 : The 2dF Galaxy Redshift Survey (2dFGRS) (2dFGRS Team, 1998-2003)", "http://www.sdss.org : SDSS Home Page"], "keyword_cds": "Surveys ; Galaxy catalogs ; Redshifts ; Magnitudes", "keyword_pub": "surveys - galaxies: distances and redshifts - cosmology: observations - large-scale structure of Universe", "abstract": ["We report the final redshift release of the 6dF Galaxy Survey (6dFGS),", "a combined redshift and peculiar velocity survey over the southern sky", "(|b|>10{deg}). Its 136304 spectra have yielded 110256 new", "extragalactic redshifts and a new catalogue of 125071 galaxies making", "near-complete samples with (K, H, J, rF, bJ)<=(12.65, 12.95, 13.75,", "15.60, 16.75). The median redshift of the survey is 0.053. Survey", "data, including images, spectra, photometry and redshifts, are", "available through an online data base. We describe changes to the", "information in the data base since earlier interim data releases.", "Future releases will include velocity dispersions, distances and", "peculiar velocities for the brightest early-type galaxies, comprising", "about 10 per cent of the sample. Here we provide redshift maps of the", "southern local Universe with z<=0.1 , showing nearby large-scale", "structures in hitherto unseen detail. A number of regions known", "previously to have a paucity of galaxies are confirmed as", "significantly underdense regions. The URL of the 6dFGS data base is", "http://www-wfau.roe.ac.uk/6dFGS ."], "description": ["Basic data for the galaxies in the 6dFGS with redshifts, using the", "best 6dFGS redshifts (Q=3 or 4) plus available redshifts from SDSS,", "2dFGRS and ZCAT (124646 entries in all)."], "date_update": "02-May-2010", "tables": [{"name": "catalog.dat", "desc": "The 6dF Galaxy Survey Redshift Catalogue Data Release 3 (Heath Jones, Anglo-Australian Observatory, 28 February 2009)", "columns": [{"name": "6dFGS", "desc": "Galaxy survey target ID (gHHMMSDDMMSS) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Nmeas", "desc": "Number of 6dFGS measurements (of any redshift Q value)"}, {"name": "Ncz", "desc": "Number of measurements used in final cz (Q=3 or 4 only)"}, {"name": "bJmag", "desc": "Recalibrated b_J magnitude (BMAG in 6dFGS database)"}, {"name": "PROGID", "desc": "Programme ID number (PROGID in database) "}, {"name": "rFmag", "desc": "Recalibrated r_F magnitude (RMAG in database) "}, {"name": "S/G", "desc": "[0/4] SuperCOSMOS star/galaxy classifier (1) "}, {"name": "Flag", "desc": "Sum of comparison flags (comparison threshold =330km/s) (2)"}, {"name": "cz", "desc": "Best available combined recession velocity cz "}, {"name": "e_cz", "desc": "Combined uncertainty in cz (3) "}, {"name": "r_cz", "desc": "Code identifying source of redshift (4) "}, {"name": "q_cz", "desc": "Best redshift quality value available for this source (5)"}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "AV", "desc": "Galactic extinction in V magnitudes (from Schlegel et al., 1998ApJ...500..525S)"}, {"name": "W", "desc": "Original weight source had for first round of fibre allocation"}, {"name": "Target", "desc": "TARGETID number from the 6dFGS database "}, {"name": "Temp", "desc": "Template code(s) (6) "}, {"name": "FileName", "desc": "Name of redshift field file containing the redshift (7)"}, {"name": "SPECID", "desc": "SPECID values of redshifts contributing to the final combined redshift"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_400_1690"}} {"id": "J/MNRAS/400/1690", "title_cds": "Ages and metallicities for quiescent galaxies", "title_create": "Smith+, 2009", "year": "2009", "author": "Smith R.J., Lucey J.R., Hudson M.J.", "title_pub": "Ages and metallicities for quiescent galaxies in the Shapley supercluster: driving parameters of the stellar populations.", "first_author": "Smith R.J.", "ref_biblio": [""], "bibcode": ["2009MNRAS.400.1690S"], "see_also": ["J/MNRAS/381/1035 : Spectroscopy in Shapley supercluster (Smith+, 2007)"], "keyword_cds": "Galaxies, spectra ; Models ; Velocity dispersion ; Abundances", "keyword_pub": "galaxies: elliptical and lenticular, cD - galaxies: evolution", "abstract": ["We use high signal-to-noise spectroscopy for a sample of 232 quiescent", "galaxies in the Shapley supercluster, to investigate how their stellar", "populations depend on velocity dispersion (sigma) luminosity and", "stellar mass. The sample spans a large range in velocity dispersion", "(30-300km/s) and in luminosity (M_R_ from -18.7 to -23.2). Estimates", "of age, total metallicity (Z/H) and alpha-element abundance ratio", "(alpha/Fe) were derived from absorption-line analysis, using", "single-burst models of Thomas and collaborators. Using the Rose CaII", "index, we conclude that recent star formation (frosting) events are", "not responsible for the intermediate ages observed in some of the", "galaxies."], "description": ["Paper I (Smith et al., 2007, Cat. ) provides a full", "description of the observations and data processing."], "type": ["MC"], "doi_pub": ["10.1111/j.1365-2966.2009.15580.x"], "orcid_pub": ["0000-0001-5998-2297"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Model inversion results ", "columns": [{"name": "---", "desc": "[NFP] "}, {"name": "NFP", "desc": "Galaxy name (JHHMMSS.s+DDMMSS) "}, {"name": "logLR", "desc": "R-band luminosity "}, {"name": "logsigma", "desc": "?=- Velocitiy dispersion "}, {"name": "e_logsigma", "desc": "?=- rms uncertainty on logsigma "}, {"name": "logAge", "desc": "Age "}, {"name": "e_logAge", "desc": "rms uncertainty on logAge "}, {"name": "[Z/H]", "desc": "Metallicity "}, {"name": "e_[Z/H]", "desc": "rms uncertainty on [Z/H] "}, {"name": "[alpha/H]", "desc": "alpha-element enhancement (1) "}, {"name": "e_[alpha/H]", "desc": "rms uncertainty on [alpha/H] "}, {"name": "C(Age,Z)", "desc": "Error correlation coefficient (2) "}, {"name": "C(Age,alpha)", "desc": "Error correlation coefficient (2) "}, {"name": "C(Z,alpha)", "desc": "Error correlation coefficient (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_400_589"}} {"id": "J/MNRAS/400/589", "title_cds": "Ionization of emission-line gas", "title_create": "Holt+, 2009", "year": "2009", "author": "Holt J., Tadhunter C.N., Morganti R.", "title_pub": "The ionization of the emission-line gas in young radio galaxies.", "first_author": "Holt J.", "ref_biblio": [""], "bibcode": ["2009MNRAS.400..589H"], "keyword_cds": "", "keyword_pub": "ISM: jets and outflows - galaxies: active - galaxies: ISM - galaxies: kinematics and dynamics", "abstract": ["This paper is the second in a series in which we present", "intermediate-resolution, wide-wavelength coverage spectra for a", "complete sample of 14 compact radio sources, taken with the aim of", "investigating the impact of the nuclear activity on the circumnuclear", "interstellar medium (ISM) in the early stages of radio source", "evolution. In the first paper (Holt, Tadhunter & Morganti,", "2008MNRAS.387..639H), we presented the kinematic results from the", "nuclear emission-line modelling and reported fast outflows in the", "circumnuclear gas. In this paper, we use the line fluxes to", "investigate the physical conditions and dominant ionization mechanisms", "of the emission-line gas. We find evidence for large electron", "densities and high reddening in the nuclear regions, particularly in", "the broader, blueshifted components."], "description": ["Our complete sample comprises 14 compact radio sources derived from", "the northern 3C and 4C samples and southern 2Jy sample and includes", "eight CSS, three GPS, two compact core sources and one compact", "flat-spectrum source. The sample has intermediate redshifts (z<0.7)", "and a radio power range of 26"], "bibcode": ["2010MNRAS.406..952S"], "see_also": ["http://www.astro.wisc.edu/glimpse/Carina_Nebula/ : Spitzer Imaging of", "II/293 : GLIMPSE Source Catalog (I + II + 3D) (IPAC 2008)"], "keyword_cds": "", "keyword_pub": "HII regions ; ISM: individual (NGC 3372) ; stars: formation ; stars: luminosity function, mass function ; stars: pre-main-sequence", "mission": "Spitzer", "abstract": ["We report the first results of imaging the Carina Nebula (NGC 3372)", "with the Infrared Array Camera (IRAC) onboard the Spitzer Space", "Telescope, providing a photometry catalog of over 44,000 point sources", "as well as a catalog of over 900 candidate young stellar objects", "(YSOs) based on fits to their spectral energy distributions (SEDs).", "We discuss several aspects of the extended emission, including the", "structure of dozens of dust pillars that result when a clumpy", "molecular cloud is shredded by feedback from massive stars. There", "are surprisingly few of the \"extended green objects\" (EGOs) that are", "normally taken as signposts of outflow activity in Spitzer data, and", "not one of the dozens of Herbig-Haro jets detected optically are seen", "as EGOs. EGOs are apparently poor tracers of outflow activity in", "strongly irradiated environments, due to the effects of massive star", "feedback. A population of \"extended red objects\" tends to be found", "around late O-type and early B-type stars, some with clear bow-shock", "morphology. These are dusty shocks where stellar winds collide with", "photoevaporative flows off nearby clouds. Finally, the relative", "distributions of O-type stars, small star clusters, and sub-clusters", "of YSOs as compared to the dust pillars shows that while smplying that", "while some YSOs are located within dust pillars, many more stars and", "YSOs reside just outside pillar heads. We suggest that pillars are", "transient phenomena, part of a continuous outwardly propagating wave", "of star formation driven by feedback from massive stars. As the", "pillars are destroyed, they leave newly formed stars in their wake,", "and these are then subsumed into the young OB association. The YSOs", "are found predominantly in the cavity between pillars and massive", "stars, arguing that their formation was in fact triggered. Altogether,", "the current generation of YSOs shows no strong deviation from a normal", "initial mass function (IMF). The number of YSOs is consistent with a", "roughly constant star-formation rate over the past ~3Myr, implying", "that propagating star formation in pillars constitutes an important", "mechanism to construct unbound OB associations. These accelerated", "pillars may give birth to massive O-type stars that, after several", "Myr, could appear to have formed in isolation."], "curator": "Francois Ochsenbein [CDS]", "alias": ["SSTCARA SSTCARC"], "type": ["OC"], "doi_pub": ["10.1111/j.1365-2966.2010.16792.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_407_870"}} {"id": "J/MNRAS/407/870", "title_cds": "Super star clusters in Haro 11", "title_create": "Adamo+, 2010", "year": "2010", "author": "Adamo A., Ostlin G., Zackrisson E., Hayes M., Cumming R.J., Micheva G.", "title_pub": "Super star clusters in Haro 11: properties of a very young starburst and evidence for a near-infrared flux excess.", "first_author": "Adamo A.", "ref_biblio": [""], "bibcode": ["2010MNRAS.407..870A"], "keyword_cds": "", "keyword_pub": "galaxies: irregular - galaxies: starburst - galaxies: star clusters: individual: Haro 11", "abstract": ["We have used multiband imaging to investigate the nature of an extreme", "starburst environment in the nearby Lyman break galaxy analogue", "Haro 11 (ESO 350\u2212IG038) by means of its stellar cluster population.", "The central starburst region has been observed in eight different", "high-resolution Hubble Space Telescope (HST) wavebands, sampling the", "stellar and gas components from UV to near-infrared. Photometric", "imaging of the galaxy was also carried out at 2.16um by NaCo AO", "instrument at the ESO Very Large Telescope. We constructed integrated", "spectral energy distributions (SEDs) for about 200 star clusters", "located in the active star-forming regions and compared them with", "single stellar population models (suitable for physical properties of", "very young cluster population) in order to derive ages, masses and", "extinctions of the star clusters."], "description": ["We have used archival\u2002HST/ACS imaging of Haro 11, with observations", "from the FUV to the optical (~8000{AA}) wavebands. We have", "supplemented these data with new\u2002HST/WFPC2 broad-band imaging in V", "(F606W), I (F814W) and H[NIC3/F160W; NICMOS near-IR (NIR)]. To sample", "further into the IR we have used the NaCo adaptive optics (AO) imager", "in the Ks band."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2010.16983.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_417_1402"}} {"id": "J/MNRAS/417/1402", "title_cds": "Groups and clusters in 2SLAQ catalogue", "title_create": "Farrens+, 2011", "year": "2011", "author": "Farrens S., Abdalla F.B., Cypriano E.S., Sabiu C., Blake C.", "title_pub": "Friends-of-friends groups and clusters in the 2SLAQ catalogue.", "first_author": "Farrens S.", "ref_biblio": [""], "bibcode": ["2011MNRAS.417.1402F"], "keyword_cds": "", "keyword_pub": "galaxies: clusters: general - galaxies: distances and redshifts", "abstract": ["We present a catalogue of galaxy groups and clusters selected using a", "friends-of-friends (FoF) algorithm with a dynamic linking length from", "the 2dF-SDSS LRG and QSO (2SLAQ) luminous red galaxy survey. The", "linking parameters for the code are chosen through an analysis of", "simulated 2SLAQ haloes. The resulting catalogue includes 313 clusters", "containing 1152 galaxies."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1111/j.1365-2966.2011.19356.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_417_3047"}} {"id": "J/MNRAS/417/3047", "title_cds": "Infrared two-colour diagrams for AGB stars", "title_create": "Suh+, 2011", "year": "2011", "author": "Suh K.-W., Kwon Y.-J.", "title_pub": "Infrared two-colour diagrams for AGB stars using AKARI, MSX, IRAS and near-infrared data.", "first_author": "Suh K.-W.", "ref_biblio": [""], "bibcode": ["2011MNRAS.417.3047S"], "keyword_cds": "Stars, giant ; Infrared sources", "keyword_pub": "radiative transfer - catalogues - stars: AGB and post-AGB - circumstellar matter - dust, extinction - infrared: stars", "abstract": ["Using a revised version of the catalogue of asymptotic giant branch", "(AGB) stars by Suh & Kwon, we present various infrared two-colour", "diagrams (2CDs) for 3003 O-rich, 1168 C-rich, 362 S-type and 35", "silicate carbon stars in our Galaxy. For each object in the new", "catalogue, we cross-identify the AKARI, Midcourse Space Experiment", "(MSX) and Two-Micron All-Sky Survey (2MASS) counterparts by finding", "the nearest object from the position information in the Infrared", "Astronomical Satellite (IRAS) Point Source Catalog (PSC)."], "description": ["For the sample of AGB stars, we use a revised version of the catalogue", "by Suh & Kwon (2009, JKAS, 42, 81). They presented a catalogue of AGB", "stars in our Galaxy from the sources listed in the IRAS PSC, compiling", "the lists of previous works with verifying processes; their catalogue", "was composed of 2193 O-rich stars, 1167 C-rich stars, 287 S stars and", "36 silicate carbon stars.", "ONLY the list of IRAS sources"], "type": ["CCC"], "doi_pub": ["10.1111/j.1365-2966.2011.19462.x"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "c-agb.dat", "desc": "C-rich AGB stars ", "columns": [{"name": "IRAS", "desc": "IRAS PSC name (HHMM+DDMMA) "}]}, {"name": "o-agb.dat", "desc": "O-rich AGB stars ", "columns": [{"name": "IRAS", "desc": "IRAS PSC name (HHMM+DDMMA) "}]}, {"name": "s.dat", "desc": "S stars ", "columns": [{"name": "IRAS", "desc": "IRAS PSC name (HHMM+DDMMA) "}]}, {"name": "sc.dat", "desc": "Silicate carbon stars ", "columns": [{"name": "IRAS", "desc": "IRAS PSC name (HHMM+DDMMA) "}]}, {"name": "alumina.dat", "desc": "Optical constants for amorphous alumina (Al2O3) dust (Density = 3.2g/cc)", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "n", "desc": "Refractive index "}, {"name": "k", "desc": "Extinction coefficient "}]}, {"name": "amc.dat", "desc": "Optical constants for amorphous carbon (Density = 2.0g/cc)", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "n", "desc": "Refractive index "}, {"name": "k", "desc": "Extinction coefficient "}]}, {"name": "silc.dat", "desc": "Optical constants for warm silicate (Density = 3.3g/cc)", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "n", "desc": "Refractive index "}, {"name": "k", "desc": "Extinction coefficient "}]}, {"name": "silw.dat", "desc": "Optical constants for cold silicate (Density = 3.3g/cc)", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "n", "desc": "Refractive index "}, {"name": "k", "desc": "Extinction coefficient "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_418_1452"}} {"id": "J/MNRAS/418/1452", "title_cds": "NIR Atlas of S0-Sa galaxies (NIRS0S)", "title_create": "Laurikainen+, 2011", "year": "2011", "author": "Laurikainen E., Salo H., Buta R., Knapen J.H.", "title_pub": "Near-infrared atlas of S0-Sa galaxies (NIRS0S).", "first_author": "Laurikainen E.", "ref_biblio": [""], "bibcode": ["2011MNRAS.418.1452L"], "keyword_cds": "", "keyword_pub": "galaxies: elliptical and lenticular, cD - galaxies: evolution - galaxies: structure", "abstract": ["We present an atlas of Ks-band images of 206 early-type galaxies,", "including 160 S0-S0/a galaxies, 12 ellipticals and 33 Sa galaxies", "(+1 later type). The majority of the atlas galaxies belong to a", "magnitude-limited (m_B_<=12.5mag) sample of 185 Near-InfraRed S0", "Survey galaxies. To ensure that misclassified S0s are not omitted,", "25 ellipticals from the Third Reference Catalogue of Bright Galaxies", "classified as S0s in the Carnegie Atlas were included in the sample.", "The observations were carried out using 3-4m class telescopes with", "subarcsecond pixel resolution (~0.25arcsec), and were obtained in good", "seeing conditions (full width at half-maximum ~1arcsec). The images", "are 2-3mag deeper than Two-Micron All-Sky Survey images, allowing the", "detection of faint outer discs in S0s. Both visual and photometric", "classifications are made, largely following the classification", "criteria of de Vaucouleurs. Special attention is paid to the", "classification of lenses, which are coded in a more systematic manner", "than in any of the previous studies. A new lens type, called a", "\"barlens\", is introduced, possibly forming part of the bar itself.", "Also, boxy/peanut/x-shaped structures are identified in many barred", "galaxies, even though the galaxies are not seen edge-on, indicating", "that vertical thickening is not enough to explain these structures.", "Photometric classification includes detection of exponential outer", "discs or other structures not directly visible in the images, but", "becoming clear in unsharp masking or residual images in", "decompositions. In our photometric classification, nuclear bars are", "assigned for 15 galaxies, which are overshadowed by bulges in visual", "classification. The mean Hubble stage in the near-infrared is found to", "be similar to that in the optical. We give dimensions of structure", "components, and radial profiles of the position angles and", "ellipticities, and show deviations from perfect elliptical isophotes.", "Shells and ripples, generally assumed to be manifestations of recent", "mergers, are detected only in six galaxies. However, multiple lenses", "appear in as much as 25 per cent of the atlas galaxies, which is a", "challenge to the hierarchical evolutionary picture of galaxies. Such", "models need to explain how the lenses were formed and then survived in", "multiple merger events that galaxies may have suffered during their", "lifetimes."], "object": [], "curator": "Patricia Vannier [CDS]", "alias": ["NIRS0S"], "doi_pub": ["10.1111/j.1365-2966.2011.19283.x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_424_1930"}} {"id": "J/MNRAS/424/1930", "title_cds": "O and N abundances of HII regions in spiral gal.", "title_create": "Gusev+, 2012", "year": "2012", "author": "Gusev A.S., Pilyugin L.S., Sakhibov F., Dodonov S.N., Ezhkova O.V., Khramtsova M.S.", "title_pub": "Oxygen and nitrogen abundances of HII regions in six spiral galaxies.", "first_author": "Gusev A.S.", "ref_biblio": [""], "bibcode": ["2012MNRAS.424.1930G"], "see_also": ["J/A+AS/123/305 : Yields of intermediate mass stars (van den Hoek+ 1997)", "J/ApJ/510/104 : Ionizing Stars of Extragalactic H II Regions (Bresolin+ 1999)"], "keyword_cds": "Galaxies, nearby ; H II regions ; Abundances", "keyword_pub": "techniques: spectroscopic - ISM: abundances - HII regions - galaxies: abundances", "abstract": ["Spectroscopic observations of 63 HII regions in six spiral", "galaxies (NGC628, NGC783, NGC2336, NGC6217, NGC7331 and NGC7678) were", "carried out with the 6-m telescope (BTA) of Russian Special", "Astrophysical Observatory with the Spectral Camera attached to the", "focal reducer SCORPIO in multislit mode with a dispersion of", "2.1{AA}/pixel and a spectral resolution of 10{AA}. These", "observations were used to estimate the oxygen and nitrogen abundances", "and the electron temperatures in HII regions through the recent", "variant of the strong-line method (NS calibration). The parameters of", "the radial distribution (the extrapolated central intercept value and", "the gradient) of the oxygen and nitrogen abundances in the discs of", "spiral galaxies NGC628, NGC783, NGC2336, NGC7331 and NGC7678 have been", "determined. The abundances in NGC783, NGC2336, NGC6217 and NGC7678 are", "measured for the first time. Galaxies from our sample follow well the", "general trend in the luminosity-central metallicity diagram for", "spiral and irregular galaxies."], "description": ["We selected galaxies with known UBVRI photometry of HII regions, as", "obtained by our team in previous works: NGC 628 (Bruevich et al.,", "2007ARep...51..222B), NGC 783 (Gusev, 2006ARep...50..167G,", "2006ARep...50..182G), NGC 2336 (Gusev & Park, 2003A&A...410..117G),", "NGC 6217 (Artamonov et al., 1999ARep...43..377A), NGC 7331", "(unpublished) and NGC 7678 (Artamonov, Bruevich & Gusev,", "1997ARep...41..577A)."], "type": ["OC"], "doi_pub": ["10.1111/j.1365-2966.2012.21322.x"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "The galaxy sample ", "columns": [{"name": "Gal", "desc": "Galaxy name "}, {"name": "MType", "desc": "Morphological type "}, {"name": "Bt", "desc": "BT magnitude "}, {"name": "RAh", "desc": "Right ascension of the galaxy centre (J2000) "}, {"name": "RAm", "desc": "Right ascension of the galaxy centre (J2000) "}, {"name": "RAs", "desc": "Right ascension of the galaxy centre (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "Incl", "desc": "Inclination "}, {"name": "PA", "desc": "Position angle "}, {"name": "HVR", "desc": "Heliocentric radial velocity "}, {"name": "Rc25", "desc": "Isophotal radius (25mag/arcsec^2^ in the B band) corrected for Galactic extinction and absorption due to the inclination of a galaxy (arcmin)"}, {"name": "Rc25k", "desc": "Isophotal radius (25mag/arcsec^2^ in the B band) corrected for Galactic extinction and absorption due to the inclination of a galaxy (kpc)"}, {"name": "d", "desc": "Distance "}, {"name": "BMAG", "desc": "Absolute B magnitude "}]}, {"name": "table3.dat", "desc": "Offsets, galactocentric distances, radial velocities of H II regions", "columns": [{"name": "Gal", "desc": "Galaxy name "}, {"name": "HII", "desc": "HII region number, within the galaxy "}, {"name": "n_HII", "desc": "[ab] Multiplicity index on HII "}, {"name": "Pos", "desc": "Slit position "}, {"name": "Name", "desc": "?=- HII region number from other works (1) "}, {"name": "RO", "desc": "? HII region number from Rosales-Ortega et al. (2011MNRAS.415.2439R)"}, {"name": "vZ", "desc": "? HII region number from van Zee et al. (1998, cat. J/A+AS/123/305)"}, {"name": "oDE", "desc": "Offsets from the Galactic Centre, positive to the north (N-S)"}, {"name": "oRA", "desc": "Offsets from the Galactic Centre, positive to the west (E-W)"}, {"name": "rd", "desc": "Deprojected galactocentric distance "}, {"name": "RV", "desc": "Radial velocity of H II region "}]}, {"name": "table4.dat", "desc": "The reddening-corrected fluxes of the main emission lines of H II regions", "columns": [{"name": "Gal", "desc": "Galaxy "}, {"name": "HII", "desc": "HII region number within the galaxy "}, {"name": "m_HII", "desc": "Multiplicty index on HII "}, {"name": "[OII]", "desc": "?=- [OII] 3727+3729 intensity normalized to H{beta} (1)"}, {"name": "e_[OII]", "desc": "?=- rms uncertainty on [OII] "}, {"name": "[OIII]", "desc": "?=- [OIII] 5007 intensity normalized to H{beta} (1)"}, {"name": "e_[OIII]", "desc": "?=- rms uncertainty on [OIII] "}, {"name": "[NII]", "desc": "?=- [NII] 6584 intensity normalized to H{beta} (1)"}, {"name": "e_[NII]", "desc": "?=- rms uncertainty on [NII] "}, {"name": "[SII]", "desc": "?=- [NII] 6717+6731 intensity normalized to H{beta} (1)"}, {"name": "e_[SII]", "desc": "?=- rms uncertainty on [NII] "}, {"name": "FHb", "desc": "H{beta} 4861 flux "}, {"name": "e_FHb", "desc": "rms uncertainty on FHb "}, {"name": "c(Hb)", "desc": "logarithmic extinction coefficient c(H{beta}) "}, {"name": "e_c(Hb)", "desc": "rms uncertainty on c(Hb) "}]}, {"name": "table5.dat", "desc": "Oxygen and nitrogen abundances and electron temperatures t2 in H II regions derived using the NS calibrations", "columns": [{"name": "Gal", "desc": "Galaxy "}, {"name": "HII", "desc": "HII region number, within the galaxy "}, {"name": "n_HII", "desc": "[ab] Multiplicity index on HII "}, {"name": "RG", "desc": "Galacto-centric radius in units of isophotal radius R25"}, {"name": "12+log(O/H)NS", "desc": "Abundance 12+log(O/H) using the NS calibration"}, {"name": "12+log(N/H)NS", "desc": "Abundance 12+log(N/H) using the NS calibration"}, {"name": "tNSB", "desc": "Electron temperatures t2 "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_428_2085"}} {"id": "J/MNRAS/428/2085", "title_cds": "Chandra X-ray measurements of galactic coronae", "title_create": "Li+, 2013", "year": "2013", "author": "Li J.-T., Wang Q.D.", "title_pub": "Chandra survey of nearby highly inclined disc galaxies. I. X-ray measurements of galactic coronae.", "first_author": "Li J.-T.", "ref_biblio": [""], "bibcode": ["2013MNRAS.428.2085L"], "keyword_cds": "", "keyword_pub": "galaxies: general - galaxies: haloes - X-rays: galaxies", "abstract": ["We present a systematical analysis of the Chandra observations of 53", "nearby highly inclined (i>~60{deg}) disc galaxies to study the coronae", "around them. This sample covers a broad range of galaxy properties:", "e.g. about three orders of magnitude in the star formation rate and", "more than two orders of magnitude in the stellar mass. The Chandra", "observations of the diffuse soft X-ray emission from 20 of these", "galaxies are presented for the first time. The data are reduced in a", "uniform manner, including the excision/subtraction of both resolved", "and unresolved stellar contributions. Various coronal properties, such", "as the scale height and luminosity, are characterized for all the", "sample galaxies. For galaxies with high enough counting statistics, we", "also examine the thermal and chemical states of the coronal gas. We", "note on galaxies with distinct multiwavelength characteristics which", "may affect the coronal properties. The uniformly processed images,", "spectra and brightness profiles, as well as the inferred hot gas", "parameters, form a large X-ray data base for studying the coronae", "around nearby disc galaxies. We also discuss various complications", "which may cause biases to this data base and their possible", "corrections or effects, such as the uncertainty in the thermal and", "chemical states of hot gas, the different galactic disc inclination", "angles, the presence of active galactic nuclei and the contribution of", "the emission from charge exchange at interfaces between hot and cool", "gases. Results from a detailed correlation analysis are presented in a", "companion paper to gain a more comprehensive statistical understanding", "of the origin of galactic coronae."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/sts183"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_428_476"}} {"id": "J/MNRAS/428/476", "title_cds": "Group members in the Leo cloud", "title_create": "Marino+, 2013", "year": "2013", "author": "Marino A., Plana H., Rampazzo R., Bianchi L., Rosado M., Bettoni D., Galletta G., Mazzei P., Buson L., Ambrocio-Cruz P., Gabbasov R.F.", "title_pub": "Galaxy evolution in nearby loose groups. II. Photometric and kinematic characterization of USGC U268 and USGC U376 group members in the Leo cloud.", "first_author": "Marino A.", "ref_biblio": [""], "bibcode": ["2013MNRAS.428..476M"], "see_also": ["VII/237 : HYPERLEDA. I. Catalog of galaxies (Paturel+, 2003)"], "keyword_cds": "Clusters, galaxy ; Galaxies, photometry ; Radial velocities", "keyword_pub": "galaxies: evolution - galaxies: groups: individual: USGC U268 - galaxies: groups: individual: USGC U376 - galaxies: kinematics and dynamics - galaxies: photometry - ultraviolet: galaxies", "abstract": ["This paper is the second of a series of papers in which we are", "exploring the coevolution of galaxies and groups in the local", "Universe, by adopting a multiwavelength approach. Here, we present the", "photometric and kinematic characterization of two groups, USGC U268", "and USGC U376 (U268 and U376 hereafter), which are located in", "different regions of the Leo cloud. We revisit the group membership,", "using results from recent redshift surveys, and we investigate their", "substructures. U268, which is composed of 10 catalogued members and 11", "new added members, has a small fraction (~24 per cent) of", "early-type galaxies (ETGs). U376 has 16 catalogued members plus eight", "new added members, with ~38 per cent of ETGs."], "description": ["The group sample has been selected from the catalogue of Ramella et", "al. (2002, Cat. J/AJ/123/2976). The cross-matching of the member", "galaxies of the catalogue with the GALEX and SDSS (York et al.", "2000AJ....120.1579Y) archives has led to a sample of 13 nearby groups", "that have almost all of the members covered by both surveys. Here, we", "focus on two of the above groups, U268 and U376."], "type": ["OC"], "data": "", "date_update": "16-Mar-2021", "tables": [{"name": "table1.dat", "desc": "*Characteristics of the galaxy members ", "columns": [{"name": "Group", "desc": "Group name "}, {"name": "Galaxy", "desc": "Galaxy name "}, {"name": "n_Galaxy", "desc": "[f,g ] Note on Galaxy (1) "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "n_Pos", "desc": "[a] Note on Position (1) "}, {"name": "MType", "desc": "Morphologycal type "}, {"name": "n_MType", "desc": "[ab] Note on MType (1) "}, {"name": "T", "desc": "? RC3 T type "}, {"name": "E(B-V)", "desc": "? Redenning (Taken from NED) "}, {"name": "Incl", "desc": "? Inclination "}, {"name": "logD25", "desc": "? Major axis diameter "}, {"name": "logr25", "desc": "? Axial ratio "}, {"name": "PA", "desc": "? Position angle "}, {"name": "n_PA", "desc": "[de] Note on PA (1) "}, {"name": "HV", "desc": "Mean heliocentric systemic velocity "}, {"name": "e_HV", "desc": "rms uncertainty on HV "}, {"name": "n_HV", "desc": "[c] Note on HV (1) "}, {"name": "BTmag", "desc": "? B total magnitude (AB mag) "}, {"name": "e_BTmag", "desc": "? rms uncertainty on BTmag "}]}, {"name": "table6.dat", "desc": "UV and optical photometry ", "columns": [{"name": "Group", "desc": "Group name "}, {"name": "Galaxy", "desc": "Galaxy name "}, {"name": "MType", "desc": "This paper morphological type "}, {"name": "FUV", "desc": "?=- FUV magnitude (AB mag) "}, {"name": "e_FUV", "desc": "? rms uncertainty on FUV "}, {"name": "NUV", "desc": "?=- NUV magnitude (AB mag) "}, {"name": "e_NUV", "desc": "? rms uncertainty on NUV "}, {"name": "umag", "desc": "?=- SDSS u magnitude (AB mag) "}, {"name": "e_umag", "desc": "? rms uncertainty on umag "}, {"name": "gmag", "desc": "?=- SDSS g magnitude (AB mag) "}, {"name": "e_gmag", "desc": "? rms uncertainty on gmag "}, {"name": "rmag", "desc": "?=- SDSS r magnitude (AB mag) "}, {"name": "e_rmag", "desc": "? rms uncertainty on rmag "}, {"name": "imag", "desc": "?=- SDSS i magnitude (AB mag) "}, {"name": "e_imag", "desc": "? rms uncertainty on imag "}, {"name": "zmag", "desc": "?=- SDSS z magnitude (AB mag) "}, {"name": "e_zmag", "desc": "? rms uncertainty on zmag "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_429_3047"}} {"id": "J/MNRAS/429/3047", "title_cds": "Observational parameters of SMGs programme", "title_create": "Bothwell+, 2013", "year": "2013", "author": "Bothwell M.S., Smail I., Chapman S.C., Genzel R., Ivison R.J., Tacconi L.J., Alaghband-zadeh S., Bertoldi F., Blain A.W., Casey C.M., Cox P., Greve T.R., Lutz D., Neri R., Omont A., Swinbank A.M.", "title_pub": "A survey of molecular gas in luminous sub-millimetre galaxies.", "first_author": "Bothwell M.S.", "ref_biblio": [""], "bibcode": ["2013MNRAS.429.3047B"], "keyword_cds": "", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: ISM - cosmology: observations", "abstract": ["We present the results from a survey of ^12^CO emission in 40 luminous", "sub-millimetre galaxies (SMGs), with 850-{mu}m fluxes of", "S_850{mu}m_=4-20mJy, conducted with the Plateau de Bure", "Interferometer. We detect ^12^CO emission in 32 SMGs at z~1.2-4.1,", "including 16 SMGs not previously published. Using multiple ^12^CO line", "(J_up_=2-7) observations, we derive a median spectral line energy", "distribution for luminous SMGs. We report the discovery of a", "fundamental relationship between ^12^CO FWHM and ^12^CO line", "luminosity in high-redshift starbursts, which we interpret as a", "natural consequence of the baryon-dominated dynamics within the", "regions probed by our observations. We use far-infrared luminosities", "to assess the star formation efficiency in our SMGs, finding that the", "slope of the L_'CO_-L_FIR_ relation is close to linear. We", "derive molecular gas masses, finding a mean gas mass of", "(5.3+/-1.0)x10^10^M_{sun}_. Combining these with dynamical masses, we", "determine the redshift evolution of the gas content of SMGs, finding", "that they do not appear to be significantly more gas rich than less", "vigorously star-forming galaxies at high redshifts. Finally, we", "collate X-ray observations, and study the interdependence of gas and", "dynamical properties of SMGs with their AGN activity and supermassive", "black hole masses (M_BH_), finding that SMGs lie significantly", "below the local M_BH_-{sigma} relation."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/sts562"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_429_L55"}} {"id": "J/MNRAS/429/L55", "title_cds": "Short Title", "title_create": "Banerji+, 2013", "year": "2013", "author": "Banerji M., Mcmahon R.G., Hewett P.C., Gonzalez-solares E., Koposov S.E.", "title_pub": "Hyperluminous reddened broad-line quasars at z ~ 2 from the VISTA Hemisphere Survey and WISE All-Sky Survey.", "first_author": "Banerji M.", "ref_biblio": [""], "bibcode": ["2013MNRAS.429L..55B"], "keyword_cds": "", "keyword_pub": "galaxies: active - quasars: emission lines - quasars: general", "abstract": ["We present the first sample of spectroscopically confirmed heavily", "reddened broad-line quasars selected using the new near-infrared VISTA", "Hemisphere Survey and Wide-field Infrared Survey Explorer} (WISE)", "all-sky survey. Observations of four candidates with (J-K)>2.5 and", "K<=16.5 over ~180deg^2^ lead to confirmation that two are highly", "dust-reddened broad-line Type 1 quasars at z~2. The typical dust", "extinctions are A_V_~ 2-2.5mag. We measure black hole masses of", "~10^9^M{sun} and extinction-corrected bolometric luminosities of", "~10^47^erg/s, making them some of the brightest Type 1 quasars", "currently known. Despite this, these quasars lie well below the", "detection limits of wide-field optical surveys like the Sloan Digital", "Sky Survey (SDSS) with i_AB_>22. We also present WISE photometry at", "3-22{mu}m, for our full sample of spectroscopically confirmed reddened", "quasars including those selected from the UKIDSS Large Area Survey. We", "demonstrate that the rest-frame infrared spectral energy distributions", "of these reddened quasars are similar to ultraviolet-luminous Type 1", "quasars with significant hot dust emission and starburst quasar hosts", "like Mrk 231. The average 12{mu}m flux density of our reddened quasars", "is similar to that of the recently discovered hyperluminous infrared", "galaxy (HyLIRG) WISE 1814+3412 (z=2.452) at similar redshifts, with", "two of our reddened quasars also having comparable 22{mu}m flux", "densities to this extreme HyLIRG. These optically faint, heavily", "reddened broad-line quasars are therefore among the most", "mid-infrared-luminous galaxies at z~2, now being discovered using", "WISE."], "description": ["VHS is a NIR photometric survey being conducted using the VISTA", "telescope in Chile that aims to survey 18000deg^2^ of the Southern", "celestial hemisphere to a depth 30 times fainter than the 2MASS survey", "in at least two wavebands (J and K). In the South Galactic Cap,", "4500deg^2^ will be imaged deeper, including the H band, and will have", "supplemental deep grizY imaging provided by the Dark Energy Survey.", "The remainder of the high galactic latitude sky will be imaged at YJHK", "and combined with optical photometry from the VST-ATLAS survey. In", "this work, we use \u223c180deg^2^ data from the VHS VST-ATLAS overlap", "region at 205{deg}"], "bibcode": ["2013MNRAS.431.1039H"], "keyword_cds": "Atomic physics", "keyword_pub": "atomic data - atomic processes - line: profiles", "abstract": ["Stark-broadening parameters have been calculated for 114 spectral", "lines of triply charged lead ion (Pbiv) using semiclassical", "perturbation approach in the impact approximation. The provided widths", "and shifts have been obtained for a set of temperatures from 20000 to", "300000K and an electron density of 10^17^cm^-3^. The studied lines", "correspond to transitions between the configurations", "5d^10^nl-5d^10^n'l' and 5d^9^6s^2^-5d^10^nl. Energy levels and", "oscillator strengths needed for this calculation have been calculated", "using a Hartree-Fock relativistic (HFR) approach. Comparison has also", "been made with available theoretical and experimental results. In", "addition, the regularity in the 5d^10^6s^2^S_1/2_-5d^10^np^2^P^o^_1/2_", "spectral series has been studied."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stt228"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_431_3510"}} {"id": "J/MNRAS/431/3510", "title_cds": "GX 339-4 X-ray binary", "title_create": "Salvesen+, 2013", "year": "2013", "author": "Salvesen G., Miller J.M., Reis R.C., Begelman M.C.", "title_pub": "Spectral hardening as a viable alternative to disc truncation in black hole state transitions.", "first_author": "Salvesen G.", "ref_biblio": [""], "bibcode": ["2013MNRAS.431.3510S"], "keyword_cds": "", "keyword_pub": "accretion, accretion discs - black hole physics - X-rays: binaries - X-rays: individual: GX 339-4", "abstract": ["Constraining the accretion flow geometry of black hole binaries in", "outburst is complicated by the inability of simplified multicolour", "disc models to distinguish between changes in the inner disc radius", "and alterations to the emergent spectrum, parametrized by the", "phenomenological colour-correction factor, f_col_. We analyse Rossi", "X-ray Timing Explorer observations of the low-mass Galactic black hole", "X-ray binary, GX 339-4, taken over seven epochs when the source was", "experiencing a state transition. The accretion disc component is", "isolated using a pipeline resulting in robust detections for disc", "luminosities, 10^-3^<~L_disc_/L_Edd_<~0.5. Assuming that the inner", "disc remains situated at the innermost stable circular orbit over the", "course of a state transition, we measure the relative degree of change", "in f_col_ required to explain the spectral evolution of the disc", "component. A variable f_col_ that increases by a factor of ~2.0-3.5 as", "the source transitions from the high/soft state to the low/hard state", "can adequately explain the observed disc spectral evolution. For the", "observations dominated by a disc component, the familiar scaling", "between the disc luminosity and effective temperature,", "L_disc_{prop.to}T_eff_^4^, is observed; however, significant", "deviations from this relation appear when GX 339-4 is in the hard", "intermediate and low/hard states. Allowing for an evolving f_col_", "between spectral states, the L_disc_-T_eff_^4^ law is recovered over", "the full range of disc luminosities, although this depends heavily on", "the physically conceivable range of f_col_. We demonstrate that", "physically reasonable changes in f_col_ provide a viable description", "for multiple state transitions of a black hole binary without invoking", "radial motion of the inner accretion disc."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stt436"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_432_2824"}} {"id": "J/MNRAS/432/2824", "title_cds": "UK IR telescope M33 monitoring project. III.", "title_create": "Javadi+, 2013", "year": "2013", "author": "Javadi A., van Loon J.T., Khosroshahi H., Mirtorabi M.T.", "title_pub": "The UK infrared telescope M33 monitoring project. III. Feedback from dusty stellar winds in the central square kiloparsec.", "first_author": "Javadi A.", "ref_biblio": [""], "bibcode": ["2013MNRAS.432.2824J"], "keyword_cds": "", "keyword_pub": "stars: AGB and post-AGB - stars: carbon - stars: mass-loss - supergiants - galaxies: individual: M33 - galaxies: structure", "abstract": ["We have conducted a near-infrared monitoring campaign at the UK", "Infrared Telescope, of the Local Group spiral galaxy M33 (Triangulum).", "The main aim was to identify stars in the very final stage of their", "evolution, and for which the luminosity is more directly related to", "the birth mass than the more numerous less evolved giant stars that", "continue to increase in luminosity. In this third paper of the series,", "we measure the dust production and rates of mass-loss by the pulsating", "asymptotic giant branch (AGB) stars and red supergiants. To this aim,", "we combined our time-averaged near-IR photometry with the multi-epoch", "mid-IR photometry obtained with the Spitzer Space Telescope. The", "mass-loss rates are seen to increase with increasing strength of", "pulsation and with increasing bolometric luminosity. Low-mass stars", "lose most of their mass through stellar winds, but even super-AGB", "stars and red supergiants lose ~ 40percent of their mass via a dusty", "stellar wind. More than three-quarters of the dust return is", "oxygenous. We construct a 2D map of the mass-return rate, showing a", "radial decline but also local enhancements due to agglomerations of", "massive stars. We estimate a total mass-loss rate of", "0.004-0.005M_{sun}_/yr/kpc^2^, increasing to ~0.006M_{sun}_/yr/kpc^2^", "when accounting for eruptive mass-loss (e.g., supernovae); comparing", "this to the current star formation rate of ~0.03M_{sun}_/yr/kpc^2^ we", "conclude that star formation in the central region of M33 can only be", "sustained if gas is accreted from further out in the disc or from", "circumgalactic regions."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stt640"], "data": "", "date_update": "11-May-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_432_3097"}} {"id": "J/MNRAS/432/3097", "title_cds": "Halpha/FUV ratios in star-forming regions", "title_create": "Hermanowicz+, 2013", "year": "2013", "author": "Hermanowicz M.T., Kennicutt R.C., Eldridge J.J.", "title_pub": "H{alpha} to FUV ratios in resolved star-forming region populations of nearby spiral galaxies.", "first_author": "Hermanowicz M.T.", "ref_biblio": [""], "bibcode": ["2013MNRAS.432.3097H"], "keyword_cds": "", "keyword_pub": "stars: formation - stars: luminosity function, mass function - HII regions - galaxies: spiral - galaxies: star formation", "abstract": ["We present a new study of H{alpha}/FUV flux ratios of star-forming", "regions within a sample of nearby spiral galaxies. We search for", "evidence of the existence of a cluster-mass-dependent truncation in", "the underlying stellar initial mass function (IMF). We use an", "automated approach to identification of extended objects based on the", "SExtractor algorithm to catalogue resolved Hii regions within a set of", "nearby spiral galaxies. Corrections due to dust attenuation effects", "are applied to avoid artificially boosted H{alpha}/FUV values. We use", "thebpass stellar population synthesis code to create a benchmark", "population of star-forming regions to act as a reference for our", "observations. Based on those models, we identify a zone of parameter", "space populated by regions that cannot be obtained with a", "cluster-mass-dependent truncation in the stellar IMF imposed. We find", "that the investigated galaxies display small subpopulations of", "star-forming regions falling within our zone of interest, which", "appears to be inconsistent with imposing an IMF truncation at maximum", "stellar mass dependent on the total cluster mass. The presence of", "those regions is expected in models using both stochastic and sorted", "sampling of the full extent of the stellar IMF. This result persists", "after taking dust attenuation effects into account. We highlight the", "significance of stochastic effects in environments with low star", "formation activity and in studies describing systems associated with", "small physical scales."], "object": [], "curator": "Patricia Vannier [CDS]", "alias": ["[HKE2013]"], "doi_pub": ["10.1093/mnras/stt665"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_437_195"}} {"id": "J/MNRAS/437/195", "title_cds": "Super and massive AGB stars nucleosynthesis", "title_create": "Doherty+, 2014", "year": "2014", "author": "Doherty C.L., Gil-pons P., Lau H.H.B., Lattanzio J.C., Siess L.", "title_pub": "Super and massive AGB stars. II. Nucleosynthesis and yields. Z = 0.02, 0.008 and 0.004.", "first_author": "Doherty C.L.", "ref_biblio": [""], "bibcode": ["2014MNRAS.437..195D"], "see_also": ["J/A+A/512/A10 : Evolution of massive AGB stars. III. (Siess, 2010)"], "keyword_cds": "Models, evolutionary ; Stars, giant", "keyword_pub": "nuclear reactions - nucleosynthesis, abundances - stars: AGB and post-AGB - ISM: abundances", "abstract": ["We have computed detailed evolution and nucleosynthesis models for", "super and massive asymptotic giant branch (AGB) stars over the mass", "range 6.5-9.0M_{sun}_ in divisions of 0.5M_{sun}_ with metallicities", "Z=0.02, 0.008 and 0.004. These calculations, in which we find third", "dredge-up and hot bottom burning, fill the gap between existing low-", "and intermediate-mass AGB star models and high-mass star models that", "become supernovae. For the considered metallicities, the composition", "of the yields is largely dominated by the thermodynamic conditions at", "the base of the convective envelope rather than by the pollution", "arising from third dredge-up. We investigate the effects of various", "uncertainties, related to the mass-loss rate, mixing length parameter,", "and the treatment of evolution after the envelope instability that", "develops near the end of the (super)AGB phase. Varying these", "parameters alters the yields mainly because of their impact on the", "amount of third dredge-up enrichment, and to a lesser extent on the", "hot bottom burning conditions. Our models produce significant amounts", "of ^4^He, ^7^Li (depending on the mass-loss formulation) ^13^C, ^14^N,", "^17^O, ^23^Na, ^25^Mg, as well the radioactive isotope ^26^Al in", "agreement with previous investigation. In addition, our results show", "enrichment of ^22^Ne, ^26^Mg and ^60^Fe, as well as a substantial", "increase in our proxy neutron capture species representing all species", "heavier than iron. These stars may provide important contributions to", "the Galaxy's inventory of the heavier Mg isotopes, ^14^N, ^7^Li and", "^27^Al."], "doi_pub": ["10.1093/mnras/stt1877"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "tableb1.dat", "desc": "VW93 model ", "columns": [{"name": "M", "desc": "Initial mass "}, {"name": "---", "desc": "[M] "}, {"name": "---", "desc": "[Z=] "}, {"name": "Z", "desc": "Initial metallicity "}, {"name": "Mod", "desc": "Model "}, {"name": "Species", "desc": "Species "}, {"name": "Yield", "desc": "Yield "}, {"name": "MassExp", "desc": " "}, {"name": "ProdFact", "desc": " "}, {"name": "E-Yield", "desc": " "}, {"name": "E-MassExp", "desc": " "}, {"name": "E-ProdFact", "desc": " "}]}, {"name": "tableb2.dat", "desc": "VW-M model ", "columns": [{"name": "M", "desc": "Initial mass "}, {"name": "---", "desc": "[M] "}, {"name": "---", "desc": "[Z=] "}, {"name": "Z", "desc": "Initial metallicity "}, {"name": "Mod", "desc": "Model "}, {"name": "Species", "desc": "Species "}, {"name": "Yield", "desc": "Yield "}, {"name": "MassExp", "desc": " "}, {"name": "ProdFact", "desc": " "}, {"name": "E-Yield", "desc": " "}, {"name": "E-MassExp", "desc": " "}, {"name": "E-ProdFact", "desc": " "}]}, {"name": "tableb3.dat", "desc": "Test cases for 8.5M ", "columns": [{"name": "M", "desc": "Initial mass "}, {"name": "---", "desc": "[M] "}, {"name": "---", "desc": "[Z=] "}, {"name": "Z", "desc": "Initial metallicity "}, {"name": "Mod", "desc": "Model "}, {"name": "Species", "desc": "Species "}, {"name": "Yield", "desc": "Yield "}, {"name": "MassExp", "desc": " "}, {"name": "ProdFact", "desc": " "}, {"name": "E-Yield", "desc": " "}, {"name": "E-MassExp", "desc": " "}, {"name": "E-ProdFact", "desc": " "}]}, {"name": "tableb4.dat", "desc": "Initial Compositions (Mass Fractions) ", "columns": [{"name": "Species", "desc": "Species "}, {"name": "IC20", "desc": "Initial composition for Z=0.02 "}, {"name": "IC8", "desc": "Initial composition for Z=0.008 "}, {"name": "IC4", "desc": "Initial composition for Z=0.004 "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_438_2753"}} {"id": "J/MNRAS/438/2753", "title_cds": "Galactic disc evolution", "title_create": "Mitschang+, 2014", "year": "2014", "author": "Mitschang A.W., De Silva G., Zucker D.B., Anguiano B., Bensby T., Feltzing S.", "title_pub": "Quantitative chemical tagging, stellar ages and the chemo-dynamical evolution of the Galactic disc.", "first_author": "Mitschang A.W.", "ref_biblio": [""], "bibcode": ["2014MNRAS.438.2753M"], "keyword_cds": "", "keyword_pub": "techniques: miscellaneous - stars: abundances - Galaxy: disc - Galaxy: evolution - open clusters and associations: general", "abstract": ["The early science results from the new generation of high-resolution", "stellar spectroscopic surveys, such as Galactic Archaeology with", "HERMES (GALAH) and the Gaia European Southern Observatory survey", "(Gaia-ESO), will represent major milestones in the quest to", "chemically tag the Galaxy. Yet this technique to reconstruct dispersed", "coeval stellar groups has remained largely untested until recently. We", "build on previous work that developed an empirical chemical tagging", "probability function, which describes the likelihood that two field", "stars are conatal, that is, they were formed in the same cluster", "environment. In this work, we perform the first ever blind chemical", "tagging experiment, i.e. tagging stars with no known or otherwise", "discernible associations, on a sample of 714 disc field stars with a", "number of high-quality high-resolution homogeneous metal abundance", "measurements. We present evidence that chemical tagging of field stars", "does identify coeval groups of stars, yet these groups may not", "represent distinct formation sites, e.g. as in dissolved open", "clusters, as previously thought. Our results point to several", "important conclusions, among them that group finding will be limited", "strictly to chemical abundance space, e.g. stellar ages, kinematics,", "colours, temperature and surface gravity do not enhance the", "detectability of groups. We also demonstrate that in addition to its", "role in probing the chemical enrichment and kinematic history of the", "Galactic disc, chemical tagging represents a powerful new stellar age", "determination technique."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stt2320"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_440_1880"}} {"id": "J/MNRAS/440/1880", "title_cds": "Eigenvectors for galaxy SED classification", "title_create": "Wild+, 2014", "year": "2014", "author": "Wild V., Almaini O., Cirasuolo M., Dunlop J., Mclure R., Bowler R., Ferreira J., Bradshaw E., Chuter R., Hartley W.", "title_pub": "A new method for classifying galaxy SEDs from multiwavelength photometry.", "first_author": "Wild V.", "ref_biblio": [""], "bibcode": ["2014MNRAS.440.1880W"], "keyword_cds": "Galaxies, photometry ; Models", "keyword_pub": "methods: statistical - galaxies: fundamental parameters - galaxies: luminosity function, mass function - galaxies: photometry - galaxies: statistics - galaxies: stellar content", "abstract": ["We present a new method to classify the broad-band", "optical-near-infrared spectral energy distributions (SEDs) of galaxies", "using three shape parameters (super-colours) based on a principal", "component analysis of model SEDs. As well as providing a compact", "representation of the wide variety of SED shapes, the method allows", "for easy visualization of information loss and biases caused by the", "incomplete sampling of the rest-frame SED as a function of redshift.", "We apply the method to galaxies in the United Kingdom Infrared", "Telescope Infrared Deep Sky Survey Ultra Deep Survey with 0.9~10 percent of their mass", "in a recent unsustained starburst event; and metal-poor quiescent", "dwarf galaxies. We find that quiescent galaxies account for 45 percent", "of galaxies with logM*/M_{sun}_>11, declining steadily to 13", "percent at logM*/M_{sun}_=10. The properties and mass function", "of the post-starburst galaxies are consistent with a scenario in which", "gas-rich mergers contribute to the growth of the low- and", "intermediate-mass range of the red sequence."], "description": ["Eigenvector used for the analysis."], "type": ["MC"], "doi_pub": ["10.1093/mnras/stu212"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "udsz.dat", "desc": "Eigenbasis information ", "columns": [{"name": "Filt", "desc": "Filter name (1) "}, {"name": "z", "desc": "Redshift of galaxy that would use this element "}, {"name": "lambda", "desc": "Effective wavelength of this filter at this redshift"}, {"name": "Flux", "desc": "Eigenbasis mean array in normalised f_lambda_ "}, {"name": "E1", "desc": "First eigenvector in normalised f_lambda__ "}, {"name": "E2", "desc": "Second eigenvector in normalised f_lambda_ "}, {"name": "E3", "desc": "Third eigenvector in normalised f_lambda_ "}]}, {"name": "vwsc_mnras_example.pro", "desc": "Program for calculating the first 3 super-colours for galaxies with 0.9"], "bibcode": ["2015MNRAS.446.4205B"], "keyword_cds": "", "keyword_pub": "stars: activity - binaries: eclipsing - stars: flare - starspots", "abstract": ["We review the results of the 1988 multiwavelength campaign on the", "late-type eclipsing binary YY Geminorum. Observations include:", "broad-band optical and near-infrared photometry, simultaneous optical", "and ultraviolet ({\\it IUE}) spectroscopy, X-ray ({\\it Ginga}) and", "radio (VLA) data. From models fitted to the optical light curves,", "fundamental physical parameters have been determined together with", "evidence for transient maculations (spots) located near quadrature", "longitudes and intermediate latitudes. Eclipses were observed at", "optical, ultraviolet and radio wavelengths. Significant drops in 6 cm", "radio emission near the phases of both primary and secondary eclipse", "indicate relatively compact radio emitting volumes that may lie", "between the binary components. {\\it IUE} observations during secondary", "eclipse are indicative of a uniform chromosphere saturated with Mg ii", "emission and an extended volume of Ly{alpha} emission. Profile fitting", "of high-dispersion H{alpha} spectra confirms the chromospheric", "saturation and indicates significant H{alpha} opacity to heights of a", "few percent of the photospheric radius. There is evidence for an", "enhanced H{alpha} emission region visible near phase 0.25-0.35 which", "may be associated with a large spot on the primary and with two small", "optical flares which were also observed at other wavelengths: one in", "microwave radiation and the other in X-rays. For both flares, {\\it", "L}X/{\\it L}opt is consistent with energy release in closed magnetic", "structures."], "object": ["07 34 37.58 +31 52 11.0 YY Geminorum = * alf Gem C"], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1093/mnras/stu2398"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_446_599"}} {"id": "J/MNRAS/446/599", "title_cds": "Seyfert and LINER galaxies", "title_create": "Singh+, 2015", "year": "2015", "author": "Singh V., Ishwara-Chandra C.H., Wadadekar Y., Beelen A., Kharb P.", "title_pub": "Kiloparsec-scale radio emission in Seyfert and LINER galaxies.", "first_author": "Singh V.", "ref_biblio": [""], "bibcode": ["2015MNRAS.446..599S"], "see_also": ["VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)", "VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)", "VIII/92 : The FIRST Survey Catalog, Version 2014Dec17 (Helfand+ 2015)"], "keyword_cds": "Galaxies, Seyfert ; Galaxies, radio", "keyword_pub": "galaxies: active - galaxies: Seyfert - radio continuum: galaxies", "abstract": ["Seyfert and LINER galaxies are known to exhibit compact radio emission", "on ~10-100pc scales, but larger Kiloparsec-Scale Radio structures", "(KSRs) often remain undetected in sub-arcsec high-resolution", "observations. We investigate the prevalence and nature of KSRs in", "Seyfert and LINER galaxies using the 1.4GHz VLA FIRST and NVSS", "observations. Our sample consists of 2651 sources detected in FIRST", "and of these 1737 sources also have NVSS counterparts. Considering the", "ratio of total to peak flux density ({theta}=(S_int_/S_peak_)^1/2^) as", "a parameter to infer the presence of extended radio emission we show", "that >=30% of FIRST-detected sources possess extended radio structures", "on scales larger than 1.0kpc. The use of low-resolution NVSS", "observations help us to recover faint extended KSRs that are resolved", "out in FIRST observations and results in >=42.5% KSR sources in", "FIRST-NVSS sub-sample. This fraction is only a lower limit owing to", "the combination of projection, resolution and sensitivity effects. Our", "study demonstrates that KSRs may be more common than previously", "thought and are found across all redshifts, luminosities and radio", "loudness. The extranuclear radio luminosity of KSR sources is found to", "be positively correlated with the core radio luminosity as well as the", "[OIII] {lambda}5007{AA} line luminosity and this can be interpreted as", "KSRs being powered by AGN rather than star formation. The", "distributions of the FIR-to-radio ratios and mid-IR colours of KSR", "sources are also consistent with their AGN origin. However,", "contribution from star formation cannot be ruled out particularly in", "sources with low radio luminosities."], "description": ["Our sample of Seyfert and LINER galaxies is derived from the 13th", "edition AGN catalogue of Veron-Cetty & Veron (2010A&A...518A..10V,", "Cat. VII/258) which is the most updated complete survey of the", "literature and lists all the quasars, BL Lacs, active galaxies known", "to the catalogue authors prior to 2009 July 1."], "doi_pub": ["10.1093/mnras/stu2124"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "tablea1.dat", "desc": "First 10 entries of our cross-matched catalogue of VV10 and FIRST and NVSS for our sample of Seyfert and LINER galaxies", "columns": [{"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sing (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "z", "desc": "Redshfit (from VV10) "}, {"name": "Type", "desc": "Seyfert type (from VV10) (1) "}, {"name": "Vmag", "desc": "V mangitude (from VV10) "}, {"name": "SpF", "desc": "FIRST 1.4GHz peak flux density "}, {"name": "SintF", "desc": "FIRST integrated 1.4GH flux density "}, {"name": "SizeF1", "desc": "FIRST fitted source size "}, {"name": "---", "desc": "[x] "}, {"name": "SizeF2", "desc": "FIRST fitted source size "}, {"name": "PAF", "desc": "Position angle of FIRST source "}, {"name": "RF", "desc": "Offset of FIRST counterpart from optical position "}, {"name": "SintN", "desc": "NVSS total flux density "}, {"name": "SizeN1", "desc": "NVSS fitted source size "}, {"name": "---", "desc": "[x] "}, {"name": "SizeN2", "desc": "NVSS fitted source size "}, {"name": "PAN", "desc": "Position angle of NVSS source "}, {"name": "RN", "desc": "Offset of NVSS position from optical position "}, {"name": "thetaF", "desc": "{theta}_FIRST_=(SintF/SpF)^1/2^ "}, {"name": "thetaN-F", "desc": "{theta}_NVSS-FIRST_=(SintN/SintF)^1/2^ "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_448_1945"}} {"id": "J/MNRAS/448/1945", "title_cds": "Short Title", "title_create": "Helminiak+, 2015", "year": "2015", "author": "Helminiak K.G., Graczyk D., Konacki M., Pilecki B., Ratajczak M., Pietrzynski G., Sybilski P., Villanova S., Gieren W., Pojmanski G., Konorski P., Suchomska K., Reichart D.E., Ivarsen K.M., Haislip J.B., Lacluyze A.P.", "title_pub": "Orbital and physical parameters of eclipsing binaries from the ASAS catalogue - VIII. The totally eclipsing double-giant system HD 187669.", "first_author": "Helminiak K.G.", "ref_biblio": [""], "bibcode": ["2015MNRAS.448.1945H"], "keyword_cds": "", "keyword_pub": "binaries: eclipsing - binaries: spectroscopic - stars: evolution - stars: fundamental parameters - stars: individual: HD 187669 - stars: late-type", "abstract": ["We present the first full orbital and physical analysis of HD 187669,", "recognized by the All-Sky Automated Survey (ASAS) as the eclipsing", "binary ASAS J195222-3233.7. We combined multi-band photometry from the", "ASAS and SuperWASP public archives and 0.41-m PROMPT robotic", "telescopes with our high-precision radial velocities from the HARPS", "spectrograph. Two different approaches were used for the analysis: (1)", "fitting to all data simultaneously with the WD code and (2) analysing", "each light curve (with jktebop) and radial velocities separately and", "combining the partial results at the end. This system also shows a", "total primary (deeper) eclipse, lasting for about 6 d. A spectrum", "obtained during this eclipse was used to perform atmospheric analysis", "with the moog and sme codes to constrain the physical parameters of", "the secondary. We found that ASAS J195222-3233.7 is a double-lined", "spectroscopic binary composed of two evolved, late-type giants, with", "masses of {\\it M}1 = 1.504+/-0.004 and {\\it M}2 = 1.505+/-0.004", "M_{sun}_, and radii of {\\it R}1 = 11.33+/-0.28 and {\\it R}2 =", "22.62+/-0.50 R_{sun}_. It is slightly less metal abundant than the", "Sun, and has a {\\it P} = 88.39 d orbit. Its properties are well", "reproduced by a 2.38-Gyr isochrone, and thanks to the metallicity", "estimation from the totality spectrum and high precision of the", "masses, it was possible to constrain the age down to 0.1Gyr. It is the", "first so evolved Galactic eclipsing binary measured with such good", "accuracy, and as such it is a unique benchmark for studying the late", "stages of stellar evolution."], "object": ["19 52 22.08 -32 33 39.7 HD 187669 = ASAS J195222-3233.7"], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1093/mnras/stu2680"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_448_3132"}} {"id": "J/MNRAS/448/3132", "title_cds": "Planetary nebula central stars binary fraction", "title_create": "Douchin+, 2015", "year": "2015", "author": "Douchin D., De Marco O., Frew D.J., Jacoby G.H., Jasniewicz G., Fitzgerald M., Passy J.-C., Harmer D., Hillwig T., Moe M.", "title_pub": "The binary fraction of planetary nebula central stars. II. A larger sample and improved technique for the infrared excess search.", "first_author": "Douchin D.", "ref_biblio": [""], "bibcode": ["2015MNRAS.448.3132D"], "see_also": ["J/MNRAS/428/2118 : Binarity in planetary nebula central stars (De Marco+ 2013)"], "keyword_cds": "", "keyword_pub": "techniques: photometric - surveys; binaries: general - stars: evolution - stars: statistics - planetary nebulae: general", "abstract": ["There is no conclusive explanation of why ~80% of planetary nebulae", "(PNe) are non-spherical. In the Binary Hypothesis, a binary", "interaction is a preferred channel to form a non-spherical PN. A", "fundamental step to corroborate or disprove the Binary Hypothesis is", "to estimate the binary fraction of central stars of PNe (CSPNe) and", "compare it with a prediction based on the binary fraction of the", "progenitor, main-sequence population. In this paper, the second in a", "series, we search for spatially unresolved I- and J-band flux excess", "in an extended sample of 34 CSPN by a refined measurement technique", "with a better quantification of the uncertainties. The detection rate", "of I- (J-)band flux excess is 32+/-16% (50+/-24%). This result is very", "close to what was obtained in with a smaller sample. We account", "conservatively for unobserved cool companions down to brown dwarf", "luminosities, increasing these fractions to 40+/-20% (62+/-30%). This", "step is very sensitive to the adopted brightness limit of our survey.", "Accounting for visual companions increases the binary fraction to", "46+/-23% (71+/-34%). These figures are lower than in. The error bars", "are better quantified, but still unacceptably large. Taken at face", "value, the current CSPN binary fraction is in line with the", "main-sequence progenitor population binary fraction. However,", "including white dwarfs companions could increase this fraction by as", "much as 13 (21) per cent points."], "description": ["Our Johnso-\u2013Cousins U, B, V and I images were taken during a seven", "night observing run at the National Optical Astronomical Observatory", "(NOAO) 2.1-m telescope at Kitt Peak between 2011 March 11 and 17."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stu2700"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_448_3382"}} {"id": "J/MNRAS/448/3382", "title_cds": "Short Title", "title_create": "Tanga+, 2015", "year": "2015", "author": "Tanga P., Carry B., Colas F., Delbo M., Matter A., Hanus J., Ali Lagoa V., Andrei A.H., Assafin M., Audejean M., Behrend R., Camargo J.I.B., Carbognani A., Cedres Reyes M., Conjat M., Cornero N., Coward D., Crippa R., De Ferra Fantin E., Devogele M., Dubos G., Frappa E., Gillon M., Hamanowa H., Jehin E., Klotz A., Kryszczynska A., Lecacheux J., Leroy A., Manfroid J., Manzini F., Maquet L., Morelle E., Mottola S., Polinska M., Roy R., Todd M., Vachier F., Vera Hernandez C., Wiggins P.", "title_pub": "The non-convex shape of (234) Barbara, the first Barbarian.", "first_author": "Tanga P.", "ref_biblio": [""], "bibcode": ["2015MNRAS.448.3382T"], "keyword_cds": "", "keyword_pub": "Techniques: photometric - Techniques: polarimetry - occultations - Minor planets - asteroids: individual: 234 Barbara", "abstract": ["Asteroid (234) Barbara is the prototype of a category of asteroids", "that has been shown to be extremely rich in refractory inclusions, the", "oldest material ever found in the Solar system. It exhibits several", "peculiar features, most notably its polarimetric behaviour. In recent", "years other objects sharing the same property (collectively known as", "`Barbarians') have been discovered. Interferometric observations in", "the mid-infrared with the ESO VLTI (Very Large Telescope", "Interferometer) suggested that (234) Barbara might have a bi-lobated", "shape or even a large companion satellite. We use a large set of 57", "optical light curves acquired between 1979 and 2014, together with the", "timings of two stellar occultations in 2009, to determine the rotation", "period, spin-vector coordinates, and 3-D shape of (234) Barbara, using", "two different shape reconstruction algorithms. By using the light", "curves combined to the results obtained from stellar occultations, we", "are able to show that the shape of (234) Barbara exhibits large", "concave areas. Possible links of the shape to the polarimetric", "properties and the object evolution are discussed. We also show that", "VLTI data can be modelled without the presence of a satellite."], "curator": "Tiphaine Pouvreau [CDS]", "doi_pub": ["10.1093/mnras/stv229"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_448_3442"}} {"id": "J/MNRAS/448/3442", "title_cds": "Galaxy Zoo", "title_create": "Galloway+, 2015", "year": "2015", "author": "Galloway M.A., Willett K.W., Fortson L.F., Cardamone C.N., Schawinski K., Cheung E., Lintott C.J., Masters K.L., Melvin T., Simmons B.D.", "title_pub": "Galaxy Zoo: the effect of bar-driven fuelling on the presence of an active galactic nucleus in disc galaxies.", "first_author": "Galloway M.A.", "ref_biblio": [""], "bibcode": ["2015MNRAS.448.3442G"], "keyword_cds": "", "keyword_pub": "galaxies: active - galaxies: Seyfert - galaxies: spiral", "abstract": ["We study the influence of the presence of a strong bar in disc", "galaxies which host an active galactic nucleus (AGN). Using data from", "the Sloan Digital Sky Survey and morphological classifications from", "the Galaxy Zoo 2 project, we create a volume-limited sample of 19756", "disc galaxies at 0.01"], "bibcode": ["2015MNRAS.452.3776G"], "keyword_cds": "", "keyword_pub": "galaxies: active - infrared: galaxies", "abstract": ["We examine the relationship between star formation and active galactic", "nuclei (AGN) activity by constructing matched samples of local", "(0"], "bibcode": ["2015MNRAS.452..884N"], "keyword_cds": "", "keyword_pub": "stars: emission-line, Be - stars: Wolf-Rayet - X-rays: binaries - X-rays: stars", "abstract": ["The nature of the low- to intermediate-luminosity (LX~10^32-34^erg/s)", "source population revealed in hard band (2-10keV) X-ray surveys of the", "Galactic plane is poorly understood. To overcome such problem, we", "cross-correlated the XMM-Newton 3XMM-DR4 survey with the infrared Two", "Micron All Sky Survey and Galactic Legacy Infrared Mid-Plane Survey", "Extraordinaire catalogues. We identified reliable X-ray-infrared", "associations for 690 sources. We selected 173 sources having hard", "X-ray spectra, typical of hard X-ray high-mass stars (kT>5keV), and", "517 sources having soft X-ray spectra, typical of active coronae.", "About 18 per cent of the soft sources are classified in the", "literature: ~91 percent as stars, with a minor fraction of Wolf-Rayet", "(WR) stars. Roughly 15 per cent of the hard sources are classified in", "the literature: ~68 percent as high-mass X-ray stars single or in", "binary systems (WR, Be and high-mass X-ray binaries - HMXBs), with a", "small fraction of G and B stars. We carried out infrared spectroscopic", "pilot observations at the William Herschel Telescope for five hard", "X-ray sources. Three of them are high-mass stars with spectral types", "WN7-8h, Ofpe/WN9 and Be, and LX~10^32^-10^33^erg/s. One source is a", "colliding-wind binary, while another source is a colliding-wind binary", "or a supergiant fast X-ray transient in quiescence. The Be star is a", "likely {gamma}-Cas system. The nature of the other two X-ray sources", "is uncertain. The distribution of hard X-ray sources in the parameter", "space made of X-ray hardness ratio, infrared colours and", "X-ray-to-infrared flux ratio suggests that many of the unidentified", "sources are new {gamma}-Cas analogues, WRs and low LX HMXBs. However,", "the nature of the X-ray population with Ks>=11 and average", "X-ray-to-infrared flux ratio remains unconstrained."], "description": ["We cross-matched the 3XMM-DR4 catalogue with the 2MASS and GLIMPSE", "catalogues using the method developed by Pineau et al.", "(2011A&A...527A.126P, Cat. J/A+A/527/A126)."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stv1020"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_453_172"}} {"id": "J/MNRAS/453/172", "title_cds": "Short Title", "title_create": "Ponti+, 2015", "year": "2015", "author": "Ponti G., Morris M.R., Terrier R., Haberl F., Sturm R., Clavel M., Soldi S., Goldwurm A., Predehl P., Nandra K., Belanger G., Warwick R.S., Tatischeff V.", "title_pub": "The XMM-Newton view of the central degrees of the Milky Way.", "first_author": "Ponti G.", "ref_biblio": [""], "bibcode": ["2015MNRAS.453..172P"], "keyword_cds": "", "keyword_pub": "plasmas - methods: data analysis - ISM: bubbles - ISM: kinematics and dynamics - ISM: supernova remnants - Galaxy: centre", "abstract": ["The deepest XMM-Newton mosaic map of the central 1.5{deg} of the", "Galaxy is presented, including a total of about 1.5Ms of EPIC-pn", "cleaned exposures in the central 15arcsec and about 200ks outside.", "This compendium presents broad-band X-ray continuum maps, soft X-ray", "intensity maps, a decomposition into spectral components and a", "comparison of the X-ray maps with emission at other wavelengths. Newly", "discovered extended features, such as supernova remnants (SNRs),", "superbubbles and X-ray filaments are reported. We provide an atlas of", "extended features within +/-1{deg} of Sgr A*. We discover the", "presence of a coherent X-ray-emitting region peaking around G0.1-0.1", "and surrounded by the ring of cold, mid-IR-emitting material known", "from previous work as the 'Radio Arc Bubble' and with the addition of", "the X-ray data now appears to be a candidate superbubble. Sgr A's", "bipolar lobes show sharp edges, suggesting that they could be the", "remnant, collimated by the circumnuclear disc, of an SN explosion that", "created the recently discovered magnetar, SGR J1745-2900. Soft X-ray", "features, most probably from SNRs, are observed to fill holes in the", "dust distribution, and to indicate a direct interaction between SN", "explosions and Galactic centre (GC) molecular clouds. We also discover", "warm plasma at high Galactic latitude, showing a sharp edge to its", "distribution that correlates with the location of known radio/mid-IR", "features such as the 'GC Lobe'. These features might be associated", "with an inhomogeneous hot 'atmosphere' over the GC, perhaps fed by", "continuous or episodic outflows of mass and energy from the GC region."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stv1331"], "orcid_pub": ["0000-0003-0293-3608"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_453_3685"}} {"id": "J/MNRAS/453/3685", "title_cds": "Shapley Supercluster Survey", "title_create": "Mercurio+, 2015", "year": "2015", "author": "Mercurio A., Merluzzi P., Busarello G., Grado A., Limatola L., Haines C.P., Brescia M., Cavuoti S., Dopita M., Dall'ora M., Capaccioli M., Napolitano N., Pimbblet K.A.", "title_pub": "Shapley Supercluster Survey: construction of the photometric catalogues and i-band data release.", "first_author": "Mercurio A.", "ref_biblio": [""], "bibcode": ["2015MNRAS.453.3685M"], "keyword_cds": "", "keyword_pub": "methods: data analysis; methods: observational; catalogues virtual observatory tools; galaxies: clusters: general galaxies: photometry", "mission": "", "abstract": ["The Shapley Supercluster Survey is a multi-wavelength survey covering an area of ~ 23 deg2 ( ~ 260 Mpc2 at {\\it z} = 0.048) around the supercluster core, including nine Abell and two poor clusters, having redshifts in the range 0.045-0.050. The survey aims to investigate the role of the cluster-scale mass assembly on the evolution of galaxies, mapping the effects of the environment from the cores of the clusters to their outskirts and along the filaments. The optical ({\\it ugri}) imaging acquired with OmegaCAM on the VLT Survey Telescope is essential to achieve the project goals providing accurate multi-band photometry for the galaxy population down to {\\it m}* + 6. We describe the methodology adopted to construct the optical catalogues and to separate extended and point-like sources. The catalogues reach average 5{sigma} limiting magnitudes within a 3 arcsec diameter aperture of {\\it ugri} = [24.4,24.6,24.1,23.3] and are 93 percent complete down to {\\it ugri} = [23.8,23.8,23.5,22.0] mag, corresponding to", "~ {\\it m}*{\\it r} + 8.5. The data are highly uniform in terms of observing conditions and all acquired with seeing less than 1.1 arcsec full width at half-maximum. The median seeing in {\\it r} band is 0.6 arcsec, corresponding to 0.56 kpc \\begin{tex}$h^{-1}_{70}$\\end{tex} at {\\it z} = 0.048. While the observations in the {\\it u}, {\\it g} and {\\it r} bands are still ongoing, the {\\it i}-band observations have been completed, and we present the {\\it i}-band catalogue over the whole survey area. The latter is released and it will be regularly updated, through the use of the Virtual Observatory tools. This includes 734 319 sources down to {\\it i} = 22.0 mag and it is the first optical homogeneous catalogue at such a depth, covering the central region of the Shapley supercluster."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stv1905"], "orcid_pub": ["0000-0001-9261-7849"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_458_1267"}} {"id": "J/MNRAS/458/1267", "title_cds": "Short Title", "title_create": "Verbiest+, 2016", "year": "2016", "author": "Verbiest J.P.W., Lentati L., Hobbs G., Van Haasteren R., Demorest P.B., Janssen G.H., Wang J.-B., Desvignes G., Caballero R.N., Keith M.J., Champion D.J., Arzoumanian Z., Babak S., Bassa C.G., Bhat N.D.R., Brazier A., Brem P., Burgay M., Burke-spolaor S., Chamberlin S.J., Chatterjee S., Christy B., Cognard I., Cordes J.M., Dai S., Dolch T., Ellis J.A., Ferdman R.D., Fonseca E., Gair J.R., Garver-daniels N.E., Gentile P., Gonzalez M.E., Graikou E., Guillemot L., Hessels J.W.T., Jones G., Karuppusamy R., Kerr M., Kramer M., Lam M.T., Lasky P.D., Lassus A., Lazarus P., Lazio T.J.W., Lee K.J., Levin L., Liu K., Lynch R.S., Lyne A.G., Mckee J., Mclaughlin M.A., Mcwilliams S.T., Madison D.R., Manchester R.N., Mingarelli C.M.F., Nice D.J., Oslowski S., Palliyaguru N.T., Pennucci T.T., Perera B.B.P., Perrodin D., Possenti A., Petiteau A., Ransom S.M., Reardon D., Rosado P.A., Sanidas S.A., Sesana A., Shaifullah G., Shannon R.M., Siemens X., Simon J., Smits R., Spiewak R., Stairs I.H., Stappers B.W., Stinebring D.R., Stovall K., Swiggum J.K., Taylor S.R., Theureau G., Tiburzi C., Toomey L., Vallisneri M., Van Straten W., Vecchio A., Wang Y., Wen L., You X.P., Zhu W.W., Zhu X.-J.", "title_pub": "The International Pulsar Timing Array: First data release.", "first_author": "Verbiest J.P.W.", "ref_biblio": [""], "bibcode": ["2016MNRAS.458.1267V"], "keyword_cds": "", "keyword_pub": "methods: data analysis - pulsars: general", "abstract": ["The highly stable spin of neutron stars can be exploited for a variety", "of (astro)physical investigations. In particular, arrays of pulsars", "with rotational periods of the order of milliseconds can be used to", "detect correlated signals such as those caused by gravitational waves.", "Three such 'pulsar timing arrays' (PTAs) have been set up around", "the world over the past decades and collectively form the", "'International' PTA (IPTA). In this paper, we describe the first", "joint analysis of the data from the three regional PTAs, i.e. of the", "first IPTA data set. We describe the available PTA data, the approach", "presently followed for its combination and suggest improvements for", "future PTA research. Particular attention is paid to subtle details", "(such as underestimation of measurement uncertainty and long-period", "noise) that have often been ignored but which become important in this", "unprecedentedly large and inhomogeneous data set. We identify and", "describe in detail several factors that complicate IPTA research and", "provide recommendations for future pulsar timing efforts. The first", "IPTA data release presented here (and available online) is used to", "demonstrate the IPTA's potential of improving upon gravitational-wave", "limits placed by individual PTAs by a factor of ~2 and provides a", "2{sigma} limit on the dimensionless amplitude of a stochastic", "gravitational-wave background of 1.7x10^-15^ at a frequency of", "1yr^-1^. This is 1.7 times less constraining than the limit placed by", "Shannon et al. (2010ApJ...725.1607S), due mostly to the more recent,", "high-quality data they used."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw347"], "orcid_pub": ["0000-0002-4088-896X"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_458_425"}} {"id": "J/MNRAS/458/425", "title_cds": "Short Title", "title_create": "van Vledder+, 2016", "year": "2016", "author": "van Vledder I., Van Der Vlugt D., Holwerda B.W., Kenworthy M.A., Bouwens R.J., Trenti M.", "title_pub": "The size and shape of the Milky Way disc and halo from M-type brown dwarfs in the BoRG survey.", "first_author": "van Vledder I.", "ref_biblio": [""], "bibcode": ["2016MNRAS.458..425V"], "keyword_cds": "", "keyword_pub": "techniques: photometric- stars: low-mass - stars: luminosity function, mass function - Galaxy: disc - Galaxy: halo - Galaxy: stellar content", "abstract": ["We have identified 274 M-type brown dwarfs in the Hubble Space", "Telescope's Wide Field Camera 3 pure parallel fields from the", "Brightest of Reionizing Galaxies (BoRG) survey for high-redshift", "galaxies. These are near-infrared observations with multiple lines of", "sight out of our Milky Way. Using these observed M-type brown dwarfs,", "we fitted a Galactic disc and halo model with a Markov chain Monte", "Carlo analysis. This model worked best with the scalelength of the", "disc fixed at h=2.6kpc. For the scaleheight of the disc, we found", "z0=0.29^+0.02^_0.019_kpc and for the central number density,", "{rho}0=0.29^+0.20^_-0.13_pc^\u22123^. For the halo, we derived a", "flattening parameter {kappa}=0.45+/-0.04 and a power-law index", "p=2.4+/-0.07. We found the fraction of M-type brown dwarfs in the", "local density that belong to the halo to be", "f_h_=0.0075^+0.0025^_-0.0019_. We found no correlation between subtype", "of M-dwarf and any model parameters. The total number of M-type brown", "dwarfs in the disc and halo was determined to be", "58.2^+9.81^_-6.70_x10^9^. We found an upper limit for the fraction of", "M-type brown dwarfs in the halo of 7^+5^_-4_ per cent. The upper limit", "for the total Galactic disc mass in M-dwarfs is", "4.34^+0.73^_-0.5_M_{sun}_, assuming all M-type brown dwarfs have a", "mass of 80M_J_."], "description": ["The brown dwarfs used in this research were found with the Brightest", "of Reionizing Galaxies (BoRG) survey. Observations were made with the", "WFC3 aboard the HST during a pure-parallel programme. The WFC3 was", "taking exposures whilst the HST was pointing for primary spectroscopic", "observations on e.g. quasars"], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw258"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_460_1846"}} {"id": "J/MNRAS/460/1846", "title_cds": "NGC 6273 intrinsic abundance spread", "title_create": "Yong+, 2016", "year": "2016", "author": "Yong D., Da Costa G.S., Norris J.E.", "title_pub": "Confirming the intrinsic abundance spread in the globular cluster NGC 6273 (M19) with calcium triplet spectroscopy.", "first_author": "Yong D.", "ref_biblio": [""], "bibcode": ["2016MNRAS.460.1846Y"], "see_also": ["II/246 : 2MASS All-Sky Catalog of Point Sources (Cutri+ 2003)", "VII/233 : The 2MASS Extended sources (IPAC/UMass, 2003-2006)", "J/MNRAS/438/3507 : NGC 5824 calcium triplet equivalent widths (Da Costa+, 2014)"], "keyword_cds": "Clusters, globular ; Photometry, infrared ; Abundances ;", "keyword_pub": "stars: abundances - stars: Population II - globular clusters: general - globular clusters: individual: NGC 6273", "abstract": ["We present metallicities for red giant stars in the globular cluster", "NGC 6273 based on intermediate resolution GMOS-S spectra of the", "calcium triplet region. For the 42 radial velocity members with", "reliable calcium triplet line strength measurements, we obtain", "metallicities, [Fe/H], using calibrations established from standard", "globular clusters. We confirm the presence of an intrinsic abundance", "dispersion identified by Johnson et al. The total range in [Fe/H] is", "~1.0dex and after taking into account the measurement errors, the", "intrinsic abundance dispersion is {sigma}_int_[Fe/H]=0.17dex. Among", "the Galactic globular clusters, the abundance dispersion in NGC 6273", "is only exceeded by {omega} Cen, which is regarded as the remnant of a", "disrupted dwarf galaxy, and M54, which is the nuclear star cluster of", "the Sagittarius dwarf galaxy. If these three globular clusters share", "the same formation mechanism, then NGC 6273 may also be the remnant", "nucleus of a disrupted dwarf galaxy."], "description": ["Programme stars (see Table 1) were selected from JK colour-magnitude", "diagrams (CMD) using 2MASS photometry (Skrutskie et al., 2006, Cat.", "VII/233). All targets occupy plausible locations in the J-K versus K", "CMD. Specifically, we required 0.68<=J-K<=1.2 and 8.572<=K<=13.0.", "Furthermore, all program stars were required to have 'AAA' 2MASS", "photometric quality flags and to lie within 3 arcmin of the cluster", "centre.", "Observations of the program stars were obtained using the GMOS-S", "multi-object spectrograph at the Gemini-S telescope in queue mode", "(GS-2012A-Q-58). All observations were taken on 2012 May 05 and the", "set-up was identical to that of Da Costa et al. (2014, Cat.", "J/MNRAS/438/3507). We used the R831 grating and the RG610 filter with", "central wavelengths of 8550 and 8600{AA} (wavelength coverage was", "typically from ~7500 to ~9000{AA})."], "type": ["OC"], "doi_pub": ["10.1093/mnras/stw1091"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Program stars ", "columns": [{"name": "2MASS", "desc": "2MASS name (HHMMSSss+DDMMSSs) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Mask", "desc": "[1/6] Mask number "}, {"name": "Jmag", "desc": "2MASS J magnitude "}, {"name": "Hmag", "desc": "2MASS H magnitude "}, {"name": "Kmag", "desc": "2MASS K magnitude "}]}, {"name": "table2.dat", "desc": "Radial velocities, equivalent widths and metallicities", "columns": [{"name": "2MASS", "desc": "2MASS name (HHMMSSss+DDMMSSs) "}, {"name": "Mask", "desc": "[1/6] Mask number "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "EW8542a", "desc": "?=- Equivalent width at 8542{AA} measured from central wavelength at 8550{AA}"}, {"name": "EW8542b", "desc": "?=- Equivalent width at 8542{AA} measured from central wavelength at 8600{AA}"}, {"name": "EW8662a", "desc": "?=- Equivalent width at 8662{AA} measured from central wavelength at 8550{AA}"}, {"name": "EW8662b", "desc": "?=- Equivalent width at 8662{AA} measured from central wavelength at 8600{AA}"}, {"name": "SW", "desc": "Sum of the equivalent widths, {Sigma}W "}, {"name": "e_SW", "desc": "rms uncertainty on SW "}, {"name": "W'", "desc": "?=- Reduced equivalent width "}, {"name": "[Fe/H]", "desc": "?=- Metallicity "}, {"name": "e_[Fe/H]", "desc": "?=- rms uncertainty on [Fe/H] "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_460_2611"}} {"id": "J/MNRAS/460/2611", "title_cds": "APOGEE K and M dwarfs", "title_create": "Schmidt+, 2016", "year": "2016", "author": "Schmidt S.J., Wagoner E.L., Johnson J.A., Davenport J.R.A., Stassun K.G., Souto D., Ge J.", "title_pub": "Examining the relationships between colour, Teff, and [M/H] for APOGEE K and M dwarfs.", "first_author": "Schmidt S.J.", "ref_biblio": [""], "bibcode": ["2016MNRAS.460.2611S"], "keyword_cds": "", "keyword_pub": "surveys - stars: abundances - stars: fundamental parameters - stars: late-type - stars: low-mass", "abstract": ["We present the effective temperatures (Teff), metallicities, and", "colours in Sloan Digital Sky Survey (SDSS), Two Micron All Sky Survey,", "and Wide-field Infrared Survey Explorer filters, of a sample of 3834", "late-K and early-M dwarfs selected from the SDSS Apache Point", "Observatory Galactic Evolution Experiment (APOGEE) spectroscopic", "survey ASPCAP (APOGEE Stellar Parameters and Chemical Abundances", "Pipeline) catalogue. We confirm that ASPCAP Teff values between", "3550"], "bibcode": ["2016MNRAS.460.3232C"], "keyword_cds": "", "keyword_pub": "radiation mechanisms: general - shock waves - gamma-ray burst: general - supernovae: general - galaxies: abundances - galaxies: high-redshift", "abstract": ["We compare the physical parameters and the relative abundances", "calculated throughout supernova (SN) and {gamma}-ray burst (GRB) host", "galaxies using a detailed modelling of the spectra. The coupled effect", "of shocks and radiation from the starburst within the host galaxy is", "considered. We have found the following. (i) Shock velocities are", "lower in long-period GRBs (LGRBs) than in SN host galaxies. (ii) O/H", "relative abundances in SN hosts are scattered within a range", "8.0<12+log(O/H)<8.85 but they are close to solar in LGRB hosts. LGRB", "galaxies hosting Wolf-Rayet stars have He/H=0.13 in a few objects.", "(iii) The starburst temperatures within a few SN hosts are relatively", "high (T*>10^5^K). The values of T* in LGRB hosts are ~3-8x10^4^K. (iv)", "The H{alpha} absolute flux calculated from the emitting clouds of a", "few SN hosts at 0.1"], "bibcode": ["2016MNRAS.462.1563M"], "keyword_cds": "Stars, nearby ; Abundances", "keyword_pub": "stars: abundances - planetary systems", "abstract": ["We conducted an analysis of the distribution of elements from lithium", "to europium in 200 dwarfs in the solar neighbourhood (~20pc)", "with temperatures in the range 4800-6200K and metallicities [Fe/H]", "higher than -0.5dex. Determinations of atmospheric parameters and the", "chemical compositions of the dwarfs were taken from our previous", "studies. We found that the lithium abundances in the planet-hosting", "solar-analogue stars of our sample were lower than those in the stars", "without planetary systems. Our results reveal no significant", "differences exceeding the determination errors for the abundances of", "investigated elements, except for aluminium and barium, which are more", "and less abundant in the planet-hosting stars, respectively. We did", "not find confident dependences of the lithium, aluminium and barium", "abundances on the ages of our target stars (which is probably because", "of the small number of stars). Furthermore, we found no correlation", "between the abundance differences in [El/Fe] and the condensation", "temperature (T_cond_) for stars in the 16 Cyg binary system, unlike", "the case for 51 Peg (HD 217014), for which a slight excess of volatile", "elements and a deficit of refractories were obtained relative to those", "of solar twins. We found that one of the components of 16 Cyg exhibits", "a slightly higher average abundance than its counterpart", "(<[El/H](A-B)>=0.08+/-0.02dex); however, no significant abundance", "trend versus T_cond_ was observed. Owing to the relatively large", "errors, we cannot provide further constraints for this system."], "description": ["Our sample consists of 200 dwarfs with temperatures in the range", "4800-6200K and metallicities from -0.4dex, corresponding to the", "range of stellar parameters of 14 stars that host planets", "(Exoplanets.eu data base; Schneider et al., 2011A&A...532A..79S) from", "our data base."], "type": ["OC"], "doi_pub": ["10.1093/mnras/stw1658"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "tablea1.dat", "desc": "Comparison of atmospheric parameters for each hosting planet stars in our sample with the data of other authors", "columns": [{"name": "HD", "desc": "HD number "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "surface gravity "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "r_[Fe/H]", "desc": "Reference for [Fe/H] "}]}, {"name": "tablea2.dat", "desc": "Abundance of hosting planet stars ", "columns": [{"name": "HD", "desc": "HD number "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "Li", "desc": "?=- Lithium abundance "}, {"name": "Liup", "desc": "?=- Upper limit on Lithium abundance "}, {"name": "[O/Fe]", "desc": "?=- Abundance [O/Fe] "}, {"name": "[Na/Fe]", "desc": "?=- Abundance [Na/Fe] "}, {"name": "[Al/Fe]", "desc": "?=- Abundance [Al/Fe] "}, {"name": "[Mg/Fe]", "desc": "?=- Abundance [Mg/Fe] "}, {"name": "[S/Fe]", "desc": "?=- Abundance [S/Fe] "}, {"name": "[Si/Fe]", "desc": "Abundance [Si/Fe] "}, {"name": "[Ca/Fe]", "desc": "Abundance [Ca/Fe] "}, {"name": "[Mn/Fe]", "desc": "?=- Abundance [Mn/Fe] "}, {"name": "[Ni/Fe]", "desc": "Abundance [Ni/Fe] "}, {"name": "[Zn/Fe]", "desc": "Abundance [Zn/Fe] "}, {"name": "[Y/Fe]", "desc": "Abundance [Y/Fe] "}, {"name": "[Zr/Fe]", "desc": "?=- Abundance [Zr/Fe] "}, {"name": "[Ba/Fe]", "desc": "Abundance [Ba/Fe] "}, {"name": "[La/Fe]", "desc": "Abundance [La/Fe] "}, {"name": "[Ce/Fe]", "desc": "Abundance [Ce/Fe] "}, {"name": "[Nd/Fe]", "desc": "?=- Abundance [Nd/Fe] "}, {"name": "[Sm/Fe]", "desc": "Abundance [Sm/Fe] "}, {"name": "[Eu/Fe]", "desc": "?=- Abundance [Eu/Fe] "}]}, {"name": "tablea3.dat", "desc": "Abundance of stars without planets (Li-Eu) ", "columns": [{"name": "Name", "desc": "Star name "}, {"name": "n_Name", "desc": "[*] * for solar-analogue stars "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "[Fe/H]", "desc": "?=- Metallicity "}, {"name": "Li", "desc": "?=- Lithium abundance "}, {"name": "Liup", "desc": "?=- Upper limit Lithium abundance "}, {"name": "[O/Fe]", "desc": "?=- Abundance [O/Fe] "}, {"name": "[Na/Fe]", "desc": "?=- Abundance [Na/Fe] "}, {"name": "[Al/Fe]", "desc": "?=- Abundance [Al/Fe] "}, {"name": "[Mg/Fe]", "desc": "?=- Abundance [Mg/Fe] "}, {"name": "[S/Fe]", "desc": "?=- Abundance [S/Fe] "}, {"name": "[Si/Fe]", "desc": "?=- Abundance [Si/Fe] "}, {"name": "[Ca/Fe]", "desc": "?=- Abundance [Ca/Fe] "}, {"name": "[Mn/Fe]", "desc": "?=- Abundance [Mn/Fe] "}, {"name": "[Ni/Fe]", "desc": "?=- Abundance [Ni/Fe] "}, {"name": "[Zn/Fe]", "desc": "?=- Abundance [Zn/Fe] "}, {"name": "[Y/Fe]", "desc": "?=- Abundance [Y/Fe] "}, {"name": "[Zr/Fe]", "desc": "?=- Abundance [Zr/Fe] "}, {"name": "[Ba/Fe]", "desc": "?=- Abundance [Ba/Fe] "}, {"name": "[La/Fe]", "desc": "?=- Abundance [La/Fe] "}, {"name": "[Ce/Fe]", "desc": "?=- Abundance [Ce/Fe] "}, {"name": "[Nd/Fe]", "desc": "?=- Abundance [Nd/Fe] "}, {"name": "[Sm/Fe]", "desc": "?=- Abundance [Sm/Fe] "}, {"name": "[Eu/Fe]", "desc": "?=- Abundance [Eu/Fe] "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_463_1213"}} {"id": "J/MNRAS/463/1213", "title_cds": "s-process enhanced barium stars", "title_create": "Mahanta+, 2016", "year": "2016", "author": "Mahanta U., Karinkuzhi D., Goswami A., Duorah K.", "title_pub": "Abundance analysis of s-process enhanced barium stars.", "first_author": "Mahanta U.", "ref_biblio": [""], "bibcode": ["2016MNRAS.463.1213M"], "keyword_cds": "Stars, peculiar ; Equivalent widths", "keyword_pub": "stars: abundances - stars: chemically peculiar stars: individual: HD 49641 - stars: individual: HD 58368 - stars: individual: HD 119650 - stars: individual: HD 191010", "abstract": ["Detailed chemical composition studies of stars with enhanced", "abundances of neutron-capture elements can provide observational", "constraints for neutron-capture nucleosynthesis studies and clues for", "understanding their contribution to the Galactic chemical enrichment.", "We present abundance results from high-resolution spectral analyses of", "a sample of four chemically peculiar stars characterized by s-process", "enhancement. High-resolution spectra (R~42000) of these objects", "spanning a wavelength range from 4000 to 6800{AA} are taken from the", "ELODIE archive. We have estimated the stellar atmospheric parameters,", "the effective temperature T_eff_, the surface gravity log g and", "metallicity [Fe/H] from local thermodynamic equilibrium analysis using", "model atmospheres. We report estimates of elemental abundances for", "several neutron-capture elements, Sr, Y, Zr, Ba, La, Ce, Pr, Nd, Sm,", "Eu and Dy. While HD 49641 and HD 58368 show [Ba/Fe]>= 1.16, the other", "two objects HD 119650 and HD 191010 are found to be mild barium stars", "with [Ba/Fe]~0.4. The derived abundances of the elements are", "interpreted on the basis of existing theories for understanding their", "origin and evolution."], "description": ["Elemental abundances are presented for four peculiar stars listed in", "the barium star catalogue of Lu (1991AJ....101.2229L, Cat. V/81). All", "the objects are found to be low-velocity objects (Vr<45km/s)."], "object": ["06 49 29.45 +03 41 30.2 HD 49641 = HIP 32713", "07 25 38.97 +07 33 39.0 HD 58368 = HIP 36042", "13 44 27.12 +00 42 07.0 HD 119650 = HIP 67050", "20 06 45.84 +25 41 06.8 HD 191010 = HIP 99067"], "type": ["OC"], "doi_pub": ["10.1093/mnras/stw1995"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table4.dat", "desc": "Equivalent widths of Fe lines used for deriving atmospheric parameters", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "Ion", "desc": "Ion "}, {"name": "Elow", "desc": "Lower value of energy potential "}, {"name": "loggf", "desc": "Oscillator strength "}, {"name": "EW1", "desc": "?=- HD 49641 equivalent width "}, {"name": "e_EW1", "desc": "? rms uncertainty on EW1 "}, {"name": "f_EW1", "desc": "[h] h for hfs-syn "}, {"name": "EW2", "desc": "?=- HD 58368 equivalent width "}, {"name": "e_EW2", "desc": "? rms uncertainty on EW3 "}, {"name": "f_EW2", "desc": "[h] h for hfs-syn "}, {"name": "EW3", "desc": "?=- HD 119650 equivalent width "}, {"name": "e_EW3", "desc": "? rms uncertainty on EW3 "}, {"name": "f_EW3", "desc": "[h] h for hfs-syn "}, {"name": "EW4", "desc": "?=- HD 191010 equivalent width "}, {"name": "e_EW4", "desc": "? rms uncertainty on EW4 "}, {"name": "f_EW4", "desc": "[h] h for hfs-syn "}, {"name": "Ref", "desc": "[1/19] Reference (1) "}]}, {"name": "table8.dat", "desc": "Equivalent widths of lines used for calculation of elemental abundances", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "Ion", "desc": "Ion "}, {"name": "Elow", "desc": "Lower value of energy potential "}, {"name": "loggf", "desc": "Oscillator strength "}, {"name": "EW1", "desc": "?=- HD 49641 equivalent width "}, {"name": "e_EW1", "desc": "? rms uncertainty on EW1 "}, {"name": "f_EW1", "desc": "[h] h for hfs-syn "}, {"name": "EW2", "desc": "?=- HD 58368 equivalent width "}, {"name": "e_EW2", "desc": "? rms uncertainty on EW3 "}, {"name": "f_EW2", "desc": "[h] h for hfs-syn "}, {"name": "EW3", "desc": "?=- HD 119650 equivalent width "}, {"name": "e_EW3", "desc": "? rms uncertainty on EW3 "}, {"name": "f_EW3", "desc": "[h] h for hfs-syn "}, {"name": "EW4", "desc": "?=- HD 191010 equivalent width "}, {"name": "e_EW4", "desc": "? rms uncertainty on EW4 "}, {"name": "f_EW4", "desc": "[h] h for hfs-syn "}, {"name": "Ref", "desc": "[1/19] Reference (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_463_2494"}} {"id": "J/MNRAS/463/2494", "title_cds": "Short Title", "title_create": "Fang+, 2016", "year": "2016", "author": "Fang X.-S., Zhao G., Zhao J.-K., Chen Y.-Q., Bharat Kumar Y.", "title_pub": "Stellar activity with LAMOST. I. Spot configuration in Pleiades.", "first_author": "Fang X.-S.", "ref_biblio": [""], "bibcode": ["2016MNRAS.463.2494F"], "keyword_cds": "", "keyword_pub": "stars: activity - stars: late-type - stars: rotation - starspots", "abstract": ["We use the spectra of Pleiades and field stars from the LAMOST DR2", "archive to study how spottedness and activity vary as a function of", "mass at young ages. We obtained the standard TiO band strength by", "measuring TiO bands near 7050{AA} from LAMOST spectra (R~=1800) for a", "large sample of field GKM dwarfs with solar metallicity. Analysis", "shows that active dwarfs, including those of late G and early K types,", "have extra TiO absorption compared to their inactive counterparts,", "indicating the presence of cool spots on their surface. Active late K", "and M dwarfs show deeper TiO2 and shallower TiO4 compared to inactive", "stars at a given TiO5, which could be partly explained through cool", "spots. We estimated the cool-spot fractional coverage for 304 Pleiades", "candidates by modelling their TiO2 (and TiO5) band strength with", "respect to the standard value. The results show that the surfaces of a", "large fraction of K- and M-type members have very large spot coverage", "(~50 per cent). We analysed the correlation between spot", "coverage, rotation and the amplitude of light variation, and found", "spot coverage on slow rotators (R_o_>0.1) increases with decreasing", "Rossby number R_o_. Interestingly, we detected a saturation-like", "feature for spot coverage in fast rotators with a saturation level of", "40-50 per cent. In addition, the spot distribution in hotter fast", "rotators is more symmetrical compared to slow rotators. More", "interestingly, we detected a large spot coverage in many M-type", "members with no or little light variation. In the bigger picture,", "these results provide important constraints for the stellar dynamos of", "these cool active stars."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw1923"], "orcid_pub": ["0000-0003-3240-1688"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_463_2640"}} {"id": "J/MNRAS/463/2640", "title_cds": "SDSS-DR12 QSOs MgII absorption systems", "title_create": "Raghunathan+, 2016", "year": "2016", "author": "Raghunathan S., Clowes R.G., Campusano L.E., Sochting I.K., Graham M.J., Williger G.M.", "title_pub": "Intervening Mg II absorption systems from the SDSS DR12 quasar spectra.", "first_author": "Raghunathan S.", "ref_biblio": [""], "bibcode": ["2016MNRAS.463.2640R"], "see_also": ["J/MNRAS/452/4153 : SDSS DR12 QSOs [OIII] doublet (Albareti+, 2015)"], "keyword_cds": "Surveys ; QSOs ; Spectroscopy ; Equivalent widths", "keyword_pub": "catalogues - quasars: absorption lines - large-scale structure of Universe", "abstract": ["We present the catalogue of the MgII absorption systems detected at a", "high significance level using an automated search algorithm in the", "spectra of quasars from the 12th data release of the Sloan Digital Sky", "Survey. A total of 266,433 background quasars were searched for the", "presence of absorption systems in their spectra. The continuum", "modelling for the quasar spectra was performed using a mean filter. A", "pseudo-continuum derived using a median filter was used to trace the", "emission lines. The absorption system catalogue contains 39,694 Mg II", "systems detected at a 6.0, 3.0{sigma} level respectively for the two", "lines of the doublet. The catalogue was constrained to an absorption", "line redshift of 0.35<=z_2796_<=2.3. The rest-frame equivalent", "width of the {lambda}2796 line ranges between 0.2<=W_r_<=6.2{AA}.", "Using Gaussian noise-only simulations, we estimate a false positive", "rate of 7.7 per cent in the catalogue. We measured the number density", "dN^2796^/dz of MgII absorbers and find evidence for steeper", "evolution of the systems with W_r_>=1.2{AA} at low redshifts", "(z_2796_<=1.0), consistent with other earlier studies. A suite of", "null tests over the redshift range 0.5<=z_2796_<=1.5 was used to", "study the presence of systematics and selection effects like the", "dependence of the number density evolution of the absorption systems", "on the properties of the background quasar spectra. The null tests do", "not indicate the presence of any selection effects in the absorption", "catalogue if the quasars with spectral signal-to-noise level less than", "5.0 are removed. The resultant catalogue contains 36,981 absorption", "systems. The Mg II absorption catalogue is publicly available and can", "be downloaded from the link http://srini.ph.unimelb.edu.au/mgii.php."], "description": ["We describe the MgII absorption catalogue detected using an automated", "search algorithm from the spectra of the SDSS DR12Q. The detection", "threshold was SNR >= 6.0, 3.0 respectively for the two lines of the", "doublet. The continuum fitting is performed using a mean filter", "algorithm which was modified with a pseudo-continuum using a median", "filter to trace the emission lines. The catalogue contains 39694", "systems distributed in the EW range 0.2<=Wr<=6.2{AA} constrained to", "the redshift range 0.35<=z<=2.3."], "type": ["OC"], "doi_pub": ["10.1093/mnras/stw2095"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "MgII absorption catalogue ", "columns": [{"name": "SDSS", "desc": "SDSS DR12 name (HHMMSS.SS+DDMMSS.s) "}, {"name": "P-M-F", "desc": "SDSS DR12 plate-mjd-fibre "}, {"name": "RAdeg", "desc": "Rigth ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "zQSO", "desc": "QSO redshift "}, {"name": "imag", "desc": "QSO PSF i-band magnitude "}, {"name": "zabs", "desc": "Absorption redshift "}, {"name": "e_zabs", "desc": "rms uncertainty on zabs "}, {"name": "EW2796", "desc": "Rest-frame MgII 2796{AA} equivalent width "}, {"name": "e_EW2796", "desc": "rms uncertainty on EW2796 "}, {"name": "EW2803", "desc": "Rest-frame MgII 1803{AA} equivalent width "}, {"name": "e_EW2803", "desc": "rms uncertainty on EW1803 "}, {"name": "Flag", "desc": "[0/1] Flag showing if the detection could be a CIV line"}, {"name": "SNRcon", "desc": "Continuum signal-to-noise ratio "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_464_274"}} {"id": "J/MNRAS/464/274", "title_cds": "New variable stars", "title_create": "Sokolovsky+, 2017", "year": "2017", "author": "Sokolovsky K.V., Gavras P., Karampelas A., Antipin S.V., Bellas-velidis I., Benni P., Bonanos A.Z., Burdanov A.Y., Derlopa S., Hatzidimitriou D., Khokhryakova A.D., Kolesnikova D.M., Korotkiy S.A., Lapukhin E.G., Moretti M.I., Popov A.A., Pouliasis E., Samus N.N., Spetsieri Z., Veselkov S.A., Volkov K.V., Yang M., Zubareva A.M.", "title_pub": "Comparative performance of selected variability detection techniques in photometric time series data.", "first_author": "Sokolovsky K.V.", "ref_biblio": [""], "bibcode": ["2017MNRAS.464..274S"], "keyword_cds": "Stars, variable ; Photometry", "keyword_pub": "methods: data analysis - methods: statistical - stars: variables: general", "abstract": ["Photometric measurements are prone to systematic errors presenting a", "challenge to low-amplitude variability detection. In search for a", "general-purpose variability detection technique able to recover a", "broad range of variability types including currently unknown ones, we", "test 18 statistical characteristics quantifying scatter and/or", "correlation between brightness measurements. We compare their", "performance in identifying variable objects in seven time series data", "sets obtained with telescopes ranging in size from a telephoto lens to", "1 m-class and probing variability on time-scales from minutes to", "decades. The test data sets together include light curves of 127 539", "objects, among them 1251 variable stars of various types and represent", "a range of observing conditions often found in ground-based", "variability surveys. The real data are complemented by simulations. We", "propose a combination of two indices that together recover a broad", "range of variability types from photometric data characterized by a", "wide variety of sampling patterns, photometric accuracies and", "percentages of outlier measurements. The first index is the", "interquartile range (IQR) of magnitude measurements, sensitive to", "variability irrespective of a time-scale and resistant to outliers. It", "can be complemented by the ratio of the light-curve variance to the", "mean square successive difference, 1/{eta}, which is efficient in", "detecting variability on time-scales longer than the typical time", "interval between observations. Variable objects have larger 1/{eta}", "and/or IQR values than non-variable objects of similar brightness.", "Another approach to variability detection is to combine many", "variability indices using principal component analysis. We present 124", "previously unknown variable stars found in the test data."], "description": ["We compare 18 variability indices quantifying the overall scatter", "and/or degree of correlations between consecutive measurements in a", "light curve. The ability of these indices to distinguish variable", "stars from non-variable ones is tested on seven data sets collected", "with various ground-based telescopes and on simulated data", "incorporating actual light curves of non-variable objects as realistic", "models of photometric noise. We apply the PCA in search for an optimal", "combination of multiple variability indices.", "We were able to identify 124 new variable stars during the test.", "The information about the new variables is summarized in Table 4."], "type": ["CCC"], "doi_pub": ["10.1093/mnras/stw2262"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table4.dat", "desc": "New variable stars found in the test data ", "columns": [{"name": "Name", "desc": "Name "}, {"name": "OName", "desc": "Other name "}, {"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "mag1", "desc": "Lower value of magnitude interval "}, {"name": "---", "desc": "[-] "}, {"name": "mag2", "desc": "Upper value of magnitude interval "}, {"name": "u_mag2", "desc": "Uncertainty flag on magnitude interval "}, {"name": "Band", "desc": "[VI] Band for magnitude interval "}, {"name": "Type", "desc": "Variable type "}, {"name": "Per", "desc": "? Period "}, {"name": "u_Per", "desc": "Uncertainty flag on Per "}, {"name": "n_Per", "desc": "Note on Per "}, {"name": "n_Epoch", "desc": "[min max] Minimum of maximum for Epoch "}, {"name": "Epoch", "desc": "? Epoch "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_464_3920"}} {"id": "J/MNRAS/464/3920", "title_cds": "GALEX/WISE early-type galaxies sample", "title_create": "Simonian+, 2017", "year": "2017", "author": "Simonian G.V., Martini P.", "title_pub": "Circumstellar dust, PAHs and stellar populations in early-type galaxies: insights from GALEX and WISE.", "first_author": "Simonian G.V.", "ref_biblio": [""], "bibcode": ["2017MNRAS.464.3920S"], "see_also": ["J/MNRAS/413/813 : ATLAS3D project. I. (Cappellari+, 2011)"], "keyword_cds": "Galaxy catalogs ; Photometry, ultraviolet ; Photometry, infrared ; Morphology", "keyword_pub": "galaxies: elliptical and lenticular, cD - galaxies: stellar content - infrared: galaxies - ultraviolet: galaxies", "abstract": ["A majority of early-type galaxies contain interstellar dust, yet the", "origin of this dust, and why the dust sometimes exhibits unusual", "polycyclic aromatic hydrocarbon (PAH) ratios, remains a mystery. If", "the dust is internally produced, it likely originates from the large", "number of asymptotic giant branch stars associated with the old", "stellar population. We present GALEX and WISE elliptical aperture", "photometry of ~310 early-type galaxies with Spitzer mid-infrared", "spectroscopy and/or ancillary data from ATLAS3D, to characterize their", "circumstellar dust and the shape of the radiation field that", "illuminates the interstellar PAHs. We find that circumstellar dust is", "ubiquitous in early-type galaxies, which indicates some tension", "between stellar population age estimates and models for circumstellar", "dust production in very old stellar populations. We also use dynamical", "masses from ATLAS3D to show that WISE W1 (3.4um) mass-to-light", "ratios are consistent with the initial mass function variation found", "by previous work. While the stellar population differences in", "early-type galaxies correspond to a range of radiation field shapes", "incident upon the diffuse dust, the ratio of the ionization-sensitive", "7.7um/11.3um PAH feature does not correlate with the shape of", "the radiation field, nor to variations with the size-sensitive", "11.3um/17um ratio. The 7.7um/11.3um PAH ratio does tend to be smaller", "in galaxies with proportionally greater H2 emission, which is evidence", "that processing of primarily smaller grains by shocks is responsible", "for the unusual ratios, rather than substantial differences in the", "overall PAH size or ionization distribution."], "description": ["We use MIR and UV photometry to study circumstellar and interstellar", "dust in early-type galaxies (ETGs). Our sample is drawn from two", "recent, comprehensive studies of ETGs: the characterizations of", "interstellar dust in ETGs with Spitzer-IRS spectra (Rampazzo et al.,", "2013MNRAS.432..374R), and the stellar population and dynamical study", "from the ATLAS3D survey (Cappellari et al., 2011, Cat.", "J/MNRAS/413/813."], "type": ["CCC"], "doi_pub": ["10.1093/mnras/stw2623"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Aperture photometry parameters for galaxies in the ATLAS3D (J/MNRAS/413/813) and Rampazzo et al. (2013MNRAS.432..374R) samples", "columns": [{"name": "Name", "desc": "Galaxy name "}, {"name": "MType", "desc": "Morphological type "}, {"name": "Dist", "desc": "Distance "}, {"name": "Sample", "desc": "Originating Sample "}, {"name": "aW1", "desc": "WISE W1 aperture semimajor axis "}, {"name": "aW4", "desc": "WISE W4 aperture semimajor axis "}, {"name": "b/aW1", "desc": "WISE W1 axis ratio "}, {"name": "b/aW4", "desc": "WISE W4 axis ratio "}, {"name": "PA", "desc": "[] Position Angle "}, {"name": "WISEDR", "desc": "WISE data release catalog "}, {"name": "GALEXNUV", "desc": "GALEX NUV tilename "}, {"name": "GALEXFUV", "desc": "GALEX NUV tilename "}]}, {"name": "table2.dat", "desc": "Galaxy magnitudes for the ATLAS3D (J/MNRAS/413/813) and Rampazzo et al. (2013MNRAS.432..374R) samples", "columns": [{"name": "Name", "desc": "Galaxy Name "}, {"name": "l_FUV", "desc": "Limit flag on FUV "}, {"name": "FUV", "desc": "?=- FUV magnitude (1) "}, {"name": "e_FUV", "desc": "?=- rms uncertainty on FUV magnitude "}, {"name": "NUV", "desc": "?=- NUV magnitude (1) "}, {"name": "e_NUV", "desc": "?=- rms uncertainty on NUV magnitude "}, {"name": "W1mag", "desc": "?=- W1 magnitude (1) "}, {"name": "e_W1mag", "desc": "?=- rms uncertainty on W1 magnitude "}, {"name": "W2mag", "desc": "?=- W2 magnitude (1) "}, {"name": "e_W2mag", "desc": "?=- rms uncertainty on W2 magnitude "}, {"name": "W3mag", "desc": "?=- W3 magnitude (1) "}, {"name": "e_W3mag", "desc": "?=- rms uncertainty on W3 magnitude "}, {"name": "l_W4mag", "desc": "Limit flag on W4mag "}, {"name": "W4mag", "desc": "?=- W4 magnitude (1) "}, {"name": "e_W4mag", "desc": "?=- rms uncertainty on W4 magnitude "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_464_4176"}} {"id": "J/MNRAS/464/4176", "title_cds": "Short Title", "title_create": "Willett+, 2017", "year": "2017", "author": "Willett K.W., Galloway M.A., Bamford S.P., Lintott C.J., Masters K.L., Scarlata C., Simmons B.D., Beck M., Cardamone C.N., Cheung E., Edmondson E.M., Fortson L.F., Griffith R.L., Haussler B., Han A., Hart R., Melvin T., Parrish M., Schawinski K., Smethurst R.J., Smith A.M.", "title_pub": "Galaxy Zoo: morphological classifications for 120 000 galaxies in HST legacy imaging.", "first_author": "Willett K.W.", "ref_biblio": [""], "bibcode": ["2017MNRAS.464.4176W"], "keyword_cds": "", "keyword_pub": "methods: data analysis - catalogues - galaxies: evolution - galaxies: high-redshift - galaxies: structure", "abstract": ["We present the data release paper for the Galaxy Zoo: Hubble (GZH)", "project. This is the third phase in a large effort to measure", "reliable, detailed morphologies of galaxies by using crowdsourced", "visual classifications of colour-composite images. Images in GZH were", "selected from various publicly released Hubble Space Telescope legacy", "programmes conducted with the Advanced Camera for Surveys, with", "filters that probe the rest-frame optical emission from galaxies out", "to z~1. The bulk of the sample is selected to have m_I814W_<23.5,", "but goes as faint as m_I814W_<26.8 for deep images combined over five", "epochs. The median redshift of the combined samples is =0.9+/-0.6,", "with a tail extending out to z~=4. The GZH morphological data include", "measurements of both bulge- and disc-dominated galaxies, details on", "spiral disc structure that relate to the Hubble type, bar", "identification, and numerous measurements of clump identification and", "geometry. This paper also describes a new method for calibrating", "morphologies for galaxies of different luminosities and at different", "redshifts by using artificially redshifted galaxy images as a", "baseline. The GZH catalogue contains both raw and calibrated", "morphological vote fractions for 119\u2009849 galaxies, providing the", "largest data set to date suitable for large-scale studies of galaxy", "evolution out to z~1."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw2568"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_465_1181"}} {"id": "J/MNRAS/465/1181", "title_cds": "Short Title", "title_create": "Liakos+, 2017", "year": "2017", "author": "Liakos A., Niarchos P.", "title_pub": "Catalogue and properties of {delta} Scuti stars in binaries.", "first_author": "Liakos A.", "ref_biblio": [""], "bibcode": ["2017MNRAS.465.1181L"], "keyword_cds": "", "keyword_pub": "binaries: close - binaries: eclipsing - stars: fundamental parameters - stars: variables: delta Scuti", "abstract": ["The catalogue contains 199 confirmed cases of binary systems", "containing at least one pulsating component of delta Sct type. The", "sample is divided into subgroups in order to describe the properties", "and characteristics of the delta Sct-type stars in binaries according", "to their Roche geometry. Demographics describing quantitatively our", "knowledge for these systems as well as the distributions of their", "pulsating components in the mass\u2013radius, colour\u2013magnitude, and", "evolutionary status\u2013temperature diagrams are presented and", "discussed. It is shown that a threshold of ~13d of the orbital", "period regarding the influence of binarity on the pulsations is", "established. Finally, the correlations between the pulsation periods", "and the orbital periods, evolutionary status, and companion's gravity", "influence are updated based on the largest sample to date."], "description": ["The catalogue consists of five lists given in Tables 1-5 of this", "paper. It contains all of the currently known binaries with a delta", "Sct component, ambiguous ones, and others that were incorrectly", "reported as being of this type. This catalogue is online", "(https://alexiosliakos.weebly.com/catalogue.html) and is frequently", "updated."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stw2756"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_467_412"}} {"id": "J/MNRAS/467/412", "title_cds": "Simulated globular clusters with Gaia", "title_create": "Pancino+, 2017", "year": "2017", "author": "Pancino E., Bellazzini M., Giuffrida G., Marinoni S.", "title_pub": "Globular clusters with Gaia.", "first_author": "Pancino E.", "ref_biblio": [""], "bibcode": ["2017MNRAS.467..412P"], "see_also": ["I/337 : Gaia DR1 (Gaia Collaboration, 2016)"], "keyword_cds": "Models ; Globular clusters", "keyword_pub": "astrometry - parallaxes - globular clusters: general", "abstract": ["The treatment of crowded fields in Gaia data will only be a reality in", "a few years from now. In particular, for globular clusters, only the", "end-of-mission data (public in 2022-2023) will have the necessary full", "crowding treatment and will reach sufficient quality for the faintest", "stars. As a consequence, the work on the deblending and", "decontamination pipelines is still ongoing. We describe the present", "status of the pipelines for different Gaia instruments, and we model", "the end-of-mission crowding errors on the basis of available", "information. We then apply the nominal post-launch Gaia performances,", "appropriately worsened by the estimated crowding errors, to a set of", "18 simulated globular clusters with different concentration, distance", "and field contamination. We conclude that there will be 10^3^-10^4^", "stars with astrometric performances virtually untouched by crowding", "(contaminated by <1mmag) in the majority of clusters. The most", "limiting factor will be field crowding, not cluster crowding: the most", "contaminated clusters will only contain 10-100 clean stars. We also", "conclude that (i) the systemic proper motions and parallaxes will be", "determined to 1 per cent or better up to ~=15kpc, and the", "nearby clusters will have radial velocities to a few km/s; (ii)", "internal kinematics will be of unprecedented quality, cluster masses", "will be determined to ~=10 per cent up to 15kpc and beyond, and", "it will be possible to identify differences of a few km/s or less", "in the kinematics (if any) of cluster sub-populations up to 10kpc and", "beyond; (iii) the brightest stars (V~=17mag) will have", "space-quality, wide-field photometry (mmag errors), and all Gaia", "photometry will have 1-3 per cent errors on the absolute photometric", "calibration."], "description": ["We used all the available information on the presently available Gaia", "deblending pipelines, along with their results on simulated data, to", "model the behaviour of Gaia in crowded areas. We computed additional", "crowding errors that were combined with the post-launch science", "performances of Gaia and applied to a set of simulated GCs with", "different concentration (c=1.0 and 2.5), distance (5, 10 and 15kpc),", "and field population (halo, disc and bulge)."], "doi_pub": ["10.1093/mnras/stx079"], "orcid_pub": ["0000-0003-0788-5879"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table2.dat", "desc": "Simulated cluster properties and crowding evaluation results", "columns": [{"name": "Cluster", "desc": "[1/18] Cluster number "}, {"name": "c", "desc": "GC concentration parameter, c=log(rt/rc) "}, {"name": "Dist", "desc": "GC projected distance "}, {"name": "Bckg", "desc": "Type of simulated background "}, {"name": "ntot", "desc": "Total number of simulated stars (GC and background) above Gaia detection limit"}, {"name": "nGC", "desc": "Number of GC members "}, {"name": "nclassic", "desc": "Number of classic blends "}, {"name": "nblends", "desc": "Number of Gaia blends "}, {"name": "ncontam", "desc": "Number of contaminated stars "}, {"name": "nclean", "desc": "Number of clean stars (1) "}, {"name": "Des", "desc": "Quick GC designation used in the paper "}, {"name": "Examp", "desc": "Some examples of GCs with similar distance, concentration and background field"}]}, {"name": "catalog.dat", "desc": "Final simulated stars (partial !!!!!) ", "columns": [{"name": "Cluster", "desc": "[1/16] Cluster number "}, {"name": "Star", "desc": "Star ID "}, {"name": "RAdeg", "desc": "Position along the RA direction (1) "}, {"name": "DEdeg", "desc": "Position along the Dec direction (1) "}, {"name": "e_pos", "desc": "Error on RA and DE "}, {"name": "pmRA", "desc": "Proper motion along RA "}, {"name": "pmDE", "desc": "Proper motion along DE "}, {"name": "e_pm", "desc": "Error on proper motion "}, {"name": "plx", "desc": "Parallax "}, {"name": "e_plx", "desc": "Parallax error "}, {"name": "Gmag", "desc": "G-band integrated magnitude "}, {"name": "e_Gmag", "desc": "G magnitude error "}, {"name": "GBPmag", "desc": "GBP integrated magnitude "}, {"name": "e_GBPmag", "desc": "GBP magnitude error "}, {"name": "GRPmag", "desc": "GRP integrated magnitude "}, {"name": "e_GRPmag", "desc": "GRP magnitude error "}, {"name": "Memb", "desc": "[0/1] True membership (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_467_3361"}} {"id": "J/MNRAS/467/3361", "title_cds": "", "title_create": "Wiegand+, 2017", "year": "2017", "author": "Wiegand A., Eisenstein D.J.", "title_pub": "The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: higher order correlations revealed by germ-grain Minkowski functionals.", "first_author": "Wiegand A.", "ref_biblio": [""], "bibcode": ["2017MNRAS.467.3361W"], "keyword_cds": "", "keyword_pub": "methods: data analysis - methods: statistical - cosmology: observations - large-scale structure of Universe", "abstract": ["We probe the higher order clustering of the galaxies in the final data", "release (DR12) of the Sloan Digital Sky Survey Baryon Oscillation", "Spectroscopic Survey (BOSS), using the method of germ-grain Minkowski", "functionals (MFs). Our sample consists of 410615 BOSS galaxies from", "the northern Galactic cap in the redshift range 0.450-0.595. We show", "the MFs to be sensitive to contributions up to the six-point", "correlation function for this data set. We ensure with a custom", "angular mask that the results are more independent of boundary effects", "than in previous analyses of this type. We extract the higher order", "part of the MFs and quantify the difference to the case without higher", "order correlations. The resulting {chi}^2^ value of over 10000 for a", "modest number of degrees of freedom, O(200), indicates a 100{sigma}", "deviation and demonstrates that we have a highly significant signal of", "the non-Gaussian contributions to the galaxy distribution. This", "statistical power can be useful in testing models with differing", "higher order correlations. Comparing the galaxy data to the quick", "particle mesh and MultiDark(MD)-Patchy mocks, we find that the latter", "better describes the observed structure. From an order-by-order", "decomposition, we expect that, for example, already a reduction of the", "amplitude of the MD-Patchy mock power spectrum by 5 per cent would", "remove the remaining tension."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stx292"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_469_1065"}} {"id": "J/MNRAS/469/1065", "title_cds": "SPIDERS catalogs", "title_create": "Dwelly+, 2017", "year": "2017", "author": "Dwelly T., Salvato M., Merloni A., Brusa M., Buchner J., Anderson S.F., Boller T., Brandt W.N., Budavari T., Clerc N., Coffey D., Del Moro A., Georgakakis A., Green P.J., Jin C., Menzel M.-L., Myers A.D., Nandra K., Nichol R.C., Ridl J., Schwope A.D., Simm T.", "title_pub": "SPIDERS: selection of spectroscopic targets using AGN candidates detected in all-sky X-ray surveys.", "first_author": "Dwelly T.", "ref_biblio": [""], "bibcode": ["2017MNRAS.469.1065D"], "keyword_cds": "", "keyword_pub": "surveys - galaxies: active - quasars: general - galaxies: Seyfert - cosmology: observations - X-rays: galaxies", "abstract": ["SPIDERS (SPectroscopic IDentification of eROSITA Sources) is a Sloan", "Digital Sky Survey IV (SDSS-IV) survey running in parallel to the", "Extended Baryon Oscillation Spectroscopic Survey (eBOSS) cosmology", "project. SPIDERS will obtain optical spectroscopy for large numbers of", "X-ray-selected active galactic nuclei (AGN) and galaxy cluster members", "detected in wide-area eROSITA, XMM-Newton and ROSAT surveys. We", "describe the methods used to choose spectroscopic targets for two", "sub-programmes of SPIDERS X-ray selected AGN candidates detected in", "the ROSAT All Sky and the XMM-Newton Slew surveys. We have exploited a", "Bayesian cross-matching algorithm, guided by priors based on mid-IR", "colour-magnitude information from the Wide-field Infrared Survey", "Explorer survey, to select the most probable optical counterpart to", "each X-ray detection. We empirically demonstrate the high fidelity of", "our counterpart selection method using a reference sample of bright", "well-localized X-ray sources collated from XMM-Newton, Chandra and", "Swift-XRT serendipitous catalogues, and also by examining blank-sky", "locations. We describe the down-selection steps which resulted in the", "final set of SPIDERS-AGN targets put forward for spectroscopy within", "the eBOSS/TDSS/SPIDERS survey, and present catalogues of these", "targets. We also present catalogues of ~12000 ROSAT and ~1500", "XMM-Newton Slew survey sources that have existing optical spectroscopy", "from SDSS-DR12, including the results of our visual inspections. On", "completion of the SPIDERS programme, we expect to have collected", "homogeneous spectroscopic redshift information over a footprint of", "~7500 deg^2^ for >85 per cent of the ROSAT and XMM-Newton Slew survey", "sources having optical counterparts in the magnitude range 17"], "bibcode": ["2017MNRAS.469..800M"], "keyword_cds": "", "keyword_pub": "Hertzsprung-Russell and colour-magnitude diagrams stars: low-mass: Population II; globular clusters: general globular clusters: individual: \\object{\u03c9 Centauri, M4, NGC2808}{}", "mission": "", "abstract": ["As part of a large investigation with Hubble Space Telescope to study the faintest stars within the globular cluster {omega} Centauri, in this work we present early results on the multiplicity of its main sequence (MS) stars, based on deep optical and near-infrared observations. By using appropriate colour-magnitude diagrams, we have identified, for the first time, the two main stellar Populations I and II along the entire MS, from the turn-off towards the hydrogen-burning limit. We have compared the observations with suitable synthetic spectra of MS stars and conclude that the two main sequences (MSs) are consistent with stellar populations with different metallicity, helium and light-element abundance. Specifically, MS-I corresponds to a metal-poor stellar population ([Fe/H]~ -1.7) with Y~ 0.25 and [O/Fe]~ 0.30. The MS-II hosts helium-rich (Y~ 0.37-0.40) stars with metallicity ranging from [Fe/H]~ -1.7 to -1.4. Below the MS knee (m_F160W_ ~ 19.5), our photometry reveals that each of the two main MSs hosts stellar subpopulations with different oxygen abundances, with very O-poor stars ([O/Fe] ~ -0.5) populating the MS-II. Such a complexity has never been observed in previous studies of M-dwarfs in globular clusters. A few months before the launch of the James Webb Space Telescope, these results demonstrate the power of optical and near-infrared photometry in the study of multiple stellar populations in globular clusters."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "30-Mar-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_471_404"}} {"id": "J/MNRAS/471/404", "title_cds": "Short Title", "title_create": "Kielty+, 2017", "year": "2017", "author": "Kielty C.L., Venn K.A., Loewen N.B., Shetrone M.D., Placco V.M., Jahandar F., Meszaros S., Martell S.L.", "title_pub": "Carbon-enhanced metal-poor stars in the SDSS-APOGEE data base.", "first_author": "Kielty C.L.", "ref_biblio": [""], "bibcode": ["2017MNRAS.471..404K"], "keyword_cds": "", "keyword_pub": "surveys; stars: abundances; stars: carbon; stars: chemically peculiar Galaxy: halo; infrared: stars", "mission": "", "abstract": ["We identify six new carbon-enhanced metal-poor (CEMP) stars ([C/Fe]>+0.7 and [Fe/H] < -1.8) and another seven likely candidates within the APOGEE data base following Data Release 12. These stars have chemical compositions typical of metal-poor halo stars, e.g. mean [{alpha}/Fe] = +0.24 {\\pm} 0.24, based on the APOGEE Stellar Parameters and Chemical Abundances Pipeline results. A lack of heavy-element spectral lines impedes further sub-classification of these CEMP stars, however, based on radial velocity (RV) scatter, we predict most are not CEMP-s stars which are typically found in binary systems. Only one object, 2M15312547+4220551, may be in a binary since it exhibits a scatter in its RV of 1.7 {\\pm} 0.6 km s^-1^ based on three visits over a 25.98 d baseline. Optical observations are now necessary to confirm the stellar parameters and low metallicities of these stars, to determine the heavy-element abundance ratios and improve the precision in the derived abundances, and to examine their CEMP sub-classifications."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "15-May-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_471_3494"}} {"id": "J/MNRAS/471/3494", "title_cds": "Short Title", "title_create": "Zhu+, 2017", "year": "2017", "author": "Zhu H., Tian W., Li A., Zhang M.", "title_pub": "The gas-to-extinction ratio and the gas distribution in the Galaxy.", "first_author": "Zhu H.", "ref_biblio": [""], "bibcode": ["2017MNRAS.471.3494Z"], "keyword_cds": "", "keyword_pub": "galaxies: active - galaxies: individual: NGC 6240 - galaxies: starburst; X-rays: galaxies", "abstract": ["We investigate the relation between the optical extinction (A_V_) and", "the hydrogen column density (N_H_) determined from X-ray observations", "of a large sample of Galactic sightlines towards 35 supernova", "remnants, 6 planetary nebulae and 70 X-ray binaries for which N_H_ was", "determined in the literature with solar abundances. We derive an", "average ratio of =(2.08+/-0.02)x10^21^Hcm^-2^mag^-1^ for", "the whole Galaxy. We find no correlation between and the", "number density of hydrogen, the distance away from the Galactic Centre", "and the distance above or below the Galactic plane. The ", "ratio is generally invariant across the Galaxy, with", "=(2.04+/-0.05)x10^21^Hcm^-2^mag^-1^ for the first and", "fourth Galactic quadrants and", "=(2.09+/-0.03)x10^21^Hcm^-2^mag^-1^ for the second and", "third Galactic quadrants. We also explore the distribution of hydrogen", "in the Galaxy by enlarging our sample with additional 74 supernova", "remnants for which both N_H_ and distances are known. We find that,", "between the Galactic radius of 2 and 10 kpc, the vertical distribution", "of hydrogen can be roughly described by a Gaussian function with a", "scaleheight of h=75.5+/-12.4pc and a mid-plane density of", "n_H_(0)=1.11+/-0.15cm^-3^, corresponding to a total gas surface", "density of {sum}_gas_~7.0 M_{sun}_/pc^2^. We also compile N_H_ from 19", "supernova remnants and 29 X-ray binaries for which N_H_ was determined", "with subsolar abundances. We obtain", "=(2.47+/-0.04)x10^21^Hcm^-2^mag^-1^ which exceeds that", "derived with solar abundances by ~20 per cent. We suggest that in", "future studies one may simply scale N_H_ derived from subsolar", "abundances"], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "28-May-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_471_4087"}} {"id": "J/MNRAS/471/4087", "title_cds": "Gaia 1 HERMES and AAOmega spectroscopy", "title_create": "Simpson+, 2017", "year": "2017", "author": "Simpson J.D., De Silva G.M., Martell S.L., Zucker D.B., Ferguson A.M.N., Bernard E.J., Irwin M., Penarrubia J., Tolstoy E.", "title_pub": "Siriusly, a newly identified intermediate-age Milky Way stellar cluster: a spectroscopic study of Gaia 1.", "first_author": "Simpson J.D.", "ref_biblio": [""], "bibcode": ["2017MNRAS.471.4087S"], "see_also": ["I/345 : Gaia DR2 (Gaia Collaboration, 2018)", "II/349 : The Pan-STARRS release 1 (PS1) Survey - DR1 (Chambers+, 2016)"], "keyword_cds": "Milky Way ; Associations, stellar ; Radial velocities", "keyword_pub": "catalogues - Galaxy: general - Galaxy: structure", "abstract": ["We confirm the reality of the recently discovered Milky Way stellar", "cluster Gaia 1 using spectra acquired with the HERMES and AAOmega", "spectrographs of the Anglo-Australian Telescope. This cluster had been", "previously undiscovered due to its close angular proximity to Sirius,", "the brightest star in the sky at visual wavelengths. Our observations", "identified 41 cluster members, and yielded an overall metallicity of", "[Fe/H]=-0.13+/-0.13 and barycentric radial velocity of", "v_r_=58.30+/-0.22km/s. These kinematics provide a dynamical mass", "estimate of 12.9^+4.6^_-3.9_x10^3^M_{sun}_. Isochrone fits to Gaia,", "2MASS, and Pan-STARRS1 photometry indicate that Gaia 1 is an", "intermediate age (~3Gyr) stellar cluster. Combining the spatial", "and kinematic data we calculate Gaia 1 has a circular orbit with a", "radius of about 12kpc, but with a large out of plane motion:", "z_max_=1.1^+0.4^_-0.3_kpc."], "description": ["Gaia 1 was observed with two of the spectrographs of the 3.9-m", "Anglo-Australian Telescope over three nights: on the night of 2017", "February 15 with the four-armed high-resolution HERMES spectrograph,", "and on the nights of 2017 February 24 and 26 with the two-armed", "AAOmega spectrograph."], "object": ["06 45 53 -16 45 00 Gaia 1 = [KBT2017] Gaia 1"], "type": ["OC"], "data": "", "date_update": "10-Feb-2021", "tables": [{"name": "tablea1.dat", "desc": "The line list used for the HERMES stellar parameter determination", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "El", "desc": "Element "}, {"name": "EP", "desc": "Energy potential "}, {"name": "loggf", "desc": "Osccilator strength "}]}, {"name": "tableb1.dat", "desc": "Parameters for members of Gaia 1 observed with HERMES", "columns": [{"name": "GaiaDR1", "desc": "Gaia DR1 source_id "}, {"name": "PS1", "desc": "PS1 objID "}, {"name": "r", "desc": "Radius "}, {"name": "SNR1", "desc": "Signa-to-noise 1 (blue: 4715-4900{AA}) "}, {"name": "SNR2", "desc": "Signa-to-noise 2 (green: 5649-5873{AA}) "}, {"name": "SNR3", "desc": "Signa-to-noise 3 (red: 6478-6737{AA}) "}, {"name": "SNR4", "desc": "Signa-to-noise 4 (near-infrared: 7585-7887{AA}) "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "e_RV", "desc": "Radial velocity error "}, {"name": "Teff", "desc": "? Effective temperature "}, {"name": "loggsp", "desc": "? Spectroscopic gravity surface "}, {"name": "loggph", "desc": "? Photometric gravity surface "}, {"name": "[Fe/H]", "desc": "? Metallicity "}, {"name": "e_[Fe/H]", "desc": "? Metallicity error "}]}, {"name": "tableb2.dat", "desc": "Parameters for members of Gaia 1 observed with AAOmega", "columns": [{"name": "GaiaDR1", "desc": "Gaia DR1 source_id "}, {"name": "PS1", "desc": "PS1 objID "}, {"name": "r", "desc": "Radius "}, {"name": "SNR", "desc": "Signal-to-noise ratio "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "e_RV", "desc": "Radial velocity error "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "e_[Fe/H]", "desc": "Metallicity error "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_472_4051"}} {"id": "J/MNRAS/472/4051", "title_cds": "Short Title", "title_create": "Calderone+, 2017", "year": "2017", "author": "Calderone G., Nicastro L., Ghisellini G., Dotti M., Sbarrato T., Shankar F., Colpi M.", "title_pub": "QSFIT: automatic analysis of optical AGN spectra.", "first_author": "Calderone G.", "ref_biblio": [""], "bibcode": ["2017MNRAS.472.4051C"], "keyword_cds": "", "keyword_pub": "methods: data analysis - catalogues; galaxies: active quasars: emission lines", "mission": "", "abstract": ["We present QSFIT (Quasar Spectral Fitting package), a new software package to automatically perform the analysis of active galactic nuclei (AGNs) optical spectra. The software provides luminosity estimates for the AGN continuum, the Balmer continuum, both optical and ultraviolet iron blended complex, host galaxy and emission lines, as well as width, velocity offset and equivalent width of 20 emission lines. Improving on a number of previous studies on AGN spectral analysis, QSFIT fits all the components simultaneously, using an AGN continuum model which extends over the entire available spectrum, and is thus a probe of the actual AGN continuum whose estimates are scarcely influenced by localized features (e.g. emission lines) in the spectrum. We used QSFIT to analyse 71 251 optical spectra of Type 1 AGN at z < 2 (obtained by the Sloan Digital Sky Survey, SDSS) and to produce a publicly available catalogue of AGN spectral properties. Such catalogueallowed us (for the first time) to estimate the AGN continuum slope and the Balmer continuum luminosity on a very large sample, and to show that there is no evident correlation between these quantities the redshift. All data in the catalogue, the plots with best-fitting model and residuals, and the IDL code we used to perform the analysis, are available on a dedicated website. The whole fitting process is customizable for specific needs, and can be extended to analysespectra from other data sources. The ultimate purpose of QSFIT is to allow astronomers to run standardized recipes to analyse the AGN data, in a simple, replicable and shareable way."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "26-Jun-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_473_2020"}} {"id": "J/MNRAS/473/2020", "title_cds": "Short Title", "title_create": "Lodieu+, 2018", "year": "2018", "author": "Lodieu N., Zapatero Osorio M.R., Bejar V.J.S., Pena Ramirez K.", "title_pub": "The optical + infrared l dwarf spectral sequence of young planetary-mass objects in the upper scorpius association.", "first_author": "Lodieu N.", "ref_biblio": [""], "bibcode": ["2018MNRAS.473.2020L"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "21-Nov-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_473_2853"}} {"id": "J/MNRAS/473/2853", "title_cds": "Short Title", "title_create": "Rosslowe+, 2018", "year": "2018", "author": "Rosslowe C.K., Crowther P.A.", "title_pub": "A deep near-infrared spectroscopic survey of the Scutum-Crux arm for Wolf-Rayet stars.", "first_author": "Rosslowe C.K.", "ref_biblio": [""], "bibcode": ["2018MNRAS.473.2853R"], "keyword_cds": "", "keyword_pub": "stars: emission-line, Be - stars: evolution - stars: Wolf\u2013Rayet \u2013 Galaxy: stellar content - infrared: stars", "abstract": ["We present a New Technology Telescope/Son-of-Isaac spectroscopic", "survey of infrared selected Wolf\u2013Rayet (WR) candidates in the", "Scutum-Crux spiral arm (298{deg}<=l<=340{deg}, |b|<=0.5{deg}). We", "obtained near-IR spectra of 127 candidates, revealing 17 WR stars \u2013", "a ~13 per cent success rate \u2013 of which 16 are newly identified here.", "The majority of the new WR stars are classified as narrow-lined", "WN5\u20137 stars, with two broad-lined WN4\u20136 stars and three WC6\u20138", "stars. The new stars, with distances estimated from previous absolute", "magnitude calibrations, have no obvious association with the", "Scutum-Crux arm. Refined near-infrared (YHJK) classification criteria", "based on over a hundred Galactic and Magellanic Cloud WR stars,", "providing diagnostics for hydrogen in WN stars, plus the", "identification of WO stars and intermediate WN/C stars. Finally, we", "find that only a quarter of WR stars in the survey region are", "associated with star clusters and/or HII regions, with similar", "statistics found for luminous blue variables (LBVs) in the Milky Way.", "The relative isolation of evolved massive stars is discussed, together", "with the significance of the co-location of LBVs and WR stars in young", "star clusters."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "21-Nov-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_473_5393"}} {"id": "J/MNRAS/473/5393", "title_cds": "Wide binaries in Tycho-Gaia", "title_create": "Andrews+, 2018", "year": "2018", "author": "Andrews J.J., Chaname J., Agueros M.A.", "title_pub": "Wide binaries in Tycho-Gaia. II: metallicities, abundances and prospects for chemical tagging.", "first_author": "Andrews J.J.", "ref_biblio": [""], "bibcode": ["2018MNRAS.473.5393A"], "see_also": ["I/337 : Gaia DR1 (Gaia Collaboration, 2016)", "III/279 : RAVE 5th data release (Kunder+, 2017)", "V/153 : LAMOST DR4 catalogs (Luo+, 2018)"], "keyword_cds": "Milky Way ; Stars, double and multiple ; Abundances ; Effective temperatures", "keyword_pub": "stars: abundances - binaries: visual - Galaxy: structure", "abstract": ["From our recent catalogue based on the first Gaia data release (TGAS),", "we select wide binaries in which both stars have been observed by the", "Radial Velocity Experiment (RAVE) or the Large Sky Area Multi-Object", "Fiber Spectroscopic Telescope (LAMOST). Using RAVE and LAMOST", "metallicities and RAVE Mg, Al, Si, Ti and Fe abundances, we find that", "the differences in the metallicities and elemental abundances of", "components of wide binaries are consistent with being due to", "observational uncertainties, in agreement with previous results for", "smaller and more restricted samples. The metallicity and elemental", "abundance consistency between wide binary components presented in this", "work confirms their common origin and bolsters the status of wide", "binaries as 'mini-open clusters'. Furthermore, this is evident that", "wide binaries are effectively co-eval and co-chemical, supporting", "their use for, e.g. constraining age-activity-rotation relations,", "the initial-final mass relation for white dwarfs and M-dwarf", "metallicity indicators. Additionally, we demonstrate that the common", "proper motion, common parallax pairs in TGAS with the most extreme", "separations (s>~0.1pc) typically have inconsistent metallicities,", "radial velocities or both and are therefore likely to be predominantly", "comprised of random alignments of unassociated stars with similar", "astrometry, in agreement with our previous results. Finally, we", "propose that wide binaries form an ideal data set with which we can", "test chemical tagging as a method to identify stars of common origin,", "particularly because the stars in wide binaries span a wide range of", "metallicities, much wider than that spanned by nearby open clusters."], "description": ["From our catalogue of 7108 wide binaries identified in TGAS in Paper I", "(Andrews et al., 2017MNRAS.472..675A, Cat. J/MNRAS/472/675, we select", "the subset of pairs in which the posterior probability is above", "99 per cent when using a power-law prior on the distribution of", "orbital separations (for details, see Paper I).", "We first cross-match these pairs with the RAVE DR5 catalogue (Kunder", "et al., 2017AJ....153...75K, Cat. III/279) and obtain 115 wide", "binaries in which both components are detected by RAVE (table1).", "We also cross-match with the LAMOST DR3 catalogue to identify", "additional 85 wide binaries with measured RVs, although only 62 of", "these have measured metallicities with uncertainties less than 0.2dex", "(table 2)."], "type": ["OC"], "doi_pub": ["10.1093/mnras/stx2685"], "orcid_pub": ["0000-0001-5261-3923"], "data": "", "date_creation": "10-Feb-2021", "date_update": "09-Mar-2021", "tables": [{"name": "table1.dat", "desc": "Wide binaries in which RAVE has observed both stars in the pair and data pass the quality cuts", "columns": [{"name": "SourceID1", "desc": "Primary Gaia DR1 designation "}, {"name": "RV1", "desc": "Primary radial velocity "}, {"name": "e_RV1", "desc": "Primary radial velocity error "}, {"name": "[M/H]1", "desc": "Primary metallicity "}, {"name": "e_[M/H]1", "desc": "Primary metallicity error "}, {"name": "Teff1", "desc": "Primary effective temperature "}, {"name": "logg1", "desc": "Primary surface gravity "}, {"name": "SourceID2", "desc": "Secondary Gaia DR1 designation "}, {"name": "RV2", "desc": "Secondary radial velocity "}, {"name": "e_RV2", "desc": "Secondary radial velocity error "}, {"name": "[M/H]2", "desc": "Secondary metallicity "}, {"name": "e_[M/H]2", "desc": "Secondary metallicity error "}, {"name": "Teff2", "desc": "Secondary effective temperature "}, {"name": "logg2", "desc": "Secondary surface gravity "}]}, {"name": "table2.dat", "desc": "Wide binaries in which LAMOST has observed both stars in the pair and data pass the quality cuts", "columns": [{"name": "SourceID1", "desc": "Primary Gaia DR1 designation "}, {"name": "RV1", "desc": "Primary radial velocity "}, {"name": "e_RV1", "desc": "Primary radial velocity error "}, {"name": "[Fe/H]1", "desc": "Primary metallicity "}, {"name": "l_e_[Fe/H]1", "desc": "Limit flag on e_[Fe/H]1 "}, {"name": "e_[Fe/H]1", "desc": "Primary metallicity error "}, {"name": "Teff1", "desc": "Primary effective temperature "}, {"name": "logg1", "desc": "Primary surface gravity "}, {"name": "SourceID2", "desc": "Secondary Gaia DR1 designation "}, {"name": "RV2", "desc": "Secondary radial velocity "}, {"name": "e_RV2", "desc": "Secondary radial velocity error "}, {"name": "[Fe/H]2", "desc": "Secondary metallicity "}, {"name": "e_[Fe/H]2", "desc": "Secondary metallicity error "}, {"name": "Teff2", "desc": "Secondary effective temperature "}, {"name": "logg2", "desc": "Secondary surface gravity "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_474_3875"}} {"id": "J/MNRAS/474/3875", "title_cds": "Galaxy And Mass Assembly (GAMA): DR3", "title_create": "Baldry+, 2018", "year": "2018", "author": "Baldry I.K., Liske J., Brown M.J.I., Robotham A.S.G., Driver S.P., Dunne L., Alpaslan M., Brough S., Cluver M.E., Eardley E., Farrow D.J., Heymans C., Hildebrandt H., Hopkins A.M., Kelvin L.S., Loveday J., Moffett A.J., Norberg P., Owers M.S., Taylor E.N., Wright A.H., Bamford S.P., Bland-hawthorn J., Bourne N., Bremer M.N., Colless M., Conselice C.J., Croom S.M., Davies L.J.M., Foster C., Grootes M.W., Holwerda B.W., Jones D.H., Kafle P.R., Kuijken K., Lara-lopez M.A., Lopez-sanchez A.R., Meyer M.J., Phillipps S., Sutherland W.J., Van Kampen E., Wilkins S.M.", "title_pub": "Galaxy And Mass Assembly: the G02 field, Herschel-ATLAS target selection and data release 3.", "first_author": "Baldry I.K.", "ref_biblio": [""], "bibcode": ["2018MNRAS.474.3875B"], "keyword_cds": "Surveys ; Galaxy catalogs ; Redshifts ; Photometry, SDSS ; Photometry, infrared", "keyword_pub": "catalogues - surveys - galaxies: distances and redshifts - galaxies: photometry", "abstract": ["We describe data release 3 (DR3) of the Galaxy And Mass Assembly", "(GAMA) survey. The GAMA survey is a spectroscopic redshift and", "multiwavelength photometric survey in three equatorial regions each of", "60.0deg^2^ (G09, G12, and G15), and two southern regions of", "55.7deg^2^ (G02) and 50.6deg^2^ (G23). DR3 consists of: the first", "release of data covering the G02 region and of data on H-ATLAS", "(Herschel \u2013 Astrophysical Terahertz Large Area Survey) sources in", "the equatorial regions; and updates to data on sources released in", "DR2. DR3 includes 154\u2009809 sources with secure redshifts across four", "regions. A subset of the G02 region is 95.5\u2009per\u2009cent redshift", "complete to r<19.8mag over an area of 19.5deg^2^, with 20086", "galaxy redshifts, that overlaps substantially with the XXL survey", "(X-ray) and VIPERS (redshift survey). In the equatorial regions, the", "main survey has even higher completeness (98.5\u2009per\u2009cent), and", "spectra for about 75\u2009per\u2009cent of H-ATLAS filler targets were also", "obtained. This filler sample extends spectroscopic redshifts, for", "probable optical counterparts to H-ATLAS submillimetre sources, to", "0.8mag deeper (r<20.6mag) than the GAMA main survey. There are", "25\u2009814 galaxy redshifts for H-ATLAS sources from the GAMA main or", "filler surveys. GAMA DR3 is available at the survey website", "(www.gama-survey.org/dr3/)."], "description": ["The third GAMA data release (DR3) provides AAT/AAOmega spectra,", "redshifts, and a wealth of ancillary information for primarily 215260", "objects from the GAMA II survey (Table 1). Of these, 178856 are", "main-survey objects and 36404 are fillers. In turn, 150465", "(84\u2009per\u2009cent) and 4344 (12\u2009per\u2009cent) of these, respectively,", "have secure redshifts. DR3 updates all data previously released in", "DR2, and significantly expands on DR2: DR3 includes both more objects", "and a wider range of data products than DR2. DR3 thus supersedes DR2", "in every way. The DR is available at: http://www.gama-survey.org/dr3/."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stx3042"], "orcid_pub": ["0000-0003-0719-9385"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_474_3344"}} {"id": "J/MNRAS/474/3344", "title_cds": "Short Title", "title_create": "Britavskiy+, 2018", "year": "2018", "author": "Britavskiy N., Pancino E., Tsymbal V., Romano D., Fossati L.", "title_pub": "A new method of measuring centre-of-mass velocities of radially pulsating stars from high-resolution spectroscopy.", "first_author": "Britavskiy N.", "ref_biblio": [""], "bibcode": ["2018MNRAS.474.3344B"], "keyword_cds": "", "keyword_pub": "methods: data analysis - techniques: radial velocities - stars: oscillations - stars: variables: Cepheids - stars: variables: RR Lyrae", "abstract": ["We present a radial velocity analysis of 20 solar neighbourhood RR", "Lyrae and three Population II Cepheid variables. We obtained", "high-resolution, moderate-to-high signal-to-noise ratio spectra for", "most stars; these spectra covered different pulsation phases for each", "star. To estimate the gamma (centre-of-mass) velocities of the", "programme stars, we use two independent methods. The first,", "\u2018classic\u2019 method is based on RR Lyrae radial velocity curve", "templates. The second method is based on the analysis of", "absorption-line profile asymmetry to determine both pulsational and", "gamma velocities. This second method is based on the least-squares", "deconvolution (LSD) technique applied to analyse the line asymmetry", "that occurs in the spectra. We obtain measurements of the pulsation", "component of the radial velocity with an accuracy of +/-3.5km/s.", "The gamma velocity was determined with an accuracy of +/-10km/s,", "even for those stars having a small number of spectra. The main", "advantage of this method is the possibility of obtaining an estimation", "of gamma velocity even from one spectroscopic observation with", "uncertain pulsation phase. A detailed investigation of LSD profile", "asymmetry shows that the projection factor p varies as a function of", "the pulsation phase - this is a key parameter, which converts", "observed spectral line radial velocity variations into photospheric", "pulsation velocities. As a by-product of our study, we present 41", "densely spaced synthetic grids of LSD profile bisectors based on", "atmospheric models of RR Lyr covering all pulsation phases."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "26-Feb-2021"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_4504"}} {"id": "J/MNRAS/475/4504", "title_cds": "Short Title", "title_create": "Barker+, 2018", "year": "2018", "author": "Barker H., Zijlstra A., De Marco O., Frew D.J., Drew J.E., Corradi R.L.M., Eisloffel J., Parker Q.A.", "title_pub": "The binary fraction of planetary nebula central stars. III. The promise of VPHAS+.", "first_author": "Barker H.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.4504B"], "keyword_cds": "", "keyword_pub": "planetary nebulae, central stars, photometry", "abstract": ["The majority of planetary nebulae (PNe) are not spherical, and current", "single-star models cannot adequately explain all the morphologies we", "observe. This has led to the Binary Hypothesis, which states that PNe", "are preferentially formed by binary systems. This hypothesis can be", "corroborated or disproved by comparing the estimated binary fraction", "of all PNe central stars (CS) to that of the supposed progenitor", "population. One way to quantify the rate of CS binarity is to detect", "near infrared excess indicative of a low-mass main-sequence companion.", "In this paper, a sample of known PNe within data release 2 of the", "ongoing VPHAS+ is investigated. We give details of the method used to", "calibrate VPHAS+ photometry, and present the expected colours of CS", "and main-sequence stars within the survey. Objects were scrutinized to", "remove PN mimics from our sample and identify true CS. Within our", "final sample of seven CS, six had previously either not been", "identified or confirmed. We detected an i-band excess indicative of a", "low-mass companion star in three CS, including one known binary,", "leading us to conclude that VPHAS+ provides the precise photometry", "required for the IR excess method presented here, and will likely", "improve as the survey completes and the calibration process finalized.", "Given the promising results from this trial sample, the entire VPHAS+", "catalogue should be used to study PNe and extend the IR excess-tested", "CS sample."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/mnras/stx3240"], "orcid_pub": ["0000-0002-2326-2885"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_716"}} {"id": "J/MNRAS/475/716", "title_cds": "Short Title", "title_create": "Green+, 2018", "year": "2018", "author": "Green A.W., Croom S.M., Scott N., Cortese L., Medling A.M., D'eugenio F., Bryant J.J., Bland-Hawthorn J., Allen J.T., Sharp R., Ho I.-T., Groves B., Drinkwater M.J., Mannering E., Harischandra L., Van De Sande J., Thomas A.D., O'Toole S., Mcdermid R.M., Vuong M., Sealey K., Bauer A.E., Brough S., Catinella B., Cecil G., Colless M., Couch W.J., Driver S.P., Federrath C., Foster C., Goodwin M., Hampton E.J., Hopkins A.M., Jones D.H., Konstantopoulos I.S., Lawrence J.S., Leon-Saval S.G., Liske J., Lopez-sanchez A.R., Lorente N.P.F., Mould J., Obreschkow D., Owers M.S., Richards S.N., Robotham A.S.G., Schaefer A.L., Sweet S.M., Taranu D.S., Tescari E., Tonini C., Zafar T.", "title_pub": "The SAMI Galaxy Survey: Data Release One with emission-line physics value-added products.", "first_author": "Green A.W.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475..716G"], "keyword_cds": "", "keyword_pub": "surveys - galaxies: general", "abstract": ["We present the first major release of data from the SAMI Galaxy", "Survey. This data release focuses on the emission-line physics of", "galaxies. Data Release One includes data for 772 galaxies, about 20", "per cent of the full survey. Galaxies included have the redshift range", "0.004"], "bibcode": ["2018MNRAS.475.1306G"], "keyword_cds": "", "keyword_pub": "galaxies: active - galaxies: statistics - radio continuum: galaxies", "abstract": ["We present high sensitivity ({sigma}_P_~=0.6mJy) polarimetric", "observations in seven bands, from 2.1 to 38GHz, of a complete sample", "of 104 compact extragalactic radio sources brighter than 200mJy at", "20GHz. Polarization measurements in six bands, in the range 5.5-38GHz,", "for 53 of these objects were reported by Galluzzi et al. We have added", "new measurements in the same six bands for another 51 sources and", "measurements at 2.1GHz for the full sample of 104 sources. Also, the", "previous measurements at 18, 24, 33, and 38GHz were re-calibrated", "using the updated model for the flux density absolute calibrator,", "PKS1934-638, not available for the earlier analysis. The observations,", "carried out with the Australia Telescope Compact Array, achieved a 90", "per cent detection rate (at 5{sigma}) in polarization. 89 of our", "sources have a counterpart in the 72-231MHz GLEAM (GaLactic and", "Extragalactic All-sky Murchison Widefield Array) survey, providing an", "unparalleled spectral coverage of 2.7 decades of frequency for these", "sources. While the total intensity data from 5.5 to 38GHz could be", "interpreted in terms of single component emission, a joint analysis of", "more extended total intensity spectra presented here, and of the", "polarization spectra, reveals that over 90 per cent of our sources", "show clear indications of at least two emission components. We", "interpret this as an evidence of recurrent activity. Our high", "sensitivity polarimetry has allowed a 5{sigma} detection of the weak", "circular polarization for ~38 per cent of the data set, and a deeper", "estimate of 20GHz polarization source counts than has been possible so", "far."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "01-Apr-2021"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_1633"}} {"id": "J/MNRAS/475/1633", "title_cds": "Photometric study of globular clusters", "title_create": "Meszaros+, 2018", "year": "2018", "author": "Meszaros S., Garcia-hernandez D.A., Cassisi S., Monelli M., Szigeti L., Dell'agli F., Derekas A., Masseron T., Shetrone M., Stetson P., Zamora O.", "title_pub": "A photometric study of globular clusters observed by the APOGEE survey.", "first_author": "Meszaros S.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.1633M"], "see_also": ["J/AJ/149/153 : Abundances of red giants in 10 globular clusters"], "keyword_cds": "Clusters, globular ; Photometry, UBVRI ; Abundances", "keyword_pub": "stars: abundances - stars: AGB and post-AGB - globular clusters: general", "abstract": ["In this paper, we describe the photometric and spectroscopic", "properties of multiple populations in seven northern globular", "clusters. In this study, we employ precise ground-based photometry", "from the private collection of Stetson, space photometry from the", "Hubble Space Telescope (HST), literature abundances of Na and O, and", "Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey", "abundances for Mg, Al, C, and N. Multiple populations are identified", "by their position in the C_U,B,I_-V pseudo colour-magnitude diagram", "(pseudo-CMD) and confirmed with their chemical composition determined", "using abundances. We confirm the expectation from previous studies", "that the red giant branches (RGBs) in all seven clusters are split and", "the different branches have different chemical compositions. The Mg-Al", "anticorrelations were well explored by the APOGEE and Gaia-ESO surveys", "for most globular clusters, some clusters showing bimodal", "distributions, while others continuous distributions. Even though the", "structure (i.e. bimodal versus continuous) of Mg-Al can greatly vary,", "the Al-rich and Al-poor populations do not seem to have very different", "photometric properties, agreeing with theoretical calculations. There", "is no one-to-one correspondence between the Mg-Al anticorrelation", "shape (bimodal versus continuous) and the structure of the RGB seen in", "the HST pseudo-CMDs, with the HSTphotometric information usually", "implying more complex formation/evolution histories than the", "spectroscopic ones. We report on finding two second-generation", "horizontal branch (HB) stars in M5, and five second-generation", "asymptotic giant branch (AGB) stars in M92, which is the most", "metal-poor cluster to date in which second-generation AGB stars have", "been observed."], "description": ["The ground-based U, B, V, R, I photometry was taken from the private", "collection of Peter Stetson and is precise to the level of", "<0.002mag in the U band and to <0.001mag for the other bands."], "type": ["OC"], "data": "", "date_update": "06-Apr-2021", "tables": [{"name": "table2.dat", "desc": "Ground-based photometry and atmospheric parameters and abundances from Meszaros et al., 2015, Cat. J/AJ/149/153", "columns": [{"name": "---", "desc": "[2M] "}, {"name": "2MASS", "desc": "2MASS ID, HHMMSSss+DDMMSSs "}, {"name": "Cluster", "desc": "Cluster ID "}, {"name": "PhotID", "desc": "Photometric ID "}, {"name": "Umag", "desc": "U magnitude "}, {"name": "Bmag", "desc": "B magnitude "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "Rmag", "desc": "?=99.99 R magnitude "}, {"name": "Imag", "desc": "I magnitude "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "[C/Fe]", "desc": "?=99.99 Abundance [C/Fe] "}, {"name": "[N/Fe]", "desc": "?=99.99 Abundance [N/Fe] "}, {"name": "[O/Fe]", "desc": "?=99.99 Abundance [O/Fe] "}, {"name": "[Mg/Fe]", "desc": "?=99.99 Abundance [Mg/Fe] "}, {"name": "[Al/Fe]", "desc": "?=99.99 Abundance [Al/Fe] "}, {"name": "[Si/Fe]", "desc": "?=99.99 Abundance [Si/Fe] "}, {"name": "[Ca/Fe]", "desc": "?=99.99 Abundance [Ca/Fe] "}, {"name": "[Ti/Fe]", "desc": "?=99.99 Abundance [Ti/Fe] "}]}, {"name": "table3.dat", "desc": "Photometric and abundances parameters collected from the literature", "columns": [{"name": "---", "desc": "[2M] "}, {"name": "2MASS", "desc": "2MASS ID, HHMMSSss+DDMMSSs "}, {"name": "Umag", "desc": "U magnitude "}, {"name": "Bmag", "desc": "B magnitude "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "Rmag", "desc": "?=99.99 R magnitude "}, {"name": "Imag", "desc": "I magnitude "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "[O/Fe]", "desc": "?=99.99 Abundance [O/Fe] "}, {"name": "[Na/Fe]", "desc": "?=99.99 Abundance [Na/Fe], NLTE corrected when it is available in the source"}, {"name": "Ref", "desc": "Literature source (1) "}]}, {"name": "table5.dat", "desc": "HST photometry and abundances from Meszaros et al., 2015, J/AJ/149/153", "columns": [{"name": "---", "desc": "[2M] "}, {"name": "2MASS", "desc": "2MASS ID, HHMMSSss+DDMMSSs "}, {"name": "Cluster", "desc": "Cluster ID "}, {"name": "F275W", "desc": "HST F275W magnitude "}, {"name": "F335W", "desc": "HST F335W magnitude "}, {"name": "F438W", "desc": "HST F438W magnitude "}, {"name": "HST", "desc": "HST ID "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "[C/Fe]", "desc": "?=99.99 Abundance [C/Fe] "}, {"name": "[N/Fe]", "desc": "?=99.99 Abundance [N/Fe] "}, {"name": "[O/Fe]", "desc": "?=99.99 Abundance [O/Fe] "}, {"name": "[Mg/Fe]", "desc": "Abundance [Mg/Fe] "}, {"name": "[Al/Fe]", "desc": "Abundance [Al/Fe] "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_1725"}} {"id": "J/MNRAS/475/1725", "title_cds": "Astrometry of double stars measured in 2011", "title_create": "Guerrero+, 2018", "year": "2018", "author": "Guerrero C.A., Orlov V.G., Borges Fernandes M., Angeles F.", "title_pub": "Speckle interferometry at the OAN-SPM Mexico: astrometry of double stars measured in 2011.", "first_author": "Guerrero C.A.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.1725G"], "keyword_cds": "Stars, double and multiple ; Interferometry", "keyword_pub": "techniques: high angular resolution - techniques: interferometric - binaries: close - binaries: visual", "abstract": ["We present speckle interferometric measurements of binary stars", "performed during 2011 February and April with the 1.5-m telescope and", "during 2011 July and November with the 2.1-m telescope of the", "Observatorio Astronomico Nacional, San Pedro Martir, Mexico, focusing", "on objects from the Washington Double Star Catalog with separations", "less than 1 arcsec. Among these objects, we have been interested in", "performing a follow-up observation of new double stars discovered by", "Hipparcos. For these observations, we developed a new detector, which", "is a combination of CCD Watec 120N with a third generation image", "intensifier. This image intensifier allows us to perform near-infrared", "speckle interferometric observations for the first time. In this", "paper, we report 761 astrometric measurements of 478 pairs, with", "angular separations ranging from 0.09 to 2.61 arcsec. We found that", "722 of our measured separations are smaller than 1 arcsec. We", "estimated a mean error in separation of 16 mas and 1.29{deg} in", "position angle. In order to overcome the usual 180{deg} ambiguity", "inherent to speckle measurements, we created a shift-and-add", "reconstructed image of each source, to establish the true quadrant of", "the secondary star. We confirmed 40 double stars discovered by", "Hipparcos and found 4 field stars resolved as interferometric pairs", "for the first time, with separations smaller than 0.60 arcsec."], "description": ["We carried out our observations in 2011, during four observing runs at", "the 1.5-m and 2.1-m telescopes of the OAN-SPM, Mexico. Specifically,", "from February 11 to 16 and April 15 to 20, we observed at the 1.5-m", "telescope, with moderate atmospheric conditions (seeing and", "transparency). From July 15 to 19 and November 7 to 13, we observed at", "the 2.1-m telescope, with excellent conditions for both runs. Our", "sample selection consisted of stars with separations shorter than", "1 arcsec, observable from the OAN-SPM, near the zenith. At the time", "of our observations, most of our sample of visual binaries were not", "observed since 20 yr ago or more. For the first two runs, most of our", "sample stars were observed through standard V, R and I filters. Half", "of the stars of the last two runs were observed through the R and I", "filters and the others were observed using just the R filter. This led", "to an apparent over population of stars resolved through the R", "passband."], "type": ["OC"], "data": "", "date_update": "08-Apr-2021", "tables": [{"name": "table3.dat", "desc": "Multi-band astrometry of known pairs observed with the 1.5m telescope", "columns": [{"name": "WDS", "desc": "WDS name (HHMMs+DDMM, J2000) "}, {"name": "n_WDS", "desc": "[*, HC] Note on WDS (1) "}, {"name": "Name", "desc": "Discoverer designation "}, {"name": "Epoch", "desc": "Epoch (Epoch-2011) "}, {"name": "theta", "desc": "Position angle "}, {"name": "e_theta", "desc": "rms uncertainty on theta "}, {"name": "rho", "desc": "Sepration angle "}, {"name": "e_rho", "desc": "rms uncertainty on rho "}, {"name": "thetaO-C", "desc": "? Observed minus computed Position angle "}, {"name": "rhoO-C", "desc": "? Observed minus computed Sepration angle "}, {"name": "Ref", "desc": "Reference, in refs.dat file "}, {"name": "lambda", "desc": "Wavelength (538, 630 or 894) "}]}, {"name": "table4.dat", "desc": "Multi-band astrometry of known pairs observed with the 2.1m telescope", "columns": [{"name": "WDS", "desc": "WDS name (HHMMs+DDMM, J2000) "}, {"name": "n_WDS", "desc": "[*, HC] Note on WDS (1) "}, {"name": "Name", "desc": "Discoverer designation "}, {"name": "Epoch", "desc": "Epoch (Epoch-2011) "}, {"name": "theta", "desc": "Position angle "}, {"name": "e_theta", "desc": "rms uncertainty on theta "}, {"name": "rho", "desc": "Sepration angle "}, {"name": "e_rho", "desc": "rms uncertainty on rho "}, {"name": "thetaO-C", "desc": "? Observed minus computed Position angle "}, {"name": "rhoO-C", "desc": "? Observed minus computed Sepration angle "}, {"name": "Ref", "desc": "Reference, in refs.dat file "}, {"name": "lambda", "desc": "Wavelength (538, 630 or 894) "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference code "}, {"name": "Text", "desc": "Reference and comments "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_2067"}} {"id": "J/MNRAS/475/2067", "title_cds": "Galaxy survey data in QSO/cluster fields", "title_create": "Burchett+, 2018", "year": "2018", "author": "Burchett J.N., Tripp T.M., Wang Q.D., Willmer C.N.A., Bowen D.V., Jenkins E.B.", "title_pub": "Warm-hot gas in X-ray bright galaxy clusters and the H I-deficient circumgalactic medium in dense environments.", "first_author": "Burchett J.N.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.2067B"], "keyword_cds": "Clusters, galaxy ; X-ray sources ; Optical ; Redshifts", "keyword_pub": "galaxies: clusters: intracluster medium - galaxies: evolution - galaxies: groups: general - galaxies: haloes - quasars: absorption lines - X-rays: galaxies: clusters", "abstract": ["We analyse the intracluster medium (ICM) and circumgalactic medium", "(CGM) in seven X-ray-detected galaxy clusters using spectra of", "background quasi-stellar objects (QSOs) (HST-COS/STIS), optical", "spectroscopy of the cluster galaxies (MMT/Hectospec and SDSS), and", "X-ray imaging/spectroscopy (XMM-Newton and Chandra). First, we report", "a very low covering fraction of HI absorption in the CGM of these", "cluster galaxies, f_c_=_25^+25^_-15_ percent, to stringent detection", "limits (N(HI)<10^13^cm^-2^). As field galaxies have an HI covering", "fraction of ~100 per cent at similar radii, the dearth of CGM HI in", "our data indicates that the cluster environment has effectively", "stripped or overionized the gaseous haloes of these cluster galaxies.", "Secondly, we assess the contribution of warm-hot (10^5^-10^6^K) gas to", "the ICM as traced by OVI and broad Ly{alpha} (BLA) absorption.", "Despite the high signal-to-noise ratio of our data, we do not detect", "OVI in any cluster, and we only detect BLA features in the QSO", "spectrum probing one cluster. We estimate that the total column", "density of warm-hot gas along this line of sight totals to ~3 per cent", "of that contained in the hot T>10^7^K X-ray emitting phase.", "Residing at high relative velocities, these features may trace", "pre-shocked material outside the cluster. Comparing gaseous galaxy", "haloes from the low-density 'field' to galaxy groups and high-density", "clusters, we find that the CGM is progressively depleted of HI with", "increasing environmental density, and the CGM is most severely", "transformed in galaxy clusters. This CGM transformation may play a key", "role in environmental galaxy quenching."], "description": ["We present the coordinates and redshifts for all galaxies", "spectroscopically measured, either through our own observations or", "through those provided by the SDSS, in the QSO/cluster fields featured", "in this work. In the table provided, the large majority of objects are", "drawn from our survey with MMT/Hectospec, for which the redshift", "measurement software provides quality scores that reflect the", "confidence of the measurement."], "type": ["OC"], "data": "", "date_update": "08-Apr-2021", "tables": [{"name": "tablea1.dat", "desc": "Galaxy survey data in QSO/cluster fields ", "columns": [{"name": "Field", "desc": "Field name (A1095, A1926 or A2246) "}, {"name": "Name", "desc": "Galaxy name "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "z", "desc": "Redshift "}, {"name": "e_z", "desc": "rms uncertainty on z "}, {"name": "Qual", "desc": "[-4/4] Quality flag (1) "}, {"name": "Class", "desc": "Object class "}, {"name": "Source", "desc": "Source (Hectospec, SDSS or La Palma) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_2480"}} {"id": "J/MNRAS/475/2480", "title_cds": "Extremely-low mass white dwarf star", "title_create": "Pelisoli+, 2018", "year": "2018", "author": "Pelisoli I., Kepler S.O., Koester D.", "title_pub": "The sdA problem. I. Physical properties.", "first_author": "Pelisoli I.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.2480P"], "see_also": ["J/A+A/600/A50 : Catalog of hot subdwarf stars (Geier+, 2017)"], "keyword_cds": "Stars, dwarfs ; Stars, subdwarf ; Stars, white dwarf ; Effective temperatures", "keyword_pub": "binaries: general - stars: evolution - stars: kinematics and dynamics - subdwarfs - white dwarfs", "abstract": ["The so-called sdA stars are defined by having H-rich spectra and", "surface gravities similar to hot subdwarf stars, but effective", "temperature below the zero-age horizontal branch. Their evolutionary", "history is an enigma: their surface gravity is too high for", "main-sequence stars, but too low for single evolution white dwarfs.", "They are most likely byproducts of binary evolution, including", "blue-stragglers, extremely-low mass white dwarf stars (ELMs) and their", "precursors (pre-ELMs). A small number of ELMs with similar properties", "to sdAs is known. Other possibilities include metal-poor A/F dwarfs,", "second generation stars, or even stars accreted from dwarf galaxies.", "In this work, we analyse colours, proper motions, and spacial", "velocities of a sample of sdAs from the Sloan Digital Sky Survey to", "assess their nature and evolutionary origin. We define a probability", "of belonging to the main sequence and a probability of being a", "(pre-)ELM based on these properties. We find that 7 per cent of the", "sdAs are more likely to be (pre-)ELMs than main-sequence stars.", "However, the spacial velocity distribution suggests that over 35 per", "cent of them cannot be explained as single metal-poor A/F stars."], "description": ["We have analysed a sample of narrow-line hydrogen spectra identified", "in the SDSS, estimating Teff and logg from their spectra using new", "spectral models derived from solar abundance atmospheric models."], "type": ["OC"], "data": "", "date_update": "08-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Obtained values of Teff and logg for the 408 analysed SDSS objects in the range 5.5<=logg<7.0 and 7000<=Teff<=20000K", "columns": [{"name": "SDSS", "desc": "SDSS designation (HHMMSS.ss+DDMMSS.s) "}, {"name": "PMF", "desc": "SDSS Plate-MJD-Fiber identifier "}, {"name": "SNRg", "desc": "Signal-to-noise ratio in g band "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "e_Teff", "desc": "rms uncertainty on Teff (1) "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "e_logg", "desc": "rms uncertainty on logg (1) "}]}, {"name": "table2.dat", "desc": "Objects with a higher probability of being (pre-)ELM compared to main sequence", "columns": [{"name": "SDSS", "desc": "SDSS designation (HHMMSS.ss+DDMMSS.s) "}, {"name": "PMF", "desc": "SDSS Plate-MJD-Fiber identifier "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "e_Teff", "desc": "rms uncertainty on Teff "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "e_logg", "desc": "rms uncertainty on logg "}, {"name": "pMS", "desc": "Probability of being main sequence "}, {"name": "pELM", "desc": "Probability of being extremely-low mass white dwarf star (ELM)"}]}, {"name": "tablec1.dat", "desc": "Objects for which our fit indicated Teff>20000K and logg<6.5, which are possible hot subdwarfs not listed in Geier et al. (2017, Cat. J/A+A/600/A50)", "columns": [{"name": "SDSS", "desc": "SDSS designation (HHMMSS.ss+DDMMSS.s) "}, {"name": "PMF", "desc": "SDSS Plate-MJD-Fiber identifier "}, {"name": "---", "desc": "[,] "}, {"name": "PMF2", "desc": "Second SDSS Plate-MJD-Fiber identifier "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_3090"}} {"id": "J/MNRAS/475/3090", "title_cds": "Predicted properties for 468 RV planets", "title_create": "Yi+, 2018", "year": "2018", "author": "Yi J.S., Chen J., Kipping D.", "title_pub": "Forecasting the detectability of known radial velocity planets with the upcoming CHEOPS mission.", "first_author": "Yi J.S.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.3090Y"], "keyword_cds": "Stars, double and multiple ; Exoplanets ; Stars, masses ; Stars, diameters", "keyword_pub": "methods: statistical - eclipses - planets and satellites: detection", "abstract": ["The CHaracterizing ExOPlanets Satellite (CHEOPS) mission is planned", "for launch next year with a major objective being to search for", "transits of known radial velocity (RV) planets, particularly those", "orbiting bright stars. Since the RV method is only sensitive to", "planetary mass, the radii, transit depths and transit signal-to-noise", "values of each RV planet are, a priori, unknown. Using an empirically", "calibrated probabilistic mass-radius relation, forecaster, we address", "this by predicting a catalogueof homogeneous credible intervals for", "these three keys terms for 468 planets discovered via RVs. Of these,", "we find that the vast majority should be detectable with CHEOPS,", "including terrestrial bodies, if they have the correct geometric", "alignment. In particular, we predict that 22 mini-Neptunes and 82", "Neptune-sized planets would be suitable for detection and that more", "than 80 per cent of these will have apparent magnitude of V<10,", "making them highly suitable for follow-up characterization work. Our", "work aims to assist the CHEOPS team in scheduling efforts and", "highlights the great value of quantifiable, statistically robust", "estimates for upcoming exoplanetary missions."], "description": ["In this work, we have predicted the planetary radii, transit depths,", "and associated SNRs using CHEOPS (Broeg et al., 2013, CHEOPS: A", "transit photometry mission for ESA's small mission programme, EPJ Web", "Conf., 47, 3005) for 468 planets listed on the \"exoplanet Orbit", "Database\" (EOD; Han et al., 2014PASP..126..827H, Exoplanets.org) as", "having been discovered using the RV method. Our SNR values assume 1h", "of cumulative integration time, no intrinsic stellar noise, employ a", "CHEOPS noise model dependent on spectral type and apparent magnitude,", "and accounts for instrument saturation."], "type": ["MC"], "data": "", "date_update": "08-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Final predicted properties for 468 RV planets using forecaster", "columns": [{"name": "Name", "desc": "Planet name "}, {"name": "Mass", "desc": "Planetary mass "}, {"name": "e_Mass", "desc": "Planetary mass +/-34.1% uncertainty "}, {"name": "Rad2.2", "desc": "Planetary radius 2.2% quantile "}, {"name": "Rad15.9", "desc": "Planetary radius 15.9% quantile "}, {"name": "Rad50.0", "desc": "Planetary radius 50.0% quantile "}, {"name": "Rad81.1", "desc": "Planetary radius 84.1% quantile "}, {"name": "Rad97.7", "desc": "Planetary radius 97.7% quantile "}, {"name": "Rad*", "desc": "Stellar radius "}, {"name": "e_Rad*", "desc": "Stellar radius -34.1% uncertainty "}, {"name": "E_Rad*", "desc": "Stellar radius +34.1% uncertainty "}, {"name": "Depht2.2", "desc": "Transit depth 2.2% quantile (in parts per thousand unit)"}, {"name": "Depht15.9", "desc": "Transit depth 15.9% quantile (in parts per thousand unit)"}, {"name": "Depht50.0", "desc": "Transit depth 50.0% quantile (in parts per thousand unit)"}, {"name": "Depht84.1", "desc": "Transit depth 84.1% quantile (in parts per thousand unit)"}, {"name": "Depht97.7", "desc": "Transit depth 97.7% quantile (in parts per thousand unit)"}, {"name": "Vmag", "desc": "V-band apparent magnitude "}, {"name": "phnoise", "desc": "CHEOPS r.m.s. photometric noise (in parts per million/hour unit)"}, {"name": "phnoise2.2", "desc": "CHEOPS signal-to-noise ratio per hour 2.2% quantile (in parts per million/hour unit)"}, {"name": "phnoise15.9", "desc": "CHEOPS signal-to-noise ratio per hour 15.9% quantile (in parts per million/hour unit)"}, {"name": "phnoise50.0", "desc": "CHEOPS signal-to-noise ratio per hour 50.0% quantile (in parts per million/hour unit)"}, {"name": "phnoise84.1", "desc": "CHEOPS signal-to-noise ratio per hour 84.1% quantile (in parts per million/hour unit)"}, {"name": "phnoise97.7", "desc": "CHEOPS signal-to-noise ratio per hour 97.7% quantile (in parts per million/hour unit)"}, {"name": "Dur", "desc": "Maximum transit duration [hours] "}, {"name": "e_Dur", "desc": "Maximum transit duration -34.1% uncertainty "}, {"name": "E_Dur", "desc": "Maximum transit duration +34.1% uncertainty "}, {"name": "Prob", "desc": "?=- Geometric transit probability "}, {"name": "Flag", "desc": "[0/3] Planet flag (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_3633"}} {"id": "J/MNRAS/475/3633", "title_cds": "Mass and age of red giant branch stars", "title_create": "Wu+, 2018", "year": "2018", "author": "Wu Y., Xiang M., Bi S., Liu X., Yu J., Hon M., Sharma S., Li T., Huang Y., Liu K., Zhang X., Li Y., Ge Z., Tian Z., Zhang J., Zhang J.", "title_pub": "Mass and age of red giant branch stars observed with LAMOST and Kepler.", "first_author": "Wu Y.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.3633W"], "see_also": ["V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)", "V/164 : LAMOST DR5 catalogs (Luo+, 2019)"], "keyword_cds": "Stars, giant ; Stars, masses ; Stars, ages ; Abundances", "keyword_pub": "asteroseismology - stars: evolution - stars: fundamental parameters", "abstract": ["Obtaining accurate and precise masses and ages for large numbers of", "giant stars is of great importance for unraveling the assemblage", "history of the Galaxy. In this paper, we estimate masses and ages of", "6940 red giant branch (RGB) stars with asteroseismic parameters", "deduced from Kepler photometry and stellar atmospheric parameters", "derived from LAMOST spectra. The typical uncertainties of mass is a", "few per cent, and that of age is ~20 per cent. The sample stars", "reveal two separate sequences in the age-[{alpha}/Fe] relation - a", "high-{alpha} sequence with stars older than ~8Gyr and a", "low-{alpha} sequence composed of stars with ages ranging from younger", "than 1Gyr to older than 11Gyr. We further investigate the", "feasibility of deducing ages and masses directly from LAMOST spectra", "with a machine learning method based on kernel based principal", "component analysis, taking a sub-sample of these RGB stars as a", "training data set. We demonstrate that ages thus derived achieve an", "accuracy of ~24 per cent. We also explored the feasibility of", "estimating ages and masses based on the spectroscopically measured", "carbon and nitrogen abundances. The results are quite satisfactory and", "significantly improved compared to the previous studies."], "type": ["CCC"], "data": "", "date_update": "08-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Deduced parameters of the 3726 uniq RGB sample stars", "columns": [{"name": "spID", "desc": "LAMOST spectrum identifier "}, {"name": "KIC", "desc": "KIC number "}, {"name": "Teff", "desc": "Effective temperature "}, {"name": "e_Teff", "desc": "rms uncertainty on Teff "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "e_logg", "desc": "rms uncertainty on logg "}, {"name": "[Fe/H]", "desc": "Metallicity "}, {"name": "e_[Fe/H]", "desc": "rms uncertainty on [Fe/H] "}, {"name": "[alpha/Fe]", "desc": "Abundance [alpha/Fe] "}, {"name": "e_[alpha/Fe]", "desc": "rms uncertainty on [alpha/Fe] "}, {"name": "[C/H]", "desc": "Abundance [C/H] "}, {"name": "e_[C/H]", "desc": "rms uncertainty on [C/H] "}, {"name": "[N/H]", "desc": "Abundance [N/H] "}, {"name": "e_[N/H]", "desc": "rms uncertainty on [N/H] "}, {"name": "dnu", "desc": "Frequency separation of two modes of the same spherical degree and consecutive"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_4148"}} {"id": "J/MNRAS/475/4148", "title_cds": "UKIDSS UDS field spectroscopic redshifts", "title_create": "Galametz+, 2018", "year": "2018", "author": "Galametz A., Pentericci L., Castellano M., Mendel T., Hartley W.G., Fossati M., Finoguenov A., Almaini O., Beifiori A., Fontana A., Grazian A., Scodeggio M., Kocevski D.D.", "title_pub": "Growing up in a megalopolis: environmental effects on galaxy evolution in a supercluster at z ~ 0.65 in UKIDSS UDS.", "first_author": "Galametz A.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.4148G"], "see_also": ["J/ApJS/206/10 : CANDELS multiwavelength catalog (Galametz+, 2013)", "J/ApJ/801/97 : GOODS-S+UDS stellar mass catalogs from CANDELS (Santini+, 2015)"], "keyword_cds": "Clusters, galaxy ; Galaxy catalogs ; Redshifts", "keyword_pub": "galaxies: clusters: individual: ClG J021734-0513 - large-scale structure of Universe", "abstract": ["We present a large-scale galaxy structure Cl J021734-0513 at z~0.65", "discovered in the UKIDSS UDS field, made of ~20 galaxy groups and", "clusters, spreading over 10Mpc. We report on a VLT/VIMOS", "spectroscopic follow-up program that, combined with past spectroscopy,", "allowed us to confirm four galaxy clusters (M_200_~10^14^M_{sun}_) and", "a dozen associated groups and star-forming galaxy overdensities. Two", "additional filamentary structures at z~0.62 and 0.69 and foreground", "and background clusters at 0.6"], "bibcode": ["2018MNRAS.475.4768T"], "keyword_cds": "", "keyword_pub": "techniques: photometric - stars: oscillations - white dwarfs - ultraviolet: stars", "abstract": ["We present results from a search for short time-scale white dwarf", "variability using gPhoton, a time-tagged data base of GALEX photon", "events and associated software package. We conducted a survey of 320", "white dwarf stars in the McCook-Sion catalogue, inspecting each for", "photometric variability with particular emphasis on variability over", "time-scales less than ~30 min. From that survey, we present the", "discovery of a new pulsating white dwarf: WD 2246-069. A CaII K line", "is found in archival ESO spectra and an IR excess is seen in WISE W1", "and W2 bands. Its independent modes are identified in follow-up", "optical photometry and used to model its interior structure.", "Additionally, we detect UV pulsations in four previously known", "pulsating ZZ Ceti-type (DAVs). Included in this group is the", "simultaneous fitting of the pulsations of WD 1401-147 in optical,", "near-ultraviolet and far-ultraviolet bands using nearly concurrent", "Whole Earth Telescope and GALEX data, providing observational insight", "into the wavelength dependence of white dwarf pulsation amplitudes."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "08-Apr-2021"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_5133"}} {"id": "J/MNRAS/475/5133", "title_cds": "3DHST CANDELS redshift compilation", "title_create": "Rodrigues+, 2018", "year": "2018", "author": "Rodrigues M., Puech M., Flores H., Hammer F., Pirzkal N.", "title_pub": "Testing the hierarchical assembly of massive galaxies using accurate merger rates out to z ~ 1.5.", "first_author": "Rodrigues M.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.5133R"], "see_also": ["J/ApJS/225/27 : 3D-HST Survey: grism spectra master catalog (Momcheva+, 2016)"], "keyword_cds": "Galaxy catalogs ; Redshifts", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: high-redshift - galaxies: interactions", "abstract": ["We established an accurate comparison between observationally and", "theoretically estimated major merger rates over a large range of mass", "(logM_bar_/M_{sun}_=9.9-11.4) and redshift (z=0.7-1.6). For this,", "we combined a new estimate of the merger rate from an exhaustive count", "of pairs within the virial radius of massive galaxies at z~1.265 and", "cross-validated with their morphology, with estimates from the", "morpho-kinematic analysis of two other samples. Theoretical", "predictions were estimated using semi-empirical models with inputs", "matching the properties of the observed samples, while specific", "visibility time-scales scaled to the observed samples were used. Both", "theory and observations are found to agree within 30 per cent of the", "observed value, which provides strong support to the hierarchical", "assembly of galaxies over the probed ranges of mass and redshift.", "Here, we find that ~60 per cent of population of local massive", "(M_stellar_=10^10.3-11.6^M_{sun}_) galaxies would have undergone a", "wet major merger since z=1.5, consistently with previous studies.", "Such recent mergers are expected to result in the (re-)formation of a", "significant fraction of local disc galaxies."], "description": ["We collected all zspec measurements available in GOODS-S and", "constructed an updated catalogue of the most accurate redshift", "measurements for 3D-HST sources in this field."], "type": ["OC"], "data": "", "date_update": "08-Apr-2021", "tables": [{"name": "tablea1.dat", "desc": "3DHST CANDELS redshift compilation ", "columns": [{"name": "ID", "desc": "[1/50502] Identification number "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "declination (J2000) "}, {"name": "Jmag", "desc": "?=- J magnitude "}, {"name": "z", "desc": "?=-1 Spectroscopic or photometric redshift "}, {"name": "q_z", "desc": "[0/3] Redshift quality flag (1) "}, {"name": "Flag", "desc": "[-1/4] Flag type (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_5179"}} {"id": "J/MNRAS/475/5179", "title_cds": "Spatially offset AGN cand. in CLASS survey", "title_create": "Skipper+, 2018", "year": "2018", "author": "Skipper C.J., Browne I.W.A.", "title_pub": "Spatially offset AGN candidates in the CLASS survey.", "first_author": "Skipper C.J.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.5179S"], "see_also": ["VIII/72 : CLASS survey of radio sources (Myers+, 2003)"], "keyword_cds": "Active gal. nuclei ; Positional data ; Redshifts", "keyword_pub": "galaxies: active - galaxies: interactions - galaxies: nuclei", "abstract": ["Prompted by a recent claim by Barrows et al. that X-ray active", "galactic nuclei (AGNs) are often found significantly offset from the", "centres of their host galaxies, we have looked for examples of compact", "radio sources that are offset from the optical centroids of nearby", "(z<0.2) galaxies. We have selected a sample of 345 galaxies from the", "Sloan Digital Sky Survey (SDSS) galaxy catalogue, which have nearby", "compact radio sources listed in the Cosmic-Lens All Sky Survey (CLASS)", "catalogue. We find only three matches ~0.87 per cent of the", "sample) with offsets greater than 600 milliarcsec (mas), which is", "considerably fewer than we would have expected from the Barrows et al.", "X-ray survey. We fit our histogram of offsets with a Rayleigh", "distribution with {sigma}=60.5mas, but find that there is an excess", "of objects with separations greater than ~150mas. Assuming that", "this excess represents AGNs with real offsets, we place an upper limit", "of ~17 per cent on the fraction of offset AGNs in our", "radio-selected sample. We select 38 objects with offsets greater than", "150mas, and find they have some diverse properties: Some are well", "known, such as Mrk 273 and Arp 220, some have dust lanes, which may", "have affected the optical astrometry, and a few are strong new", "candidates for offset AGNs."], "description": ["Our sample was constructed from the SDSS galaxy catalogue by cross", "matching sources with the z<0.2 OSSY catalogue (Oh et al.,", "2011ApJS..195...13O), and the CLASS catalogue (Myers et al.,", "2003MNRAS.341....1M, Browne et al., 2003MNRAS.341...13B, Cat. VIII/72)", "of compact radio sources. Our sample comprised 374 galaxies."], "type": ["CCC"], "data": "", "date_update": "08-Apr-2021", "tables": [{"name": "table1.dat", "desc": "*The high-offset galaxies ", "columns": [{"name": "SDSS", "desc": "SDSS catalog ID (SDSS JHHMMSS.ss+DDMMSS.s) "}, {"name": "OSSY", "desc": "OSSY catalog ID "}, {"name": "RAdeg", "desc": "OSSY right ascension (J2000) "}, {"name": "DEdeg", "desc": "OSSY declination (J2000) "}, {"name": "z", "desc": "Redshift of galaxy from OSSY catalog "}, {"name": "OName", "desc": "Other common galaxy names (i.e. NGC, Messier, UGC, IC, Markarian catalog IDs)"}, {"name": "Sy/LINER", "desc": "[SEYFERT LINER] Seyfert or LINER, based upon the line strengths from the OSSY catalog"}, {"name": "CLASS", "desc": "CLASS catalog ID (GB6JHHMMSS+DDMMSS) "}, {"name": "RANdeg", "desc": "Right ascension (J2000) of nearest CLASS source to galaxy position"}, {"name": "DENdeg", "desc": "Declination (J2000) of nearest CLASS source to galaxy position"}, {"name": "OffsetN", "desc": "Offset between galaxy position and nearest CLASS source"}, {"name": "FluxN", "desc": "Flux density at 8.46GHz of nearest CLASS source"}, {"name": "RABdeg", "desc": "? Right ascension (J2000) of brightest CLASS source (1)"}, {"name": "DEBdeg", "desc": "? Declination (J2000) of brightest CLASS source (1)"}, {"name": "OffsetB", "desc": "? Offset between galaxy position and brightest CLASS source (1)"}, {"name": "FluxB", "desc": "? Flux density at 8.46GHz of brightest CLASS source (1)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_475_5487"}} {"id": "J/MNRAS/475/5487", "title_cds": "Stellar properties of KIC stars", "title_create": "Silva Aguirre+, 2018", "year": "2018", "author": "Silva Aguirre V., Bojsen-Hansen M., Slumstrup D., Casagrande L., Kawata D., Ciuca I., Handberg R., Lund M.N., Mosumgaard J.R., Huber D., Johnson J.A., Pinsonneault M.H., Serenelli A.M., Stello D., Tayar J., Bird J.C., Cassisi S., Hon M., Martig M., Nissen P.E., Rix H.W., Schonrich R., Sahlholdt C., Trick W.H., Yu J.", "title_pub": "Confirming chemical clocks: asteroseismic age dissection of the Milky Way disc(s).", "first_author": "Silva Aguirre V.", "ref_biblio": [""], "bibcode": ["2018MNRAS.475.5487S"], "see_also": ["V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)", "J/MNRAS/452/2127 : Fundamental parameters of Kepler stars", "J/ApJ/835/173 : Kepler asteroseismic LEGACY sample. II."], "keyword_cds": "Stars, giant ; Stars, masses ; Stars, diameters ; Stars, ages ; Stars, distances", "keyword_pub": "asteroseismology - stars: fundamental parameters - stars: kinematics and dynamic - Galaxy: disc - Galaxy: evolution - Galaxy: structure", "abstract": ["Investigations of the origin and evolution of the Milky Way disc have", "long relied on chemical and kinematic identifications of its", "components to reconstruct our Galactic past. Difficulties in", "determining precise stellar ages have restricted most studies to small", "samples, normally confined to the solar neighbourhood. Here, we break", "this impasse with the help of asteroseismic inference and perform a", "chronology of the evolution of the disc throughout the age of the", "Galaxy. We chemically dissect the Milky Way disc population using a", "sample of red giant stars spanning out to 2 kpc in the solar annulus", "observed by the Kepler satellite, with the added dimension of", "asteroseismic ages. Our results reveal a clear difference in age", "between the low- and high-{alpha} populations, which also show", "distinct velocity dispersions in the V and W components. We find no", "tight correlation between age and metallicity nor [{alpha}/Fe] for the", "high-{alpha} disc stars. Our results indicate that this component", "formed over a period of more than 2 Gyr with a wide range of [M/H] and", "[{alpha}/Fe] independent of time. Our findings show that the kinematic", "properties of young {alpha}-rich stars are consistent with the rest of", "the high-{alpha} population and different from the low-{alpha} stars", "of similar age, rendering support to their origin being old stars that", "went through a mass transfer or stellar merger event, making them", "appear younger, instead of migration of truly young stars formed close", "to the Galactic bar."], "description": ["The set of stars considered in this study are the 1989 red giants", "comprising the first combined APOGEE and Kepler catalogues, in which", "the Kepler spacecraft detected oscillations during its nominal", "mission.", "We determined stellar properties for the APOKASC sample combining the", "photometric, spectroscopic, and asteroseismic observables using the", "BAyesian STellar Algorithm (BASTA, Silva Aguirre et al. 2015, Cat.", "J/MNRAS/452/2127, 2017, Cat. J/ApJ/835/173)."], "type": ["CCC"], "data": "", "date_update": "08-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Stellar properties determined with BASTA for the APOKASC sample", "columns": [{"name": "KIC", "desc": "Kepler Input Catalogue Identifier "}, {"name": "Mass", "desc": "Mass "}, {"name": "e_Mass", "desc": "rms uncertainty on Mass "}, {"name": "Rad", "desc": "Radius "}, {"name": "e_Rad", "desc": "rms uncertainty on Rad "}, {"name": "logg", "desc": "Surface gravity "}, {"name": "e_logg", "desc": "rms uncertainty on logg "}, {"name": "Age", "desc": "Age "}, {"name": "e_Age", "desc": "rms uncertainty on Age "}, {"name": "Lum", "desc": "Luminosity "}, {"name": "e_Lum", "desc": "rms uncertainty on Lum "}, {"name": "Dist", "desc": "Distance "}, {"name": "e_Dist", "desc": "rms uncertainty on Dist "}, {"name": "Prob", "desc": "Target selection probability "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_114"}} {"id": "J/MNRAS/476/114", "title_cds": "Stellar properties of Kron 3 stars", "title_create": "Hollyhead+, 2018", "year": "2018", "author": "Hollyhead K., Lardo C., Kacharov N., Bastian N., Hilker M., Rejkuba M., Koch A., Grebel E.K., Georgiev I.", "title_pub": "Kron 3: a fourth intermediate age cluster in the SMC with evidence of multiple populations.", "first_author": "Hollyhead K.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476..114H"], "keyword_cds": "Magellanic Clouds ; Associations, stellar ; Stars, giant ; Effective temperatures ; Abundances", "keyword_pub": "Magellanic Clouds - galaxies: star clusters: individual: Kron 3", "abstract": ["We present the results of a spectroscopic study of the intermediate", "age (~=6.5Gyr) massive cluster Kron 3 in the Small Magellanic", "Cloud. We measure CN and CH band strengths (at ~=3839 and 4300{AA},", "respectively) using VLT FORS2 spectra of 16 cluster members and find a", "sub-population of five stars enriched in nitrogen. We conclude that", "this is evidence for multiple populations in Kron 3, the fourth", "intermediate age cluster, after Lindsay 1, NGC 416 and NGC 339 (ages", "6-8Gyr), to display this phenomenon originally thought to be a unique", "characteristic of old globular clusters. At ~=6.5Gyr this is one of", "the youngest clusters with multiple populations, indicating that the", "mechanism responsible for their onset must operate until a redshift of", "at least 0.75, much later than the peak of globular cluster formation", "at redshift ~3."], "description": ["FORS2 spectroscopy of 35 RGB stars in the intermediate age massive", "cluster Kron 3 in the SMC have yielded 16 member stars after a", "conservative membership selection process. We were able to derive CN", "and CH index measurements and C and N abundances for 16 stars."], "type": ["OC"], "data": "", "date_update": "08-Apr-2021", "tables": [{"name": "table1.dat", "desc": "*Stellar properties for all 35 stars in our programme", "columns": [{"name": "Star", "desc": "Star identification number "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Vmag", "desc": "V magnitude "}, {"name": "Teff", "desc": "?=- Effective temperature "}, {"name": "e_Teff", "desc": "?=- rms uncertainty on Teff "}, {"name": "logg", "desc": "?=- Surface gravity "}, {"name": "e_logg", "desc": "?=- rms uncertainty on logg "}, {"name": "[C/Fe]", "desc": "?=- Abundance [C/Fe] "}, {"name": "e_[C/Fe]", "desc": "?=- rms uncertainty on [C/Fe] "}, {"name": "[N/Fe]", "desc": "?=- Abundance [N/Fe] "}, {"name": "e_[N/Fe]", "desc": "?=- rms uncertainty on [N/Fe] "}, {"name": "CN", "desc": "?=- CN index "}, {"name": "e_CN", "desc": "?=- rms uncertainty on CN "}, {"name": "CH", "desc": "?=- CH index "}, {"name": "e_CH", "desc": "?=- rms uncertainty on CH "}, {"name": "Ca(HK)", "desc": "?=- Ca(HK) index "}, {"name": "e_Ca(HK)", "desc": "?=- rms uncertainty on Ca(HK) "}, {"name": "Fe", "desc": "?=- Fe index "}, {"name": "e_Fe", "desc": "?=- rms uncertainty on Fe "}, {"name": "RV", "desc": "Radial velocity "}, {"name": "Notes", "desc": "Notes "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_307"}} {"id": "J/MNRAS/476/307", "title_cds": "Short Title", "title_create": "Moreno-Raya+, 2018", "year": "2018", "author": "Moreno-Raya M.E., Galbany L., Lopez-Sanchez A.R., Molla M., Gonzalez-Gaitan S., Vilchez J.M., Carnero A.", "title_pub": "Elemental gas-phase abundances of intermediate redshift type Ia supernova star-forming host galaxies.", "first_author": "Moreno-Raya M.E.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476..307M"], "keyword_cds": "", "keyword_pub": "methods: data analysis - techniques: spectroscopic - supernovae: general - ISM: abundances - HII regions - galaxies: abundances", "abstract": ["The maximum luminosity of type Ia supernovae (SNe Ia) depends on the", "oxygen abundance of the regions of the host galaxies, where they", "explode. This metallicity dependence reduces the dispersion in the", "Hubble diagram (HD) when included with the traditional two-parameter", "calibration of SN Ia light-curve parameters and absolute magnitude. In", "this work, we use empirical calibrations to carefully estimate the", "oxygen abundance of galaxies hosting SNe Ia from the SDSS-II/SN (Sloan", "Digital Sky Survey-II Supernova) survey at intermediate redshift by", "measuring their emission-line intensities. We also derive electronic", "temperature with the direct method for a small fraction of objects for", "consistency. We find a trend of decreasing oxygen abundance with", "increasing redshift for the most massive galaxies. Moreover, we study", "the dependence of the HD residuals (HR) with galaxy oxygen abundance", "obtaining a correlation in line with those found in other works. In", "particular, the HR versus oxygen abundance shows a slope of", "-0.186+/-0.123mag/dex (1.52{sigma}) in good agreement with theoretical", "expectations. This implies smaller distance modulii after corrections", "for SNe Ia in metal-rich galaxies. Based on our previous results on", "local SNe Ia, we propose this dependence to be due to the lower", "luminosity of the SNe Ia produced in more metal-rich environments."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "13-Apr-2021"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_528"}} {"id": "J/MNRAS/476/528", "title_cds": "Short Title", "title_create": "El-badry+, 2018", "year": "2018", "author": "El-badry K., Ting Y.-S., Rix H.-W., Quataert E., Weisz D.R., Cargile P., Conroy C., Hogg D.W., Bergemann M., Liu C.", "title_pub": "Discovery and characterization of 3000+ main-sequence binaries from APOGEE spectra.", "first_author": "El-badry K.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476..528E"], "keyword_cds": "", "keyword_pub": "methods: data analysis - binaries: spectroscopic - Galaxy: stellar content", "abstract": ["We develop a data-driven spectral model for identifying and", "characterizing spatially unresolved multiple-star systems and apply it", "to APOGEE DR13 spectra of main-sequence stars. Binaries and triples", "are identified as targets whose spectra can be significantly better", "fit by a superposition of two or three model spectra, drawn from the", "same isochrone, than any single-star model. From an initial sample of", "~20000 main-sequence targets, we identify ~2500 binaries in", "which both the primary and secondary stars contribute detectably to", "the spectrum, simultaneously fitting for the velocities and stellar", "parameters of both components. We additionally identify and fit", "~200 triple systems, as well as ~700 velocity-variable systems in", "which the secondary does not contribute detectably to the spectrum.", "Our model simplifies the process of simultaneously fitting single- or", "multi-epoch spectra with composite models and does not depend on a", "velocity offset between the two components of a binary, making it", "sensitive to traditionally undetectable systems with periods of", "hundreds or thousands of years. In agreement with conventional", "expectations, almost all the spectrally identified binaries with", "measured parallaxes fall above the main sequence in the", "colour-magnitude diagram. We find excellent agreement between", "spectrally and dynamically inferred mass ratios for the ~600", "binaries in which a dynamical mass ratio can be measured from", "multi-epoch radial velocities. We obtain full orbital solutions for 64", "systems, including 14 close binaries within hierarchical triples. We", "make available catalogues of stellar parameters, abundances, mass", "ratios, and orbital parameters."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "13-Apr-2021"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_724"}} {"id": "J/MNRAS/476/724", "title_cds": "EW of 4 primary stars and the Sun", "title_create": "Kong+, 2018", "year": "2018", "author": "Kong X.M., Zhao G., Zhao J.K., Shi J.R., Bharat Kumar Y., Wang L., Zhang J.B., Wang Y., Zhou Y.T.", "title_pub": "Chemical abundances of primary stars in the Sirius-like binary systems.", "first_author": "Kong X.M.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476..724K"], "keyword_cds": "Stars, barium ; Abundances, peculiar", "keyword_pub": "stars: abundances - binaries: general - stars: chemically peculiar - stars: fundamental parameters - white dwarfs", "abstract": ["Study of primary stars lying in Sirius-like systems with various", "masses of white dwarf (WD) companions and orbital separations is one", "of the key aspects to understand the origin and nature of barium (Ba)", "stars. In this paper, based on high-resolution and high-S/N spectra,", "we present systematic analysis of photospheric abundances for 18 FGK", "primary stars of Sirius-like systems including six giants and 12", "dwarfs. Atmospheric parameters, stellar masses, and abundances of 24", "elements (C, Na, Mg, Al, Si, S, K, Ca, Sc, Ti, V, Cr, Mn, Fe, Co, Ni,", "Cu, Sr, Y, Zr, Ba, La, Ce, and Nd) are determined homogeneously. The", "abundance patterns in these sample stars show that most of the", "elements in our sample follow the behaviour of field stars with", "similar metallicity. As expected, s-process elements in four known Ba", "giants show overabundance. A weak correlation was found between", "anomalies of s-process elemental abundance and orbital separation,", "suggesting that the orbital separation of the binaries could not be", "the main constraint to differentiate strong Ba stars from mild Ba", "stars. Our study shows that the large mass (>0.51M_{sun}_) of a WD", "companion in a binary system is not a sufficient condition to form a", "Ba star, even if the separation between the two components is small.", "Although not sufficient, it seems to be a necessary condition since Ba", "stars with lower mass WDs in the observed sample were not found. Our", "results support that [s/Fe] and [hs/ls] ratios of Ba stars are", "anti-correlated with the metallicity. However, the different levels of", "s-process overabundance among Ba stars may not be dominated mainly by", "the metallicity."], "description": ["This paper presents a complete analysis of chemical abundances in a", "sample of 18 FGK stars belonging to binary systems with a white dwarf", "(Sirius-like systems). The purpose of the work is to compare the", "characteristics of those systems to try to understand what is", "necessary to produce a Ba-rich star. We show that the orbital", "separation of these systems is not important to determine whether a", "star becomes a Ba star. We also conclude that a companion white dwarf", "with a large mass is not enough to produce such objects either."], "object": ["22 19 34.36 +21 22 01.8 BD+20 5125 = HIP 110218", "14 57 53.57 +29 52 32.5 BD+30 2592 = HIP 73224", "07 04 02.88 +71 11 41.5 BD+71 380 = HIP 34082", "05 53 58.75 +12 25 10.0 HD 39570 = HIP 27878"], "type": ["OC"], "data": "", "date_update": "13-Apr-2021", "tables": [{"name": "table3.dat", "desc": "All atomic-line data used and their corresponding EWs and abundances of program stars and the Sun", "columns": [{"name": "Star", "desc": "Star name (1) "}, {"name": "Ion", "desc": "Ion designation "}, {"name": "lambda", "desc": "Wavelength "}, {"name": "EP", "desc": "Excitation potential "}, {"name": "loggf", "desc": "log of Oscillator Strength "}, {"name": "EW", "desc": "Line equivalent width "}, {"name": "A(X)", "desc": "Absolute element abundances "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_908"}} {"id": "J/MNRAS/476/908", "title_cds": "Chromospheric activity in 4 open clusters", "title_create": "Fang+, 2018", "year": "2018", "author": "Fang X.-S., Zhao G., Zhao J.-K., Bharat Kumar Y.", "title_pub": "Stellar activity with LAMOST. II. Chromospheric activity in open clusters.", "first_author": "Fang X.-S.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476..908F"], "see_also": ["V/153 : LAMOST DR4 catalogs (Luo+, 2018)"], "keyword_cds": "Clusters, open ; Stars, late-type ; Equivalent widths", "keyword_pub": "stars: activity - stars: chromospheres - stars: late-type - stars: rotation", "abstract": ["We use the LAMOST spectra of member stars in Pleiades, M34, Praesepe,", "and Hyades to study how chromospheric activity varies as a function of", "mass and rotation at different age. We measured excess equivalent", "widths of H{alpha}, H{beta}, and CaII K based on estimated", "chromospheric contributions from old and inactive field dwarfs, and", "excess luminosities are obtained by normalizing bolometric luminosity,", "for more than 700 late-type stars in these open clusters. Results", "indicate two activity sequences in cool spot coverage and H{alpha}", "excess emission among GK dwarfs in Pleiades and M dwarfs in Praesepe", "and Hyades, paralleling with well-known rotation sequences. A weak", "dependence of chromospheric emission on rotation exists among", "ultrafast rotators in saturated regime with Rossby number Ro<=0.1. In", "the unsaturated regime, chromospheric and coronal emission show", "similar dependence on Ro, but with a shift towards larger Ro,", "indicating chromospheric emission gets easily saturated than coronal", "emission, and/or convective turnover time-scales based on X-ray data", "do not work well with chromospheric emission. More interestingly, our", "analysis shows fully convective slow rotators obey the", "rotation-chromospheric activity relation similar to hotter stars,", "confirming the previous finding. We found correlations among H{alpha},", "H{beta}, and CaII K emissions, in which H{alpha} losses are more", "important than CaII K for cooler and more active stars. In addition, a", "weak correlation is seen between chromospheric emission and", "photospheric activity that shows dependence on stellar spectral type", "and activity level, which provides some clues on how spot", "configuration varies as a function of mass and activity level."], "description": ["We have selected four nearby open clusters with a range of ages from", "100 to 700Myr (Pleiades, M34, Praesepe, and Hyades), and retrieved", "the available spectra of good quality from LAMOST DR3 archive."], "type": ["OC"], "data": "", "date_update": "13-Apr-2021", "tables": [{"name": "tablef1.dat", "desc": "Measurements for stars in Pleiades ", "columns": [{"name": "Name", "desc": "Star designation "}, {"name": "Teff", "desc": "Effective (quiescent) temperature "}, {"name": "EWHa", "desc": "?=-9999 Equivalent width of Halpha line "}, {"name": "EWHb", "desc": "?=-9999 Equivalent width of Hbeta line "}, {"name": "EWCaK", "desc": "?=-9999 Equivalent width of Ca II K line "}, {"name": "EW'Ha", "desc": "?=-9999 Excess equivalent width of Halpha line "}, {"name": "EW'Hb", "desc": "?=-9999 Excess equivalent width of Hbeta line "}, {"name": "EW'CaK", "desc": "?=-9999 Excess equivalent width of Ca II K line "}, {"name": "R'Ha", "desc": "?=-9999 Fractional excess luminosity of Halpha (1)"}, {"name": "R'Hb", "desc": "?=-9999 Fractional excess luminosity of Hbeta (1)"}, {"name": "R'CaK", "desc": "?=-9999 Fractional excess luminosity of Ca IIK (1)"}, {"name": "fs", "desc": "?=-9999 Spot filling factor (based on TiO2) "}, {"name": "Tspot", "desc": "?=-9999 Spot temperature "}, {"name": "multi", "desc": "Photometric single/binary member/non-member (2) "}, {"name": "RAdeg", "desc": "Right ascension J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}]}, {"name": "tablef2.dat", "desc": "Measurements for stars in M34 ", "columns": [{"name": "Name", "desc": "Star designation "}, {"name": "Teff", "desc": "Effective (quiescent) temperature "}, {"name": "EWHa", "desc": "?=-9999 Equivalent width of Halpha line "}, {"name": "EWHb", "desc": "?=-9999 Equivalent width of Hbeta line "}, {"name": "EWCaK", "desc": "?=-9999 Equivalent width of Ca II K line "}, {"name": "EW'Ha", "desc": "?=-9999 Excess equivalent width of Halpha line "}, {"name": "EW'Hb", "desc": "?=-9999 Excess equivalent width of Hbeta line "}, {"name": "EW'CaK", "desc": "?=-9999 Excess equivalent width of Ca II K line "}, {"name": "R'Ha", "desc": "?=-9999 Fractional excess luminosity of Halpha (1)"}, {"name": "R'Hb", "desc": "?=-9999 Fractional excess luminosity of Hbeta (1)"}, {"name": "R'CaK", "desc": "?=-9999 Fractional excess luminosity of Ca IIK (1)"}, {"name": "fs", "desc": "?=-9999 Spot filling factor (based on TiO2) "}, {"name": "Tspot", "desc": "?=-9999 Spot temperature "}, {"name": "multi", "desc": "Photometric single/binary member/non-member (2) "}, {"name": "RAdeg", "desc": "Right ascension J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}]}, {"name": "tablef3.dat", "desc": "Measurements for stars in Praesepe ", "columns": [{"name": "Name", "desc": "Star designation "}, {"name": "Teff", "desc": "Effective (quiescent) temperature "}, {"name": "EWHa", "desc": "?=-9999 Equivalent width of Halpha line "}, {"name": "EWHb", "desc": "?=-9999 Equivalent width of Hbeta line "}, {"name": "EWCaK", "desc": "?=-9999 Equivalent width of Ca II K line "}, {"name": "EW'Ha", "desc": "?=-9999 Excess equivalent width of Halpha line "}, {"name": "EW'Hb", "desc": "?=-9999 Excess equivalent width of Hbeta line "}, {"name": "EW'CaK", "desc": "?=-9999 Excess equivalent width of Ca II K line "}, {"name": "R'Ha", "desc": "?=-9999 Fractional excess luminosity of Halpha (1)"}, {"name": "R'Hb", "desc": "?=-9999 Fractional excess luminosity of Hbeta (1)"}, {"name": "R'CaK", "desc": "?=-9999 Fractional excess luminosity of Ca IIK (1)"}, {"name": "fs", "desc": "?=-9999 Spot filling factor (based on TiO2) "}, {"name": "Tspot", "desc": "?=-9999 Spot temperature "}, {"name": "multi", "desc": "Photometric single/binary member/non-member (2) "}, {"name": "RAdeg", "desc": "Right ascension J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}]}, {"name": "tablef4.dat", "desc": "Measurements for stars in Hyades ", "columns": [{"name": "Name", "desc": "Star designation "}, {"name": "Teff", "desc": "Effective (quiescent) temperature "}, {"name": "EWHa", "desc": "?=-9999 Equivalent width of Halpha line "}, {"name": "EWHb", "desc": "?=-9999 Equivalent width of Hbeta line "}, {"name": "EWCaK", "desc": "?=-9999 Equivalent width of Ca II K line "}, {"name": "EW'Ha", "desc": "?=-9999 Excess equivalent width of Halpha line "}, {"name": "EW'Hb", "desc": "?=-9999 Excess equivalent width of Hbeta line "}, {"name": "EW'CaK", "desc": "?=-9999 Excess equivalent width of Ca II K line "}, {"name": "R'Ha", "desc": "?=-9999 Fractional excess luminosity of Halpha (1)"}, {"name": "R'Hb", "desc": "?=-9999 Fractional excess luminosity of Hbeta (1)"}, {"name": "R'CaK", "desc": "?=-9999 Fractional excess luminosity of Ca IIK (1)"}, {"name": "fs", "desc": "?=-9999 Spot filling factor (based on TiO2) "}, {"name": "Tspot", "desc": "?=-9999 Spot temperature "}, {"name": "multi", "desc": "Photometric single/binary member/non-member (2) "}, {"name": "RAdeg", "desc": "Right ascension J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_1213"}} {"id": "J/MNRAS/476/1213", "title_cds": "Ages for stars in 19 clusters", "title_create": "Getman+, 2018", "year": "2018", "author": "Getman K.V., Feigelson E.D., Kuhn M.A., Bate M.R., Broos P.S., Garmire G.P.", "title_pub": "Intracluster age gradients in numerous young stellar clusters.", "first_author": "Getman K.V.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476.1213G"], "see_also": ["J/ApJ/787/108 : Age estimates for massive SFR stellar populations", "J/ApJ/787/109 : Age estimates for NGC 2024 and ONC stars (Getman+, 2014)", "J/ApJS/209/32 : Probable young stars in the MYStIX project (Broos+, 2013)", "J/ApJS/229/28 : SFiNCs: X-ray, IR and membership catalogs (Getman+, 2017)"], "keyword_cds": "Clusters, open ; Stars, ages", "keyword_pub": "stars: early-type - stars: formation - stars: pre-main sequence - open clusters and associations: general - infrared: stars - X-rays: stars", "abstract": ["The pace and pattern of star formation leading to rich young stellar", "clusters is quite uncertain. In this context, we analyse the spatial", "distribution of ages within 19 young (median t<=3Myr on the Siess et", "al. time-scale), morphologically simple, isolated, and relatively rich", "stellar clusters. Our analysis is based on young stellar object (YSO)", "samples from the Massive Young Star-Forming Complex Study in Infrared", "and X-ray and Star Formation in Nearby Clouds surveys, and a new", "estimator of pre-main sequence (PMS) stellar ages, Age_JX_, derived", "from X-ray and near-infrared photometric data. Median cluster ages are", "computed within four annular subregions of the clusters. We confirm", "and extend the earlier result of Getman et al. (2014ApJ...787..108G,", "Cat. J/ApJ/787/108; 2014ApJ...787..109G. Cat. J/ApJ/787/109): 80 per", "cent of the clusters show age trends where stars in cluster cores are", "younger than in outer regions. Our cluster stacking analyses establish", "the existence of an age gradient to high statistical significance in", "several ways. Time-scales vary with the choice of PMS evolutionary", "model; the inferred median age gradient across the studied clusters", "ranges from 0.75 to 1.5Myr/pc. The empirical finding reported in the", "present study - late or continuing formation of stars in the cores of", "star clusters with older stars dispersed in the outer regions - has a", "strong foundation with other observational studies and with the", "astrophysical models like the global hierarchical collapse model of", "Vazquez-Semadeni et al. (2017MNRAS.467.1313V)."], "description": ["Among the 141 MYStIX (Kuhn et al., 2014ApJ...787..107K, Cat.", "J/ApJ/787/107) and 52 SFiNCs (Getman et al., 2018, MNRAS, in prep.)", "clusters that are identified by an objective likelihood-based", "statistical procedure (Kuhn et al. 2014ApJ...787..107K), we select the", "ones that : (1) have a simple morphology (a single dense core", "surrounded by a sparser halo); (2) are relatively isolated (without or", "with only weak secondary sub-clusters present in their vicinity); 3)", "and have a relatively high number of stars with available age", "estimates. A total of 19 clusters, with 2487 AgeJX stars, satisfy", "these criteria."], "type": ["CCC"], "data": "", "date_update": "13-Apr-2021", "tables": [{"name": "table2.dat", "desc": "AgeJX Stars. All MYStIX and SFiNCs stars with available age estimates across the 19 clusters of interest", "columns": [{"name": "Region", "desc": "Star-forming region name "}, {"name": "Source", "desc": "Source name (HHMMSS.ss+DDMMSS.sa) (1) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "AgeJX", "desc": "Stellar age estimated using the AgeJX method of Getman et al. (2014ApJ...787..108G)"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_1224"}} {"id": "J/MNRAS/476/1224", "title_cds": "Starspot variability as X-ray radiation proxy", "title_create": "Arkhypov+, 2018", "year": "2018", "author": "Arkhypov O.V., Khodachenko M.L., Lammer H., Gudel M., Luftinger T., Johnstone C.P.", "title_pub": "Starspot variability as an X-ray radiation proxy.", "first_author": "Arkhypov O.V.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476.1224A"], "see_also": ["V/133 : Kepler Input Catalog (Kepler Mission Team, 2009)", "J/ApJ/743/48 : Stars with rotation periods & X-ray luminosities (Wright+ 2011)", "J/A+A/557/L10 : Rotation periods of 12000 Kepler stars (Nielsen+, 2013)", "J/ApJS/211/24 : Rotation periods of Kepler MS stars (McQuillan+, 2014)", "J/ApJS/229/30 : Q1-17 Kepler targets revised stellar properties (Mathur+, 2017)"], "keyword_cds": "Stars, variable ; X-ray sources ; Effective temperatures", "keyword_pub": "stars: activity - starspots - ultraviolet: stars - X-rays: stars", "abstract": ["Stellar X-ray emission plays an important role in the study of", "exoplanets as a proxy for stellar winds and as a basis for the", "prediction of extreme ultraviolet (EUV) flux, unavailable for direct", "measurements, which in their turn are important factors for the", "mass-loss of planetary atmospheres. Unfortunately, the detection", "thresholds limit the number of stars with the directly measured X-ray", "fluxes. At the same time, the known connection between the sunspots", "and X-ray sources allows using of the starspot variability as an", "accessible proxy for the stellar X-ray emission. To realize this", "approach, we analysed the light curves of 1729 main-sequence stars", "with rotation periods 0.5)", "desc": "Our active index, averaged over a whole light curve, A_1_^2^"}, {"name": "e_log()", "desc": "Estimated error of log() "}, {"name": "(B-V)o", "desc": "Colour index according to the transformation Teff-->(B-V)o in equation (1)"}, {"name": "tauMLT", "desc": "Turnover time according to equation (4) in Noyes et al. (1984ApJ...279..763N)"}, {"name": "log(Rx)reg", "desc": "Logarithm of the ratio of X-ray to bolometric luminosities which are estimated from equations (6)-(8) of the paper"}, {"name": "log(Lx)reg", "desc": "Logarithm of the predicted X-ray luminosity using equations (10)-(14) of the paper"}]}, {"name": "table3.dat", "desc": "Parameters and predictions for stars in the catalogue by Wright et al. (2011ApJ...743...48W, Cat. J/ApJ/743/48)", "columns": [{"name": "RAdeg", "desc": "?=- Right ascension for epoch 2000.0 (1) "}, {"name": "DEdeg", "desc": "?=- Declination for epoch 2000.0 (1) "}, {"name": "Field", "desc": "Afiliation "}, {"name": "Teff", "desc": "Effective temperature (1) "}, {"name": "P", "desc": "Period (1) "}, {"name": "tauMLT", "desc": "Turnover time (2) "}, {"name": "log(Rx)reg", "desc": "Logarithm of the ratio of X-ray to bolometric luminosities which are estimated from equations (6)-(8) of the paper"}, {"name": "log(Lx)reg", "desc": "Logarithm of the predicted X-ray luminosity using equations (10)-(14) of the paper"}, {"name": "log(Lx)", "desc": "Logarithm of the measured X-ray luminosity (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_1765"}} {"id": "J/MNRAS/476/1765", "title_cds": "MaNGA E and S galaxies properties", "title_create": "Li+, 2018", "year": "2018", "author": "Li H., Mao S., Cappellari M., Ge J., Long R.J., Li R., Mo H.J., Li C., Zheng Z., Bundy K., Thomas D., Brownstein J.R., Roman Lopes A., Law D.R., Drory N.", "title_pub": "SDSS-IV MaNGA: global stellar population and gradients for about 2000 early-type and spiral galaxies on the mass-size plane.", "first_author": "Li H.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476.1765L"], "see_also": ["J/AJ/154/86 : MaNGA catalog, DR15 (Wake+, 2017)"], "keyword_cds": "Galaxies ; Morphology ; Velocity dispersion", "keyword_pub": "galaxies: evolution - galaxies: formation - galaxies: kinematics and dynamics - galaxies: structure", "abstract": ["We perform full spectrum fitting stellar population analysis and Jeans", "Anisotropic modelling of the stellar kinematics for about 2000", "early-type galaxies (ETGs) and spiral galaxies from the MaNGA DR14", "sample. Galaxies with different morphologies are found to be located", "on a remarkably tight mass plane which is close to the prediction of", "the virial theorem, extending previous results for ETGs. By examining", "an inclined projection ('the mass-size' plane), we find that spiral", "and early-type galaxies occupy different regions on the plane, and", "their stellar population properties (i.e. age, metallicity, and", "stellar mass-to-light ratio) vary systematically along roughly the", "direction of velocity dispersion, which is a proxy for the bulge", "fraction. Galaxies with higher velocity dispersions have typically", "older ages, larger stellar mass-to-light ratios and are more metal", "rich, which indicates that galaxies increase their bulge fractions as", "their stellar populations age and become enriched chemically. The age", "and stellar mass-to-light ratio gradients for low-mass galaxies in our", "sample tend to be positive (centre=2x 10^11^M_{sun}_, where slow rotator ETGs", "start dominating, have much flatter gradients. This may be due to", "differences in their evolution histories, e.g. mergers."], "description": ["The galaxies in this study are from the MaNGA Product Launch 5 (MPL5)", "catalogue (internal release, nearly identical to SDSS-DR14, Abolfathi", "et al., 2018ApJS..235...42A), which includes 2778 galaxies of", "different morphologies.", "We perform Jeans Anisotropic modelling (JAM, Cappellari,", "2008MNRAS.390...71C) for all the galaxies in our sample."], "type": ["CCC"], "data": "", "date_update": "23-Apr-2021", "tables": [{"name": "tablea1.dat", "desc": "Properties of all the galaxies in the sample ", "columns": [{"name": "MaNGA", "desc": "MaNGA ID of the galaxy "}, {"name": "Morph", "desc": "[SE] Galaxy morphology, E for ETGs, S for spiral galaxies"}, {"name": "logsigmae", "desc": "Velocity dispersion within 1Re, as defined in equation (2) in the paper"}, {"name": "logM1/2", "desc": "Enclosed total mass within three-dimensional half-light radius from dynamical model"}, {"name": "logRe", "desc": "Major axis of the half-light isophote for the best-fitting MGE model"}, {"name": "logAge", "desc": "Mean logAge within the effective radius "}, {"name": "[Z/H]", "desc": "Mean metallicity within the effective radius"}, {"name": "logM*/L", "desc": "Mean stellar mass-to-light ratio within the effective radius in SDSS r band"}, {"name": "DlogAge", "desc": "Age gradient "}, {"name": "D[Z/H]", "desc": "Metallicity gradient "}, {"name": "DlogM*/L", "desc": "Stellar mass-to-light ratio gradient in SDSS r band"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_2501"}} {"id": "J/MNRAS/476/2501", "title_cds": "AGN short time-scale optical variability", "title_create": "Aranzana+, 2018", "year": "2018", "author": "Aranzana E., Kording E., Uttley P., Scaringi S., Bloemen S.", "title_pub": "Short time-scale optical variability properties of the largest AGN sample observed with Kepler/K2.", "first_author": "Aranzana E.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476.2501A"], "see_also": ["VII/283 : The Million Quasars (Milliquas) catalog (6.3) (Flesch, 2019)"], "keyword_cds": "Active gal. nuclei ; QSOs ; Redshifts", "keyword_pub": "accretion, accretion discs - galaxies: active - quasars: general - quasars: supermassive black holes", "abstract": ["We present the first short time-scale (~ hours to days) optical", "variability study of a large sample of active galactic nuclei (AGNs)", "observed with the Kepler/K2 mission. The sample contains 252 AGN", "observed over four campaigns with ~30 min cadence selected from", "the Million Quasar Catalogue with R magnitude <19. We performed time", "series analysis to determine their variability properties by means of", "the power spectral densities (PSDs) and applied Monte Carlo techniques", "to find the best model parameters that fit the observed power spectra.", "A power-law model is sufficient to describe all the PSDs of our", "sample. A variety of power-law slopes were found indicating that there", "is not a universal slope for all AGNs. We find that the rest-frame", "amplitude variability in the frequency range of 6x10^-6^-10^-4^Hz", "varies from 1 to 10 per cent with an average of 1.7 per cent. We explore", "correlations between the variability amplitude and key parameters of", "the AGN, finding a significant correlation of rest-frame short-term", "variability amplitude with redshift. We attribute this effect to the", "known 'bluer when brighter' variability of quasars combined with the", "fixed bandpass of Kepler data. This study also enables us to", "distinguish between Seyferts and blazars and confirm AGN candidates.", "For our study, we have compared results obtained from light curves", "extracted using different aperture sizes and with and without", "detrending. We find that limited detrending of the optimal photometric", "precision light curve is the best approach, although some systematic", "effects still remain present."], "description": ["In this work, we presented a catalogue of the optical variability", "properties in the high-frequency domain of a large sample of 252", "sources. Using light curves of extremely high quality from Kepler/K2,", "we studied their power spectra by using the PSRESP Monte Carlo method."], "type": ["CCC"], "data": "", "date_update": "26-Apr-2021", "tables": [{"name": "tableb1.dat", "desc": "Parameters for all the MQ AGN analysed in this work ", "columns": [{"name": "EPIC", "desc": "EPIC number "}, {"name": "n_EPIC", "desc": "[*] Note on EPIC (1) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Type", "desc": "Type of AGN (2) "}, {"name": "b'mag", "desc": "b' magnitude (2) "}, {"name": "r'mag", "desc": "r' magnitude (2) "}, {"name": "z", "desc": "Redshift (2) "}, {"name": "betaopt", "desc": "Negative power-law index of the simulated PSD for the 'optimal' aperture"}, {"name": "---", "desc": "[+] "}, {"name": "E_betaopt", "desc": "Error on betaopt (upper value) "}, {"name": "---", "desc": "[-] "}, {"name": "e_betaopt", "desc": "Error on betaopt (lower value) "}, {"name": "betaPRF9", "desc": "Negative power-law index of the simulated PSD for the PRF aperture"}, {"name": "---", "desc": "[+] "}, {"name": "E_betaPRF9", "desc": "Error on betaPRF9 (upper value) "}, {"name": "---", "desc": "[-] "}, {"name": "e_betaPRF9", "desc": "Error on betaPRF9 (lower value) "}, {"name": "betadet", "desc": "Negative power-law index of the simulated PSD for the 'optimal' detrended light curves"}, {"name": "---", "desc": "[+] "}, {"name": "E_betadet", "desc": "Error on betadet (upper value) "}, {"name": "---", "desc": "[-] "}, {"name": "e_betadet", "desc": "Error on betadet (lower value) "}, {"name": "Norm", "desc": "Best normalisation "}, {"name": "Noise", "desc": "Poisson noise level obtained in the minimisation"}, {"name": "Prob", "desc": "Acceptance probability for the model "}, {"name": "sigmaobs", "desc": "?=- Fractional rms measured in the observed power spectra"}, {"name": "sigmalit", "desc": "Fractional rms measured in the simulated power spectra"}, {"name": "sigmarestfit", "desc": "Rest-frame fractional rms "}, {"name": "e_sigmarestfit", "desc": "Rms uncertainty on sigmarestfit "}, {"name": "Lbol", "desc": "Estimated bolometric luminosity "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_MNRAS_476_2717"}} {"id": "J/MNRAS/476/2717", "title_cds": "AT20G-MWACS catalogue", "title_create": "Harvey+, 2018", "year": "2018", "author": "Harvey V.M., Franzen T., Morgan J., Seymour N.", "title_pub": "A novel approach for characterizing broad-band radio spectral energy distributions.", "first_author": "Harvey V.M.", "ref_biblio": [""], "bibcode": ["2018MNRAS.476.2717H"], "see_also": ["VIII/98 : 180MHz Murchison Commissioning Survey (MWACS)", "J/MNRAS/402/2403 : Australia Telescope 20GHz Survey Catalog, AT20G"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio", "keyword_pub": "methods: analytical - techniques: photometric - catalogues - radio continuum: galaxies", "abstract": ["We present a new broad-band radio frequency catalogue across", "0.12GHz<={nu}<=20GHz created by combining data from the Murchison", "Widefield Array Commissioning Survey, the Australia Telescope 20GHz", "survey, and the literature. Our catalogue consists of 1285 sources", "limited by S_20GHz_>40mJy at 5{sigma}, and contains flux density", "measurements (or estimates) and uncertainties at 0.074, 0.080, 0.119,", "0.150, 0.180, 0.408, 0.843, 1.4, 4.8, 8.6, and 20GHz. We fit a", "second-order polynomial in log-log space to the spectral energy", "distributions of all these sources in order to characterize their", "broad-band emission. For the 994 sources that are well described by a", "linear or quadratic model we present a new diagnostic plot arranging", "sources by the linear and curvature terms. We demonstrate the", "advantages of such a plot over the traditional radio colour-colour", "diagram. We also present astrophysical descriptions of the sources", "found in each segment of this new parameter space and discuss the", "utility of these plots in the upcoming era of large area, deep,", "broad-band radio surveys."], "description": ["We have created a new source catalogue, AT20G-MWACS, by building on", "the solid high-frequency foundation of the AT20G survey and combining", "it with the results of a fresh run of source finding algorithms on the", "original MWACS images. The catalogue covers an area of 5760deg^2^ and", "contains 1285 sources."], "type": ["CCC"], "data": "", "date_update": "26-Apr-2021", "tables": [{"name": "catalog.dat", "desc": "AT20G-MWACS catalogue ", "columns": [{"name": "AT20G", "desc": "AT20G IAU designation (JHHMMSS+DDMMSS) "}, {"name": "RAJ2000", "desc": "AT20G right ascension (J2000) "}, {"name": "DEJ2000", "desc": "AT20G declination (J2000) "}, {"name": "S20G", "desc": "?=- AT20G Peak brightness at 20GHz "}, {"name": "e_S20G", "desc": "?=- Uncertainty on S20G with an additional 10% of S20G added"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASJ_55_771"}} {"id": "J/PASJ/55/771", "title_cds": "Hdelta-strong galaxies in SDSS", "title_create": "Goto+, 2003", "year": "2003", "author": "Goto T., Nichol R.C., Okamura S., Sekiguchi M., Miller C.J., Bernardi M., Hopkins A., Tremonti C., Connolly A., Castander F.J., Brinkmann J., Fukugita M., Harvanek M., Ivezic Z., Kleinman S.J., Krzesinski J., Long D., Loveday J., Neilsen E.H., Newman P.R., Nitta A., Snedden S.A., Subbarao M.", "title_pub": "Hdelta-strong galaxies in the Sloan Digital Sky Survey : I. The Catalog.", "first_author": "Goto T.", "ref_biblio": [""], "bibcode": ["2003PASJ...55..771G"], "keyword_cds": "", "keyword_pub": "galaxies: evolution - galaxies: interaction - galaxies: peculiar - galaxies: starburst", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/pasj/55.4.771"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASJ_59_245"}} {"id": "J/PASJ/59/245", "title_cds": "High-Resolution and S/N Spectrum Atlas of Vega", "title_create": "Takeda+, 2006", "year": "2006", "author": "Takeda Y., Kawanomoto S., and Ohishi N.", "title_pub": "High-Resolution and High-S/N Spectrum Atlas of Vega", "first_author": "Takeda Y.", "ref_biblio": [""], "bibcode": ["2007PASJ...59..245T"], "see_also": ["J/ApJ/380/223 : Metallic line profiles of the AO V star VEGA", "J/A&A/420/183 : S4N: A spectroscopic survey of stars in the solar", "J/PASP/116/693 : The ELODIE Archive (Moultaka+ 2004)", "J/other/PBeiO/33.34 : The high resolution spectrum of Vega.I. Spectral", "J/other/PBeiO/33.58 : The high resolution spectrum of Vega.II. Spectral", "J/PASJ/57/13 : High-Dispersion Spectra Collection of Nearby F--K Stars", "at Okayama Astrophysical Observatory: A Basis for"], "keyword_cds": "Abundances ; Atlases ; Spectroscopy ; Stars, early-type ; Stars, A-type ; Line Profiles", "keyword_pub": "atlases - line: profiles - stars: early-type - stars: individual({alpha}Lyr, {alpha}Leo) - techniques: spectroscopic", "abstract": ["We present a digital spectral atlas of Vega covering from", "violet to near-IR region (~3900-8800A), which has so high", "resolution (R~100000) and high signal-to-noise ratio", "(typically ~1000-2000 on the average) as to allow a detailed", "line-profile analysis. In addition, theoretically simulated", "spectra and lists of lines predicted to have appreciable", "strengths are also provided, which may be useful for identifying", "or searching lines on the atlas. Besides, the spectra of", "Regulus (a representative rapid rotator) obtained at the same", "night are appended as a reference of telluric lines."], "description": ["The data contained in the five directories (\"fitsfiles\",", "\"finalspectra\", \"synthespec\", \"lineprediction\", and \"appendix\")", "constitute the electronic data table of our paper \"High-Resolution", "and High-S/N Spectrum Atlas of Vega\" published in PASJ, Vol. 59,", "pp245-261 (2007)."], "object": ["18 36 56.3 +38 47 01 {alpha} Lyr = HD 172167", "10 08 22.3 +11 58 02 {alpha} Leo = HD 87901"], "doi_pub": ["10.1093/pasj/59.1.245"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "obslog_vega.dat", "desc": "basic data of our Vega observations ", "columns": [{"name": "frameNo", "desc": "[1-9hb] serial number of each spectral frame "}, {"name": "region", "desc": "[bgri] wavelength region indicator "}, {"name": "date", "desc": "date of observation "}, {"name": "UT", "desc": "observation time (in UT) at mid-exposure "}, {"name": "secz", "desc": "air mass at the time of observation "}, {"name": "texp", "desc": "exposure time (in second) "}, {"name": "count", "desc": "mean spectrum count "}]}, {"name": "fitsfiles/*", "desc": "FITS files of spectrum of Vega ", "columns": []}, {"name": "obslog_regu.dat", "desc": "basic data of our Regulus observations ", "columns": [{"name": "frameNo", "desc": "[1-9hb] serial number of each spectral frame "}, {"name": "region", "desc": "[bgri] wavelength region indicator "}, {"name": "date", "desc": "date of observation "}, {"name": "UT", "desc": "observation time (in UT) at mid-exposure "}, {"name": "secz", "desc": "air mass at the time of observation "}, {"name": "texp", "desc": "exposure time (in second) "}, {"name": "count", "desc": "mean spectrum count "}]}, {"name": "appendix/*", "desc": "FITS files of spectrum of Regulus ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASJ_60_1267"}} {"id": "J/PASJ/60/1267", "title_cds": "Old open clusters photometric data", "title_create": "Hasegawa+, 2008", "year": "2008", "author": "Hasegawa T., Sakamoto T., Malasan H.L.", "title_pub": "New photometric data of old open clusters. II. A dataset for 36 clusters.", "first_author": "Hasegawa T.", "ref_biblio": [""], "bibcode": ["2008PASJ...60.1267H"], "see_also": ["J/PASJ/56/295 : BVIc photometry of old open clusters (Hasegawa+, 2004)"], "keyword_cds": "Clusters, open ; Photometry, UBVRI", "keyword_pub": "Galaxy: evolution - Galaxy: open clusters and associations: general - Galaxy: open clusters and associations: HR diagram - Galaxy: structure", "abstract": ["We present new photometric data on 36 old open clusters using the", "65-cm telescope at Gunma Astronomical Observatory. This dataset is a", "continuation of photometric data of old open clusters (Hasegawa et al.", "2004, Cat. ) collected mainly in the antigalactic", "center region. By constructing a color-magnitude diagram, we inspected", "the main sequence and (if richly populated) red-clump stars to", "evaluate the cluster parameters, that is, the age, distance, and", "reddening, by applying an isochrone provided by the Padova group. Now,", "49 old clusters have consistently measured parameters (36 clusters in", "this study and 13 from Hasegawa et al. 2004, Cat. ).", "The clusters are exclusively older than the Hyades cluster, and the", "age is distributed in the range 0.6-5.0Gyr."], "description": ["Optical observations were conducted using the 65-cm telescope (F/12.0,", "f=7800mm) at Gunma Astronomical Observatory. Data were collected", "between 2000 December 4 and 2006 December 22, mostly in 2004 and 2006."], "type": ["OC"], "doi_pub": ["10.1093/pasj/60.6.1267"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "List of open clusters observed in this study ", "columns": [{"name": "Name", "desc": "Cluster name "}, {"name": "RAh", "desc": "Revised central right ascension (J2000.0) "}, {"name": "RAm", "desc": "Revised central right ascension (J2000.0) "}, {"name": "RAs", "desc": "Revised central right ascension (J2000.0) "}, {"name": "DE-", "desc": "Revised central declination sign (J2000.0) "}, {"name": "DEd", "desc": "Revised central declination (J2000.0) "}, {"name": "DEm", "desc": "Revised central declination (J2000.0) "}, {"name": "GLON", "desc": "Revised central Galactic longitude "}, {"name": "GLAT", "desc": "Revised central Galactic latitude "}, {"name": "Morph", "desc": "Morphological parameters given in COCD; contrast (1,2), richness (m,p), and detachment (I-IIII) (1)"}]}, {"name": "table2.dat", "desc": "Log of optical photometric observations using the 65-cm telescope", "columns": [{"name": "Name", "desc": "Cluster name "}, {"name": "Cam", "desc": "Adopted camera system "}, {"name": "FWHM", "desc": "Typical seeing size at I-band "}, {"name": "TexpB", "desc": "Total exposure time in B band "}, {"name": "TexpV", "desc": "Total exposure time in V band "}, {"name": "TexpI", "desc": "Total exposure time in I band "}, {"name": "Bmaglim", "desc": "Limiting B magnitude "}, {"name": "Vmaglim", "desc": "Limiting V magnitude "}, {"name": "Imaglim", "desc": "Limiting I magnitude "}]}, {"name": "table4.dat", "desc": "Parameters of the open clusters, as determined in this study", "columns": [{"name": "Name", "desc": "Cluster name "}, {"name": "Age", "desc": "Age (Isochrone fitting) "}, {"name": "Z", "desc": "Assumed metallicity Z (Isochrone fitting) "}, {"name": "E(V-I)", "desc": "V-I colour excess (Isochrone fitting) "}, {"name": "(m-M)0", "desc": "Deredenned distance modulus (Isochrone fitting) "}, {"name": "rGC", "desc": "Galactocentric distance (Isochrone fitting) (1) "}, {"name": "z", "desc": "Distance from the galactic plane (Isochrone fitting)"}, {"name": "l_E(V-I)D", "desc": "[~] Limit flag on E(V-I)D "}, {"name": "E(V-I)D", "desc": "V-I color excess quoted from the DIRBE/ISSA "}, {"name": "dE(V-I)D", "desc": "Differential reddening, which is the peak-to-peak difference of the DIRBE/ISSA color excess in the 10' box area"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASJ_65_8"}} {"id": "J/PASJ/65/8", "title_cds": "Catalog of SDSS quasar absorption redshift", "title_create": "Qin+, 2013", "year": "2013", "author": "Qin Y.-P., Chen Z.-F., Lu L.-Z., Huang W.-R., Li M.-S., Li G.-Q., Wang M.P., Zhong Y.-Q., Wen S.-Q., Liao R.-H., Ye F.", "title_pub": "Catalog of SDSS quasar absorption redshifts measured from MgII absorption lines. I. For sources with z_em_ <= 0.8.", "first_author": "Qin Y.-P.", "ref_biblio": [""], "bibcode": ["2013PASJ...65....8Q"], "keyword_cds": "", "keyword_pub": "line: identification - quasars: absorption lines - quasars: general", "abstract": ["We are going to analyze the whole Sloan Digital Sky Survey (SDSS)", "quasar spectra by visually identifying Mg II absorption line systems", "one by one. In this paper, we limit our analysis to quasars with $", "z_em_<=0.8, which leaves 8006 quasars in total. Based on this, we are", "able to present the first catalog of these redshifts (in the interval", "of 0.36=0.3{AA}, and about 71% (2957/4158) of the absorbers", "have W__r{lambda}2803>=0.3{AA}, showing that the main portion of our", "catalog is likely to be occupied by strong absorbers."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/pasj/65.1.8"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASJ_71_62"}} {"id": "J/PASJ/71/62", "title_cds": "Short Title", "title_create": "Gao, 2019", "year": "2019", "author": "Gao X.-H.", "title_pub": "Membership and fundamental parameters of the intermediate-age open clusters NGC 2281 and NGC 2539 based on Gaia-DR2.", "first_author": "Gao X.-H.", "ref_biblio": [""], "bibcode": ["2019PASJ...71...62G"], "keyword_cds": "", "keyword_pub": "", "abstract": ["This paper presents an investigation on the two intermediate-age open", "clusters NGC 2281 and NGC 2539 based on Gaia Data Release 2", "(Gaia-DR2). A combined machine-learning method is used to identify", "likely cluster members of the two clusters, taking into account the", "astrometric and photometric data of Gaia-DR2. It is found that NGC", "2281 and NGC 2539 each have more than 600 likely cluster members,", "which are highly suitable for further investigation of the fundamental", "parameters of the two clusters. Robust estimates of the distances,", "proper motions, and radial velocities for the two clusters are", "obtained via a Monte Carlo simulation technique. NGC 2281 is found to", "have a distance of 522+/-12pc, a proper motion of", "(, =(\u22122.94+/-0.014, -8.344+/-0.014)mas/yr,", "and a radial velocity of +20.0+/-0.7km/s. The distance, proper motion,", "and radial velocity of NGC 2539 are determined to be 1271+/-70pc,", "()=(-2.33+/-\u00b10.007, -0.583+/-0.006)mas/yr, and", "+29.6+/-0.4km/s, respectively. We find that NGC 2281 has a core radius", "of 8.89'+/-0.27' (1.3pc) and a limiting radius of 79.26'+/-2.86'", "(12.0pc). The core and limiting radius of NGC 2539 are determined to", "be 5.62'+/-0.28' (2.1pc) and 33.65'+/-1.96 (12.4pc), respectively. In", "addition, we find strong evidence for the existence of mass", "segregation in the two clusters."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1093/pasj/psz039"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASJ_72_43"}} {"id": "J/PASJ/72/43", "title_cds": "FUGIN. VII. Galactic plane HI clouds", "title_create": "Nakanishi+, 2020", "year": "2020", "author": "Nakanishi H., Fujita S., Tachihara K., et AL.", "title_pub": "FOREST unbiased Galactic plane imaging survey with the Nobeyama 45 m telescope (FUGIN). VII. Molecular fraction of HI clouds.", "first_author": "Nakanishi H.", "ref_biblio": [""], "bibcode": ["2020PASJ...72...43N"], "see_also": ["J/AJ/122/3155 : Peculiar HI cloud near galactic plane (Higgs+, 2001)", "J/ApJ/626/887 : HI clouds in Southern Galactic Plane Survey (Kavars+, 2005)", "J/ApJ/722/367 : HI clouds in Quadrant I of the Milky Way (Ford+, 2010)", "J/ApJ/770/L4 : HI clouds around the Galactic Center (McClure-Griffiths+, 2013)"], "keyword_cds": "Galactic plane ; Molecular clouds ; H I data ; Velocity dispersion", "abstract": ["We analyze molecular-gas formation in neutral atomic hydrogen (HI)", "clouds using the latest CO data, obtained from the FOREST (four-beam", "receiver system on the 45m telescope) unbiased Galactic plane imaging", "survey with the Nobeyama 45m telescope, and using HI data taken from", "the Very Large Array Galactic plane survey. We applied a dendrogram", "algorithm to the HI data cube to identify HI clouds, and we calculated", "the HI mass and molecular-gas mass by summing the CO line intensity", "within each HI cloud. On the basis of the results, we created a", "catalog of 5737 identified HI clouds with local standard of rest (LSR)", "velocity of VLSR<=-20km/s in galactic longitude and latitude ranges of", "20{deg}<=l<=50{deg} and -1{deg}<=b<=1{deg}, respectively. We found", "that most of the HI clouds are distributed within a Galactocentric", "distance of 16kpc, and most of them are in the cold neutral medium", "phase. In addition, we determined that the high-mass end of the HI", "mass function is fitted well with a power-law function with an index", "of 2.3. Although two sequences of self-gravitating and diffuse clouds", "are expected to appear in the M_tot_-M_H2_ diagram according to", "previous works based on a plane-parallel model, the observational data", "show only a single sequence with large scattering within these two", "sequences. This implies that most of the clouds are mixtures of these", "two types of clouds. Moreover, we suggest the following scenario of", "molecular-gas formation: an HI-dominant cloud evolved with increasing", "H2 mass along a path of M_H2_{prop.to}M^2^_tot_ by collecting diffuse", "gas before reaching and moving along the curves of the two sequences."], "description": ["We applied the dendrogram analysis to the VGPS HI data cube to create", "a catalog of HI clouds of the outer Galaxy, including the masses of", "H_2_ gas within each HI cloud, which were estimated by using FUGIN CO", "survey data."], "alias": ["[NFT2020]"], "type": ["OC"], "data": "", "date_update": "22-Apr-2021", "tables": [{"name": "table1.dat", "desc": "Identified HI clouds ", "columns": [{"name": "ID", "desc": "[1/5737] Sequential number "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic longitude "}, {"name": "VLSR", "desc": "LSR velocity "}, {"name": "D", "desc": "Heliocentric distance "}, {"name": "R", "desc": "Galactocentric distance "}, {"name": "Rmin", "desc": "Minor-axis radius "}, {"name": "Rmaj", "desc": "Major-axis radius "}, {"name": "PA", "desc": "[] Position angle "}, {"name": "sigma", "desc": "Velocity dispersion "}, {"name": "MHI", "desc": "HI mass "}, {"name": "e_MHI", "desc": "rms uncertainty on MHI "}, {"name": "MH2", "desc": "H_2_ mass "}, {"name": "e_MH2", "desc": "rms uncertainty on MH2 "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_102_865"}} {"id": "J/PASP/102/865", "title_cds": "Stars in the field of NGC 2353.", "title_create": "Fitzgerald+, 1990", "year": "1990", "author": "Fitzgerald M.P., Harris G.L.H., Reed B.C.", "title_pub": "The moderately young open cluster NGC 2353.", "first_author": "Fitzgerald M.P.", "ref_biblio": [""], "bibcode": ["1990PASP..102..865F"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/132711"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_108_o.277"}} {"id": "J/PASP/108/277", "title_cds": "Night-Sky High-Res Spectral Atlas of OH and O2", "title_create": "Osterbrock+ 1996", "year": "1996", "author": "Osterbrock D.E., Fulbright J.P., Martel A.R., Keane M.J, Trager S.C. and Basri G.", "title_pub": "Night-Sky High-Resolution Spectral Atlas of OH and O2 Emission Lines for Echelle Spectrograph Wavelength Calibration", "first_author": "Osterbrock D.E.", "ref_biblio": [""], "bibcode": ["1995PASP..108..277O"], "see_also": ["http://ucowww.ucsc.edu/~jfulb/OH.html : the original data distribution"], "keyword_cds": "Atomic and molecular data", "keyword_pub": "OH; O2", "description": ["This catalog provides a list of atmospheric OH and O2 lines that are", "useful for wavelength calibration of high resolution spectra.", "Tables of observed OH lines supplemented by calculated values from the", "literature, observed and calculated wavelengths for molecular oxygen", "(O2), atomic lines of O I and Na I and postscript files for all", "spectral regions with identifications from all the figures of the paper", "are given."], "date_update": "31-Jan-2000", "tables": [{"name": "table2.dat", "desc": "Observed OH Lines Not Listed in Abrams et al. (1994) ", "columns": [{"name": "trans", "desc": "OH transition nu'-nu\" "}, {"name": "ID", "desc": "OH line Identification "}, {"name": "lambda", "desc": "wavelength observed OH line "}]}, {"name": "table3.dat", "desc": "Calculated Wavelengths for O2 (0-1) ", "columns": [{"name": "ID1", "desc": "O2 line identification "}, {"name": "lambda1", "desc": "? calculated wavelength "}, {"name": "ID2", "desc": "O2 line identification "}, {"name": "lambda2", "desc": "? calculated wavelength "}]}, {"name": "table4.dat", "desc": "Atomic Lines ", "columns": [{"name": "ID", "desc": "Ion identification "}, {"name": "lambda", "desc": "wavelength of atomic night-sky lines "}]}, {"name": "tablea.dat", "desc": "Supplemental Table of OH Wavelengths (Abrams et al.) ", "columns": [{"name": "trans", "desc": "OH transition nu'-nu\" "}, {"name": "ID", "desc": "OH identification "}, {"name": "lambda", "desc": "wavelength from Abrams et al. (1994) "}]}, {"name": "figures.tar", "desc": "Postscript files for all figures ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_109_289"}} {"id": "J/PASP/109/289", "title_cds": "Emission lines in PNe", "title_create": "Kaler+ 1997", "year": "1997", "author": "Kaler J.B., Shaw R.A., Browning L.", "title_pub": "Title of the paper", "first_author": "Kaler J.B.", "ref_biblio": [""], "bibcode": ["1997PASP..109..289K\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/133887"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_110_1342"}} {"id": "J/PASP/110/1342", "title_cds": "Unusual objects in the SDSS", "title_create": "Krisciunas+ 1998", "year": "1998", "author": "Authors", "title_pub": "Title of the paper", "first_author": "Authors", "ref_biblio": [""], "bibcode": ["1998PASP..110.1342K\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/316264"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_111_221"}} {"id": "J/PASP/111/221", "title_cds": "Detection of O VII in PNe from IUE spectra", "title_create": "Feibelman, 1999", "year": "1999", "author": "Authors", "title_pub": "Title of the paper", "first_author": "Authors", "ref_biblio": [""], "bibcode": ["1999PASP..111..221F\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/316317"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_112_1008"}} {"id": "J/PASP/112/1008", "title_cds": "Near-infrared galaxy morphology atlas", "title_create": "Jarrett+, 2000", "year": "2000", "author": "Jarrett T.H.", "title_pub": "Near-infrared galaxy morphology atlas.", "first_author": "Jarrett T.H.", "ref_biblio": [""], "bibcode": ["2000PASP..112.1008J\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "James Marcout, Patricia Bauer [CDS]", "doi_pub": ["10.1086/316603"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_122_516"}} {"id": "J/PASP/122/516", "title_cds": "Hogg 12 and NGC 3590", "title_create": "Piatti+, 2010", "year": "2010", "author": "Piatti A.E., Claria J.J., Ahumada A.V.", "title_pub": "Hogg 12 and NGC 3590: a new open cluster binary system candidate.", "first_author": "Piatti A.E.", "ref_biblio": [""], "bibcode": ["2010PASP..122..516P"], "keyword_cds": "", "abstract": ["We have obtained CCD UBVI_KC_ photometry down to V~22.0 for the open", "clusters Hogg 12 and NGC 3590 and the fields surrounding them. Based", "on photometric and morphological criteria, as well as on the stellar", "density in the region, our evidence is sufficient to confirm that Hogg", "12 is a genuine open cluster. NGC 3590 was used as a control cluster.", "The color-magnitude diagrams of Hogg 12, cleaned from field star", "contamination, reveal that this is a solar metal content cluster,", "affected by E(B-V)=0.40+/-0.05, located at a heliocentric", "distance d=2.0+/-0.5kpc, and of an age similar to that of NGC 3590", "(t=30Myr). Both clusters are surprisingly small objects whose radii", "are barely ~1pc, andthey are separated in the sky by scarcely 3.6pc.", "These facts, added to their similar ages, reddenings, and", "metallicities, allow us to consider them a new open cluster binary", "system candidate. Of the 180 open cluster binary systems estimated to", "exist in the Galaxy, of which 27 are actually well known, Hogg 12 and", "NGC 3590 appear to be one of the two closest pairs."], "description": ["We obtained CCD images for Hogg 12 on the nights of 2000 27 December", "and 29 December with the UBVIKC filters and a 2048x2048pixel", "Tektronix CCD attached to the 0.9m telescope (scale 0.4\"/pixel)", "at Cerro Tololo Inter-American Observatory (CTIO) Chile."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1086/652501"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_81_804"}} {"id": "J/PASP/81/804", "title_cds": "Four southern photoelectric sequences", "title_create": "Fitzgerald+, 1969", "year": "1969", "author": "Fitzgerald M.P., Wilson W., Stegman J.E.", "title_pub": "Four southern photoelectric sequences.", "first_author": "Fitzgerald M.P.", "ref_biblio": [""], "bibcode": ["1969PASP...81..804F"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_86_829"}} {"id": "J/PASP/86/829", "title_cds": "Transmission grating spectra", "title_create": "Miller+ 1974", "year": "1974", "author": "Miller E.W., Graham J.A.", "title_pub": "Transmission grating spectra: a new search technique for faint blue stars.", "first_author": "Miller E.W.", "ref_biblio": [""], "bibcode": ["1974PASP...86..829M"], "keyword_cds": "Stars, blue", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "doi_pub": ["10.1086/129681"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PASP_96_707"}} {"id": "J/PASP/96/707", "title_cds": "Hyades lower main sequence", "title_create": "Duncan+, 1984", "year": "1984", "author": "Duncan D.K., Baliunas S.L., Noyes R.W., Vaughan A.H., Frazer J., Lanning H.H.", "title_pub": "Chromospheric emission and rotation of the Hyades lower main sequence.", "first_author": "Duncan D.K.", "ref_biblio": [""], "bibcode": ["1984PASP...96..707D"], "keyword_cds": "Clusters, open ; Stars, emission ; Spectroscopy", "keyword_pub": "Stellar rotation - emission lines - late-type stars", "abstract": ["The identity of chromospheric CaII H- and K-line emission has been", "monitored for two seasons in a large sample of Hyades F and G dwarfs.", "Mean emission levels vary smoothly with spectral type, suggesting that", "the rotation rate at a given spectral type varies relatively little,", "and that the rotation rate decreases smoothly as a function of mass.", "In this case the mechanism which controls pre-main-sequence angular", "momentum loss in late-type stars must be self-regulating to a high", "degree."], "object": [], "doi_pub": ["10.1086/131409"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "stars.dat", "desc": " ", "columns": [{"name": "VB", "desc": "van Bueren number (1952BAN....11..385V) "}, {"name": "logRhk", "desc": " "}, {"name": "logR'hk", "desc": "Chromospheric activity index "}, {"name": "logP", "desc": "Period "}, {"name": "SimbadName", "desc": "Designation of the star in SIMBAD "}, {"name": "RAdeg", "desc": "Right ascension in decimal degrees (J2000) "}, {"name": "DEdeg", "desc": "Declination in decimal degrees (J2000) "}, {"name": "TYC1", "desc": "Tycho-2 designation (Cat. I/259) "}, {"name": "TYC2", "desc": "Tycho-2 designation (Cat. I/259) "}, {"name": "TYC3", "desc": "Tycho-2 designation (Cat. I/259) "}, {"name": "HIP", "desc": "? Hipparcos number (Cat. I/239/hip_main) "}, {"name": "HD", "desc": "Henry Draper number (III/135) "}, {"name": "ASCC", "desc": "ASCC number (Kharchenko et al., Cat. I/280) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_PAZh_26_843"}} {"id": "J/PAZh/26/843", "title_cds": "Catalog of high- and low-mass X-ray binaries", "title_create": "Guseinov+, 2000", "year": "2000", "author": "Guseinov O.H., Sayagac A.T., Allakhverdiev A., Caliskan H., Ozdemir S., Yerli S.K., Ankay A.", "title_pub": "A preliminary version of a catalog of high-low-mass X-ray binaries", "first_author": "Guseinov O.H.", "ref_biblio": [""], "bibcode": ["2000PAZh...26..843G", "2000AstL...26..725G"], "see_also": ["V/106 : High- and low mass X-ray binaries catalogue (Liu+ 2000)"], "keyword_cds": "Binaries, X-ray ; Photometry, UBV ; Cross identifications", "keyword_pub": "catalogs, X-ray binaries, neutron stars, X-rays", "abstract": ["The aim of this catalogue is to provide basic information on X-ray", "sources and their counterparts. The catalogue contains positions,", "information about distances and counterparts, spectral, photometric", "and timing properties of the X-ray sources in X-ray and optical bands", "as well as references. The list of references, comments and the", "catalogue as a whole will be periodically updated to include the most", "up to date information on all X-ray binaries and guide users to the", "recent literature on individual sources. In some cases, there is some", "doubt about the nature of the X-ray source, which has been noted. The", "sources are ordered according to their right ascension.", "The first comprehensive catalogue of X-ray binaries was presented by", "van Paradijs (1995, Cat. ). Our catalogue includes, as X-ray", "binaries, the point X-ray sources powered by accretion onto neutron", "stars and blackholes. The weak sources powered by stellar coronae,", "Wolf-Rayet stars, and cataclysmic variables are not included. Among", "those X-ray binaries presented in the catalogue there are 78 HMXBs (35", "and 5 of which are pulsars and possible pulsars, respectively) and 138", "LMXBs (only 9 of which are pulsars), 89 transient and possible", "transient sources, and 25 possible blackholes (6 HMXBs+19 LMXBs).", "There are also 43 bursters (all of which are Galactic LMXBs) and 21", "QPOs. The present catalogue extends the work by van Paradijs,", "tabulates further information on the compact objects and their", "companions as well as attempting a more comprehensive guide to the", "literature. Where different authors obtained different values for", "system parameters, we have quoted all parameter values together with", "the references to guide the reader to the relevant literature for the", "derivation of the parameters."], "description": ["The catalogue mainly consists of 2 parts, 'hmxb' and 'lmxb', each of", "which has 4 files:", "1) The main catalogue is consisted of 'hmxbcat.dat' and 'lmxbcat.dat'.", "The most recent and/or the most reliable data are given in these files.", "2) All of the cross catalogue names of the sources and the names of", "the optical counterparts are given in 'hmxbnam.dat' and 'lmxbnam.dat'.", "3) The intensity values, energy bands, dates of observations, names of", "satellites for these observations, and the references of all of these", "data are given in 'hmxbobs.dat' and 'lmxbobs.dat'.", "4) All of the data other than the most recent and/or the most reliable", "ones are presented in 'hmxbrem.dat' and 'lmxbrem.dat'. The values given", "in intervals are also presented in these two files (e.g. A distance value", "of 4-5kpc of a source is given in 'hmxbrem.dat' or'lmxbrem.dat' (not in", "'hmxbcat.dat' or 'lmxbcat.dat') even if it is the most recent and/or the", "most reliable distance value of that source)."], "type": ["CCC"], "data": "", "date_update": "07-Sep-2011", "tables": [{"name": "lmxbcat.dat", "desc": "Low-Mass X-ray Binaries catalogue ", "columns": [{"name": "Name", "desc": "*Object name "}, {"name": "Location", "desc": "*[GOLS] Object's location "}, {"name": "Supersoft", "desc": "[S] Supersoft flag "}, {"name": "Type", "desc": "*Object's type "}, {"name": "RAh", "desc": "? Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "? Right Ascension 2000 (minutes) "}, {"name": "RAs", "desc": "? Right Ascension 2000 (seconds) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "? Declination 2000 (degrees) "}, {"name": "DEm", "desc": "? Declination 2000 (minutes) "}, {"name": "DEs", "desc": "? Declination 2000 (seconds) "}, {"name": "RA1950h", "desc": "? Right Ascension 1950 (hours) "}, {"name": "RA1950m", "desc": "? Right Ascension 1950 (minutes) "}, {"name": "RA1950s", "desc": "? Right Ascension 1950 (seconds) "}, {"name": "DE1950-", "desc": "Declination 1950 (sign) "}, {"name": "DE1950d", "desc": "? Declination 1950 (degrees) "}, {"name": "DE1950m", "desc": "? Declination 1950 (minutes) "}, {"name": "DE1950s", "desc": "? Declination 1950 (seconds) "}, {"name": "GLON", "desc": "? Galactic Longtitude "}, {"name": "GLAT", "desc": "? Galactic Latitude "}, {"name": "l_Porb", "desc": "[~<>= ] Limit flag on Porb "}, {"name": "Porb", "desc": "? Orbital Period "}, {"name": "u_Porb", "desc": "[:] Uncertainity flag on Porb "}, {"name": "n_Porb", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Ppulse", "desc": "[~<>= ] Limit flag on Ppulse "}, {"name": "Ppulse", "desc": "? Pulse Period "}, {"name": "u_Ppulse", "desc": "[:] Uncertainity flag on Ppulse "}, {"name": "n_Ppulse", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "n_Period", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Energy", "desc": "[~<>= ] Limit flag on Energy "}, {"name": "Energy", "desc": "? Energy, kT "}, {"name": "u_Energy", "desc": "[:] Uncertainity flag on Energy "}, {"name": "n_Energy", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Sp+Index", "desc": "[~<>= ] Limit flag on Sp+Index "}, {"name": "Sp+Index", "desc": "? Spectral Index "}, {"name": "u_Sp+Index", "desc": "[:] Uncertainity flag on Sp+Index "}, {"name": "n_Sp+Index", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "n_Fieldmag", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Dist", "desc": "[~<>= ] Limit flag on Dist "}, {"name": "Dist", "desc": "? Distance "}, {"name": "u_Dist", "desc": "[:] Uncertainity flag on Dist "}, {"name": "n_Dist", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_logNH", "desc": "[~<>= ] Limit flag on logNH "}, {"name": "logNH", "desc": "? log NH "}, {"name": "u_logNH", "desc": "[:] Uncertainity flag on logNH "}, {"name": "n_logNH", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_AV", "desc": "[~<>= ] Limit flag on AV "}, {"name": "AV", "desc": "? Total optical absorption "}, {"name": "u_AV", "desc": "[:] Uncertainity flag on AV "}, {"name": "n_AV", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_LX", "desc": "[~<>= ] Limit flag on LX "}, {"name": "LX", "desc": "? X-ray luminosity "}, {"name": "u_LX", "desc": "[:] Uncertainity flag on LX "}, {"name": "n_LX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_LX/Lopt", "desc": "[~<>= ] Limit flag on LX/Lopt "}, {"name": "LX/Lopt", "desc": "? Ratio of X-ray to optical luminosity "}, {"name": "u_LX/Lopt", "desc": "[:] Uncertainity flag on LX/Lop "}, {"name": "n_LX/Lopt", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "SpType", "desc": "*Spectral Type (Spectral type part 1) "}, {"name": "SpClass", "desc": "*Spectral Class (Spectal type part 2) "}, {"name": "SpType3", "desc": "*[dnefp ] Spectral Type (part 3) "}, {"name": "u_SpType", "desc": "*[:] Uncertainity flag on SpType "}, {"name": "l_Vmag1", "desc": "[~<>= ] Limit flag on Vmag1 "}, {"name": "Vmag1", "desc": "? V magnitude (1st component) "}, {"name": "Vmag2", "desc": "? V magnitude (2nd component) "}, {"name": "u_Vmag1", "desc": "[:] Uncertainity flag on Vmag1 "}, {"name": "n_Vmag1", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_B-V", "desc": "[~<>= ] Limit flag on B-V "}, {"name": "B-V", "desc": "? B-V magnitude "}, {"name": "u_B-V", "desc": "[:] Uncertainity flag on B-V "}, {"name": "n_B-V", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_U-B", "desc": "[~<>= ] Limit flag on U-B "}, {"name": "U-B", "desc": "? U-B magnitude "}, {"name": "u_U-B", "desc": "[:] Uncertainity flag on U-B "}, {"name": "n_U-B", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_E(B-V)", "desc": "[~<>= ] Limit flag on E(B-V) "}, {"name": "E(B-V)", "desc": "? E(B-V) colour excess "}, {"name": "u_E(B-V)", "desc": "[:] Uncertainity flag on E(B-V) "}, {"name": "n_E(B-V)", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassX", "desc": "[~<>= ] Limit flag on MassX "}, {"name": "MassX", "desc": "? Mass of compact object "}, {"name": "u_MassX", "desc": "[:] Uncertainity flag on MassX "}, {"name": "n_MassX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassO", "desc": "[~<>= ] Limit flag on MassO "}, {"name": "MassO", "desc": "? Mass of companion "}, {"name": "u_MassO", "desc": "[:] Uncertainity flag on MassO "}, {"name": "n_MassO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassFX", "desc": "[~<>= ] Limit flag on Mass FX "}, {"name": "MassFX", "desc": "? Mass function of compact object "}, {"name": "u_MassFX", "desc": "[:] Uncertainity flag on Mass FX "}, {"name": "n_MassFX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassFO", "desc": "[~<>= ] Limit flag on Mass FO "}, {"name": "MassFO", "desc": "? Mass function of companion "}, {"name": "u_MassFO", "desc": "[:] Uncertainity flag on Mass FO "}, {"name": "n_MassFO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_eOpt", "desc": "[~<>= ] Limit flag on eOpt "}, {"name": "eOpt", "desc": "? Eccentricity of the orbit "}, {"name": "u_eOpt", "desc": "[:] Uncertainity flag on eOpt "}, {"name": "n_eOpt", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelKX", "desc": "[~<>= ] Limit flag on VelKX "}, {"name": "VelKX", "desc": "? Semi-amplitude velocity of compact "}, {"name": "u_VelKX", "desc": "[:] Uncertainity flag on VelKX "}, {"name": "n_VelKX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelKO", "desc": "[~<>= ] Limit flag on VelKO "}, {"name": "VelKO", "desc": "? Semi-amplitude velocity of companion "}, {"name": "u_VelKO", "desc": "[:] Uncertainity flag on VelKO "}, {"name": "n_VelKO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelVG", "desc": "[~<>= ] Limit flag on VelVG "}, {"name": "VelVG", "desc": "? Center-of-mass velocity "}, {"name": "u_VelVG", "desc": "[:] Uncertainity flag on VelVG "}, {"name": "n_VelVG", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_a1sini", "desc": "[~<>= ] Limit flag on a1sini "}, {"name": "a1sini", "desc": "? A sin(I) for compact object "}, {"name": "u_a1sini", "desc": "[:] Uncertainity flag on a1sini "}, {"name": "n_a1sini", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_a2sini", "desc": "[~<>= ] Limit flag on a2sini "}, {"name": "a2sini", "desc": "? A sin(I) for companion "}, {"name": "u_a2sini", "desc": "[:] Uncertainity flag on a2sini "}, {"name": "n_a2sini", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Incl", "desc": "[~<>= ] Limit flag on Incl "}, {"name": "Incl", "desc": "? Inclination of orbit "}, {"name": "u_Incl", "desc": "[:] Uncertainity flag on Incl "}, {"name": "n_Incl", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "---", "desc": "[|] "}]}, {"name": "hmxbcat.dat", "desc": "High-Mass X-ray Binaries catalogue ", "columns": [{"name": "Name", "desc": "*Object name "}, {"name": "Location", "desc": "*[GOLS] Object's location "}, {"name": "Supersoft", "desc": "[S] Supersoft flag "}, {"name": "Type", "desc": "*Object's type "}, {"name": "RAh", "desc": "? Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "? Right Ascension 2000 (minutes) "}, {"name": "RAs", "desc": "? Right Ascension 2000 (seconds) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "? Declination 2000 (degrees) "}, {"name": "DEm", "desc": "? Declination 2000 (minutes) "}, {"name": "DEs", "desc": "? Declination 2000 (seconds) "}, {"name": "RA1950h", "desc": "? Right Ascension 1950 (hours) "}, {"name": "RA1950m", "desc": "? Right Ascension 1950 (minutes) "}, {"name": "RA1950s", "desc": "? Right Ascension 1950 (seconds) "}, {"name": "DE1950-", "desc": "Declination 1950 (sign) "}, {"name": "DE1950d", "desc": "? Declination 1950 (degrees) "}, {"name": "DE1950m", "desc": "? Declination 1950 (minutes) "}, {"name": "DE1950s", "desc": "? Declination 1950 (seconds) "}, {"name": "GLON", "desc": "? Galactic Longtitude "}, {"name": "GLAT", "desc": "? Galactic Latitude "}, {"name": "l_Porb", "desc": "[~<>= ] Limit flag on Porb "}, {"name": "Porb", "desc": "? Orbital Period "}, {"name": "u_Porb", "desc": "[:] Uncertainity flag on Porb "}, {"name": "n_Porb", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Ppulse", "desc": "[~<>= ] Limit flag on Ppulse "}, {"name": "Ppulse", "desc": "? Pulse Period "}, {"name": "u_Ppulse", "desc": "[:] Uncertainity flag on Ppulse "}, {"name": "n_Ppulse", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "n_Period", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Energy", "desc": "[~<>= ] Limit flag on Energy "}, {"name": "Energy", "desc": "? Energy, kT "}, {"name": "u_Energy", "desc": "[:] Uncertainity flag on Energy "}, {"name": "n_Energy", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Sp+Index", "desc": "[~<>= ] Limit flag on Sp+Index "}, {"name": "Sp+Index", "desc": "? Spectral Index "}, {"name": "u_Sp+Index", "desc": "[:] Uncertainity flag on Sp+Index "}, {"name": "n_Sp+Index", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "n_Fieldmag", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Dist", "desc": "[~<>= ] Limit flag on Dist "}, {"name": "Dist", "desc": "? Distance "}, {"name": "u_Dist", "desc": "[:] Uncertainity flag on Dist "}, {"name": "n_Dist", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_logNH", "desc": "[~<>= ] Limit flag on logNH "}, {"name": "logNH", "desc": "? log NH "}, {"name": "u_logNH", "desc": "[:] Uncertainity flag on logNH "}, {"name": "n_logNH", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_AV", "desc": "[~<>= ] Limit flag on AV "}, {"name": "AV", "desc": "? Total optical absorption "}, {"name": "u_AV", "desc": "[:] Uncertainity flag on AV "}, {"name": "n_AV", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_LX", "desc": "[~<>= ] Limit flag on LX "}, {"name": "LX", "desc": "? X-ray luminosity "}, {"name": "u_LX", "desc": "[:] Uncertainity flag on LX "}, {"name": "n_LX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_LX/Lopt", "desc": "[~<>= ] Limit flag on LX/Lopt "}, {"name": "LX/Lopt", "desc": "? Ratio of X-ray to optical luminosity "}, {"name": "u_LX/Lopt", "desc": "[:] Uncertainity flag on LX/Lop "}, {"name": "n_LX/Lopt", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "SpType", "desc": "*Spectral Type (Spectral type part 1) "}, {"name": "SpClass", "desc": "*Spectral Class (Spectal type part 2) "}, {"name": "SpType3", "desc": "*[dnefp ] Spectral Type (part 3) "}, {"name": "u_SpType", "desc": "*[:] Uncertainity flag on SpType "}, {"name": "l_Vmag1", "desc": "[~<>= ] Limit flag on Vmag1 "}, {"name": "Vmag1", "desc": "? V magnitude (1st component) "}, {"name": "Vmag2", "desc": "? V magnitude (2nd component) "}, {"name": "u_Vmag1", "desc": "[:] Uncertainity flag on Vmag1 "}, {"name": "n_Vmag1", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_B-V", "desc": "[~<>= ] Limit flag on B-V "}, {"name": "B-V", "desc": "? B-V magnitude "}, {"name": "u_B-V", "desc": "[:] Uncertainity flag on B-V "}, {"name": "n_B-V", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_U-B", "desc": "[~<>= ] Limit flag on U-B "}, {"name": "U-B", "desc": "? U-B magnitude "}, {"name": "u_U-B", "desc": "[:] Uncertainity flag on U-B "}, {"name": "n_U-B", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_E(B-V)", "desc": "[~<>= ] Limit flag on E(B-V) "}, {"name": "E(B-V)", "desc": "? E(B-V) colour excess "}, {"name": "u_E(B-V)", "desc": "[:] Uncertainity flag on E(B-V) "}, {"name": "n_E(B-V)", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassX", "desc": "[~<>= ] Limit flag on MassX "}, {"name": "MassX", "desc": "? Mass of compact object "}, {"name": "u_MassX", "desc": "[:] Uncertainity flag on MassX "}, {"name": "n_MassX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassO", "desc": "[~<>= ] Limit flag on MassO "}, {"name": "MassO", "desc": "? Mass of companion "}, {"name": "u_MassO", "desc": "[:] Uncertainity flag on MassO "}, {"name": "n_MassO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassFX", "desc": "[~<>= ] Limit flag on Mass FX "}, {"name": "MassFX", "desc": "? Mass function of compact object "}, {"name": "u_MassFX", "desc": "[:] Uncertainity flag on Mass FX "}, {"name": "n_MassFX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_MassFO", "desc": "[~<>= ] Limit flag on Mass FO "}, {"name": "MassFO", "desc": "? Mass function of companion "}, {"name": "u_MassFO", "desc": "[:] Uncertainity flag on Mass FO "}, {"name": "n_MassFO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_eOpt", "desc": "[~<>= ] Limit flag on eOpt "}, {"name": "eOpt", "desc": "? Eccentricity of the orbit "}, {"name": "u_eOpt", "desc": "[:] Uncertainity flag on eOpt "}, {"name": "n_eOpt", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelKX", "desc": "[~<>= ] Limit flag on VelKX "}, {"name": "VelKX", "desc": "? Semi-amplitude velocity of compact "}, {"name": "u_VelKX", "desc": "[:] Uncertainity flag on VelKX "}, {"name": "n_VelKX", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelKO", "desc": "[~<>= ] Limit flag on VelKO "}, {"name": "VelKO", "desc": "? Semi-amplitude velocity of companion "}, {"name": "u_VelKO", "desc": "[:] Uncertainity flag on VelKO "}, {"name": "n_VelKO", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_VelVG", "desc": "[~<>= ] Limit flag on VelVG "}, {"name": "VelVG", "desc": "? Center-of-mass velocity "}, {"name": "u_VelVG", "desc": "[:] Uncertainity flag on VelVG "}, {"name": "n_VelVG", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_a1sini", "desc": "[~<>= ] Limit flag on a1sini "}, {"name": "a1sini", "desc": "? A sin(I) for compact object "}, {"name": "u_a1sini", "desc": "[:] Uncertainity flag on a1sini "}, {"name": "n_a1sini", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_a2sini", "desc": "[~<>= ] Limit flag on a2sini "}, {"name": "a2sini", "desc": "? A sin(I) for companion "}, {"name": "u_a2sini", "desc": "[:] Uncertainity flag on a2sini "}, {"name": "n_a2sini", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "l_Incl", "desc": "[~<>= ] Limit flag on Incl "}, {"name": "Incl", "desc": "? Inclination of orbit "}, {"name": "u_Incl", "desc": "[:] Uncertainity flag on Incl "}, {"name": "n_Incl", "desc": "[*] indicates remark in [lh]mxbrem.dat "}, {"name": "---", "desc": "[|] "}]}, {"name": "lmxbobs.dat", "desc": "LMXB observations ", "columns": [{"name": "Seq", "desc": "[001/139]+= Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "OBSS.D", "desc": "? Start Day of observation date "}, {"name": "OBSS.M", "desc": "? Start Month of observation date "}, {"name": "OBSS.Y", "desc": "? Start Year of observation date "}, {"name": "OBSE.D", "desc": "? End Day of observation date "}, {"name": "OBSE.M", "desc": "? End Month of observation date "}, {"name": "OBSE.Y", "desc": "? End Year of observation date "}, {"name": "SAT", "desc": "*Satellite abbreviation "}, {"name": "EnergyS", "desc": "? Start of energy range "}, {"name": "EnergyE", "desc": "? End of energy range "}, {"name": "l_Flux1", "desc": "[<>~] Limit flag "}, {"name": "Flux1", "desc": "? Flux in {mu}Jy "}, {"name": "---", "desc": "[-] "}, {"name": "Flux1u", "desc": "? Upper limit of Flux1 when interval "}, {"name": "l_Flux2S", "desc": "[<>~ =] Limit flag "}, {"name": "Flux2S", "desc": "? Start of flux range in mW/m^2^ "}, {"name": "Flux2E", "desc": "? End of flux range in mW/m^2^ "}, {"name": "l_Flux3", "desc": "[<> ~ ] Limit flag on Flux3 "}, {"name": "Flux3", "desc": "? Flux (in count/s if x_Flux3=\" \") "}, {"name": "---", "desc": "[-] "}, {"name": "Flux3u", "desc": "? Upper limit of Flux3 when interval "}, {"name": "x_Flux3", "desc": "*[pmc] Units of Flux3 if not ct/s "}, {"name": "---", "desc": "[|] "}]}, {"name": "hmxbobs.dat", "desc": "HMXB observations ", "columns": [{"name": "Seq", "desc": "[001/139]+= Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "OBSS.D", "desc": "? Start Day of observation date "}, {"name": "OBSS.M", "desc": "? Start Month of observation date "}, {"name": "OBSS.Y", "desc": "? Start Year of observation date "}, {"name": "OBSE.D", "desc": "? End Day of observation date "}, {"name": "OBSE.M", "desc": "? End Month of observation date "}, {"name": "OBSE.Y", "desc": "? End Year of observation date "}, {"name": "SAT", "desc": "*Satellite abbreviation "}, {"name": "EnergyS", "desc": "? Start of energy range "}, {"name": "EnergyE", "desc": "? End of energy range "}, {"name": "l_Flux1", "desc": "[<>~] Limit flag "}, {"name": "Flux1", "desc": "? Flux in {mu}Jy "}, {"name": "---", "desc": "[-] "}, {"name": "Flux1u", "desc": "? Upper limit of Flux1 when interval "}, {"name": "l_Flux2S", "desc": "[<>~ =] Limit flag "}, {"name": "Flux2S", "desc": "? Start of flux range in mW/m^2^ "}, {"name": "Flux2E", "desc": "? End of flux range in mW/m^2^ "}, {"name": "l_Flux3", "desc": "[<> ~ ] Limit flag on Flux3 "}, {"name": "Flux3", "desc": "? Flux (in count/s if x_Flux3=\" \") "}, {"name": "---", "desc": "[-] "}, {"name": "Flux3u", "desc": "? Upper limit of Flux3 when interval "}, {"name": "x_Flux3", "desc": "*[pmc] Units of Flux3 if not ct/s "}, {"name": "---", "desc": "[|] "}]}, {"name": "hmxbname.dat", "desc": "HMXB cross-identifications ", "columns": [{"name": "Seq", "desc": "[1/139]? Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "n_Name", "desc": "[?E] Flag on name, not explicited in the paper "}, {"name": "Opt", "desc": "Optical name "}, {"name": "HD", "desc": "HD or HDE name "}, {"name": "SAO", "desc": "SAO name "}, {"name": "BD", "desc": "BD number "}, {"name": "Other", "desc": "Other name "}, {"name": "Xname", "desc": "X name "}, {"name": "3A", "desc": "3A name "}, {"name": "AX", "desc": "AX name "}, {"name": "1E", "desc": "1E/2E name "}, {"name": "EXO", "desc": "EXO name "}, {"name": "1H", "desc": "H/1H name "}, {"name": "RX", "desc": "RX/1RXS name "}, {"name": "2S", "desc": "2S nam,e "}, {"name": "SAX", "desc": "SAX name "}, {"name": "4U", "desc": "2U/3U/4U name "}, {"name": "1XRS", "desc": "1XRS name "}, {"name": "Names", "desc": "Other names "}, {"name": "---", "desc": "[|] "}]}, {"name": "lmxbname.dat", "desc": "LMXB cross-identifications ", "columns": [{"name": "Seq", "desc": "[1/139]? Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "n_Name", "desc": "[?E] Flag on name, not explicited in the paper "}, {"name": "Opt", "desc": "Optical name "}, {"name": "HD", "desc": "HD or HDE name "}, {"name": "SAO", "desc": "SAO name "}, {"name": "BD", "desc": "BD number "}, {"name": "Other", "desc": "Other name "}, {"name": "Xname", "desc": "X name "}, {"name": "3A", "desc": "3A name "}, {"name": "AX", "desc": "AX name "}, {"name": "1E", "desc": "1E/2E name "}, {"name": "EXO", "desc": "EXO name "}, {"name": "1H", "desc": "H/1H name "}, {"name": "RX", "desc": "RX/1RXS name "}, {"name": "2S", "desc": "2S nam,e "}, {"name": "SAX", "desc": "SAX name "}, {"name": "4U", "desc": "2U/3U/4U name "}, {"name": "1XRS", "desc": "1XRS name "}, {"name": "Names", "desc": "Other names "}, {"name": "---", "desc": "[|] "}]}, {"name": "lmxbrem.dat", "desc": "Other data for LMXB ", "columns": [{"name": "Seq", "desc": "[001/139]+= Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "Data", "desc": "Data "}, {"name": "f_Data", "desc": "[prvd] "}, {"name": "Value", "desc": "Value(s) of Data "}]}, {"name": "hmxbrem.dat", "desc": "Other data for HMXB ", "columns": [{"name": "Seq", "desc": "[001/139]+= Sequential number "}, {"name": "Name", "desc": "Object name "}, {"name": "Data", "desc": "Data "}, {"name": "f_Data", "desc": "[prvd] "}, {"name": "Value", "desc": "Value(s) of Data "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_A&A_543_o.A100"}} {"id": "J/A+A/543/A100", "title_cds": "GaiaSimu Universe Model Snapshot", "title_create": "Robin+, 2012", "year": "2012", "author": "Robin A.C., Luri X., Reyle C., Isasi Y., Grux E., Blanco-Cuaresma S., Arenou F., Babusiaux C., Belcheva M., Drimmel R., Jordi C., Krone-Martins A., Masana E., Mauduit J.C., Mignard F., Mowlavi N., Rocca-Volmerange B., Sartoretti P., Slezak E., Sozzetti A.", "title_pub": "Gaia Universe model snapshot. A statistical analysis of the expected contents of the Gaia catalogue.", "first_author": "Robin A.C.", "ref_biblio": [""], "bibcode": ["2012A&A...543A.100R"], "keyword_cds": "Positional data ; Surveys ; Models", "keyword_pub": "methods: data analysis - Galaxy: stellar content - catalogs - Galaxy: structure - galaxies: statistics - stars: statistics", "mission": "GAIA", "abstract": ["This study has been developed in the framework of the computational", "simulations that are executed for the preparation of the ESA Gaia", "astrometric mission.", "We focus on describing the objects and characteristics that Gaia will", "potentially observe without taking into consideration instrumental", "effects (detection efficiency, observing errors).", "The theoretical Universe model prepared for the Gaia simulation has", "been statistically analysed at a given time. Ingredients of the model", "are described, with the greatest emplasis on the stellar content, the", "double and multiple stars, and variability.", "**************************************************************************", "* *", "* The simulated catalogue will be soon available *", "* *", "**************************************************************************"], "curator": "Patricia Vannier [CDS]", "date_update": "09-Jul-2012"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_A&A_548_o.A66"}} {"id": "J/A+A/548/A66", "title_cds": "SDSS Quasar Catalog, DR9Q", "title_create": "Paris+, 2012", "year": "2012", "author": "Paris I., Petitjean P., Aubourg E., Bailey S., Ross N.P., Myers A.D., Strauss M.A., Anderson S.F., Arnau E., Bautista J., Bizyaev D., Bolton A.S., Bovy J., Brandt W.N., Brewington H., Brownstein J.R., Busca N., Capellupo D., Carithers W., Croft R.A.C., Dawson K., Delubac T., Ebelke G., Eisenstein D.J., Engelke P., Fan X., Filiz Ak N., Finley H., Font-Ribera A., Ge J., Gibson R.R., Hall P.B., Hamann F., Hennawi J.F., Ho S., Hogg D.W., Ivezic Z., Jiang L., Kimball A.E., Kirky D., Kirkpatrick J.A., Lee K-G., Le Goff J.-M., Lundgren B., MacLeod C.L., Malanushenko E., Malanushenko V., Maraston C., McGreer I.D., McMahon R.G., Miralda-Escude J., Muna D., Noterdaeme P., Oravetz D., Palanque-Delabrouille N., Pan K., Perez-Fournon I., Pieri M.M., Richards G.T., Rollinde E., Sheldon E.S., Schlegel D.J., Schneider D.P., Slosar A., Shelden A., Shen Y., Simmons A., Snedden S., Suzuki N., Tinker J., Viel M., Weaver B.A., Weinberg D.W., White M., Wood-Vasey W.M., Yeche C.", "title_pub": "The Sloan Digital Sky Survey Quasar Catalog: ninth data release.", "first_author": "Paris I.", "ref_biblio": [""], "bibcode": ["2012A&A...548A..66P"], "see_also": ["VII/260 : The SDSS-DR7 quasar catalog (Schneider+, 2010)", "J/A+A/547/L1 : SDSS-III DR9 DLA catalogue (Noterdaeme+, 2012)", "http://www.sdss.org : SDSS Home Page"], "keyword_cds": "Surveys ; QSOs ; Active gal. nuclei", "keyword_pub": "catalogs - surveys - quasars: general", "abstract": ["We present the Data Release 9 Quasar (DR9Q) catalog from the Baryon", "Oscillation Spectroscopic Survey (BOSS) of the Sloan Digital Sky", "Survey III. The catalog includes all BOSS objects that were targeted", "as quasar candidates during the survey, are spectroscopically confirmed", "as quasars via visual inspection. This catalog contains 87,822 quasars", "(78,086 are new discoveries) detected over 3,275{deg}^2^ with robust", "identification and redshift measured by a combination of principal", "component eigenspectra newly derived from a training set of 8,632", "spectra from SDSS-DR7. The number of quasars with z>2.15 (61,931) is", "2.8 times larger than the number of z>2.15 quasars previously known.", "Redshifts and FWHMs are provided for the strongest emission lines", "(CIV, CIII], MgII). The catalog identifies 7,533 broad absorption line", "quasars and gives their characteristics. For each object the catalog", "presents five-band (u,g,r,i,z) CCD-based photometry with typical", "accuracy of 0.03mag, and information on the morphology and selection", "method. The catalog also contains X-ray, ultraviolet, near-infrared,", "and radio emission properties of the quasars, when available, from", "other large-area surveys. We also provide a supplemental list of an", "additional 949 quasars that have been identified, among galaxy targets", "of the BOSS or among quasar targets after DR9 was frozen."], "description": ["The SDSS-DR9 Quasar Catalog presents photometric and spectroscopic", "properties of 87,822 quasars observed by the SDSS-III/BOSS survey. We", "provide the catalog in the form of a fits file but also an ascii file.", "We also provide a supplemental list containing 949 quasars with", "exactly the same format as the main catalog."], "date_update": "16-Mar-2013", "tables": [{"name": "dr9q.dat", "desc": "Main DR9 Quasar catalog ", "columns": [{"name": "SDSS", "desc": "SDSS-DR9 designation (HHMMSS.ss+DDMMSS.s) "}, {"name": "RAdeg", "desc": "Right ascension (J2000.0) "}, {"name": "DEdeg", "desc": "Declination (J2000.0) "}, {"name": "THINGID", "desc": "[26159535/512342668] Unique identifier "}, {"name": "Plate", "desc": "SDSS Plate number "}, {"name": "MJD", "desc": "SDSS Spectroscopic MJD "}, {"name": "Fiber", "desc": "SDSS Fiber number "}, {"name": "z.v", "desc": "Visual inspection redshift "}, {"name": "z.b", "desc": "BOSS pipeline redshift "}, {"name": "e_z.b", "desc": "?=-1 Error on pipeline redshift "}, {"name": "f_z.b", "desc": "[0/196] zwarning flag (G2) "}, {"name": "z.p", "desc": "?=-1 PCA redshift (G3) "}, {"name": "e_z.p", "desc": "?=-1 Error on PCA redshift (G3) "}, {"name": "qCont", "desc": "[0/1]?=-1 Quality of PCA continuum (G3) "}, {"name": "zCIV", "desc": "?=-1 CIV redshift "}, {"name": "zCIII", "desc": "?=-1 CIII] complex redshift "}, {"name": "zMgII", "desc": "?=-1 MgII redshift "}, {"name": "Morph", "desc": "[0/1] Morphology flag (0=point, 1=extended) "}, {"name": "Btarg1", "desc": "?=0 Main (BOSS) survey primary target selection flags (G4)"}, {"name": "Atarg1", "desc": "?=0 Ancillary target selection flag 1 (G4) "}, {"name": "Atarg2", "desc": "?=0 Ancillary target selection flag 2 (G4) "}, {"name": "f7", "desc": "[0/1] 1=quasar in SDSS-DR7 (Cat. VII/260) "}, {"name": "Plate7", "desc": "?=-1 SDSS DR7 Plate number "}, {"name": "MJD7", "desc": "?=-1 SDSS DR7 spectroscopic MJD "}, {"name": "Fiber7", "desc": "?=-1 SDSS DR7 Fiber number "}, {"name": "US", "desc": "[0/2]?=-1 Uniform sample flag (G6) "}, {"name": "iMAG", "desc": "?=-9999. Absolute Magnitude Mi[z=2] (G5) "}, {"name": "D(g-i)", "desc": "?=-9999. Diff. color {Delta}(g-i) (G7) "}, {"name": "alpha", "desc": "Spectral index {alpha}_{nu}_ "}, {"name": "SNRsp", "desc": "Median S/N ratio (whole spectrum) "}, {"name": "SNR1700", "desc": "?=-1 Median SNR (1650-175nm rest) "}, {"name": "SNR3000", "desc": "?=-1 Median SNR (2950-305nm rest) "}, {"name": "SNR5150", "desc": "?=-1 Median SNR (5100-525nm rest) "}, {"name": "FW(CIV)", "desc": "?=-1 FWHM of CIV emission "}, {"name": "HW(CIV)b", "desc": "?=-1 Blue HWHM of CIV emission "}, {"name": "HW(CIV)r", "desc": "?=-1 Red HWHM of CIV emission "}, {"name": "A(CIV)", "desc": "?=-1 Amplitude of CIV emission "}, {"name": "W(CIV)", "desc": "?=-1 Rest equivalent width of CIV emission "}, {"name": "e_W(CIV)", "desc": "?=-1 Error on rest EW of CIV emission "}, {"name": "FW(CIII)", "desc": "?=-1 FWHM of CIII] complex "}, {"name": "HW(CIII)b", "desc": "?=-1 Blue HWHM of CIII] complex "}, {"name": "HW(CIII)r", "desc": "?=-1 Red HWHM of CIII] complex "}, {"name": "A(CIII)", "desc": "?=-1 Amplitude of CIII] complex "}, {"name": "W(CIII)", "desc": "?=-1 Rest equivalent width of CIII] complex "}, {"name": "e_W(CIII)", "desc": "?=-1 Error on rest EW of CIII] complex "}, {"name": "FW(MgII)", "desc": "?=-1 FWHM of MgII emission "}, {"name": "HW(MgII)b", "desc": "?=-1 Blue HWHM of MgII emission "}, {"name": "HW(MgII)r", "desc": "?=-1 Red HWHM of MgII emission "}, {"name": "A(MgII)", "desc": "?=-1 Amplitude of MgII emission "}, {"name": "W(MgII)", "desc": "?=-1 Rest equivalent width of MgII emission "}, {"name": "e_W(MgII)", "desc": "?=-1 Error on rest EW of MgII emission "}, {"name": "BAL-VI", "desc": "[0/1] BAL flag from visual inspection "}, {"name": "BI(CIVt)", "desc": "?=-1 Balnicity index (BI) of CIV trough "}, {"name": "e_BI(CIVt)", "desc": "?=-1 Error on BI of CIV trough "}, {"name": "AI(CIVt)", "desc": "?=-1 AI index of CIV trough "}, {"name": "e_AI(CIVt)", "desc": "?=-1 Error on AI of CIV trough "}, {"name": "DI(CIVt)", "desc": "?=-1 Detection index (DI) of CIV trough "}, {"name": "e_DI(CIVt)", "desc": "?=-1 Error on the DI of CIV trough "}, {"name": "Chi2CIVt", "desc": "Chi2 of the CIV troughs "}, {"name": "N2t", "desc": "[0/5] Number of CIV troughs > 1999km/s "}, {"name": "Vmin2t", "desc": "?=0 Min velocity of CIV troughs (NCIV2) "}, {"name": "Vmax2t", "desc": "?=0 Max velocity of CIV troughs (NCIV2) "}, {"name": "N.45t", "desc": "[0/13] Number of CIV troughs > 449km/s "}, {"name": "Vmin.45t", "desc": "Min velocity of CIV troughs (NCIV4.5) "}, {"name": "Vmax.45t", "desc": "Max velocity of CIV troughs (NCIV4.5) "}, {"name": "W(SiIVt)", "desc": "?=0 Rest equivalent width of SiIV trough "}, {"name": "W(CIVt)", "desc": "?=0 Rest equivalent width of CIV trough "}, {"name": "W(AlIIIt)", "desc": "?=0 Rest equivalent width of AlIII trough "}, {"name": "Run", "desc": "Imaging Run Number "}, {"name": "Ph-MJD", "desc": "Photometric MJD "}, {"name": "Rerun", "desc": "Photometric Processing Rerun number "}, {"name": "Colcam", "desc": "[1/6] camera column number "}, {"name": "Field", "desc": "Field number "}, {"name": "objID", "desc": "?=-9999. Object Identification number "}, {"name": "Fu", "desc": "?=-9999. u-band flux (in nanomaggies) (G1) "}, {"name": "e_Fu", "desc": "?=-9999. Error on Fu (in nanomaggies) (G1) "}, {"name": "Fg", "desc": "?=-9999. g-band flux (in nanomaggies) (G1) "}, {"name": "e_Fg", "desc": "?=-9999. Error on Fg (in nanomaggies) (G1) "}, {"name": "Fr", "desc": "?=-9999. r-band flux (in nanomaggies) (G1) "}, {"name": "e_Fr", "desc": "?=-9999. Error on Fr (in nanomaggies) (G1) "}, {"name": "Fi", "desc": "?=-9999. i-band flux (in nanomaggies) (G1) "}, {"name": "e_Fi", "desc": "?=-9999. Error on Fi (in nanomaggies) (G1) "}, {"name": "Fz", "desc": "?=-9999. z-band flux (in nanomaggies) (G1) "}, {"name": "e_Fz", "desc": "?=-9999. Error on Fz (in nanomaggies) (G1) "}, {"name": "Fut", "desc": "?=-9999 TARGET flux in the u-band (in nanomaggies) (G1)"}, {"name": "Fgt", "desc": "?=-9999 TARGET flux in the g-band (in nanomaggies) (G1)"}, {"name": "Frt", "desc": "?=-9999 TARGET flux in the r-band (in nanomaggies) (G1)"}, {"name": "Fit", "desc": "?=-9999 TARGET flux in the i-band (in nanomaggies) (G1)"}, {"name": "Fzt", "desc": "?=-9999 TARGET flux in the z-band (in nanomaggies) (G1)"}, {"name": "Extu", "desc": "u-band Galactic extinction "}, {"name": "logNHI", "desc": "?=-9 log of Galactic HI column density "}, {"name": "logXcr", "desc": "?=-9 log RASS full band count rate "}, {"name": "SNR(X)", "desc": "?=-9 SNR of RASS count rate "}, {"name": "sepX", "desc": "[0] SDSS-RASS separation "}, {"name": "FNUV", "desc": "NUV flux (GALEX) (in nanomaggies) (G1) "}, {"name": "e_FNUV", "desc": "?=0 Error on NUV flux (in nanomaggies)(G1) "}, {"name": "FFUV", "desc": "FUV flux (GALEX) (in nanomaggies) (G1) "}, {"name": "e_FFUV", "desc": "?=0 Error on FUV flux (in nanomaggies)(G1) "}, {"name": "Jmag", "desc": "?=0 J-band magnitude (Vega, 2MASS) "}, {"name": "e_Jmag", "desc": "?=-1 Error on J-band magnitude "}, {"name": "SNR(J)", "desc": "?=-1 J-band SNR "}, {"name": "f_Jmag", "desc": "[0/6] J-band photometry flag "}, {"name": "Hmag", "desc": "?=0 H-band magnitude (Vega, 2MASS) "}, {"name": "e_Hmag", "desc": "?=-1 Error on H-band magnitude "}, {"name": "SNR(H)", "desc": "?=-1 H-band SNR "}, {"name": "f_Hmag", "desc": "[0/6] H-band photometry flag "}, {"name": "Kmag", "desc": "?=0 K-band magnitude (Vega, 2MASS) "}, {"name": "e_Kmag", "desc": "?=-1 Error on K-band magnitude "}, {"name": "SNR(K)", "desc": "?=-1 K-band SNR "}, {"name": "f_Kmag", "desc": "[0/6] K-band photometry flag "}, {"name": "sep2", "desc": "?=0 SDSS-2MASS separation "}, {"name": "W1mag", "desc": "?=0 W1 magnitude (Vega, WISE=Cat. II/311) "}, {"name": "e_W1mag", "desc": "?=0 Error on W1 magnitude "}, {"name": "W1SNR", "desc": "?=0 SNR in W1 band "}, {"name": "W1chi2", "desc": "?=0 Chi2 in W1 band "}, {"name": "W2mag", "desc": "?=0 W2 magnitude (Vega, WISE=Cat. II/311) "}, {"name": "e_W2mag", "desc": "?=0 Error on W2 magnitude "}, {"name": "W2SNR", "desc": "?=0 SNR in W2 band "}, {"name": "W2chi2", "desc": "?=0 Chi2 in W2 band "}, {"name": "W3mag", "desc": "?=0 W3 magnitude (Vega, WISE=Cat. II/311) "}, {"name": "e_W3mag", "desc": "?=0 Error on W3 magnitude "}, {"name": "W3SNR", "desc": "?=0 SNR in W3 band "}, {"name": "W3chi2", "desc": "?=0 Chi2 in W3 band "}, {"name": "W4mag", "desc": "?=0 W4 magnitude (Vega, WISE=Cat. II/311) "}, {"name": "e_W4mag", "desc": "?=0 Error on W4 magnitude "}, {"name": "W4SNR", "desc": "?=0 SNR in W4 band "}, {"name": "W4chi2", "desc": "?=0 Chi2 in W4 band "}, {"name": "sepW", "desc": "?=0 SDSS-WISE separation "}, {"name": "F1p", "desc": "?=0 FIRST (Cat. VIII/90) peak flux density at 20cm"}, {"name": "SNR(1)", "desc": "?=0 SNR of the FIRST flux density "}, {"name": "sep1", "desc": "?=0 SDSS-FIRST separation "}]}, {"name": "dr9q.fits", "desc": "Main DR9 Quasar catalog, FITS format ", "columns": []}, {"name": "dr9qsup.dat", "desc": "Supplemental list ", "columns": [{"name": "SDSS", "desc": "SDSS-DR9 designation (HHMMSS.ss+DDMMSS.s) (1) "}, {"name": "RAdeg", "desc": "? Right ascension (J2000.0) (1) "}, {"name": "DEdeg", "desc": "? Declination (J2000.0) (1) "}, {"name": "THINGID", "desc": "?=-1 Unique identifier (1) "}, {"name": "Plate", "desc": "SDSS Plate number "}, {"name": "MJD", "desc": "SDSS Spectroscopic MJD "}, {"name": "Fiber", "desc": "SDSS Fiber number "}, {"name": "z.v", "desc": "Visual inspection redshift "}, {"name": "z.b", "desc": "BOSS pipeline redshift "}, {"name": "e_z.b", "desc": "?=-1 Error on pipeline redshift "}, {"name": "f_z.b", "desc": "[0/134] zwarning flag (G2) "}, {"name": "z.p", "desc": "?=-1 PCA redshift (G3) "}, {"name": "e_z.p", "desc": "?=-1 Error on PCA redshift (G3) "}, {"name": "qCont", "desc": "?=-1 Quality of PCA continuum (G3) "}, {"name": "zCIV", "desc": "?=-1 CIV redshift "}, {"name": "zCIII", "desc": "?=-1 CIII] complex redshift "}, {"name": "zMgII", "desc": "?=-1 MgII redshift "}, {"name": "Morph", "desc": "[0/1] Morphology flag (0=point, 1=extended) "}, {"name": "Btarg1", "desc": "?=1 Main (BOSS) survey primary target selection flags (G4)"}, {"name": "Atarg1", "desc": "?=1 Ancillary target selection flag 1 (G4) "}, {"name": "Atarg2", "desc": "?=1 Ancillary target selection flag 2 (G4) "}, {"name": "alpha", "desc": "Spectral index {alpha}_{nu}_ "}, {"name": "SNRsp", "desc": "Median SNR (whole spectrum) "}, {"name": "SNR1700", "desc": "?=-1 Median SNR (1650-175nm rest) "}, {"name": "SNR3000", "desc": "?=-1 Median SNR (2950-305nm rest) "}, {"name": "SNR5150", "desc": "?=-1 Median SNR (5100-525nm rest) "}, {"name": "FW(CIV)", "desc": "?=-1 FWHM of CIV emission "}, {"name": "HW(CIV)b", "desc": "?=-1 Blue HWHM of CIV emission "}, {"name": "HW(CIV)r", "desc": "?=-1 Red HWHM of CIV emission "}, {"name": "A(CIV)", "desc": "?=-1 Amplitude of CIV emission "}, {"name": "W(CIV)", "desc": "?=-1 Rest equivalent width of CIV emission "}, {"name": "e_W(CIV)", "desc": "?=-1 Error on rest EW of CIV emission "}, {"name": "FW(CIII)", "desc": "?=-1 FWHM of CIII] complex "}, {"name": "HW(CIII)b", "desc": "?=-1 Blue HWHM of CIII] complex "}, {"name": "HW(CIII)r", "desc": "?=-1 Red HWHM of CIII] complex "}, {"name": "A(CIII)", "desc": "?=-1 Amplitude of CIII] complex "}, {"name": "W(CIII)", "desc": "?=-1 Rest equivalent width of CIII] complex "}, {"name": "e_W(CIII)", "desc": "?=-1 Error on rest EW of CIII] complex "}, {"name": "FW(MGII)", "desc": "?=-1 FWHM of MgII emission "}, {"name": "HW(MGII)b", "desc": "?=-1 Blue HWHM of MgII emission "}, {"name": "HW(MGII)r", "desc": "?=-1 Red HWHM of MgII emission "}, {"name": "A(MGII)", "desc": "?=-1 Amplitude of MgII emission "}, {"name": "W(MGII)", "desc": "?=-1 Rest equivalent width of MgII emission "}, {"name": "e_W(MGII)", "desc": "?=-1 Error on rest EW of MgII emission "}, {"name": "BAL-VI", "desc": "[0/1] BAL flag from visual inspection "}, {"name": "BI(CIVt)", "desc": "?=-1 Balnicity index (BI) of CIV trough "}, {"name": "e_BI(CIVt)", "desc": "?=-1 Error on BI of CIV trough "}, {"name": "AI(CIVt)", "desc": "?=-1 AI index of CIV trough "}, {"name": "e_AI(CIVt)", "desc": "?=-1 Error on AI of CIV trough "}, {"name": "DI(CIVt)", "desc": "?=-1 Detection index (DI) of CIV trough "}, {"name": "e_DI(CIVt)", "desc": "?=-1 Error on the DI of CIV trough "}, {"name": "Chi2CIVt", "desc": "?=-1 Chi2 of the CIV troughs "}, {"name": "N2t", "desc": "?=-1 Number of CIV troughs > 1999km/s "}, {"name": "Vmin2t", "desc": "?=0 Min velocity of CIV troughs (NCIV2) "}, {"name": "Vmax2t", "desc": "?=0 Max velocity of CIV troughs (NCIV2) "}, {"name": "N.45t", "desc": "?=-1 Number of CIV troughs > 449km/s "}, {"name": "Vmin.45t", "desc": "Min velocity of CIV troughs (NCIV4.5) "}, {"name": "Vmax.45t", "desc": "Max velocity of CIV troughs (NCIV4.5) "}, {"name": "Run", "desc": "?=0 Imaging Run Number "}, {"name": "Ph-MJD", "desc": "?=0 Photometric MJD "}, {"name": "Rerun", "desc": "? Photometric Processing Rerun number "}, {"name": "Colcam", "desc": "?=0 camera column number "}, {"name": "Field", "desc": "?=0 Field number "}, {"name": "OBJID", "desc": "? Object Identification number "}, {"name": "Fu", "desc": "?=-999. u-band flux (in nanomaggies) (G1) "}, {"name": "e_Fu", "desc": "?=-9. Error on Fu (in nanomaggies) (G1) "}, {"name": "Fg", "desc": "?=-999. g-band flux (in nanomaggies) (G1) "}, {"name": "e_Fg", "desc": "?=-9. Error on Fg (in nanomaggies) (G1) "}, {"name": "Fr", "desc": "?=-999. r-band flux (in nanomaggies) (G1) "}, {"name": "e_Fr", "desc": "?=-9. Error on Fr (in nanomaggies) (G1) "}, {"name": "Fi", "desc": "?=-999. i-band flux (in nanomaggies) (G1) "}, {"name": "e_Fi", "desc": "?=-9. Error on Fi (in nanomaggies) (G1) "}, {"name": "Fz", "desc": "?=-999. z-band flux (in nanomaggies) (G1) "}, {"name": "e_Fz", "desc": "?=-9. Error on Fz (in nanomaggies) (G1) "}, {"name": "Extu", "desc": "u-band Galactic extinction "}]}, {"name": "dr9q_sup.fits", "desc": "Supplemental list, FITS format ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_Ap+SS_163.275"}} {"id": "J/other/ApSS/163.275", "title_cds": "UV & Geneva photometry around HD 173009", "title_create": "Reichen+, 1990", "year": "1990", "author": "Reichen M., Lanz T., Golay M., Huguenin D.", "title_pub": "A detailed study of a 6{deg} diameter field in Scutum. I. Data presentation and overall description of the interstellar matter distribution.", "first_author": "Reichen M.", "ref_biblio": [""], "bibcode": ["1990Ap&SS.163..275R"], "see_also": ["II/59 : Catalogue of stellar UV fluxes (TD1) (Thompson+ 1978)"], "keyword_cds": "Surveys ; Photometry, ultraviolet ; Photometry, Geneva ; MK spectral classification", "abstract": ["A 6{deg} diameter field centered on the star {epsilon} Scutum has been", "selected from the SCAP-2000 balloon-borne UV survey for its high", "apparent stellar density contrast and relatively good transparency on", "a small projected portion of the galactic plane. In view of a detailed", "study of the absorption and interstellar matter distribution in this", "field, a large collection of data has been made and is presented here.", "Ultraviolet magnitudes at 2000{AA} have been obtained from the", "reduction of three SCAP frames. In addition, 322 stars among the 487", "stars detected on the UV frames have been measured in the Geneva", "photometric system. For a small number of photometrically distant", "objects, medium resolution spectra have been obtained in order to", "determine spectral types and confirm the distances determination. An", "overall description of the distribution of interstellar material in", "the ultraviolet is made using star counting methods, and is confronted", "to similar studies in the visible range. A discussion of the", "variations of the extinction law in different parts of the field is", "made. A new distance determination of the Sct OB2 association is", "proposed, as well as a list of additional probable members of the", "association. A certain number of distant hot stars seem to indicate", "the presence of an unknown OB association at the edge of the Scutum", "spiral arm, at a distance of over 3 kpc from the Sun."], "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Calibration stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (see Table2) "}, {"name": "Name", "desc": "HD, BD or CSI identification "}, {"name": "SpType", "desc": "Spectral type (see table 2) "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude from the Geneva system"}, {"name": "UVmag", "desc": "UV magnitude at 2000{AA} deduced from calibration"}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag "}, {"name": "n_UVmag", "desc": "[abcd ] Note on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965{AA} passband of the TD1 catalogue (Thompson et al., 1978, Cat. ). (2)"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "n_UVmagTD1", "desc": "[)] ) indicates that the UV magnitude UVmagboxes was preferred for the calibration"}, {"name": "UVmagboxes", "desc": "UV magnitude deduced by the method of the so-called \"photometric boxes\" (see text.) (3)"}, {"name": "e_UVmagboxes", "desc": "rms uncertainty on UVmagboxes "}, {"name": "n_UVmagboxes", "desc": "[)] ) indicates that the UV magnitude UVmagTD1 was preferred for the calibration"}, {"name": "N", "desc": "Number of stars in the photometric box "}, {"name": "Rem", "desc": "Remarks related to the UV_TD1_ magnitudes (G2) "}]}, {"name": "table2.dat", "desc": "All stars measured on SCAP frames 11.65/14.48/14.49 ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (1) "}, {"name": "n_SCAP", "desc": "[* o] \"*\" star measured in the Geneva system (see Table 3) \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[+*] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (see Table 3) "}, {"name": "Vmag", "desc": "? Visual magnitude (3) "}, {"name": "UVmag", "desc": "UV magnitude at 2000A from the SCAP frames "}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag (4) "}, {"name": "n_UVmag", "desc": "[abcd ] Notes on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965A passband of the TD1 catalogue (Thompson et al., 1978, )"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "UV-V", "desc": "? (UVmag-Vmag) color index "}, {"name": "(UV-V)0", "desc": "? Intrinsic (UV-V)_0_ color index taken from Carnochan (1982) following the MK, photometric or other spectra type"}, {"name": "E(UV-V)", "desc": "? UV color excess (from (UV-V) and (UV-V)0) "}, {"name": "Rem", "desc": "Various remarks and comments (G2) "}]}, {"name": "table3.dat", "desc": "All stars with Geneva photometry ", "columns": [{"name": "SCAP", "desc": "SCAP identification (see Table 2) "}, {"name": "n_SCAP", "desc": "[o] \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[*+] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "GLONd", "desc": "Galactic longitude "}, {"name": "GLONm", "desc": "Galactic longitude "}, {"name": "GLATd", "desc": "Galactic latitude "}, {"name": "GLATm", "desc": "Galactic latitude "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (1) "}, {"name": "[U-B]", "desc": "Geneva [U-B] colour index "}, {"name": "[B-V]", "desc": "Geneva [B-V] colour index "}, {"name": "[B1-B]", "desc": "Geneva [B1-B] colour index "}, {"name": "[B2-B]", "desc": "Geneva [B2-B] colour index "}, {"name": "[V1-B]", "desc": "Geneva [V1-B] colour index "}, {"name": "[G-B]", "desc": "Geneva [G-B] colour index "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude "}, {"name": "E[B-V]", "desc": "? Color excess deduced from the X,Y,Z parameters (Cramer, 1982A&A...112..330C) unless stated otherwise in the remarks"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters (Cramer and Maeder, 1979A&A....78..305C) unless stated otherwise in the remarks"}, {"name": "r", "desc": "? Decuced heliocentric distance "}, {"name": "Rem", "desc": "Various remarks (2) "}]}, {"name": "table4.dat", "desc": "Spectroscopic standard stars ", "columns": [{"name": "HD", "desc": "HD identification "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "? Visible absorption derived from E[B-V]. "}, {"name": "n_AV", "desc": "[)] ): values deduced from Johnson's U-B/B-V diagram"}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypeH", "desc": "Spectral type given by Houk and Cowley (1975, ) or Houk (1978, , 1982, )"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHg", "desc": "Equivalent width of the H{gamma} line derived from our spectroscopic observations"}, {"name": "VMAGHg", "desc": "Absolute magnitude derived from EW_H{gamma}_ using calibrations by Millward and Walker (1985ApJS...57...63M) or Hill et al. (1986PASP...98.1186H)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}]}, {"name": "table5.dat", "desc": "Spectroscopy of Scutum field stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "Visible absorption derived from E[B-V] "}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHa", "desc": "Equivalent width of the H{alpha} line derived from our spectroscopic observations"}, {"name": "u_EWHa", "desc": "[)] Uncertainty flag on EWHa "}, {"name": "VMAGHa", "desc": "? Absolute magnitude derived from EW_H{alpha}_ (See notes to Table 4)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}, {"name": "Rem", "desc": "Individual remarks (1) "}]}, {"name": "notes2.dat", "desc": "Individual notes to table2.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "notes3.dat", "desc": "Individual notes to table3.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_Natur_585.363"}} {"id": "J/other/Nat/585.363", "title_cds": "WD 1856+534 transit curves", "title_create": "Vanderburg+, 2020", "year": "2020", "author": "Vanderburg A., Rappaport S.A., Xu S., Crossfield I.J.M., Becker J.C., Gary B., Murgas F., Blouin S., Kaye T.G., Palle E., Melis C., Morris B.M., Kreidberg L., Gorjian V., Morley C.V., Mann A.W., Parviainen H., Pearce L.A., Newton E.R., Carrillo A., Zuckerman B., Nelson L., Zeimann G., Brown W.R., Tronsgaard R., Klein B., Ricker G.R., Vanderspek R.K., Latham D.W., Seager S., Winn J.N., Jenkins J.M., Adams F.C., Benneke B., Berardo D., Buchhave L.A., Caldwell D.A., Christiansen J.L., Collins K.A., Colon K.D., Daylan T., Doty J., Doyle A.E., Dragomir D., Dressing C., Dufour P., Fukui A., Glidden A., Guerrero N.M., Guo X., Heng K., Henriksen A.I., Huang C.X., Kaltenegger L., Kane S.R., Lewis J.A., Lissauer J.J., Morales F., Narita N., Pepper J., Rose M.E., Smith J.C., Stassun K.G., Yu L.", "title_pub": "A giant planet candidate transiting a white dwarf.", "first_author": "Vanderburg A.", "ref_biblio": [""], "bibcode": ["2020Natur.585..363V"], "keyword_cds": "Stars, white dwarf ; Spectra, optical ; Photometry, SDSS", "abstract": ["Astronomers have discovered thousands of planets outside the Solar", "System, most of which orbit stars that will eventually evolve into red", "giants and then into white dwarfs. During the red giant phase, any", "close-orbiting planets will be engulfed by the star, but more distant", "planets can survive this phase and remain in orbit around the white", "dwarf. Some white dwarfs show evidence for rocky material floating in", "their atmospheres5, in warm debris disks or orbiting very closely,", "which has been interpreted as the debris of rocky planets that were", "scattered inwards and tidally disrupted. Recently, the discovery of", "a gaseous debris disk with a composition similar to that of ice giant", "planets14 demonstrated that massive planets might also find their way", "into tight orbits around white dwarfs, but it is unclear whether these", "planets can survive the journey. So far, no intact planets have been", "detected in close orbits around white dwarfs. Here we report the", "observation of a giant planet candidate transiting the white dwarf", "WD 1856+534 (TIC 267574918) every 1.4days. We observed and modelled", "the periodic dimming of the white dwarf caused by the planet candidate", "passing in front of the star in its orbit. The planet candidate is", "roughly the same size as Jupiter and is no more than 14 times as", "massive (with 95 per cent confidence). Other cases of white dwarfs", "with close brown dwarf or stellar companions are explained as the", "consequence of common-envelope evolution, wherein the original orbit", "is enveloped during the red giant phase and shrinks owing to friction.", "In this case, however, the long orbital period (compared with other", "white dwarfs with close brown dwarf or stellar companions) and low", "mass of the planet candidate make common-envelope evolution less", "likely. Instead, our findings for the WD 1856+534 system indicate that", "giant planets can be scattered into tight orbits without being tidally", "disrupted, motivating the search for smaller transiting planets around", "white dwarfs."], "description": ["We show spectra from four observatories, using the Low Resolution", "Spectrograph 2 on the Hobby-Eberly Telescope (HET/LRS2), the Gemini", "Near InfraRed Spectrograph on the Gemini North Telescope", "(Gemini/GNIRS), the Kast Double Spectrograph on the Shane Telescope at", "Lick Observatory (Lick/Kast) and the Blue Channel spectrograph at MMT", "Observatory. The data have been scaled to remove offsets in their", "absolute flux calibrations. The optical spectra show a pure continuum,", "confirming the DC spectral classification, whereas the near-infrared", "spectrum from Gemini North shows only spurious features, owing to", "imperfect correction of the telluric absorption and sky emission from", "Earth's atmosphere.", "We show the light curves from TESS; data from several private", "telescopes in Arizona (operated by B.G. and T.G.K.) with odd and", "even-numbered transits shown separately; simultaneous light curves in", "four colours from MuSCAT2; a light curve from the GTC, and a light", "curve from Spitzer. The individual two-minute-cadence TESS flux", "measurements are shown as grey points, and the rose-coloured points", "are averages of the brightness in roughly 30s in orbital phase. The", "TESS data have been corrected for dilution from nearby stars so that", "the transit depth matches that of the GTC data."], "object": ["18 57 39.34 +53 30 33.3 WD 1856+534 = TOI 1690"], "date_update": "17-Nov-2020", "tables": [{"name": "fig2.dat", "desc": "Spectroscopic observation of WD 1856+534 ", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "RelFlux", "desc": "? Relative Flux "}, {"name": "Inst", "desc": "Observatory/Spectrograph (1) "}]}, {"name": "fig2ext.dat", "desc": "All transit observation of WD 1856+534 ", "columns": [{"name": "Time", "desc": "Observation date (TDB) "}, {"name": "Relmag", "desc": "Relative Brightness "}, {"name": "Inst", "desc": "Observatory/Filter (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_Ap_32.252"}} {"id": "J/other/Ap/32.252", "title_cds": "Second Byurakan Spectral Sky Survey. VII.", "title_create": "Stepanyan+, 1990", "year": "1990", "author": "Stepanyan D.A., Lipovetskii V.A., Erastova L.K.", "title_pub": "Second Byurakan Spectral Sky Survey. VII. Results fo R region centered on alpha=12h00m, delta=+59d00.", "first_author": "Stepanyan D.A.", "ref_biblio": [""], "bibcode": ["1990Ap.....32..252S"], "keyword_cds": "", "abstract": ["The paper gives the seventh list of objects of the Second Byurakan", "Spectral Sky Survey situated in an area measuring 4{deg}x4{deg} with", "coordinates of its center RA=12:00, DE=+59:00. The observations", "were made with the 40\"-52\" Schmidt telescope of the Byurakan", "Astrophysical Observatory with a set of three objective prisms. The", "list contains data on 94 peculiar objects and galaxies and 12 blue", "stars. This part of the survey has revealed II QSOs, two galaxies", "exhibiting Seyfert features, 20 BSOs, 29 galaxies with appreciable", "ultraviolet continuum, and 34 emission galaxies without significant", "ultraviolet radiation. The surface density of QSOs and Seyferts in the", "investigated area is about unity, while for emission galaxies it is of", "the order of four per square degree down to the 19th magnitude."], "object": [], "curator": "Alexandra Bauer, Patricia Vannier [CDS]", "doi_pub": ["10.1007/BF01005507"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_Ap_43.413"}} {"id": "J/other/Ap/43.413", "title_cds": "Ellipticity of nearby elliptical galaxies", "title_create": "Andreasyan+, 2000", "year": "2000", "author": "Andreasyan R.R., Sol H.", "title_pub": "Ellipticity of nearby elliptical galaxies identified with extended extragalactic radio sources.", "first_author": "Andreasyan R.R.", "ref_biblio": [""], "bibcode": ["2000Ap.....43..413A"], "keyword_cds": "Radio sources ; Galaxies, radio ; Morphology", "abstract": ["The dependence of the ellipticity of nearby optical galaxies", "associated with extragalactic radio sources on the type of radio", "galaxy is considered. It is shown that elliptical galaxies identified", "with radio galaxies of the FRI type and with radio sources having a", "radio image with a small elongation have a smaller ellipticity, on the", "average, than those associated with radio galaxies of the FRII type", "and with radio sources with greater elongation. As one possible", "explanation for this phenomenon, one can assume that the optical", "galaxies associated with radio galaxies of type FRI and with radio", "sources of small elongation are oriented in space so that they are", "observed edge-on relatively rarely."], "doi_pub": ["10.1023/A:1010962807367"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Parameters of the radio sources ", "columns": [{"name": "Name", "desc": "Radio source designation (based on B1950 position) "}, {"name": "E", "desc": "Ellipticity "}, {"name": "l_K", "desc": "Limit flag on K "}, {"name": "K", "desc": "? Ratio of the major to the minor axes "}, {"name": "FR", "desc": "Fanaroff & Riley (1974MNRAS.167p..31F) FR type "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_ApSS_163.275"}} {"id": "J/other/ApSS/163.275", "title_cds": "UV & Geneva photometry around HD 173009", "title_create": "Reichen+, 1990", "year": "1990", "author": "Reichen M., Lanz T., Golay M., Huguenin D.", "title_pub": "A detailed study of a 6{deg} diameter field in Scutum. I. Data presentation and overall description of the interstellar matter distribution.", "first_author": "Reichen M.", "ref_biblio": [""], "bibcode": ["1990Ap&SS.163..275R"], "see_also": ["II/59 : Catalogue of stellar UV fluxes (TD1) (Thompson+ 1978)"], "keyword_cds": "Surveys ; Photometry, ultraviolet ; Photometry, Geneva ; MK spectral classification", "abstract": ["A 6{deg} diameter field centered on the star {epsilon} Scutum has been", "selected from the SCAP-2000 balloon-borne UV survey for its high", "apparent stellar density contrast and relatively good transparency on", "a small projected portion of the galactic plane. In view of a detailed", "study of the absorption and interstellar matter distribution in this", "field, a large collection of data has been made and is presented here.", "Ultraviolet magnitudes at 2000{AA} have been obtained from the", "reduction of three SCAP frames. In addition, 322 stars among the 487", "stars detected on the UV frames have been measured in the Geneva", "photometric system. For a small number of photometrically distant", "objects, medium resolution spectra have been obtained in order to", "determine spectral types and confirm the distances determination. An", "overall description of the distribution of interstellar material in", "the ultraviolet is made using star counting methods, and is confronted", "to similar studies in the visible range. A discussion of the", "variations of the extinction law in different parts of the field is", "made. A new distance determination of the Sct OB2 association is", "proposed, as well as a list of additional probable members of the", "association. A certain number of distant hot stars seem to indicate", "the presence of an unknown OB association at the edge of the Scutum", "spiral arm, at a distance of over 3 kpc from the Sun."], "doi_pub": ["10.1007/BF00655749"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Calibration stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (see Table2) "}, {"name": "Name", "desc": "HD, BD or CSI identification "}, {"name": "SpType", "desc": "Spectral type (see table 2) "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude from the Geneva system"}, {"name": "UVmag", "desc": "UV magnitude at 2000{AA} deduced from calibration"}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag "}, {"name": "n_UVmag", "desc": "[abcd ] Note on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965{AA} passband of the TD1 catalogue (Thompson et al., 1978, Cat. ). (2)"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "n_UVmagTD1", "desc": "[)] ) indicates that the UV magnitude UVmagboxes was preferred for the calibration"}, {"name": "UVmagboxes", "desc": "UV magnitude deduced by the method of the so-called \"photometric boxes\" (see text.) (3)"}, {"name": "e_UVmagboxes", "desc": "rms uncertainty on UVmagboxes "}, {"name": "n_UVmagboxes", "desc": "[)] ) indicates that the UV magnitude UVmagTD1 was preferred for the calibration"}, {"name": "N", "desc": "Number of stars in the photometric box "}, {"name": "Rem", "desc": "Remarks related to the UV_TD1_ magnitudes (G2) "}]}, {"name": "table2.dat", "desc": "All stars measured on SCAP frames 11.65/14.48/14.49 ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (1) "}, {"name": "n_SCAP", "desc": "[* o] \"*\" star measured in the Geneva system (see Table 3) \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[+*] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (see Table 3) "}, {"name": "Vmag", "desc": "? Visual magnitude (3) "}, {"name": "UVmag", "desc": "UV magnitude at 2000A from the SCAP frames "}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag (4) "}, {"name": "n_UVmag", "desc": "[abcd ] Notes on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965A passband of the TD1 catalogue (Thompson et al., 1978, )"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "UV-V", "desc": "? (UVmag-Vmag) color index "}, {"name": "(UV-V)0", "desc": "? Intrinsic (UV-V)_0_ color index taken from Carnochan (1982) following the MK, photometric or other spectra type"}, {"name": "E(UV-V)", "desc": "? UV color excess (from (UV-V) and (UV-V)0) "}, {"name": "Rem", "desc": "Various remarks and comments (G2) "}]}, {"name": "table3.dat", "desc": "All stars with Geneva photometry ", "columns": [{"name": "SCAP", "desc": "SCAP identification (see Table 2) "}, {"name": "n_SCAP", "desc": "[o] \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[*+] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "GLONd", "desc": "Galactic longitude "}, {"name": "GLONm", "desc": "Galactic longitude "}, {"name": "GLATd", "desc": "Galactic latitude "}, {"name": "GLATm", "desc": "Galactic latitude "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (1) "}, {"name": "[U-B]", "desc": "Geneva [U-B] colour index "}, {"name": "[B-V]", "desc": "Geneva [B-V] colour index "}, {"name": "[B1-B]", "desc": "Geneva [B1-B] colour index "}, {"name": "[B2-B]", "desc": "Geneva [B2-B] colour index "}, {"name": "[V1-B]", "desc": "Geneva [V1-B] colour index "}, {"name": "[G-B]", "desc": "Geneva [G-B] colour index "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude "}, {"name": "E[B-V]", "desc": "? Color excess deduced from the X,Y,Z parameters (Cramer, 1982A&A...112..330C) unless stated otherwise in the remarks"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters (Cramer and Maeder, 1979A&A....78..305C) unless stated otherwise in the remarks"}, {"name": "r", "desc": "? Decuced heliocentric distance "}, {"name": "Rem", "desc": "Various remarks (2) "}]}, {"name": "table4.dat", "desc": "Spectroscopic standard stars ", "columns": [{"name": "HD", "desc": "HD identification "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "? Visible absorption derived from E[B-V]. "}, {"name": "n_AV", "desc": "[)] ): values deduced from Johnson's U-B/B-V diagram"}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypeH", "desc": "Spectral type given by Houk and Cowley (1975, ) or Houk (1978, , 1982, )"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHg", "desc": "Equivalent width of the H{gamma} line derived from our spectroscopic observations"}, {"name": "VMAGHg", "desc": "Absolute magnitude derived from EW_H{gamma}_ using calibrations by Millward and Walker (1985ApJS...57...63M) or Hill et al. (1986PASP...98.1186H)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}]}, {"name": "table5.dat", "desc": "Spectroscopy of Scutum field stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "Visible absorption derived from E[B-V] "}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHa", "desc": "Equivalent width of the H{alpha} line derived from our spectroscopic observations"}, {"name": "u_EWHa", "desc": "[)] Uncertainty flag on EWHa "}, {"name": "VMAGHa", "desc": "? Absolute magnitude derived from EW_H{alpha}_ (See notes to Table 4)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}, {"name": "Rem", "desc": "Individual remarks (1) "}]}, {"name": "notes2.dat", "desc": "Individual notes to table2.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "notes3.dat", "desc": "Individual notes to table3.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AstBu_64.123_o64.123"}} {"id": "J/other/AstBu/64.123", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. I: Construction of the sample.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..123K"], "see_also": ["J/other/AstBu/64.276 : Paper II. Photometry (Khabibullina+, 2009)", "J/other/AstBu/64.357 : Paper III. Sizes & flux densities (Khabibullina+, 2009)", "ftp://cats.sao.ru/pub/CATS/RGLIST : CATS Home Page"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio", "keyword_pub": "elliptical galaxies - quasars - active or peculiar galaxies, objects, and systems - radio galaxies - statistical and correlative studies of properties - radio sources - observational cosmology", "abstract": ["The procedure of the construction of a sample of distant (z>0.3)", "radio galaxies using NED, SDSS, and CATS databases for further", "application in statistical tests is described. The sample is assumed", "to be cleaned from objects with quasar properties. Primary statistical", "analysis of the list is performed and the regression dependence of the", "spectral index on redshift is found."], "date_update": "09-Dec-2009", "tables": [{"name": "table1.dat", "desc": "Spectral indexes and redshifts for 2442 galaxies ", "columns": [{"name": "Name", "desc": "Name of the source catalog or source name (1) "}, {"name": "n_Name", "desc": "Note on source (2) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "alf1", "desc": "? Spectral index for frequency 325MHz (3) "}, {"name": "alf2", "desc": "? Spectral index for frequency 1400MHz (3) "}, {"name": "alf3", "desc": "? Spectral index for frequency 4850MHz (3) "}, {"name": "z", "desc": "Spectroscopic redshift "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AstBu_64.123_o64.276"}} {"id": "J/other/AstBu/64.276", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. II: Photometric data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..276K"], "see_also": ["J/other/AstBu/64.123 : Paper I. Sample (Khabibullina+, 2009)", "J/other/AstBu/64.357 : Paper III. Sizes & flux densities (Khabibullina+, 2009)", "ftp://cats.sao.ru/pub/cats/RGLIST : Catalog Home Page"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio ; Galaxies, photometry", "keyword_pub": "astronomical catalogs - elliptical galaxies - active or peculiar galaxies, objects, and systems - radio galaxies - magnitudes and colors - radio sources - cosmology", "abstract": ["We describe the procedure of the construction of a sample of distant", "(z>0.3) radio galaxies using the NED, SDSS, and CATS databases. We", "believe the sample to be free of objects with quasar properties. This", "paper is the second part of the description of the radio galaxies", "catalog we plan to use for cosmological tests. We report the", "photometric parameters for the objects of the list, and perform its", "preliminary statistical analysis including the construction of the", "Hubble diagrams."], "date_update": "12-Nov-2009", "tables": [{"name": "table2.dat", "desc": "Magnitudes for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "Name", "desc": "Name of galaxies "}, {"name": "Band1", "desc": "Band name (1) "}, {"name": "l_mag1", "desc": "[=>] Limit flag on Band1 "}, {"name": "mag1", "desc": "? Magnitude in mag1 "}, {"name": "e_mag1", "desc": "? rms uncertainty on mag1 "}, {"name": "u_mag1", "desc": "[)] Uncertainty flag on mag1 "}, {"name": "Band2", "desc": "Band name (1) "}, {"name": "l_mag2", "desc": "[=>] Limit flag on mag2 "}, {"name": "mag2", "desc": "? Magnitude in Band2 "}, {"name": "e_mag2", "desc": "? rms uncertainty on mag2 "}, {"name": "u_mag2", "desc": "[)] Uncertainty flag on mag2 "}, {"name": "Band3", "desc": "Band name (1) "}, {"name": "l_mag3", "desc": "[=>] Limit flag on mag3 "}, {"name": "mag3", "desc": "? Magnitude in Band3 "}, {"name": "e_mag3", "desc": "? rms uncertainty on mag3 "}, {"name": "Band4", "desc": "Band name (1) "}, {"name": "l_mag4", "desc": "[=><] Limit flag on mag4 "}, {"name": "mag4", "desc": "? Magnitude in Band4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "Band5", "desc": "Band name (1) "}, {"name": "l_mag5", "desc": "[=>] Limit flag on mag5 "}, {"name": "mag5", "desc": "? Magnitude in Band5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "Band6", "desc": "Band name (1) "}, {"name": "l_mag6", "desc": "[=>] Limit flag on mag6 "}, {"name": "mag6", "desc": "? 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Magnitude in Band10 "}, {"name": "Band11", "desc": "Band name (1) "}, {"name": "l_mag11", "desc": "[=>] Limit flag on mag11 "}, {"name": "mag11", "desc": "? Magnitude in Band11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AstBu_64.123_o64.357"}} {"id": "J/other/AstBu/64.357", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. III: Sizes and flux density according to the NVSS data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..357K"], "see_also": ["J/other/AstBu/64.123 : Spectral indexes and redshifts (I) (Khabibullina+, 2009)", "J/other/AstBu/64.276 : Magnitudes (II) (Khabibullina+, 2009)"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio ; Redshifts", "keyword_pub": "radio galaxies - spatial distribution of galaxies - radio sources - observational cosmology", "abstract": ["We describe the procedure of the construction of a sample of distant", "(z>0.3) radio galaxies using the NED, CATS and SDSS databases for", "further use in various statistical tests. We believe the sample to be", "free of objects with quasar properties. This paper is the third part", "of the description of the radio galaxies catalog that we plan to use", "for cosmological tests. We report the results of the sample of angular", "sizes for the NVSS survey list objects, and its preliminary", "statistical analysis. Three-parameter diagrams \"angular", "size-redshift-flux density\" and \"angular size-redshift-spectral", "index\", and their two-parameter projections are constructed. Three", "subsamples of radio galaxies are separated in the \"source size-flux", "density\" diagram."], "date_update": "12-Nov-2009", "tables": [{"name": "table3.dat", "desc": "Sizes and flux density for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "RAh", "desc": "? NVSS Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "? NVSS Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "? NVSS Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? NVSS Declination J2000 (degrees) "}, {"name": "DEm", "desc": "? NVSS Declination J2000 (minutes) "}, {"name": "DEs", "desc": "? NVSS Declination J2000 (seconds) "}, {"name": "l_MajAxis", "desc": "Limit flag on MajAxis "}, {"name": "MajAxis", "desc": "? Max diameter of source in arcsec (NVSS) "}, {"name": "l_MinAxis", "desc": "Limit flag on MinAxis "}, {"name": "MinAxis", "desc": "? Min diameter of source in arcsec (NVSS) "}, {"name": "Flux", "desc": "? 1.4GHz flux density of source (NVSS) "}, {"name": "z", "desc": "Redshift "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AstBu_64.276_o64.123"}} {"id": "J/other/AstBu/64.123", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. I: Construction of the sample.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..123K"], "see_also": ["J/other/AstBu/64.276 : Paper II. Photometry (Khabibullina+, 2009)", "J/other/AstBu/64.357 : Paper III. Sizes & flux densities (Khabibullina+, 2009)", "ftp://cats.sao.ru/pub/CATS/RGLIST : CATS Home Page"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio", "keyword_pub": "elliptical galaxies - quasars - active or peculiar galaxies, objects, and systems - radio galaxies - statistical and correlative studies of properties - radio sources - observational cosmology", "abstract": ["The procedure of the construction of a sample of distant (z>0.3)", "radio galaxies using NED, SDSS, and CATS databases for further", "application in statistical tests is described. The sample is assumed", "to be cleaned from objects with quasar properties. Primary statistical", "analysis of the list is performed and the regression dependence of the", "spectral index on redshift is found."], "date_update": "09-Dec-2009", "tables": [{"name": "table1.dat", "desc": "Spectral indexes and redshifts for 2442 galaxies ", "columns": [{"name": "Name", "desc": "Name of the source catalog or source name (1) "}, {"name": "n_Name", "desc": "Note on source (2) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "alf1", "desc": "? Spectral index for frequency 325MHz (3) "}, {"name": "alf2", "desc": "? Spectral index for frequency 1400MHz (3) "}, {"name": "alf3", "desc": "? Spectral index for frequency 4850MHz (3) "}, {"name": "z", "desc": "Spectroscopic redshift "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AstBu_64.276_o64.276"}} {"id": "J/other/AstBu/64.276", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. II: Photometric data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..276K"], "see_also": ["J/other/AstBu/64.123 : Paper I. Sample (Khabibullina+, 2009)", "J/other/AstBu/64.357 : Paper III. 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We report the", "photometric parameters for the objects of the list, and perform its", "preliminary statistical analysis including the construction of the", "Hubble diagrams."], "date_update": "12-Nov-2009", "tables": [{"name": "table2.dat", "desc": "Magnitudes for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "Name", "desc": "Name of galaxies "}, {"name": "Band1", "desc": "Band name (1) "}, {"name": "l_mag1", "desc": "[=>] Limit flag on Band1 "}, {"name": "mag1", "desc": "? Magnitude in mag1 "}, {"name": "e_mag1", "desc": "? rms uncertainty on mag1 "}, {"name": "u_mag1", "desc": "[)] Uncertainty flag on mag1 "}, {"name": "Band2", "desc": "Band name (1) "}, {"name": "l_mag2", "desc": "[=>] Limit flag on mag2 "}, {"name": "mag2", "desc": "? Magnitude in Band2 "}, {"name": "e_mag2", "desc": "? rms uncertainty on mag2 "}, {"name": "u_mag2", "desc": "[)] Uncertainty flag on mag2 "}, {"name": "Band3", "desc": "Band name (1) "}, {"name": "l_mag3", "desc": "[=>] Limit flag on mag3 "}, {"name": "mag3", "desc": "? Magnitude in Band3 "}, {"name": "e_mag3", "desc": "? rms uncertainty on mag3 "}, {"name": "Band4", "desc": "Band name (1) "}, {"name": "l_mag4", "desc": "[=><] Limit flag on mag4 "}, {"name": "mag4", "desc": "? Magnitude in Band4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "Band5", "desc": "Band name (1) "}, {"name": "l_mag5", "desc": "[=>] Limit flag on mag5 "}, {"name": "mag5", "desc": "? Magnitude in Band5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "Band6", "desc": "Band name (1) "}, {"name": "l_mag6", "desc": "[=>] Limit flag on mag6 "}, {"name": "mag6", "desc": "? Magnitude in Band6 "}, {"name": "e_mag6", "desc": "? rms uncertainty on mag6 "}, {"name": "Band7", "desc": "Band name (1) "}, {"name": "l_mag7", "desc": "[=>] Limit flag on mag7 "}, {"name": "mag7", "desc": "? Magnitude in Band7 "}, {"name": "e_mag7", "desc": "? rms uncertainty on mag7 "}, {"name": "Band8", "desc": "Band name (1) "}, {"name": "l_mag8", "desc": "[=>] Limit flag on mag8 "}, {"name": "mag8", "desc": "? Magnitude in Band8 "}, {"name": "e_mag8", "desc": "? rms uncertainty on mag8 "}, {"name": "Band9", "desc": "Band name (1) "}, {"name": "l_mag9", "desc": "[=>] Limit flag on mag9 "}, {"name": "mag9", "desc": "? Magnitude in Band9 "}, {"name": "e_mag9", "desc": "? rms uncertainty on mag9 "}, {"name": "Band10", "desc": "Band name (1) "}, {"name": "l_mag10", "desc": "[=>] Limit flag on mag10 "}, {"name": "mag10", "desc": "? Magnitude in Band10 "}, {"name": "Band11", "desc": "Band name (1) "}, {"name": "l_mag11", "desc": "[=>] Limit flag on mag11 "}, {"name": "mag11", "desc": "? Magnitude in Band11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AstBu_64.276_o64.357"}} {"id": "J/other/AstBu/64.357", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. III: Sizes and flux density according to the NVSS data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..357K"], "see_also": ["J/other/AstBu/64.123 : Spectral indexes and redshifts (I) (Khabibullina+, 2009)", "J/other/AstBu/64.276 : Magnitudes (II) (Khabibullina+, 2009)"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio ; Redshifts", "keyword_pub": "radio galaxies - spatial distribution of galaxies - radio sources - observational cosmology", "abstract": ["We describe the procedure of the construction of a sample of distant", "(z>0.3) radio galaxies using the NED, CATS and SDSS databases for", "further use in various statistical tests. We believe the sample to be", "free of objects with quasar properties. This paper is the third part", "of the description of the radio galaxies catalog that we plan to use", "for cosmological tests. We report the results of the sample of angular", "sizes for the NVSS survey list objects, and its preliminary", "statistical analysis. Three-parameter diagrams \"angular", "size-redshift-flux density\" and \"angular size-redshift-spectral", "index\", and their two-parameter projections are constructed. Three", "subsamples of radio galaxies are separated in the \"source size-flux", "density\" diagram."], "date_update": "12-Nov-2009", "tables": [{"name": "table3.dat", "desc": "Sizes and flux density for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "RAh", "desc": "? NVSS Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "? NVSS Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "? NVSS Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? NVSS Declination J2000 (degrees) "}, {"name": "DEm", "desc": "? NVSS Declination J2000 (minutes) "}, {"name": "DEs", "desc": "? NVSS Declination J2000 (seconds) "}, {"name": "l_MajAxis", "desc": "Limit flag on MajAxis "}, {"name": "MajAxis", "desc": "? Max diameter of source in arcsec (NVSS) "}, {"name": "l_MinAxis", "desc": "Limit flag on MinAxis "}, {"name": "MinAxis", "desc": "? Min diameter of source in arcsec (NVSS) "}, {"name": "Flux", "desc": "? 1.4GHz flux density of source (NVSS) "}, {"name": "z", "desc": "Redshift "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AstBu_64.357_o64.123"}} {"id": "J/other/AstBu/64.123", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. 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Primary statistical", "analysis of the list is performed and the regression dependence of the", "spectral index on redshift is found."], "date_update": "09-Dec-2009", "tables": [{"name": "table1.dat", "desc": "Spectral indexes and redshifts for 2442 galaxies ", "columns": [{"name": "Name", "desc": "Name of the source catalog or source name (1) "}, {"name": "n_Name", "desc": "Note on source (2) "}, {"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "Declination J2000 (seconds) "}, {"name": "alf1", "desc": "? Spectral index for frequency 325MHz (3) "}, {"name": "alf2", "desc": "? Spectral index for frequency 1400MHz (3) "}, {"name": "alf3", "desc": "? Spectral index for frequency 4850MHz (3) "}, {"name": "z", "desc": "Spectroscopic redshift "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AstBu_64.357_o64.276"}} {"id": "J/other/AstBu/64.276", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. II: Photometric data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..276K"], "see_also": ["J/other/AstBu/64.123 : Paper I. Sample (Khabibullina+, 2009)", "J/other/AstBu/64.357 : Paper III. 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We report the", "photometric parameters for the objects of the list, and perform its", "preliminary statistical analysis including the construction of the", "Hubble diagrams."], "date_update": "12-Nov-2009", "tables": [{"name": "table2.dat", "desc": "Magnitudes for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "Name", "desc": "Name of galaxies "}, {"name": "Band1", "desc": "Band name (1) "}, {"name": "l_mag1", "desc": "[=>] Limit flag on Band1 "}, {"name": "mag1", "desc": "? Magnitude in mag1 "}, {"name": "e_mag1", "desc": "? rms uncertainty on mag1 "}, {"name": "u_mag1", "desc": "[)] Uncertainty flag on mag1 "}, {"name": "Band2", "desc": "Band name (1) "}, {"name": "l_mag2", "desc": "[=>] Limit flag on mag2 "}, {"name": "mag2", "desc": "? Magnitude in Band2 "}, {"name": "e_mag2", "desc": "? rms uncertainty on mag2 "}, {"name": "u_mag2", "desc": "[)] Uncertainty flag on mag2 "}, {"name": "Band3", "desc": "Band name (1) "}, {"name": "l_mag3", "desc": "[=>] Limit flag on mag3 "}, {"name": "mag3", "desc": "? Magnitude in Band3 "}, {"name": "e_mag3", "desc": "? rms uncertainty on mag3 "}, {"name": "Band4", "desc": "Band name (1) "}, {"name": "l_mag4", "desc": "[=><] Limit flag on mag4 "}, {"name": "mag4", "desc": "? Magnitude in Band4 "}, {"name": "e_mag4", "desc": "? rms uncertainty on mag4 "}, {"name": "Band5", "desc": "Band name (1) "}, {"name": "l_mag5", "desc": "[=>] Limit flag on mag5 "}, {"name": "mag5", "desc": "? Magnitude in Band5 "}, {"name": "e_mag5", "desc": "? rms uncertainty on mag5 "}, {"name": "Band6", "desc": "Band name (1) "}, {"name": "l_mag6", "desc": "[=>] Limit flag on mag6 "}, {"name": "mag6", "desc": "? 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Magnitude in Band10 "}, {"name": "Band11", "desc": "Band name (1) "}, {"name": "l_mag11", "desc": "[=>] Limit flag on mag11 "}, {"name": "mag11", "desc": "? Magnitude in Band11 "}, {"name": "e_mag11", "desc": "? rms uncertainty on mag11 "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AstBu_64.357_o64.357"}} {"id": "J/other/AstBu/64.357", "title_cds": "Catalog of radio galaxies with z>0.3", "title_create": "Khabibullina+, 2009", "year": "2009", "author": "Khabibullina M.L., Verkhodanov O.V.", "title_pub": "Catalog of radio galaxies with z>0.3. III: Sizes and flux density according to the NVSS data.", "first_author": "Khabibullina M.L.", "ref_biblio": [""], "bibcode": ["2009AstBu..64..357K"], "see_also": ["J/other/AstBu/64.123 : Spectral indexes and redshifts (I) (Khabibullina+, 2009)", "J/other/AstBu/64.276 : Magnitudes (II) (Khabibullina+, 2009)"], "keyword_cds": "Galaxy catalogs ; Galaxies, radio ; Redshifts", "keyword_pub": "radio galaxies - spatial distribution of galaxies - radio sources - observational cosmology", "abstract": ["We describe the procedure of the construction of a sample of distant", "(z>0.3) radio galaxies using the NED, CATS and SDSS databases for", "further use in various statistical tests. We believe the sample to be", "free of objects with quasar properties. This paper is the third part", "of the description of the radio galaxies catalog that we plan to use", "for cosmological tests. We report the results of the sample of angular", "sizes for the NVSS survey list objects, and its preliminary", "statistical analysis. Three-parameter diagrams \"angular", "size-redshift-flux density\" and \"angular size-redshift-spectral", "index\", and their two-parameter projections are constructed. Three", "subsamples of radio galaxies are separated in the \"source size-flux", "density\" diagram."], "date_update": "12-Nov-2009", "tables": [{"name": "table3.dat", "desc": "Sizes and flux density for 2442 galaxies ", "columns": [{"name": "GName", "desc": "Name of galaxies as coordinates (HHMMSS+DDMMSS, J2000)"}, {"name": "RAh", "desc": "? NVSS Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "? NVSS Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "? NVSS Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "? NVSS Declination J2000 (degrees) "}, {"name": "DEm", "desc": "? NVSS Declination J2000 (minutes) "}, {"name": "DEs", "desc": "? NVSS Declination J2000 (seconds) "}, {"name": "l_MajAxis", "desc": "Limit flag on MajAxis "}, {"name": "MajAxis", "desc": "? Max diameter of source in arcsec (NVSS) "}, {"name": "l_MinAxis", "desc": "Limit flag on MinAxis "}, {"name": "MinAxis", "desc": "? Min diameter of source in arcsec (NVSS) "}, {"name": "Flux", "desc": "? 1.4GHz flux density of source (NVSS) "}, {"name": "z", "desc": "Redshift "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AuJPA_14.1"}} {"id": "J/other/AuJPA/14.1", "title_cds": "5000MHz galactic radio sources", "title_create": "Goss+, 1970", "year": "1970", "author": "Goss W.M., Shaver P.A.", "title_pub": "Galactic radio sources. I. High resolution 5000 MHz observations.", "first_author": "Goss W.M.", "ref_biblio": [""], "bibcode": ["1970AuJPA..14....1G"], "see_also": ["J/other/AuJPA/14.77 : Paper II, 408MHz galactic radio sources (Shaver+ 1970)", "J/other/AuJPA/14.133 : Paper III, galactic radio sources spectra (Shaver+ 1970)"], "keyword_cds": "Radio sources", "abstract": ["Contour maps of 63 regions in the galactic plane are presented. The", "half-power beamwidth was 4'arc at 5000 MHZ. Positions and composite", "flux densities are given for 206 sources."], "data": "", "date_update": "28-Jun-1999", "tables": [{"name": "table1.dat", "desc": "Flux Densities and Positions of Calactic Sources ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "RAh", "desc": "Right ascension (1950.0) "}, {"name": "RAm", "desc": "Right ascension (1950.0) "}, {"name": "RAs", "desc": "Right ascension (1950.0) "}, {"name": "DE-", "desc": "Declination sign (1950.0) "}, {"name": "DEd", "desc": "Declination (1950.0) "}, {"name": "DEm", "desc": "Declination (1950.0) "}, {"name": "Tb", "desc": "? Baselevel (in brightness temperature) above which the composite flux was measured"}, {"name": "n_Tb", "desc": "Note on Tb (1) "}, {"name": "F5GHz", "desc": "? Composite flux at 5000MHz "}, {"name": "n_F5GHz", "desc": "Note on Flux (1) "}, {"name": "FigNo", "desc": "? Number of figure "}, {"name": "Note", "desc": "[a-d] Notes (2) "}, {"name": "Names", "desc": "Other names "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_AuJPA_14.133"}} {"id": "J/other/AuJPA/14.133", "title_cds": "Galactic radio sources. III.", "title_create": "shaver+ 1970", "year": "1970", "author": "Shaver P.A., Goss W.M.", "title_pub": "Galactic radio sources. III. Spectra and physical characteristics", "first_author": "Shaver P.A.", "ref_biblio": [""], "bibcode": ["1970AuJPA..14..133S"], "see_also": ["J/other/AuJPA/14.1 : 5000MHz galactic radio sources (Goss+, 1970)", "J/other/AuJPA/14.77 : 408MHz galactic radio sources (Shaver+ 1970)"], "keyword_cds": "Radio sources", "abstract": ["Spectral indices for over 250 galactic radio sources have been", "determined from high resolution observations at 408 and 5000MHz. About", "14% of the sources have nonthermal spectra. A comparison with results", "from an H109{alpha} line survey shows that the line-to-continuum", "temperature ratios for thermal sources are greater than about 2.5%,", "and no recombination line above the detectable threshold has been", "found in a nonthermal source. A search for optical emission from the", "vicinity of the thermal and nonthermal radio sources resulted in", "positive identifications for one-third of them. In 16 cases the radio", "contours are shown superimposed on optical photographs.", "Electron temperatures have been determined directly from the 408MHz", "brightness distribution for 50 thermal sources and are found to be", "consistent with values obtained from H109{alpha} recombination line", "work, indicating that any departures from local thermodynamic", "equilibrium, and their effects on the recombination lines, are small.", "Physical properties of the thermal sources have been computed assuming", "a spherical HII region model. It is shown that HII regions have a", "strong tendency to cluster, and that the cluster sizes are comparable", "with those of open star clusters. No HII regions were found with", "turnover frequencies greater than 1400MHz, indicating that high", "density sources (N_e_>5x10^3^cm^-3^ over a region >0.1pc in extent)", "are very rare. The largest, least dense HII regions have shell", "structure which is consistent with current ideas about the dynamical", "effects of radiation pressure on the dust within HII regions. Fifteen", "new supernova remnants have been identified and distances and physical", "properties computed for them. For the well-resolved supernova remnants", "the shell thickness is a constant fraction of the diameter. It is", "shown that supernova remnants are frequently located in OB", "associations."], "data": "", "date_update": "08-Jul-1999", "tables": [{"name": "table1.dat", "desc": "Measured continuum data for all sources ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "Tb408MHz", "desc": "? Base-level (in brightness temperature) for 408MHz flux density"}, {"name": "Tp408MHz", "desc": "? Peak temperature for 408MHz flux density "}, {"name": "M1RA", "desc": "? Half-power width in right ascension at 408MHz "}, {"name": "M1DE", "desc": "? Half-power width in declination at 408MHz "}, {"name": "S408MHz", "desc": "? Flux density at 408MHz "}, {"name": "n_S408MHz", "desc": "[+] Note on S408MHz (1) "}, {"name": "Tb5GHz", "desc": "? Base-level (in brightness temperature) for 5GHz flux density"}, {"name": "Tp5GHz", "desc": "? Peak temperature for 5GHz flux density "}, {"name": "M2RA", "desc": "? Half-power width in right ascension at 5GHz "}, {"name": "M2DE", "desc": "? Half-power width in declination at 5GHz "}, {"name": "S5GHz", "desc": "? Flux density a 5GHz "}, {"name": "n_S5GHz", "desc": "[*] *: S5GHz is an upper limit "}, {"name": "C1/C2", "desc": "? Half-power width ratio (2) "}, {"name": "T2/T1", "desc": "? Peak temperature ratio (2) "}, {"name": "e_T2/T1", "desc": "? rms uncertainty on T2/T1 "}, {"name": "Source", "desc": "Nature of source (3) "}, {"name": "l_TL/TC", "desc": "Limit flag on TL/TC "}, {"name": "TL/TC", "desc": "? Line-to-continuum temperature ratio from the H109{alpha} recombination line and 5GHz continuum surveys"}, {"name": "Note", "desc": "[N] N: H109{alpha} line observations have been made in the northern survey"}]}, {"name": "table2.dat", "desc": "Flux Densities from Other References ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "n_[GS70]", "desc": "[abc] For same letter, the other values are for the group of sources"}, {"name": "Freq", "desc": "Frequency "}, {"name": "l_SFreq", "desc": "[~ <=] Limit flag on SFreq "}, {"name": "SFreq", "desc": "Flux density "}, {"name": "l_SI", "desc": "[<= ] Limit flag on SI "}, {"name": "SI", "desc": "? Spectral index (1) "}, {"name": "n_SI", "desc": "[n] n: value not significantly different from zero "}, {"name": "Ref", "desc": "[1/15] Reference (2) "}]}, {"name": "table3.dat", "desc": "Optical identifications ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "n_[GS70]", "desc": "[a-n] Group "}, {"name": "Fig", "desc": "Figure number "}, {"name": "OptID", "desc": "Optical identification, comments "}]}, {"name": "table4.dat", "desc": "Electron Temperatures ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "n_[GS70]", "desc": "[*] *: notes in file notes4.dat "}, {"name": "Tb", "desc": "Base-level of 408MHz maps "}, {"name": "T1b", "desc": "Observed 408MHz peak brightness temperature "}, {"name": "T'1", "desc": "Restored 408MHz peak brightness temperature "}, {"name": "T'2", "desc": "? Restored value of T2 "}, {"name": "l_tau1", "desc": "[<= ] Limit flag on tau1 "}, {"name": "tau1", "desc": "? 408MHz optical depth "}, {"name": "l_Tec", "desc": "[>= ] Limit flag on Tec "}, {"name": "Tec", "desc": "Continuum estimate of electron temperature "}, {"name": "Ter", "desc": "? H109{alpha} line estimate of electron temperature"}, {"name": "l_Tec/Ter", "desc": "[ >=] Limit flag on Tec/Ter "}, {"name": "Tec/Ter", "desc": "? Continuum to H109{alpha} line electron temperature ratio"}]}, {"name": "notes4.dat", "desc": "Individual notes to table4.dat ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "table5.dat", "desc": "Properties of HII Regions ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "W1", "desc": "? 408MHz corrected geometric mean half-power source width"}, {"name": "W2", "desc": "? 5GHz corrected geometric mean half-power source width"}, {"name": "EM", "desc": "? Emission measure "}, {"name": "Te", "desc": "? Electron temperature "}, {"name": "Distn", "desc": "? Near distance "}, {"name": "Diam", "desc": "? Linear diameter "}, {"name": "Ne", "desc": "? Electron density "}, {"name": "Mass", "desc": "? Mass "}, {"name": "U", "desc": "? Excitation parameter "}, {"name": "Disf", "desc": "? Far distance "}, {"name": "DiamC", "desc": "? Linear diameter computed for the spherical model"}, {"name": "NeC", "desc": "? Electron density computed for the spherical model"}, {"name": "MassC", "desc": "? Mass computed for the spherical model "}, {"name": "UC", "desc": "? Excitation parameter computed for the spherical model"}]}, {"name": "table6.dat", "desc": "Unresolved HII Regions ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "Freq", "desc": "? Turnover frequency "}, {"name": "W", "desc": "Computed width "}, {"name": "n_W", "desc": "[*+] Note (1) "}]}, {"name": "table7.dat", "desc": "References for distances of HII Regions ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "n_[GS70]", "desc": "[a-j] Group "}, {"name": "Dist", "desc": "Distance (1) "}, {"name": "Ref", "desc": "References (2) "}]}, {"name": "table8.dat", "desc": "Extragalactic sources ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "l_SI", "desc": "[<= ] Limit flag on SI "}, {"name": "SI", "desc": "Spectral index "}, {"name": "S408MHz", "desc": "408MHz flux density "}]}, {"name": "table9.dat", "desc": "Properties of Supernova Remnants ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "SI", "desc": "Spectral index "}, {"name": "Diam", "desc": "Angular diameter "}, {"name": "S1GHz", "desc": "1GHz flux density "}, {"name": "Dist", "desc": "Distance "}, {"name": "Z", "desc": "Displacement above of below the Galactic Plane "}, {"name": "2R", "desc": "Diameter "}, {"name": "P1GHz", "desc": "Power output at 1GHz "}, {"name": "Power", "desc": "Total power "}]}, {"name": "appen.dat", "desc": "Notes on individual sources ", "columns": [{"name": "[GS70]", "desc": "Galactic source name (GLLL.l+BB.b) "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_BAN_14.265"}} {"id": "J/other/BAN/14.265", "title_cds": "UBV photometry in 3 clusters", "title_create": "Koelbloed+, 1959", "year": "1959", "author": "Koelbloed D.", "title_pub": "Three-colour photometry of the three southern open clusters NGC 3532, 6475 (M7) and 6124.", "first_author": "Koelbloed D.", "ref_biblio": [""], "bibcode": ["1959BAN....14..265K"], "keyword_cds": "Clusters, open ; Photometry, UBV", "keyword_pub": "", "object": ["NGC 6475 (Koelbloed)"], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_BASI_40.65"}} {"id": "J/other/BASI/40.65", "title_cds": "Spatial orientation of galaxies in ZoA", "title_create": "Aryal+, 2012", "year": "2012", "author": "Aryal B., Yadav S.N., Saurer W.", "title_pub": "Spatial orientation of galaxies in the Zone of Avoidance.", "first_author": "Aryal B.", "ref_biblio": [""], "bibcode": ["2012BASI...40...65A"], "see_also": ["J/A+AS/110/269 : Galaxies in the \"zone of avoidance\". I. (Weinberger+, 1995)", "J/A+AS/117/1 : Galaxies in the \"zone of avoidance\". II. (Seeberger+, 1996)", "J/A+AS/117/369 : Galaxies in the \"zone of avoidance\". III. (Lercher+, 1996)", "J/A+AS/126/247 : Galaxies in the \"zone of avoidance\". IV. (Saurer+, 1997)", "J/A+AS/127/101 : Galaxies in the \"zone of avoidance\". V. (Seeberger+ 1998)"], "keyword_cds": "Galaxy catalogs ; Morphology", "keyword_pub": "catalogues - surveys - galaxies: evolution - galaxies: statistics", "abstract": ["We present spatial orientation of spin vectors of galaxies found in", "the region 20{deg}<=l<=80{deg}, -10{deg}<=b<=-5{deg} in the first", "Palomar Observatory Sky Survey. The inclination angle and intrinsic", "flatness of a galaxy are used to determine the spin vector and spin", "vector projections of the galaxy. We studied the preferred alignments", "of spin vectors of galaxies with respect to equatorial, Galactic and", "supergalactic coordinate systems."], "type": ["OC"], "data": "", "date_update": "10-Jul-2012", "tables": [{"name": "table.dat", "desc": "*Position angle (PA) and diameters of the galaxies ", "columns": [{"name": "RAh", "desc": "Right ascension (J2000) "}, {"name": "RAm", "desc": "Right ascension (J2000) "}, {"name": "RAs", "desc": "Right ascension (J2000) "}, {"name": "DE-", "desc": "Declination sign (J2000) "}, {"name": "DEd", "desc": "Declination (J2000) "}, {"name": "DEm", "desc": "Declination (J2000) "}, {"name": "DEs", "desc": "Declination (J2000) "}, {"name": "PA", "desc": "Position angle "}, {"name": "a", "desc": "Semi-major axis "}, {"name": "b", "desc": "Semi-minor axis "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_BSAO_49.53"}} {"id": "J/other/BSAO/49.53", "title_cds": "Catalogue of radio decametric sources", "title_create": "Verkhodanov+, 2000", "year": "2000", "author": "Verkhodanov O.V., Andernach H., Verkhodanova N.V.", "title_pub": "Radio identification of decametric sources. I. Catalogue", "first_author": "Verkhodanov O.V.", "ref_biblio": [""], "bibcode": ["2000BSAO...49...53V"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "James Marcout, Patricia Bauer [CDS]", "data": "", "date_update": "16-Jul-2002"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_ChJAA_2.501"}} {"id": "J/other/ChJAA/2.501", "title_cds": "Seyfert 1 galaxies", "title_create": "Zhou+, 2002", "year": "2002", "author": "Zhou H.-Y., Wang T.-G.", "title_pub": "Properties of broad band continuum of narrow line Seyfert 1 galaxies.", "first_author": "Zhou H.-Y.", "ref_biblio": [""], "bibcode": ["2002ChJAA...2..501Z"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1088/1009-9271/2/6/501"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_CoVVO_2.33"}} {"id": "J/other/CoVVO/2.33", "title_cds": "Southern M-type stars", "title_create": "Lu+, 1984", "year": "1984", "author": "Lu P.K., Macconnell D.J.", "title_pub": "A search for southern M-type stars.", "first_author": "Lu P.K.", "ref_biblio": [""], "bibcode": ["1984CoVVO...2...33L"], "keyword_cds": "Stars, late-type", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_JAD_20.5"}} {"id": "J/other/JAD/20.5", "title_cds": "Detectability of micro-variables in ASAS", "title_create": "David+, 2014", "year": "2014", "author": "David M., Hensberge H., Nitschelm C.", "title_pub": "Detectability of micro-variables in the ASAS database: the Scorpius - Centaurus Complex.", "first_author": "David M.", "ref_biblio": [""], "bibcode": ["2014JAD....20....5D\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "stars: variables: general - techniques: photometric - open clusters and associations: individual: Sco - Cen Complex - stars: individual: HD 46057, HD 146285, HD 116794, HD 119022", "abstract": ["We present a star-by-star discussion of the light variability of stars", "belonging to the Sco-Cen Complex, as detected in the ASAS\u2013V", "database by David et al. (2013A&A...557A..47D). Most of the variables", "(30) are young stars with irregular and/or cyclic patterns of", "variability, almost all with spectral types that indicate that they", "did not yet reach the zero-age main-sequence. The ZAMS starts at A3,", "F2 and F4 for the Upper-Scorpius, the Upper Centaurus-Lupus and the", "Lower Centaurus-Crux subgroups, respectively. A minority of stars (7),", "mainly of spectral type B or late-A, show strictly (multi-)periodic", "variability induced by rigid rotation of a spotted magnetic star, by", "slight deformation of the stellar shape in a binary, or by pulsation", "of stars situated in the instability domain of either SPB, {delta} Sct", "or {gamma} Dor stars. For some stars comments on yet unpublished", "high-resolution spectra are included."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "08-Oct-2016"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_JAD_9.1"}} {"id": "J/other/JAD/9.1", "title_cds": "Munster Red Sky Survey", "title_create": "Seitter+, 2015", "year": "2015", "author": "Seitter W.C., Duerbeck H.W.", "title_pub": "The Munster Red Sky Survey. Large=scale structures in the universe.", "first_author": "Seitter W.C.", "ref_biblio": ["<(various journals) JAD, 9.1 (2015)>"], "bibcode": ["2015other.JAD..9.1.\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "sky surveys: stars - sky surveys: galaxies - CCD photometry: galaxy clusters", "abstract": ["We present"], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "08-Oct-2016"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_JApA_33.227"}} {"id": "J/other/JApA/33.227", "title_cds": "Photoelectric radial velocities", "title_create": "Griffin, 2012", "year": "2012", "author": "Griffin R.F.", "title_pub": "Photoelectric radial velocities. Paper XIX: Additional spectroscopic binaries among the Redman K stars.", "first_author": "Griffin R.F.", "ref_biblio": [""], "bibcode": ["2012JApA...33..227G"], "keyword_cds": "", "keyword_pub": "stars: late-type - stars: radial velocities - spectroscopic binaries - orbits", "mission": "", "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1007/s12036-012-9140-x"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_Nat_585.363"}} {"id": "J/other/Nat/585.363", "title_cds": "WD 1856+534 transit curves", "title_create": "Vanderburg+, 2020", "year": "2020", "author": "Vanderburg A., Rappaport S.A., Xu S., Crossfield I.J.M., Becker J.C., Gary B., Murgas F., Blouin S., Kaye T.G., Palle E., Melis C., Morris B.M., Kreidberg L., Gorjian V., Morley C.V., Mann A.W., Parviainen H., Pearce L.A., Newton E.R., Carrillo A., Zuckerman B., Nelson L., Zeimann G., Brown W.R., Tronsgaard R., Klein B., Ricker G.R., Vanderspek R.K., Latham D.W., Seager S., Winn J.N., Jenkins J.M., Adams F.C., Benneke B., Berardo D., Buchhave L.A., Caldwell D.A., Christiansen J.L., Collins K.A., Colon K.D., Daylan T., Doty J., Doyle A.E., Dragomir D., Dressing C., Dufour P., Fukui A., Glidden A., Guerrero N.M., Guo X., Heng K., Henriksen A.I., Huang C.X., Kaltenegger L., Kane S.R., Lewis J.A., Lissauer J.J., Morales F., Narita N., Pepper J., Rose M.E., Smith J.C., Stassun K.G., Yu L.", "title_pub": "A giant planet candidate transiting a white dwarf.", "first_author": "Vanderburg A.", "ref_biblio": [""], "bibcode": ["2020Natur.585..363V"], "keyword_cds": "Stars, white dwarf ; Spectra, optical ; Photometry, SDSS", "abstract": ["Astronomers have discovered thousands of planets outside the Solar", "System, most of which orbit stars that will eventually evolve into red", "giants and then into white dwarfs. During the red giant phase, any", "close-orbiting planets will be engulfed by the star, but more distant", "planets can survive this phase and remain in orbit around the white", "dwarf. Some white dwarfs show evidence for rocky material floating in", "their atmospheres5, in warm debris disks or orbiting very closely,", "which has been interpreted as the debris of rocky planets that were", "scattered inwards and tidally disrupted. Recently, the discovery of", "a gaseous debris disk with a composition similar to that of ice giant", "planets14 demonstrated that massive planets might also find their way", "into tight orbits around white dwarfs, but it is unclear whether these", "planets can survive the journey. So far, no intact planets have been", "detected in close orbits around white dwarfs. Here we report the", "observation of a giant planet candidate transiting the white dwarf", "WD 1856+534 (TIC 267574918) every 1.4days. We observed and modelled", "the periodic dimming of the white dwarf caused by the planet candidate", "passing in front of the star in its orbit. The planet candidate is", "roughly the same size as Jupiter and is no more than 14 times as", "massive (with 95 per cent confidence). Other cases of white dwarfs", "with close brown dwarf or stellar companions are explained as the", "consequence of common-envelope evolution, wherein the original orbit", "is enveloped during the red giant phase and shrinks owing to friction.", "In this case, however, the long orbital period (compared with other", "white dwarfs with close brown dwarf or stellar companions) and low", "mass of the planet candidate make common-envelope evolution less", "likely. Instead, our findings for the WD 1856+534 system indicate that", "giant planets can be scattered into tight orbits without being tidally", "disrupted, motivating the search for smaller transiting planets around", "white dwarfs."], "description": ["We show spectra from four observatories, using the Low Resolution", "Spectrograph 2 on the Hobby-Eberly Telescope (HET/LRS2), the Gemini", "Near InfraRed Spectrograph on the Gemini North Telescope", "(Gemini/GNIRS), the Kast Double Spectrograph on the Shane Telescope at", "Lick Observatory (Lick/Kast) and the Blue Channel spectrograph at MMT", "Observatory. The data have been scaled to remove offsets in their", "absolute flux calibrations. The optical spectra show a pure continuum,", "confirming the DC spectral classification, whereas the near-infrared", "spectrum from Gemini North shows only spurious features, owing to", "imperfect correction of the telluric absorption and sky emission from", "Earth's atmosphere.", "We show the light curves from TESS; data from several private", "telescopes in Arizona (operated by B.G. and T.G.K.) with odd and", "even-numbered transits shown separately; simultaneous light curves in", "four colours from MuSCAT2; a light curve from the GTC, and a light", "curve from Spitzer. The individual two-minute-cadence TESS flux", "measurements are shown as grey points, and the rose-coloured points", "are averages of the brightness in roughly 30s in orbital phase. The", "TESS data have been corrected for dilution from nearby stars so that", "the transit depth matches that of the GTC data."], "object": ["18 57 39.34 +53 30 33.3 WD 1856+534 = TOI 1690"], "type": ["OC"], "data": "", "date_update": "17-Nov-2020", "tables": [{"name": "fig2.dat", "desc": "Spectroscopic observation of WD 1856+534 ", "columns": [{"name": "lambda", "desc": "Wavelength "}, {"name": "RelFlux", "desc": "? Relative Flux "}, {"name": "Inst", "desc": "Observatory/Spectrograph (1) "}]}, {"name": "fig2ext.dat", "desc": "All transit observation of WD 1856+534 ", "columns": [{"name": "Time", "desc": "Observation date (TDB) "}, {"name": "Relmag", "desc": "Relative Brightness "}, {"name": "Inst", "desc": "Observatory/Filter (1) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_NewA_27.102"}} {"id": "J/other/NewA/27.102", "title_cds": "HAT-P-16b photometric observations", "title_create": "Pearson+, 2014", "year": "2014", "author": "Pearson K.A., Turner J.D., Sagan T.G.", "title_pub": "Photometric observation of HAT-P-16b in the near-UV.", "first_author": "Pearson K.A.", "ref_biblio": [""], "bibcode": ["2014NewA...27..102P"], "keyword_cds": "", "keyword_pub": "planetary systems - techniques: photometric - planets and satellites: magnetic fields", "abstract": ["We present the first primary transit light curve of the hot Jupiter", "HAT-P-16b in the near-UV photometric band. We observed this object on", "December 29, 2012 in order to update the transit ephemeris, constrain", "its planetary parameters and search for magnetic field interference.", "Vidotto et al. (2011MNRAS.414.1573V) postulate that the magnetic field", "of HAT-P-16b can be constrained if its near-UV light curve shows an", "early ingress compared to its optical light curve, while its egress", "remains unchanged. However, we did not detect an early ingress in our", "night of observing when using a cadence of 60 seconds and an average", "photometric precision of 2.26 mmag. We find a near-UV planetary radius", "of Rp=1.274+/-0.057R_Jup_ which is consistent with its near-IR radius", "of Rp=1.289+/-0.066R_Jup_ (Buchhave et al., 2010, Cat.", "J/ApJ/720/1118). We developed an automated reduction pipeline and a", "modeling package to process our data. The data reduction package", "synthesizes a set of IRAF scripts to calibrate images and perform", "aperture photometry. The modeling package utilizes the", "Levenberg\u2013Marquardt minimization algorithm to find a least-squares", "best fit and a differential evolution Markov Chain Monte Carlo", "algorithm to find the best fit to the light curve. To constrain the", "red noise in both fitting models we use the residual permutation", "(rosary bead) method and time-averaging method."], "description": ["Our observation was conducted on December 29, 2012 at the Steward", "Observatory 1.55-m Kuiper Telescope on Mt. Bigelow, using the Mont4k", "CCD. The Mont4k CCD contains a 4096x4096 pixel sensor with a field", "of view (FOV) of 9.7arcminx9.7arcmin."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1016/j.newast.2013.08.002"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_NewA_34.27"}} {"id": "J/other/NewA/34.27", "title_cds": "Sh2-311 region deep optical survey", "title_create": "Yadav+, 2015", "year": "2015", "author": "Yadav R.K., Pandey A.K., Sharma S., Jose J., Ogura K., Kobayashi N., Samal M.R., Eswaraiah C., Chandola H.C.", "title_pub": "Deep optical survey of the stellar content of Sh2-311 region.", "first_author": "Yadav R.K.", "ref_biblio": [""], "bibcode": ["2015NewA...34...27Y"], "keyword_cds": "", "keyword_pub": "stars: clusters - star clusters: individual (Haffner 18, Haffner 19 and NGC 2467) - stars: pre-main sequence - stars: formation", "abstract": ["The stellar content in and around Sh2-311 region have been studied", "using the deep optical observations as well as near-infrared (NIR)", "data from 2MASS. The region contains three clusters, viz. NGC 2467,", "Haffner 18 and Haffner 19. We have made an attempt to distinguish the", "stellar content of these individual regions as well as to re-determine", "their fundamental parameters such as distance, reddening, age, onto", "the basis of a new and more extended optical and infrared photometric", "data set. NGC 2467 and Haffner 19 are found to be located in the", "Perseus arm at the distances of 5.0+/-0.4kpc and 5.7+/-0.4kpc,", "respectively, whereas Haffner 18 is located at the distance of", "11.2+/-1.0kpc. The clusters NGC 2467 and Haffner 19 might have formed", "from the same molecular cloud, whereas the cluster Haffner 18 is", "located in the outer galactic arm, i.e. the Norma\u2013Cygnus arm. We", "identify 8 class II young stellar objects (YSOs) using the NIR", "(J-H)/(H-K)(J-H)/(H-K) two colour diagram. We have estimated the age", "and mass of the YSOs identified in the present work and those by", "Snider et al. (2009) using the V/(V-I)V/(V-I) colour-magnitude", "diagram. The estimated ages and mass range of the majority of the YSOs", "are <~1Myr and ~0.4-3.5M_{sun}_, respectively, indicating that these", "sources could be T-Tauri stars or their siblings. Spatial distribution", "of the YSOs shows that some of the YSOs are distributed around the Hii", "region Sh2-311, suggesting a triggered star formation at its", "periphery."], "description": ["The data used in this work are a combination of archived optical UBVI", "images taken with the Wide Field Imager (WFI) camera at the 2.2-m MPG", "Telescope of the European Southern Observatory (ESO) and NIR data from", "the 2MASS Point Source catalogue (Cutri et al., 2003, Cat. II/246)", "available on the WEB. Low resolution spectroscopic observation of", "three stars were also taken using the 2.0-m Himalayan Chandra", "Telescope (HCT) of Indian Astronomical Observatory (IAO), Hanle.", "The archived optical observations of Sh2-311 region used in this study", "were taken using the WFI camera (PI: Rubio, M.) mounted at the", "Cassegrain focus of the ESO 2.2-m Telescope."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1016/j.newast.2014.05.004"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_NewA_52.96"}} {"id": "J/other/NewA/52.96", "title_cds": "Short Title", "title_create": "Cakirli+, 2017", "year": "2017", "author": "Cakirli O., Ibanoglu C., Sipahi E., Akan M.C.", "title_pub": "V850 Cyg: An eclipsing binary with a giant {gamma} Dor pulsator.", "first_author": "Cakirli O.", "ref_biblio": [""], "bibcode": ["2017NewA...52...96C"], "keyword_cds": "", "keyword_pub": "stars: fundamental parameters - stars: individual: V850 Cyg - binaries: eclipses", "abstract": ["We present new spectroscopic observations of the double-lined", "eclipsing binary V850 Cyg. The long-cadence photometric observations", "obtained by Kepler were analysed and combined with the analysis of", "radial velocities for deriving the absolute parameters of the", "components. Masses and radii were determined as", "Mp=1.601+/-0.076M_{sun}_ and Rp=4.239+/-0.076R_{sun}_,", "Ms=0.851+/-0.053M_{sun}_ and Rs=5.054+/-0.087R_{sun}_ for the", "components of V850 Cyg. We estimate an interstellar reddening of", "0.28+/-0.12mag and a distance of 1040+/-160pc for the system. The", "measured rotational velocity of the secondary appears to lower than", "that of synchronize rotation. However its spectral lines are too weak", "to be measured the rotational velocity with reasonable accuracy. We", "have extracted the synthetic light curve from the observations and", "excluded the data within the eclipses for the frequency analysis. We", "obtained at least nine frequencies in the {gamma} Dor regime. It seems", "that the primary component oscillates with a dominant period of about", "1.152549+/-0.000009-days. We also compare pulsational properties of", "the primary star of V850 Cyg with the {gamma} Dor type pulsating", "components in other binaries."], "description": ["V850 Cyg was observed in both long- and short-cadence by the Kepler", "satellite. Detailed descriptions of the characteristics of these", "observations can be found in Slawson (2011, Cat. J/AJ/142/160). The", "short-cadence observations comprise about 24,000 data points obtained", "in the Quarters 0, 1, 2a, 2b, 2c, 3a, 3b, 3c, 4a, 4b, 4c, 8, 12, and", "16, and the long-cadence data encompass 57,535 data points in the", "Quarters 0,... ,17 obtained over four years. The corrected flux", "measurements were used in our analysis. The times of the observational", "data are transformed to the heliocentric Julian dates and the flux", "measurements converted to Kepler magnitude scale."], "object": [], "curator": "Patricia Vannier [CDS]", "doi_pub": ["10.1016/j.newast.2016.10.008"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_OEJV_185"}} {"id": "J/other/OEJV/185", "title_cds": "Short Title", "title_create": "Author+, ", "title_pub": "CzeV - The Czech Variable Star Catalogue.", "first_author": "Skarka M.", "author": "Skarka M., Masek M., Brat L., Cagas Pa., Jurysek J., Honkova K., Zejda M., Smelcer L., Jelinek M., Lomoz F., Tylsar M., Trnka J., Pejcha O., Pintr P., Lehky M., Janik J., Cervinka L., Pribik V., Motl D., Walter F., Zasche P., Koss K., Hajek P., Bilek F., Liska J., Kucakova H., Bodnar F., Beranek J., Safar J., Moudra M., Orsulak M., Pintr M., Sobotka P., Dreveny R., Juranova A., Polak J., Polster J., Onderkova K., Smolka M., Auer R.F., Kocian R., Hladik B., Cagas P., Gres A., Muller D., Capkova H., Kysely J., Hornoch K., Truparova K., Timko L., Broz M., Bilek M., Sebela P., Hanzl D., Zampachova E., Secka J., Pravec , P., Mrnak P., Svoboda P., Ehrenberger R., Novotny F., Poddany S., Prudil Z., Kuchtak B., Stegner D.", "ref_biblio": [""], "bibcode": ["2017OEJV..185....1S\t(SIMBAD/NED"], "keyword_cds": "", "abstract": ["We present the first release of the Czech Variable star catalogue that", "currently contains 1228 stars whose variability was discovered by 60", "Czech observers. The catalogue contains confirmed variable stars of", "various types, but also candidates. We give precise coordinates, cross", "identification with other catalogues, information about constellation,", "variability type, brightness, light elements, name of the discoverer", "and year of discovery. In eighty-eight percent of stars the", "variability type is estimated, for more than 60 % of the stars the", "light ephemerides are given."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "29-May-2018"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_PASA_16.175"}} {"id": "J/other/PASA/16.175", "title_cds": "-73<=DE<=+27 X-ray sources catalog", "title_create": "Meliani, 1999", "year": "1999", "author": "Meliani M.T.", "title_pub": "A catalogue of X-ray sources in the sky region between {delta}=-73{deg} and {delta}=+27{deg}.", "first_author": "Meliani M.T.", "ref_biblio": [""], "bibcode": ["1999PASA...16..175M"], "keyword_cds": "X-ray sources ; Binaries, X-ray ; Pulsars ; Active gal. nuclei ; Cross identifications ; Photometry, UBV", "abstract": ["This catalogue lists coordinates, X-ray fluxes in different energy", "ranges, magnitudes and color indices, optical counterparts, orbital", "periods of binaries, pulsar periods and other characteristics of", "226 X-ray sources (HMXBs, LMXBs, pulsars and galaxies) between", "DE=-73{deg} and DE=+27{deg}."], "doi_pub": ["10.1071/AS99175"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "position.dat", "desc": "X-ray names and positions ", "columns": [{"name": "Bname", "desc": "Source B or J name "}, {"name": "Type", "desc": "Type of source (1) "}, {"name": "RAh", "desc": "Right ascension (2000) "}, {"name": "RAm", "desc": "Right ascension (2000) "}, {"name": "RAs", "desc": "? Right ascension (2000) "}, {"name": "DE-", "desc": "Declination sign (2000) "}, {"name": "DEd", "desc": "Declination (2000) "}, {"name": "DEm", "desc": "Declination (2000) "}, {"name": "DEs", "desc": "? Declination (2000) "}, {"name": "RA1h", "desc": "Right ascension (1950) "}, {"name": "RA1m", "desc": "Right ascension (1950) "}, {"name": "RA1s", "desc": "? Right ascension (1950) "}, {"name": "DE1-", "desc": "Declination sign (1950) "}, {"name": "DE1d", "desc": "Declination (1950) "}, {"name": "DE1m", "desc": "? Declination (1950) "}, {"name": "DE1s", "desc": "? Declination (1950) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "ObsType", "desc": "[oxir, ] Type of observation "}, {"name": "PosErr", "desc": "? Source position error "}, {"name": "x_PosErr", "desc": "Unit of PosErr (\", ' or {deg}) "}, {"name": "Names", "desc": "Other names "}]}, {"name": "optical.dat", "desc": "UBV photometry, optical counterpart ", "columns": [{"name": "Name", "desc": "Usual name "}, {"name": "l_Vmag", "desc": "[->] Limit flag on Vmag "}, {"name": "Vmag", "desc": "? V magnitude "}, {"name": "---", "desc": "[-] - when interval of magnitudes "}, {"name": "Vmag2", "desc": "? Lower V magnitude when interval "}, {"name": "u_Vmag", "desc": "[:v] \":\" : uncertainty flag on Vmag, v: var "}, {"name": "Band", "desc": "[BK] When Vmag contains B or K magnitude "}, {"name": "r_Vmag", "desc": "References for Vmag (1) "}, {"name": "n_Vmag", "desc": "[*] Note for B1608-522, B1657-415 (2) "}, {"name": "B-V", "desc": "? B-V colour index (3) "}, {"name": "---", "desc": "[-] - when interval of B-V colour index "}, {"name": "B-V2", "desc": "? Lower B-V colour index when interval "}, {"name": "u_B-V", "desc": "Uncertainty flag on B-V "}, {"name": "r_B-V", "desc": "Reference for B-V (1) "}, {"name": "U-B", "desc": "? U-B colour index "}, {"name": "r_U-B", "desc": "Reference for U-B (1) "}, {"name": "l_E(B-V)", "desc": "Limit flag on E(B-V) "}, {"name": "E(B-V)", "desc": "? Interstellar reddening "}, {"name": "---", "desc": "[-] - when interval on interstellar reddening "}, {"name": "E(B-V)2", "desc": "? Upper value of E(B-V) when interval "}, {"name": "u_E(B-V)", "desc": "Uncertainty flag on E(B-V) "}, {"name": "r_E(B-V)", "desc": "Reference for E(B-V) (1) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "OName", "desc": "Optical counterpart, if known, and associations "}]}, {"name": "xfluxes.dat", "desc": "X-ray fluxes and periods ", "columns": [{"name": "Bname", "desc": "Source B or J name "}, {"name": "n_F2-10", "desc": "[*] *: 0.1-2.4KeV flux in F2-10 "}, {"name": "l_F2-10", "desc": "[> <] Limit flag on F2-10 "}, {"name": "F2-10", "desc": "? X-ray flux in the range 2-10 keV (or 0.1-2.4keV if *)"}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F2-10u", "desc": "? Upper limit on F2-10 when interval "}, {"name": "r_F2-10", "desc": "References for F2-10 (1) "}, {"name": "n_F40-80", "desc": "[*] *: 10-40keV flux in F10-40 "}, {"name": "l_F40-80", "desc": "Limit flag on F40-80 "}, {"name": "F40-80", "desc": "? X-ray flux in the range 40-80KeV (or 10-40keV if *)"}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F40-80u", "desc": "? Upper limit on F40-80 when interval "}, {"name": "r_F40-80", "desc": "Reference for F40-80 (1) "}, {"name": "l_F80-120", "desc": "Limit flag on F80-120 "}, {"name": "F80-120", "desc": "? X-ray flux in the range 80-120keV "}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F80-120u", "desc": "? Upper limit on F80-120 for interval "}, {"name": "r_F80-120", "desc": "Reference on F80-120 (1) "}, {"name": "F100-200", "desc": "? X-ray flux in the range 100-200keV "}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F100-200u", "desc": "? Upper limit on F100-200 if interval "}, {"name": "l_F200-600", "desc": "Limit flag on F200-600 "}, {"name": "F200-600", "desc": "? X-ray flux in the range 200-600keV "}, {"name": "---", "desc": "[-] - if interval "}, {"name": "F200-600u", "desc": "? Upper limit on F200-600 if interval "}, {"name": "l_F1000+", "desc": "Limit flag on F1000+ "}, {"name": "F1000+", "desc": "? X-ray flux in the range >1000keV "}, {"name": "---", "desc": "[-] - when interval "}, {"name": "F1000+u", "desc": "? Upper limit on F1000+ if interval "}, {"name": "r_F1000+", "desc": "Reference for F1000+ (1) "}, {"name": "l_Porb", "desc": "Limit flag on Porb "}, {"name": "Porb", "desc": "? Orbital period "}, {"name": "x_Porb", "desc": "Units of Porb (d, h) "}, {"name": "u_Porb", "desc": "[: ?] Uncertainty flag on Porb "}, {"name": "r_Porb", "desc": "Reference for Porb (1) "}, {"name": "n_Porb", "desc": "Second possible period or upper value if interval"}, {"name": "Ppul", "desc": "? Pulsar period "}, {"name": "x_Ppul", "desc": "Units of Pulsar period (s or ms) "}, {"name": "n_Ppul", "desc": "Reference or second possible value for Ppul (1)"}, {"name": "Char", "desc": "Characteristics (2) "}, {"name": "Cat.", "desc": "X-ray catalogues and experiments in which the source was listed and/or detected (3)"}]}, {"name": "notes.dat", "desc": "Individual notes ", "columns": [{"name": "Bname", "desc": "Name "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference number "}, {"name": "BibCode", "desc": "BibCode "}, {"name": "Authors", "desc": "Author's names "}, {"name": "Com", "desc": "Comments "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_PASAu_5.290"}} {"id": "J/other/PASAu/5.290", "title_cds": "MDS2 survey", "title_create": "Author+, ", "title_pub": "Title of the paper", "first_author": "Authors", "author": "Authors", "ref_biblio": ["<(various journals) PASAu, 5.290 (2000)>"], "bibcode": ["2000PASAu5.290.\t(SIMBAD/NED"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["MDS2"], "data": "", "date_update": "09-Aug-2006"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_POAN_2.59"}} {"id": "J/other/POAN/2.59", "title_cds": "Peculiar stars in 5 southern fields", "title_create": "Stock+, 1972", "year": "1972", "author": "Stock J., Wroblewski H.", "title_pub": "A southern objective prism survey.", "first_author": "Stock J.", "ref_biblio": [""], "bibcode": ["1972POAN....2...59S"], "keyword_cds": "", "keyword_pub": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "12-Jul-2006"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_RAA_16.138"}} {"id": "J/other/RAA/16.138", "title_cds": "Short Title", "title_create": "Hou+, 2016", "year": "2016", "author": "Hou W., Luo A-L., Hu J.-Y., Yang H.-F., Du C.-D., Liu C., Lee C.-D., Lin C.-C., Wang Y.-F., Zhang Y., Cao Z.-H., Hou Y.-H.", "title_pub": "A catalog of early-type emission-line stars and H{alpha}\u03b1line profiles from LAMOST DR2.", "first_author": "Hou W.", "ref_biblio": [""], "bibcode": ["2016RAA....16..138H"], "see_also": ["J/A+AS/25/25 : HII regions of the Northern Milky Way (Dubout-Crillon+ 1976)"], "keyword_cds": "", "keyword_pub": "stars: early-type - stars: emission-line, Be \u2014 stars: pre-main sequence - binaries: close", "abstract": ["We present a catalog including 11204 spectra of 10436 early-type", "emission-line stars from LAMOST DR2, among which 9752 early-type", "emission-line spectra are newly discovered. For these earlytype", "emission-line stars, we discuss the morphological and physical", "properties of their low-resolution spectra. In this spectral sample,", "the H{alpha} emission profiles display a wide variety of shapes. Based", "on the H{alpha} line profiles, these spectra are categorized into five", "distinct classes: single-peak emission, single-peak emission in", "absorption, double-peak emission, double-peak emission in absorption,", "and P-Cygni profiles. To better understand what causes the H{alpha}", "line profiles, we divide these objects into four types from the", "perspective of physical classification, which include classical Be", "stars, Herbig Ae/Be stars, close binaries and spectra contaminated by", "HII regions. The majority of Herbig Ae/Be stars and classical Be stars", "are identified and separated using a (H-K, K-W1) color-color", "diagram.We also discuss 31 binary systems that are listed in the", "SIMBAD on-line catalog and identify 3600 spectra contaminated by HII", "regions after cross-matching with positions in the Dubout-Crillon", "catalog (1976, Cat. J/A+AS/25/25. A statistical analysis of line", "profiles versus classifications is then conducted in order to", "understand the distribution of H{alpha} profiles for each type in our", "sample. Finally, we also provide a table of 172 spectra with FeII", "emission lines and roughly calculate stellar wind velocities for seven", "spectra with P-Cygni profiles."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "31-Aug-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_RMxAA_22.43"}} {"id": "J/other/RMxAA/22.43", "title_cds": "IR stellar population in the Galaxy", "title_create": "Ruelas-Mayorga, 1991", "year": "1991", "author": "Ruelas-Mayorga R.A.", "title_pub": "Distribution and studies of the infrared stellar population in the Galaxy. II. The data base.", "first_author": "Ruelas-Mayorga R.A.", "ref_biblio": [""], "bibcode": ["1991RMxAA..22...43R"], "see_also": ["J/A+AS/93/61 : IR Stellar Population in Baade's window (Ruelas-Mayorga+ 1992)", "J/A+AS/97/587 : JHK photometry of Galactic center stars (Ruelas-Mayorga+ 1993)"], "keyword_cds": "Populations, stellar; Photometry, infrared ; Infrared sources", "keyword_pub": "Galaxy: stellar content - Galaxy: structure - Interstellar: dust", "abstract": ["In this paper we utilised the galactic model developed in", "Ruelas-Mayorga (1991RMxAA..22...27R) in order to predict the", "Cumulative Counts Function (CCF) (log. of the number of sources down", "to a given K-magnitude per unit of area) in 39 directions of the sky.", "We present stellar-counts observations for these directions and", "compare the observational results with the predictions of the model.", "We conclude that the global description of the distribution of the", "stellar population responsible for the 2.2{mu}m radiation in our galaxy", "is very well represented by the model's predictions. There are a few", "regions for which the global description is not satisfactory. We", "present evidence for some cases that this is due to anomalous stellar", "concentrations or to excess or deficiency of absorption."], "data": "", "date_update": "24-Oct-2000", "tables": [{"name": "tables.dat", "desc": "Infrared sources ", "columns": [{"name": "Table", "desc": "Table number (A2 to A30) "}, {"name": "---", "desc": "[l=] "}, {"name": "GLON", "desc": "Region field center galactic longitude "}, {"name": "---", "desc": "[b=] "}, {"name": "GLAT", "desc": "Region field center galactic latitude "}, {"name": "Scan", "desc": "Row number in the scan "}, {"name": "---", "desc": "[/] "}, {"name": "Source", "desc": "Source number along scan-line "}, {"name": "RAh", "desc": "Right ascension (1950.0) "}, {"name": "RAm", "desc": "Right ascension (1950.0) "}, {"name": "RAs", "desc": "[0/60] Right ascension (1950.0) "}, {"name": "DE-", "desc": "Declination sign (1950.0) "}, {"name": "DEd", "desc": "Declination (1950.0) "}, {"name": "DEm", "desc": "Declination (1950.0) "}, {"name": "DEs", "desc": "Declination (1950.0) "}, {"name": "Kmag", "desc": "? K magnitude "}, {"name": "n_Kmag", "desc": "[SAT ] SAT: saturated, for sources brighter than K~+8.5"}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_RMxAA_6.83"}} {"id": "J/other/RMxAA/6.83", "title_cds": "Carbon stars", "title_create": "Fuenmayor, 1981", "year": "1981", "author": "Fuenmayor F.J.", "title_pub": "A deep near infrared objective prism survey for carbon stars toward the galactic center and anticenter.", "first_author": "Fuenmayor F.J.", "ref_biblio": [""], "bibcode": ["1981RMxAA...6...83F"], "keyword_cds": "", "keyword_pub": "", "mission": "", "object": [], "curator": "Francois Ochsenbein [CDS]", "data": "", "date_update": "08-Dec-2013"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_Sci_368.1477"}} {"id": "J/other/Sci/368.1477", "title_cds": "Short Title", "title_create": "Author+, ", "title_pub": "A multiplanet system of super-Earths orbiting the brightest red dwarf star GJ 887.", "first_author": "Jeffers S.V.", "author": "Jeffers S.V., Dreizler S., Barnes J.R., Haswell C.A., Nelson R.P., Rodriguez E., Lopez-Gonzalez M.J., Morales N., Luque R., Zechmeister M., Vogt S.S., Jenkins J.S., Palle E., Berdinas Z.M., Coleman G.A.L., Diaz M.R., Ribas I., Jones H.R.A., Butler R.P., Tinney C.G., Bailey J., Carter B.D., O'Toole S., Wittenmyer R.A., Crane J.D., Feng F., Shectman S.A., Teske J., Reiners A., Amado P.J., Anglada-Escude G.", "ref_biblio": [""], "bibcode": ["2020Sci...368.1477J"], "keyword_cds": "", "abstract": ["The closet exoplanets to the Sun provide opportunities for detailed", "characterization of planets outside the Solar System. We report the", "discovery, using radial velocity measurements, of a compact", "multiplanet system of super-Earth exoplanets orbiting the nearby red", "dwarf star GJ 887. The two planets have orbital periods of 9.3 and", "21.8 days. Assuming an Earth-like albedo, the equilibrium temperature", "of the 21.8-day planet is ~350 kelvin. The planets are interior to,", "but close to the inner edge of, the liquid-water habitable zone. We", "also detect an unconfirmed signal with a period of ~50 days, which", "could correspond to a third super-Earth in a more temperate orbit. Our", "observations show that GJ 887 has photometric variability below 500", "parts per million, which is unusually quiet for a red dwarf."], "object": [], "curator": "Patricia Vannier [CDS]", "data": "", "date_update": "16-Nov-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_A+SP_163.275"}} {"id": "J/other/ApSS/163.275", "title_cds": "UV & Geneva photometry around HD 173009", "title_create": "Reichen+, 1990", "year": "1990", "author": "Reichen M., Lanz T., Golay M., Huguenin D.", "title_pub": "A detailed study of a 6{deg} diameter field in Scutum. I. Data presentation and overall description of the interstellar matter distribution.", "first_author": "Reichen M.", "ref_biblio": [""], "bibcode": ["1990Ap&SS.163..275R"], "see_also": ["II/59 : Catalogue of stellar UV fluxes (TD1) (Thompson+ 1978)"], "keyword_cds": "Surveys ; Photometry, ultraviolet ; Photometry, Geneva ; MK spectral classification", "abstract": ["A 6{deg} diameter field centered on the star {epsilon} Scutum has been", "selected from the SCAP-2000 balloon-borne UV survey for its high", "apparent stellar density contrast and relatively good transparency on", "a small projected portion of the galactic plane. In view of a detailed", "study of the absorption and interstellar matter distribution in this", "field, a large collection of data has been made and is presented here.", "Ultraviolet magnitudes at 2000{AA} have been obtained from the", "reduction of three SCAP frames. In addition, 322 stars among the 487", "stars detected on the UV frames have been measured in the Geneva", "photometric system. For a small number of photometrically distant", "objects, medium resolution spectra have been obtained in order to", "determine spectral types and confirm the distances determination. An", "overall description of the distribution of interstellar material in", "the ultraviolet is made using star counting methods, and is confronted", "to similar studies in the visible range. A discussion of the", "variations of the extinction law in different parts of the field is", "made. A new distance determination of the Sct OB2 association is", "proposed, as well as a list of additional probable members of the", "association. A certain number of distant hot stars seem to indicate", "the presence of an unknown OB association at the edge of the Scutum", "spiral arm, at a distance of over 3 kpc from the Sun."], "date_update": "19-Jan-2020", "tables": [{"name": "table1.dat", "desc": "Calibration stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (see Table2) "}, {"name": "Name", "desc": "HD, BD or CSI identification "}, {"name": "SpType", "desc": "Spectral type (see table 2) "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude from the Geneva system"}, {"name": "UVmag", "desc": "UV magnitude at 2000{AA} deduced from calibration"}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag "}, {"name": "n_UVmag", "desc": "[abcd ] Note on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965{AA} passband of the TD1 catalogue (Thompson et al., 1978, Cat. ). (2)"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "n_UVmagTD1", "desc": "[)] ) indicates that the UV magnitude UVmagboxes was preferred for the calibration"}, {"name": "UVmagboxes", "desc": "UV magnitude deduced by the method of the so-called \"photometric boxes\" (see text.) (3)"}, {"name": "e_UVmagboxes", "desc": "rms uncertainty on UVmagboxes "}, {"name": "n_UVmagboxes", "desc": "[)] ) indicates that the UV magnitude UVmagTD1 was preferred for the calibration"}, {"name": "N", "desc": "Number of stars in the photometric box "}, {"name": "Rem", "desc": "Remarks related to the UV_TD1_ magnitudes (G2) "}]}, {"name": "table2.dat", "desc": "All stars measured on SCAP frames 11.65/14.48/14.49 ", "columns": [{"name": "SCAP", "desc": "SCAP identification number (1) "}, {"name": "n_SCAP", "desc": "[* o] \"*\" star measured in the Geneva system (see Table 3) \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[+*] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (see Table 3) "}, {"name": "Vmag", "desc": "? Visual magnitude (3) "}, {"name": "UVmag", "desc": "UV magnitude at 2000A from the SCAP frames "}, {"name": "e_UVmag", "desc": "? rms uncertainty on UVmag (4) "}, {"name": "n_UVmag", "desc": "[abcd ] Notes on UVmag (G1) "}, {"name": "UVmagTD1", "desc": "? UV magnitude in the 1965A passband of the TD1 catalogue (Thompson et al., 1978, )"}, {"name": "e_UVmagTD1", "desc": "? rms uncertainty on UVmagTD1 "}, {"name": "UV-V", "desc": "? (UVmag-Vmag) color index "}, {"name": "(UV-V)0", "desc": "? Intrinsic (UV-V)_0_ color index taken from Carnochan (1982) following the MK, photometric or other spectra type"}, {"name": "E(UV-V)", "desc": "? UV color excess (from (UV-V) and (UV-V)0) "}, {"name": "Rem", "desc": "Various remarks and comments (G2) "}]}, {"name": "table3.dat", "desc": "All stars with Geneva photometry ", "columns": [{"name": "SCAP", "desc": "SCAP identification (see Table 2) "}, {"name": "n_SCAP", "desc": "[o] \"o\" UBV photometry is available (Mermilliod, 1987, Cat. )"}, {"name": "Name", "desc": "HD, BD or CSI identification. "}, {"name": "n_Name", "desc": "[*+] \"+\" BD numbers not included in Simbad \"*\" BD numbers included in Simbad after publication of the paper"}, {"name": "GLONd", "desc": "Galactic longitude "}, {"name": "GLONm", "desc": "Galactic longitude "}, {"name": "GLATd", "desc": "Galactic latitude "}, {"name": "GLATm", "desc": "Galactic latitude "}, {"name": "SpType", "desc": "Spectral type "}, {"name": "r_SpType", "desc": "Origin of SpType (2) "}, {"name": "SpPhot", "desc": "Photometric spectral type (1) "}, {"name": "[U-B]", "desc": "Geneva [U-B] colour index "}, {"name": "[B-V]", "desc": "Geneva [B-V] colour index "}, {"name": "[B1-B]", "desc": "Geneva [B1-B] colour index "}, {"name": "[B2-B]", "desc": "Geneva [B2-B] colour index "}, {"name": "[V1-B]", "desc": "Geneva [V1-B] colour index "}, {"name": "[G-B]", "desc": "Geneva [G-B] colour index "}, {"name": "Vmag", "desc": "Photoelectric visual magnitude "}, {"name": "E[B-V]", "desc": "? Color excess deduced from the X,Y,Z parameters (Cramer, 1982A&A...112..330C) unless stated otherwise in the remarks"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters (Cramer and Maeder, 1979A&A....78..305C) unless stated otherwise in the remarks"}, {"name": "r", "desc": "? Decuced heliocentric distance "}, {"name": "Rem", "desc": "Various remarks (2) "}]}, {"name": "table4.dat", "desc": "Spectroscopic standard stars ", "columns": [{"name": "HD", "desc": "HD identification "}, {"name": "RAh", "desc": "Right ascension (1950) "}, {"name": "RAm", "desc": "Right ascension (1950) "}, {"name": "DE-", "desc": "Declination sign (1950) "}, {"name": "DEd", "desc": "Declination (1950) "}, {"name": "DEm", "desc": "Declination (1950) "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "? Visible absorption derived from E[B-V]. "}, {"name": "n_AV", "desc": "[)] ): values deduced from Johnson's U-B/B-V diagram"}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypeH", "desc": "Spectral type given by Houk and Cowley (1975, ) or Houk (1978, , 1982, )"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHg", "desc": "Equivalent width of the H{gamma} line derived from our spectroscopic observations"}, {"name": "VMAGHg", "desc": "Absolute magnitude derived from EW_H{gamma}_ using calibrations by Millward and Walker (1985ApJS...57...63M) or Hill et al. (1986PASP...98.1186H)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}]}, {"name": "table5.dat", "desc": "Spectroscopy of Scutum field stars ", "columns": [{"name": "SCAP", "desc": "SCAP identification "}, {"name": "Vmag", "desc": "Apparent visual magnitude "}, {"name": "AV", "desc": "Visible absorption derived from E[B-V] "}, {"name": "SpTypes", "desc": "Spectral type derived from our medium resolution spectra"}, {"name": "SpTypep", "desc": "Photometric spectral type deduced from the position of the star in the (X Y) diagram"}, {"name": "EWHa", "desc": "Equivalent width of the H{alpha} line derived from our spectroscopic observations"}, {"name": "u_EWHa", "desc": "[)] Uncertainty flag on EWHa "}, {"name": "VMAGHa", "desc": "? Absolute magnitude derived from EW_H{alpha}_ (See notes to Table 4)"}, {"name": "VMAG", "desc": "? Absolute visual magnitude deduced from the X,Y,Z parameters of the Geneva photometry"}, {"name": "Rem", "desc": "Individual remarks (1) "}]}, {"name": "notes2.dat", "desc": "Individual notes to table2.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}, {"name": "notes3.dat", "desc": "Individual notes to table3.dat ", "columns": [{"name": "SCAP", "desc": "SCAP number "}, {"name": "Note", "desc": "Text of the note "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"J_other_RNAAS_4.12"}} {"id": "J/other/RNAAS/4.12", "title_cds": "Galactic RSG+B binary systems", "title_create": "Pantaleoni Gonzalez+, 2020", "year": "2020", "author": "Pantaleoni Gonzalez M., Maiz Apellaniz J., Barba R.H., Negueruela I.", "title_pub": "A catalog of Galactic multiple systems with a red supergiant and a B star.", "first_author": "Pantaleoni Gonzalez M.", "ref_biblio": [""], "bibcode": ["2020RNAAS...4...12P"], "see_also": ["B/sb9 : SB9: 9th Cat. of Spectroscopic Binary Orbits (Pourbaix+ 2004-2014)", "B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)", "B/wds : The Washington Visual Double Star Catalog (Mason+ 2001-2020)", "B/mk : Catalogue of Stellar Spectral Classifications (Skiff, 2009- )", "III/117 : MK Classifications of Close Visual Binaries (Corbally, 1984)", "III/135 : Henry Draper Catalogue and Extension (Cannon+ 1918-1924; ADC 1989)", "III/150 : Perkins Revised MK Types for the Cooler Stars (Keenan+ 1989)", "III/274 : Galactic O-Star Spectroscopic Survey (GOSSS) (Sota+, 2014)", "J/ApJS/99/135 : A-type stars rotation and spectral peculiarities (Abt+ 1995)", "J/ApJS/119/83 : IUE sample of binaries with hot component (Parsons+, 1998)", "J/ApJS/143/513 : Spectral classification of close binaries (Ginestet+, 2002)", "J/MNRAS/427/3209 : Galactic and MC O-AGBs and RSGs stars (Jones+, 2012)", "J/A+A/571/A43 : Red supergiants in Galactic clusters (Messineo+, 2014)", "J/ApJS/224/4 : GOSSS III. Additional O-type systems (Maiz Apellaniz+, 2016)", "J/MNRAS/469/1330 : NGC 6067 stars (Alonso-Santiago+, 2017)", "J/MNRAS/475/2003 : Red supergiant population in Perseus arm (Dorda+, 2018)", "J/A+A/616/A124 : NGC 3105 UBVR photometry (Alonso-Santiago+, 2018)", "J/AJ/158/20 : K-M stars of class I cand. RSGs in Gaia (Messineo+, 2019)"], "keyword_cds": "Stars, double and multiple; Stars, giant; Stars, B-type; References", "keyword_pub": "Binary stars ; Catalogs ; Early-type stars ; Late-type stars ; Late-type supergiant stars ; Red supergiant stars ; B stars", "description": ["We have searched the literature and Simbad to find Galactic red", "supergiant (RSG)+B binary systems. More specifically, we define RSGs", "as objects with spectral type G, K, or M and luminosity classes II to", "Ia for consistency with Neugent+ (2019ApJ...875..124N), but we note", "that criterion includes some Cepheids, which can be of spectral type", "G-K0 in some phases. Results are listed in Table 1.", "We have found 108 Galactic RSG+B binary systems in the literature,", "with 61% of the sample already present in two references alone", "(Ginestet & Carquillat 2002, J/ApJS/143/513 and", "Samus'+ 2017ARep...61...80S). A significant number of the objects have", "two entries in the HD catalog, a likely consequence of the composite", "nature of the spectra. The total number in the sample has to be taken", "with care, as literature spectral classifications can include gross", "errors."], "type": ["GCC"], "data": "", "date_update": "09-Sep-2020", "tables": [{"name": "table1.dat", "desc": "Objects, spectral classifications, Galactic coordinates, V magnitudes, separations, references, and comments", "columns": [{"name": "Name", "desc": "Identifier "}, {"name": "AName", "desc": "Alternate name "}, {"name": "SpT-RSG", "desc": "Red supergiant spectral type "}, {"name": "LC-RSG", "desc": "Red supergiant luminosity class "}, {"name": "Q-RSG", "desc": "[ep ] Red supergiant qualifier "}, {"name": "SpT-B", "desc": "B star spectral type "}, {"name": "LC-B", "desc": "B star luminosity class "}, {"name": "Q-B", "desc": "B star qualifier "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "[-39.4/21] Galactic latitude "}, {"name": "Vmag", "desc": "[0.9/14.4]?=99.9 Apparent V band magnitude "}, {"name": "Sep", "desc": "[0/9.4]? Binary separation (1) "}, {"name": "Ref", "desc": "Reference code (see refs.dat file) "}, {"name": "Comm", "desc": "Additional comments "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference code "}, {"name": "BibCode", "desc": "Bibcode of the reference "}, {"name": "Auth", "desc": "Author's name(s) "}, {"name": "Comm", "desc": "Comment "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"V_100"}} {"id": "V/100", "title_cds": "Strasbourg-ESO Catalogue of Galactic Planetary Nebulae", "title_create": "Acker+ 1996", "year": "1996", "author": "Acker A., Ochsenbein F., Stenholm B., Tylenda R., Marcout J., Schohn C.", "title_pub": "Strasbourg-ESO Catalogue of Galactic Planetary Nebulae and First Supplement", "first_author": "Acker A.", "ref_biblio": [""], "bibcode": ["1992ESOPN...1....1A"], "see_also": ["J/A+A/307/215 : Spectrophotometry of PNe (Cuisinier+, 1996)"], "keyword_cds": "Planetary nebulae ; Spectroscopy", "description": ["This new edition of the \"Catalogue of Galactic Planetary Nebulae\" is a", "merging of the \"Strasbourg-ESO Catalogue of Galactic Planetary", "Nebulae\" published by ESO in 1992 and the \"First Supplement to the", "Strasbourg-ESO Catalogue of Galactic Planetary Nebulae\" prepared at", "Strasbourg for the Mexico meeting...", "Compared to the previous edition, 384 new objects discovered since", "1991/92 have been added: 242 have been added as \"true or probable\"", "PNe, and 142 which status is stilll unclear were classified among", "the \"possible\" planetary nebulae.", "Errors reported until ... were also corrected."], "alias": ["GPN", "PNG"], "data": "", "date_update": "31-Aug-2010", "tables": [{"name": "main.dat", "desc": "Discoverers, Designations, and Positions of True and Possible Planetary Nebulae (1)", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "*Designation of the Galactic Planetary Nebula (blank for Possible PNe from 1992)"}, {"name": "RAh", "desc": "Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension 2000 (minutes) "}, {"name": "RAs", "desc": "? Right Ascension 2000 (seconds) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "Declination 2000 (degrees) "}, {"name": "DEm", "desc": "Declination 2000 (minutes) "}, {"name": "DEs", "desc": "[0/60[? Declination 2000 (seconds) "}, {"name": "qualPos", "desc": "*[ad*] Accuracy on the 2000 Position: "}, {"name": "r_Pos", "desc": "Reference of position "}, {"name": "Name", "desc": "Main designation "}, {"name": "PK", "desc": "Designation in PK67 "}, {"name": "IRAS", "desc": "Designation in IRAS catalogue "}, {"name": "Disc", "desc": "*Discoverer name and publication year "}, {"name": "Idents", "desc": "Other names separated by commas "}]}, {"name": "diam.dat", "desc": "Diameters of PN (optical and radio) (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "l_oDiam", "desc": "Limit flag on oDiam "}, {"name": "oDiam", "desc": "? Optical diameter "}, {"name": "u_oDiam", "desc": "[:e] Uncertainty flag (:) on oDiam, or e for \"extended\" (without value)"}, {"name": "r_oDiam", "desc": "References for oDiam "}, {"name": "l_rDiam", "desc": "Limit flag on Radio diameter "}, {"name": "rDiam", "desc": "? Radio diameter "}, {"name": "u_rDiam", "desc": "Uncertainty flag (:) on oDiam "}, {"name": "r_rDiam", "desc": "Reference on Radio diameter "}]}, {"name": "dist.dat", "desc": "Distance estimations (2) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "Method", "desc": "*[EKSWXDCM] Method used for distance determination"}, {"name": "Dist1", "desc": "? Lower distance if l_Dist is '-' "}, {"name": "l_Dist", "desc": "[-<>] '-' if Dist1 is a lower limit; '<' or '>' apply to Dist."}, {"name": "Dist", "desc": "Distance in kiloparsecs. "}, {"name": "u_Dist", "desc": "[?:] Uncertainty flag on Dist "}, {"name": "r_Dist", "desc": "Reference of Dist determination. "}]}, {"name": "dista.dat", "desc": "Statistical distances (2) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "Method", "desc": "*[EKSWXDCM] Method used for distance determination"}, {"name": "Dist1", "desc": "? Lower distance if l_Dist is '-' "}, {"name": "l_Dist", "desc": "[-<>] '-' if Dist1 is a lower limit; '<' or '>' apply to Dist."}, {"name": "Dist", "desc": "Distance in kiloparsecs. "}, {"name": "u_Dist", "desc": "[?:] Uncertainty flag on Dist "}, {"name": "r_Dist", "desc": "Reference of Dist determination. "}]}, {"name": "hbeta.dat", "desc": "H-beta fluxes (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "log(Fbeta)", "desc": "[-15/-9] log of flux in H-beta "}, {"name": "e_log(Fbeta)", "desc": "? Mean error on log(Fbeta) "}, {"name": "r_log(Fbeta)", "desc": "References "}]}, {"name": "intens.dat", "desc": "Line intensities results (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "ObsLabel", "desc": "Observation name (includes the date) "}, {"name": "LineRef", "desc": "[ab] Line taken as reference (value=100): 'a'=H-alpha (6563), 'b'=H-beta (4861)"}, {"name": "I4363", "desc": "]0/15000]? Line intensity of [OIII] at 436.3nm "}, {"name": "u_I4363", "desc": "Uncertainty flag on I4363 "}, {"name": "I4686", "desc": "]0/15000]? Line intensity of HeII at 468.6nm "}, {"name": "u_I4686", "desc": "Uncertainty flag on I4686 "}, {"name": "n_I5007", "desc": "[*] '*' if the measurement refers to 495.9nm because 500.7nm line is saturated"}, {"name": "I5007", "desc": "]0/15000]? Line intensity of [OIII] at 500.7nm "}, {"name": "u_I5007", "desc": "Uncertainty flag on I5007 "}, {"name": "I5876", "desc": "]0/15000]? Line intensity of HeI "}, {"name": "u_I5876", "desc": "Uncertainty flag on I5876 at 587.6nm "}, {"name": "I6563", "desc": "]0/15000]? Line intensity of H-alpha at 656.3nm"}, {"name": "u_I6563", "desc": "Uncertainty flag on I6563 "}, {"name": "I6584", "desc": "[0/15000]? Line intensity of [NII] at 658.4nm "}, {"name": "u_I6584", "desc": "Uncertainty flag on I6584 "}, {"name": "n_I6717", "desc": "[B] 'B' if line is blended "}, {"name": "I6717", "desc": "]0/15000]? Line intensity of [SII] at 671.7nm "}, {"name": "u_I6717", "desc": "Uncertainty flag on I6717 "}, {"name": "n_I6731", "desc": "[B] 'B' if line is blended "}, {"name": "I6731", "desc": "]0/15000]? Line intensity of [SII] at 673.1nm "}, {"name": "u_I6731", "desc": "Uncertainty flag on I6731 "}, {"name": "r_Line", "desc": "Reference of the spectroscopic values "}]}, {"name": "iue.dat", "desc": "IUE observations log (2) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "IUEname", "desc": "Name as found in the IUE Merged Log "}, {"name": "1950Pos", "desc": "Position as found in the IUE Merged Log "}, {"name": "ObsDate", "desc": "Date and time (hours, minutes) of the Observation"}, {"name": "OType", "desc": "Object class as found in the IUE Merged Log "}, {"name": "Camera", "desc": "designation, LW=Long Wavelength, SW=Short Wavelength"}, {"name": "Image", "desc": "identification of the Observation "}]}, {"name": "iras.dat", "desc": "IRAS Point Source Catalogue fluxes (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "IRAS", "desc": "IRAS source name "}, {"name": "RAIRASh", "desc": "Hours RA, equinox 1950.0, epoch 1983.5 "}, {"name": "RAIRASm", "desc": "Minutes RA, equinox 1950.0, epoch 1983.5 "}, {"name": "RAIRASds", "desc": "Seconds RA, equinox 1950.0, epoch 1983.5 "}, {"name": "DEIRAS-", "desc": "Sign Dec, equinox 1950.0, epoch 1983.5 "}, {"name": "DEIRASd", "desc": "Degrees Dec, equinox 1950.0, epoch 1983.5 "}, {"name": "DEIRASm", "desc": "Minutes Dec, equinox 1950.0, epoch 1983.5 "}, {"name": "DEIRASs", "desc": "Seconds Dec, equinox 1950.0, epoch 1983.5 "}, {"name": "Major", "desc": "Uncertainty ellipse major axis "}, {"name": "Minor", "desc": "Uncertainty ellipse minor axis "}, {"name": "PosAng", "desc": "Uncertainty ellipse position angle (1) "}, {"name": "NHcon", "desc": "Number of times observed "}, {"name": "Fnu12", "desc": "Average non-color corrected flux density, 12um"}, {"name": "Fnu25", "desc": "Average non-color corrected flux density, 25um"}, {"name": "Fnu60", "desc": "Average non-color corrected flux density, 60um"}, {"name": "Fnu100", "desc": "Average non-color corrected flux density, 100um"}, {"name": "q_Fnu12", "desc": "[1/3] Flux density quality, 12um (1) "}, {"name": "q_Fnu25", "desc": "[1/3] Flux density quality, 25um (1) "}, {"name": "q_Fnu60", "desc": "[1/3] Flux density quality, 60um (1) "}, {"name": "q_Fnu100", "desc": "[1/3] Flux density quality, 100um (1) "}]}, {"name": "nir.dat", "desc": "Near infra-red observations (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "Jmag", "desc": "? Magnitude in J filter (1.25um) "}, {"name": "l_Hmag", "desc": "Limit flag on Hmag "}, {"name": "Hmag", "desc": "? Magnitude in H filter (1.65um) "}, {"name": "l_Kmag", "desc": "Limit flag on Kmag "}, {"name": "Kmag", "desc": "? Magnitude in K filter (2.22um) "}, {"name": "l_Lmag", "desc": "Limit flag on Lmag "}, {"name": "Lmag", "desc": "? Magnitude in L/L' filter (3.5/3.8um) "}, {"name": "n_Lmag", "desc": "['] the apostrophe indicates the L' filter "}, {"name": "l_Mmag", "desc": "Limit flag on Mmag "}, {"name": "Mmag", "desc": "? Magnitude in M (5.0um) "}, {"name": "Class", "desc": "*[NDSP,?+ ] Class based on the near-IR "}, {"name": "r_Phot", "desc": "References for JHKL "}, {"name": "r_Sp", "desc": "References describing the Spectrum "}]}, {"name": "radio.dat", "desc": "Radio observations (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "l_Rad2cm", "desc": "Limit flag on Rad2cm "}, {"name": "Rad2cm", "desc": "? Radio flux density at 2cm (14.7GHz) "}, {"name": "r_Rad2cm", "desc": "Reference of Rad2cm "}, {"name": "l_Rad6cm", "desc": "Limit flag on Rad6cm "}, {"name": "Rad6cm", "desc": "? Radio flux density at 6cm (5GHz) "}, {"name": "u_Rad6cm", "desc": "Uncertainty flag on Rad6cm "}, {"name": "r_Rad6cm", "desc": "Reference of Rad6cm "}]}, {"name": "vel.dat", "desc": "Radial and Expansion Velocities (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "RVel", "desc": "? Radial Velocity "}, {"name": "e_RVel", "desc": "? Mean error on RVel "}, {"name": "r_RVel", "desc": "Source of the Radial Velocity "}, {"name": "l_ExpVel", "desc": "Limit flag on ExpVel "}, {"name": "ExpVel", "desc": "? Expansion velocity [OIII] "}, {"name": "u_ExpVel", "desc": "[*] Note on ExpVel (1) "}, {"name": "r_ExpVel", "desc": "Source of ExpVel "}, {"name": "n_ExpVel", "desc": "[+-] Note on the elements (2) "}, {"name": "l_ExpVel2", "desc": "Limit flag on ExpVel2 "}, {"name": "ExpVel2", "desc": "? Expansion velocity [NII] "}, {"name": "u_ExpVel2", "desc": "[*] Note on ExpVel2 (1) "}, {"name": "r_ExpVel2", "desc": "Reference of ExpVel2 "}, {"name": "n_ExpVel2", "desc": "[+-] Note on the elements (2) "}]}, {"name": "cstar.dat", "desc": "Data concerning Central Stars of PN (1) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "AG82", "desc": "Name in ref. AG82 (Acker et al., Publ. Speciale CDS 3, 1982)"}, {"name": "Umag", "desc": "? Johnson's U filter mag. of central star "}, {"name": "l_Bmag", "desc": "Limit flag on Bmag "}, {"name": "Bmag", "desc": "? Johnson's B filter mag. of central star "}, {"name": "l_Vmag", "desc": "Limit flag on Vmag "}, {"name": "Vmag", "desc": "? Johnson's V filter mag. of central star "}, {"name": "Quality", "desc": "*[ABCDP] Accuracy of the photometry "}, {"name": "r_UBV", "desc": "References of Photometry "}, {"name": "Remarks", "desc": "Remarks on Photometry "}, {"name": "Sp", "desc": "Spectral type of central star "}, {"name": "r_Sp", "desc": "Reference of Spectral type "}, {"name": "Sp2", "desc": "Other spectral classification "}, {"name": "r_Sp2", "desc": "Reference of Sp2 "}, {"name": "Sp3", "desc": "Other spectral classification "}, {"name": "r_Sp3", "desc": "Reference of Sp3 "}, {"name": "Names", "desc": "Various designations of the Central Star separated by a semi-colon (;)"}]}, {"name": "notes.dat", "desc": "Notes and remarks about some nebulae (2) ", "columns": [{"name": "Sup", "desc": "[+AaBbQq?] Origin of the PN (G1) "}, {"name": "PNG", "desc": "Designation of the Galactic Planetary Nebula "}, {"name": "Text", "desc": "Text of the note "}]}, {"name": "refs.dat", "desc": "References ", "columns": [{"name": "Ref", "desc": "Reference code (repeated on each line) "}, {"name": "Text", "desc": "Text if reference (authors and titles) "}]}, {"name": "pospn.dat", "desc": "Possible PN (table 2) ", "columns": [{"name": "Name", "desc": "Usual name "}, {"name": "n_PK", "desc": "[*] The '*' indicates that PK was not published in the PK67 reference"}, {"name": "PK", "desc": "Designation in PK67 (or later, see n_PK) "}, {"name": "RAh", "desc": "Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension 2000 (minutes) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "Declination 2000 (degrees) "}, {"name": "DEm", "desc": "Declination 2000 (minutes) "}, {"name": "GLON", "desc": "Galactic longitude "}, {"name": "GLAT", "desc": "Galactic latitude "}, {"name": "Class", "desc": "*[UHPLNE?*2 ] Class of the object "}, {"name": "OtherNames", "desc": "separated by a comma (,) "}]}, {"name": "notpn.dat", "desc": "Objects rejected as PN (table 3) ", "columns": [{"name": "Name", "desc": "Usual name "}, {"name": "n_PK", "desc": "[*] The '*' indicates that PK was not published in the PK67 reference"}, {"name": "PK", "desc": "Designation in PK67 (or later, see n_PK) "}, {"name": "RAh", "desc": "[0/24[? Right Ascension 2000 (hours) (1) "}, {"name": "RAm", "desc": "[0/60[? Right Ascension 2000 (minutes) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "[0/90[? Declination 2000 (degrees) "}, {"name": "DEm", "desc": "[0/60[? Declination 2000 (minutes) "}, {"name": "GLON", "desc": "[0/360[? Galactic longitude "}, {"name": "GLAT", "desc": "[-90/90]? Galactic latitude "}, {"name": "Notes", "desc": "*Notes concerning the object "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"V_5"}} {"id": "V/5A", "title_cds": "Colours, Luminosities, and Motions Nearer K-M Giants", "title_create": "Eggen 1966", "year": "1966", "author": "Eggen O.J.", "title_pub": "Colours, Luminosities, and Motions of the Nearer Giants of Types K and M", "first_author": "Eggen O.J.", "ref_biblio": [""], "keyword_cds": "Colors - 235; Space velocities - 730; Stars, giant - 880; Stars, late-type - 895", "description": ["The data compilation Colours, Luminosities and Motions of the Nearer", "Giants of Types of K and M (Eggen 1966) contains all stars in the", "Yale Catalogue of Bright Stars (Hoffleit 1964) that have visual", "magnitudes brighter than 5.5 and that have been observed to have B-V", "redder than +0.8 mag, with the exception of a few K-type dwarfs. In", "addition to mostly K- and M-type giants, a few subgiants and", "supergiants are included. The data result from some 1600", "photoelectric observations of 600 stars with the 50.8-cm reflector", "of the Hale Observatories. Approximately one-third of the stars had", "been observed at the Cape Observatory (Cousins and Stoy 1963).", "Although spectral types are given in the published catalog, they", "were taken from a variety of sources, are very inhomogeneous, and", "are not included in this catalog."], "date_update": "20-Nov-1995", "tables": [{"name": "giantkm.dat", "desc": "Catalog Data ", "columns": [{"name": "HR", "desc": "HR number from the Yale Catalogue of Bright Stars (Hoffleit 1964)."}, {"name": "HR2", "desc": "A slash (/) and additional digit if a second HR star is included in the measurements."}, {"name": "flag1", "desc": "An asterisk (*) is present if there are remarks in the published catalog."}, {"name": "GCRV", "desc": "GCRV number in the General Catalogue of Stellar Radial Velocities (Wilson 1953)."}, {"name": "GCRV2", "desc": "A slash and additional digit if a GCRV star is included in the value given"}, {"name": "V", "desc": "? Photoelectric V(E) magnitude. The precision varies within the data field."}, {"name": "flag2", "desc": "A \"v\" if the magnitude is variable; a colon (:) for uncertainty. If the magnitude given is considered to be a maximum, a code M is given in byte 46."}, {"name": "B-V", "desc": "? B-V color. The precision varies. "}, {"name": "flag3", "desc": "uncertainty flag: colon (:) for uncertainty, \"V\" for variable."}, {"name": "U-B", "desc": "? U-B color. The precision varies. "}, {"name": "flag4", "desc": "U-B flag (see byte 32). A question mark (?) is present if the value is surrounded by parentheses in the published table."}, {"name": "ObsNum", "desc": "? Number of observations, n, for UBV data. "}, {"name": "UBVcode", "desc": "*Code for UBV measurements "}, {"name": "M(V)", "desc": "? Absolute visual magnitude, M(V), taken from various sources, as indicated by the codes in bytes 53-54. Precision varies."}, {"name": "flag5", "desc": "*Flag for M(V) "}, {"name": "Source", "desc": "*Source of M(V) "}, {"name": "U-", "desc": "Sign of U component "}, {"name": "U", "desc": "? U component of the space velocity relative to Sun."}, {"name": "u_U", "desc": "Colon if U uncertain. "}, {"name": "V-", "desc": "Sign of V component "}, {"name": "V", "desc": "? V component of the space velocity "}, {"name": "u_V", "desc": "Colon (:) if V uncertain. "}, {"name": "W-", "desc": "Sign of W component "}, {"name": "W", "desc": "? W component of the space velocity "}, {"name": "u_W", "desc": "Colon (:) if W uncertain. "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VI_115"}} {"id": "VI/115", "title_cds": "Second Epoch Sky Survey Plate List", "title_create": "Read 2005", "year": "2005", "author": "Read M.", "title_pub": "Second Epoch Sky Survey Plate List", "first_author": "Read M.", "ref_biblio": [""], "see_also": ["VI/25 : POSS Plate Data (Palomar Obs. 1960)", "VI/30 : Plates of the ESO Sky Survey (Holmberg+ 1974-)", "VI/114 : second epoch Palomar Oschin Schmidt Sky Survey (POSS2)", "http://www.roe.ac.uk/ifa/wfau/ukstu/pltcat.html : ROE Plate Catalogue"], "keyword_cds": "Surveys; Plate data", "type": ["OC"], "records": ["606 fields"], "data": "", "date_update": "03-Feb-2006", "tables": [{"name": "ukstu.dat", "desc": "List plats for 606 fields ", "columns": [{"name": "FE", "desc": "[OR] Plate prefix, a one- or two-character code for the filter/emulsion combination"}, {"name": "Plate", "desc": "Plate number "}, {"name": "---", "desc": "[*] "}, {"name": "---", "desc": "[R] Color "}, {"name": "Tpl", "desc": "? Non-survey field code "}, {"name": "Field", "desc": "Field number "}, {"name": "RAh", "desc": "Right Ascension 1950 of plate centre (hours) "}, {"name": "RAm", "desc": "Right Ascension 1950 of plate centre (minutes) "}, {"name": "DE-", "desc": "Declination 1950 of plate centre (sign) "}, {"name": "DEd", "desc": "Declination 1950 of plate centre (deg) "}, {"name": "DEm", "desc": "Declination 1950 of plate centre (min) "}, {"name": "Obs.Y", "desc": "Observation date (year) "}, {"name": "Obs.M", "desc": "Observation date (month) "}, {"name": "Obs.D", "desc": "Observation date (day) "}, {"name": "---", "desc": "[:] "}, {"name": "LST", "desc": "Local Sideral Time of start of exposure "}, {"name": "Emuls", "desc": "Plate emulsion "}, {"name": "Filter", "desc": "Filter name "}, {"name": "Exp", "desc": "Exposure time "}, {"name": "Grade", "desc": "Image quality (2) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VI_123"}} {"id": "VI/123", "title_cds": "Photometrical Catalogues and Standards, 1953-1968", "title_create": "Sharov+ 1970", "year": "1970", "author": "Sharov A.S., Jakimova N.N.", "title_pub": "A new, machine-readable version of the compilation \"Photometrical Catalogues and Standards\", updated and revised by M. Morel, 2006 Oct. 24", "first_author": "Sharov A.S.", "ref_biblio": [""], "bibcode": ["1970TrSht..40..106S"], "keyword_cds": "Photometry, sequences; Photometry, standards; Photometry, UBV; Photometry, UcBV; Photometry, UBVRI; Photometry, Eggen", "description": ["The Sharov & Jakimova compilation of published photometrical standards", "is presented as computer readable files. Two main tables (References", "and Catalogue) are presented, plus an Errors file. Russian", "script/terms are replaced by the English equivalents. The original", "coordinate system (1950) are replaced by J2000 positions. A number of", "errors or ambiguous entries have been amended. SIMBAD bibcodes are", "provided for papers cited by Sharov and Jakimova."], "records": ["734 stars"], "data": "", "date_update": "24-Oct-2006", "tables": [{"name": "catalog.dat", "desc": "List of photometric standards/sequences ", "columns": [{"name": "Object", "desc": "Name of object / field / sequence "}, {"name": "RAh", "desc": "Right Ascension (J2000), hours "}, {"name": "RAmin", "desc": "Right Ascension (J2000), minutes "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (J2000), degrees "}, {"name": "DEm", "desc": "Declination (J2000), minutes "}, {"name": "Ref.", "desc": "Ref. number assigned by Sharov & Jakimova "}, {"name": "System", "desc": "Photometric system "}, {"name": "Stars", "desc": "Number of stars in sequence "}, {"name": "Vmag1", "desc": "Bright limit of sequence "}, {"name": "Hyphen", "desc": "Range separator "}, {"name": "Vmag2", "desc": "Faint limit of sequence "}, {"name": "Notes", "desc": "Supplementary remarks "}]}, {"name": "refs.dat", "desc": "SIMBAD Bibcodes for all cited papers ", "columns": [{"name": "Ref.No.", "desc": "Number assigned by Sharov & Jakimova (Table 1). "}, {"name": "Bibcode", "desc": "SIMBAD / NED bibcode "}, {"name": "Reference", "desc": "Full reference from Sharov & Jakimova (Table 1). "}]}, {"name": "errors.dat", "desc": "Amendments included in file Catalog.txt ", "columns": [{"name": "Object", "desc": "Name of object / field / sequence "}, {"name": "RAh", "desc": "Right Ascension (J2000), hours "}, {"name": "RAmin", "desc": "Right Ascension (J2000), minutes "}, {"name": "DE-", "desc": "Declination sign "}, {"name": "DEd", "desc": "Declination (J2000), degrees "}, {"name": "DEm", "desc": "Declination (J2000), minutes "}, {"name": "Ref.", "desc": "Ref. number assigned by Sharov & Jakimova "}, {"name": "Problem", "desc": "Correction or amendment made "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VI_124"}} {"id": "VI/124", "title_cds": "Plate centers of the Direct observations of UKST", "title_create": "SuperCOSMOS, 2002", "year": "2002", "author": "SuperCOSMOS Sky Surveys", "title_pub": "Plate centers of the Direct observations of UKST", "first_author": "SuperCOSMOS Sky Surveys", "ref_biblio": [""], "keyword_cds": "Plate data ; Observatory log", "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["UKST"], "type": ["OC"], "records": ["records"], "data": "", "date_update": "24-Jun-2007"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VI_126"}} {"id": "VI/126", "title_cds": "Catalogue of Wide-Field Plate Archives", "title_create": "Tsvetkova+ 2008", "year": "2008", "author": "Tsvetkova K., Tsvetkov M.", "title_pub": "Catalogue of Wide-Field Plate Archives (V5.2, July 2008)", "first_author": "Tsvetkova K.", "ref_biblio": [""], "see_also": ["http://www.wfpa.bas.bg/ : Wide-Field Plate Database home page", "VI/90 : Wide-Field Plate Database (Tsvetkov+ 1997)"], "keyword_cds": "Observatory log ; Plate data", "keyword_pub": "Catalogues; Photographic plate archives; Plate data", "description": ["The Catalogue of Wide-Field Plate Archives (CWFPAs, version 5.2 from", "July 2008) contains the information for 440 plate archives stored in", "astronomical observatories and institutions all over the world. It is", "an integrated part of the Wide-Field Plate Database (WFPDB) aiming to", "store the valuable astronomical plate observations (more than", "2,200,000 wide-field plates or films) and quickly to offer the", "opportunity to see back in time records of interesting astronomical", "phenomena. The Catalogue provides information for the location", "(storage) of the plate archives - site and country; for the", "observatory, where the archive was made - name, site, country,", "Marsden's number, time zone, coordinates and altitude; for the archive", "instrument - original name, clear aperture, mirror diameter, focal", "length, scale, type, field size and years of operation; for the number", "of direct and objective prism plates; for the archive type, quality", "and the name of astronomer in charge for possible contacts. Search for", "plate archives can be made using the WFPDB instrument identifier", "(equal to archive identifier), which constitutes from the WFPDB", "observatory identifier, instrument aperture, and possible suffix to", "the instrument identifier in the cases when more instruments with the", "same aperture exist in the observatory."], "alias": ["CWFPA"], "type": ["BCC"], "records": ["records"], "data": "", "date_update": "06-Oct-2008", "tables": [{"name": "cwfpa.dat", "desc": "Catalogue of wide-field plate archives ", "columns": [{"name": "IDobs", "desc": "*WFPDB observatory identifier "}, {"name": "IDins", "desc": "*? Instrument aperture "}, {"name": "m_IDins", "desc": "*[A-Z ] Suffix to the instrument identifier "}, {"name": "ORI", "desc": "Original name of the instrument "}, {"name": "LOC.site", "desc": "Location of the plate archive, town (site) "}, {"name": "LOC.ctry", "desc": "Location of the plate archive, country "}, {"name": "OBS.name", "desc": "Observatory, name "}, {"name": "OBS.site", "desc": "Observatory, site "}, {"name": "OBS.ctry", "desc": "Observatory, country "}, {"name": "MNo", "desc": "? Marsden's number "}, {"name": "TZ", "desc": "? Time zone "}, {"name": "LON-", "desc": "? Observatory longitude, sign "}, {"name": "LONd", "desc": "? Observatory longitude, deg "}, {"name": "LONm", "desc": "? Observatory longitude, arcmin "}, {"name": "LAT-", "desc": "? Observatory latitude, sign "}, {"name": "LATd", "desc": "? Observatory latitude, deg "}, {"name": "LATm", "desc": "? Observatory latitude, arcmin "}, {"name": "ALT", "desc": "? Observatory altitude "}, {"name": "MULT", "desc": "? Multiplicity of telescope cameras "}, {"name": "---", "desc": "[x] Sign 'x' "}, {"name": "APR", "desc": "? Clear aperture of the telescope "}, {"name": "MD", "desc": "? Diameter of telescope mirror "}, {"name": "FL", "desc": "? Focal length of the telescope "}, {"name": "SCL", "desc": "? Plate scale "}, {"name": "ITYPE", "desc": "*Instrument type "}, {"name": "FIELD", "desc": "? Field angular dimension "}, {"name": "YEAR1", "desc": "? Year of beginning of telescope operation "}, {"name": "YEAR2", "desc": "? Year of end of telescope operation "}, {"name": "PF", "desc": "Indication F for film, PF for plate and film "}, {"name": "NPd", "desc": "? Number of direct plates "}, {"name": "NPUNd", "desc": "[: ] Uncertainty of the number of plates "}, {"name": "NOT", "desc": "? Notes to the number of plates "}, {"name": "CFORMd", "desc": "*Plate catalog form (direct plates) "}, {"name": "NPs", "desc": "? Number of objective prism plates "}, {"name": "CFORMs", "desc": "*Plate catalog form (obj. prism plates) "}, {"name": "QUAL", "desc": "*[ABD ] Code for plte archive quality "}, {"name": "ANAME", "desc": "Astronomer in charge "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VI_61"}} {"id": "VI/61", "title_cds": "O2 Absorption Cross Sections", "title_create": "Yoshino+ 1992", "year": "1992", "author": "Yoshino K., Esmond J.R., Cheung A.S.-C., Freeman D.E., Parkinson W.H", "title_pub": "High resolution absorption cross sections in the transmission window region of the Schumann-Runge bands and Herzberg continuum of O_2_", "first_author": "Yoshino K.", "ref_biblio": [""], "bibcode": ["1992P&SS...40..185Y"], "keyword_cds": "Atomic physics ; Spectra, ultraviolet", "abstract": ["The absorption cross sections of the Schumann-Runge bands in the", "window region between the rotational lines have been measured in the", "wavelength region 180-195 nm. The measurements have been done with", "many different pressures of oxygen, 2.5-760 torr, so that the", "pressure- dependent absorption can be separated from the main cross", "sections. The published cross sections [Yoshino et al., Planet. Space", "Sci. 31, 339 (1983)] in the window region are superseded by the", "present cross sections. The combined cross sections are available at", "wavenumber intervals of ~0.1 cm-1. The Herzberg continuum cross", "sections are derived after subtracting calculated contributions from", "the Schumann-Runge bands and are significantly smaller than any", "previous measurements."], "type": ["OC"], "records": ["94384 points"], "doi_pub": ["10.1016/0032-0633(92)90056-T"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "o2wb01x0.dat", "desc": "Data file (wave num 49362. - 50050.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb02x0.dat", "desc": "Data file (wave num 50050. - 50720.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb03x0.dat", "desc": "Data file (wave num 50720. - 51370.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb04x0.dat", "desc": "Data file (wave num 50370. - 51980.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb05x0.dat", "desc": "Data file (wave num 51980. - 52661.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb06x0.dat", "desc": "Data file (wave num 52661. - 53250.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb07x0.dat", "desc": "Data file (wave num 53250. - 53746.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb08x0.dat", "desc": "Data file (wave num 53746. - 54256.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb09x0.dat", "desc": "Data file (wave num 54260. - 54685.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb10x0.dat", "desc": "Data file (wave num 54685. - 55115.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb11x0.dat", "desc": "Data file (wave num 55115. - 55485.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}, {"name": "o2wb12x0.dat", "desc": "Data file (wave num 55485. - 55800.) ", "columns": [{"name": "wavenum", "desc": "wave number in cm-1 "}, {"name": "sigma", "desc": "Oxigen cross section/ molecule measured "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VI_77"}} {"id": "VI/77", "title_cds": "Theoretical Stellar Fluxes", "title_create": "Kurucz+Buser, 1994", "year": "1994", "author": "Kurucz R.L., Buser R.B.", "title_pub": "A Library of Theoretical Stellar Fluxes for F- to K-type stars", "first_author": "Kurucz R.L.", "ref_biblio": ["2) abundance relative to Sun (logarithmic scale)"}, {"name": "Vturb", "desc": "[2] Microturbulence velocity "}, {"name": "l/H", "desc": "[0/1.25] Mixing-length-to-scale-height ratio "}]}, {"name": "fm50k2.dat", "desc": "Fluxes, [Fe/H]=-5.00 ", "columns": []}, {"name": "fm45k2.dat", "desc": "Fluxes, [Fe/H]=-4.50 ", "columns": []}, {"name": "fm40k2.dat", "desc": "Fluxes, [Fe/H]=-4.00 ", "columns": []}, {"name": "fm35k2.dat", "desc": "Fluxes, [Fe/H]=-3.50 ", "columns": []}, {"name": "fm30k2.dat", "desc": "Fluxes, [Fe/H]=-3.00 ", "columns": []}, {"name": "fm25k2.dat", "desc": "Fluxes, [Fe/H]=-2.50 ", "columns": []}, {"name": "fm20k2.dat", "desc": "Fluxes, [Fe/H]=-2.00 ", "columns": []}, {"name": "fm15k2.dat", "desc": "Fluxes, [Fe/H]=-1.50 ", "columns": []}, {"name": "fm10k2.dat", "desc": "Fluxes, [Fe/H]=-1.00 ", "columns": []}, {"name": "fm05k2.dat", "desc": "Fluxes, [Fe/H]=-0.50 ", "columns": []}, {"name": "fm03k2.dat", "desc": "Fluxes, [Fe/H]=-0.30 ", "columns": []}, {"name": "fm02k2.dat", "desc": "Fluxes, [Fe/H]=-0.20 ", "columns": []}, {"name": "fp00k2.dat", "desc": "Fluxes, [Fe/H]=+0.00 ", "columns": []}, {"name": "fm01k2.dat", "desc": "Fluxes, [Fe/H]=-0.10 ", "columns": []}, {"name": "fp01k2.dat", "desc": "Fluxes, [Fe/H]=+0.10 ", "columns": []}, {"name": "fp02k2.dat", "desc": "Fluxes, [Fe/H]=+0.20 ", "columns": []}, {"name": "fp03k2.dat", "desc": "Fluxes, [Fe/H]=+0.30 ", "columns": []}, {"name": "fp05k2.dat", "desc": "Fluxes, [Fe/H]=+0.50 ", "columns": []}, {"name": "fp10k2.dat", "desc": "Fluxes, [Fe/H]=+1.00 ", "columns": []}, {"name": "fsun.dat", "desc": "Fluxes, Sun ", "columns": []}, {"name": "fvega.dat", "desc": "Fluxes, Vega ", "columns": []}, {"name": "uvby.f", "desc": "FORTRAN program to compute uvby colors ", "columns": []}, {"name": "uvbyca.f", "desc": "FORTRAN program to compute uvbyca colors ", "columns": []}, {"name": "ubvm50.dat", "desc": "Theoretical UBV, [Fe/H]=-5.00 ", "columns": []}, {"name": "ubvm45.dat", "desc": "Theoretical UBV, [Fe/H]=-4.50 ", "columns": []}, {"name": "ubvm40.dat", "desc": "Theoretical UBV, [Fe/H]=-4.00 ", "columns": []}, {"name": "ubvm35.dat", "desc": "Theoretical UBV, [Fe/H]=-3.50 ", "columns": []}, {"name": "ubvm30.dat", "desc": "Theoretical UBV, [Fe/H]=-3.00 ", "columns": []}, {"name": "ubvm25.dat", "desc": "Theoretical UBV, [Fe/H]=-2.50 ", "columns": []}, {"name": "ubvm20.dat", "desc": "Theoretical UBV, [Fe/H]=-2.00 ", "columns": []}, {"name": "ubvm15.dat", "desc": "Theoretical UBV, [Fe/H]=-1.50 ", "columns": []}, {"name": "ubvm10.dat", "desc": "Theoretical UBV, [Fe/H]=-1.00 ", "columns": []}, {"name": "ubvm05.dat", "desc": "Theoretical UBV, [Fe/H]=-0.50 ", "columns": []}, {"name": "ubvm03.dat", "desc": "Theoretical UBV, [Fe/H]=-0.30 ", "columns": []}, {"name": "ubvm02.dat", "desc": "Theoretical UBV, [Fe/H]=-0.20 ", "columns": []}, {"name": "ubvm01.dat", "desc": "Theoretical UBV, [Fe/H]=-0.10 ", "columns": []}, {"name": "ubvp00.dat", "desc": "Theoretical UBV, [Fe/H]=+0.00 ", "columns": []}, {"name": "ubvp01.dat", "desc": "Theoretical UBV, [Fe/H]=+0.10 ", "columns": []}, {"name": "ubvp02.dat", "desc": "Theoretical UBV, [Fe/H]=+0.20 ", "columns": []}, {"name": "ubvp03.dat", "desc": "Theoretical UBV, [Fe/H]=+0.30 ", "columns": []}, {"name": "ubvp05.dat", "desc": "Theoretical UBV, [Fe/H]=+0.50 ", "columns": []}, {"name": "ubvp10.dat", "desc": "Theoretical UBV, [Fe/H]=+1.00 ", "columns": []}, {"name": "ubvsun.dat", "desc": "UBV, Sun ", "columns": []}, {"name": "ubvvega.dat", "desc": "UBV, Vega ", "columns": []}, {"name": "uvbym50.dat", "desc": "Theoretical uvby, [Fe/H]=-5.00 ", "columns": []}, {"name": "uvbym45.dat", "desc": "Theoretical uvby, [Fe/H]=-4.50 ", "columns": []}, {"name": "uvbym40.dat", "desc": "Theoretical uvby, [Fe/H]=-4.00 ", "columns": []}, {"name": "uvbym35.dat", "desc": "Theoretical uvby, [Fe/H]=-3.50 ", "columns": []}, {"name": "uvbym30.dat", "desc": "Theoretical uvby, [Fe/H]=-3.00 ", "columns": []}, {"name": "uvbym25.dat", "desc": "Theoretical uvby, [Fe/H]=-2.50 ", "columns": []}, {"name": "uvbym20.dat", "desc": "Theoretical uvby, [Fe/H]=-2.00 ", "columns": []}, {"name": "uvbym15.dat", "desc": "Theoretical uvby, [Fe/H]=-1.50 ", "columns": []}, {"name": "uvbym10.dat", "desc": "Theoretical uvby, [Fe/H]=-1.00 ", "columns": []}, {"name": "uvbym05.dat", "desc": "Theoretical uvby, [Fe/H]=-0.50 ", "columns": []}, {"name": "uvbym03.dat", "desc": "Theoretical uvby, [Fe/H]=-0.30 ", "columns": []}, {"name": "uvbym02.dat", "desc": "Theoretical uvby, [Fe/H]=-0.20 ", "columns": []}, {"name": "uvbym01.dat", "desc": "Theoretical uvby, [Fe/H]=-0.10 ", "columns": []}, {"name": "uvbyp00.dat", "desc": "Theoretical uvby, [Fe/H]=+0.00 ", "columns": []}, {"name": "uvbyp01.dat", "desc": "Theoretical uvby, [Fe/H]=+0.10 ", "columns": []}, {"name": "uvbyp02.dat", "desc": "Theoretical uvby, [Fe/H]=+0.20 ", "columns": []}, {"name": "uvbyp03.dat", "desc": "Theoretical uvby, [Fe/H]=+0.30 ", "columns": []}, {"name": "uvbyp05.dat", "desc": "Theoretical uvby, [Fe/H]=+0.50 ", "columns": []}, {"name": "uvbyp10.dat", "desc": "Theoretical uvby, [Fe/H]=+1.00 ", "columns": []}, {"name": "uvbysun.dat", "desc": "uvby, Sun ", "columns": []}, {"name": "uvbyvega.dat", "desc": "uvby, Vega ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VI_80A"}} {"id": "VI/80", "title_cds": "Opacities from the Opacity Project", "title_create": "Seaton+, 1995", "year": "1995", "author": "Seaton M.J., Yan Y., Mihalas D., Pradhan A.K.", "title_pub": "Opacities for stellar envelopes", "first_author": "Seaton M.J.", "ref_biblio": ["", " (OPF)"], "bibcode": ["1994MNRAS.266..805S", "1994MNRAS.265L..25S"], "keyword_pub": "Opacities", "description": ["1 CODES.", "*****", "1.1 Code rop.for", "************", "This code reads opacity files written in standard OP format.", "Its main purpose is to provide documentation on the contents of the", "files.", "This code, like the other codes provided, prompts for the name of", "the file (or files) to be read.", "The file names read in response to the prompt may have up to 128", "characters.", "1.2 Code opfit.for", "**************", "This code reads opacity files in standard OP format, and", "provides for interpolation of opacities to any required values", "of temperature and mass-density. The method used is described in OPF.", "The code prompts for the name of a file giving all required control", "parameters. As an example, the file opfit.dat is provided (users", "will need to change directory names and file names).", "The use of opfit.for is illustrated using opfit.dat.", "Most users will probably want to adapt opfit.for for use as a subroutine", "in other codes.", "Timings for DEC 7000 ALPHA: 0.3 sec for data read and initialisations;", "then 0.0007 sec for each temperature-density point.", "Users who like OPAL formats should note that opfit.for has a facility", "to produce files of OP data in OPAL-type formats.", "1.3 Code ixz.for", "************", "This code provides for interpolations to any required values of X and", "Z. See S95A. It prompts for the name of a file giving all required control", "parameters. An example of such a file if provided, ixz.dat (the user", "will need to change directory and file names).", "The output files have names s92INT.'nnn'. The user specifies the first", "value of nnn, and the number of files to be produced.", "2. DATA FILES", "**********", "2.1 Data files for solar metal-mix", "******************************", "Data for solar metal-mix s92 as defined in SYMP. These files are", "from version 2 runs of December 1994 (see S95A for details on Version 2).", "There are 213 files with names s92.'nnn', 'nnn'=201 to 413.", "Each file occupies 83762 bytes.", "The file s92.version2 gives values of X (hydrogen mass-faction) and", "Z (metals mass-fraction) for each value of 'nnn'. The user can get", "s92.version2, select the values of 'nnn' required, then get the", "required files s92.'nnn'. The user can see the file in ftp,", "displayed on the screen, by typing \"get s92.version2 -\".", "The files s92.'nnn' can be used with opfit.for to obtain opacities", "for any requires value of temperature and mass density.", "Files for other metal-mixtures will be added in due course.", "Send requests to mjs@star.ucl.ac.uk.", "2.2 Files for interpolation in X and Z", "**********************************", "The data files have names s92xz.'mmm', where 'mmm'=001 to 096.", "They differ from the standard OP files (such as s92.'nnn' ---", "section 2.1 above) in that they contain information", "giving derivatives of opacities with respect to X and Z.", "Each file s92xz.'mmm' occupies 148241 bytes.", "The interpolations to any required values of X and Z are made using", "ixz.for.", "Timings: on DEC 7000 ALPHA, 2.16 sec for each new-mixture file.", "For interpolations to some specified values of X and Z, one requires just", "4 files s92xz.'mmm'. Most users will not require the complete set", "of files s92xz.'mmm'. The file s92xz.index includes a table (starting", "on line 3) giving values, for each 'mmm' file, of x,y,z (abundances by", "number-factions) and X,Y,Z (abundances by mass-fractions). Users are", "advised to get the file s92.index, and select values of 'mmm' for", "files required, then get those files.", "The files produced by ixz.for are in standard OP format and can be", "used with opfit.for to obtain opacities for any required values of", "temperature and mass density.", "3 RECOMMENDED PROCEDURE FOR USE OF OPACITY FILES", "**********************************************", "(1) Get the file s92.version2.", "(2) If the values of X and Z you require are available in the", "files s92.'nnn' then get those files.", "(3) If not, get the file s92xz.index.", "(4) Select from s92xz.index the values of 'mmm' which cover the", "range of X and Z in which your are interested. Get those", "files and use ixz.for to generate files for your exact", "required values of X and Z.", "(5) Note that the exact abundance mixtures used are specified in each", "file (see rop.for). Also each run of opfit.for produces a", "table of abundances.", "(6) If you want a metal-mix different from that of s92, contact", "mjs@star.ucl.ac.uk.", "4 FUTURE DEVELOPMENTS", "*******************", "(1) Files will be added very shortly for calculation of radiative", "forces.", "(2) Facilities will be added later which will enable the user", "to make calculations giving files for any required mixtures."], "date_update": "04-Sep-1995", "tables": [{"name": "rop.for", "desc": "Code to read opacity files (s92.* files) ", "columns": []}, {"name": "opfit.for", "desc": "Code to read opacity files and interpolate to any temperature and mass-density.", "columns": []}, {"name": "ixz.for", "desc": "Code for interpolations to any X and Z values ", "columns": []}, {"name": "ixz.dat", "desc": "Example of input for ixz code ", "columns": []}, {"name": "opfit.dat", "desc": "Example of input for opfit code ", "columns": []}, {"name": "s92.version2", "desc": "Summary of solar metal-mix s92 data ", "columns": [{"name": "Version", "desc": "Version designation \"OP Version 2.0 S92\" "}, {"name": "Mix", "desc": "[201/413]+ Mixture number "}, {"name": "text", "desc": "\"X=\" "}, {"name": "X", "desc": "[0/1] Hydrogen mass-fraction "}, {"name": "text", "desc": "\", Z=\" "}, {"name": "Z", "desc": "[0/1] Metal (Z>=3) mass-fraction "}, {"name": "Date", "desc": "Computation date "}]}, {"name": "s92.*", "desc": "Solar metal-mix s92 as defined in SYMP in standard OP format (213 files)", "columns": []}, {"name": "s92xz.*", "desc": "Opacity derivatives with respect to X and Z (96 files)", "columns": []}, {"name": "s92xz.index", "desc": "Summary of s92xz.* files ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VI_93"}} {"id": "VI/93", "title_cds": "Archive of spectrogrammes of AGNs.", "title_create": "Denisyuk+, 1984", "year": "1984", "author": "Denisyuk E.K., Kondrat'eva L.N.", "title_pub": "Archive of spectrogrammes of the active galaxies nuclei.", "first_author": "Denisyuk E.K.", "ref_biblio": [""], "bibcode": ["1984Afz....20..525D"], "keyword_cds": "Active gal. nuclei; Spectroscopy", "description": ["The archive of the spectrogrammes of the active galaxy nucleis", "obtained in the Fessenkov Astrophysical Institute by Denisyuk E.K. and", "Kondrat'eva L.N. during 25 years has been presented. The spectral", "observations have been carried out using the slit spectrograph with", "three-cascades image-tube, attached to 70-cm reflector. The spectral", "region 370 - 850 nm is available. The optical system allows to choose", "the dispersion in the range: 12-200 0.1nm/mm. The spectral resolution", "is 0.8-13 A in dependence on the dispersion. It is the first part of", "the archive."], "records": ["81 AGNs"], "data": "", "date_update": "06-May-2020", "tables": [{"name": "objects.dat", "desc": "List of Objects ", "columns": [{"name": "RAh", "desc": "Right Ascension 2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension 2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension 2000 (seconds) "}, {"name": "DE-", "desc": "Declination 2000 (sign) "}, {"name": "DEd", "desc": "Declination 2000 (degrees) "}, {"name": "DEm", "desc": "Declination 2000 (minutes) "}, {"name": "DEs", "desc": "Declination 2000 (seconds) "}, {"name": "Name", "desc": "Principal Name of galaxies, as in table "}, {"name": "---", "desc": "[=] "}, {"name": "Other", "desc": "Other names of galaxies "}]}, {"name": "table", "desc": "The archive of the spectrograms ", "columns": [{"name": "Name", "desc": "*The name of the galaxy "}, {"name": "Date", "desc": "Observation date "}, {"name": "Disp", "desc": "Dispersion "}, {"name": "Grt", "desc": "Grating parameter "}, {"name": "Ord", "desc": "*Order of grating "}, {"name": "N", "desc": "Number of the spectrogrammes "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VI_94"}} {"id": "VI/94", "title_cds": "Archive of spectrogrammes of planetary nebulae", "title_create": "Kondrat'eva, 1994", "year": "1994", "author": "Kondrat'eva L.N.", "title_pub": "The archive of spectrogrammes of the planetary nebulae", "first_author": "Kondrat'eva L.N.", "ref_biblio": ["="], "bibcode": ["1994PAZh..20...644K"], "keyword_cds": "Planetary nebulae; Spectrophotometry", "description": ["The archive of the spectrogrammes of the planetary nebulae", "obtained in the Fessenkov Astrophysical Institute by Kondrat'eva", "L.N. during 25 years. The spectral observations have been carried", "out using the slit spectrograph with three-cascades image-tube,", "attached to 70-cm reflector. The spectral region is 3700 - 8500A.", "Dispersion is in the range: 12-200 A/mm. The spectral resolution", "is 0.8-13 A in dependence on the dispersion. The part of the", "spectrogrammes has been treated and the results have been", "published [1-7]."], "alias": [""], "records": ["165 PNe"], "data": "", "date_update": "12-Oct-2000", "tables": [{"name": "table", "desc": "The archive of the spectrogrammes ", "columns": [{"name": "name", "desc": "The name of the planetary nebula "}, {"name": "LLpb", "desc": "Lower limit of the passband "}, {"name": "ULpb", "desc": "Upper limit of the passband "}, {"name": "Date", "desc": "Date of observation "}, {"name": "n", "desc": "the number of the spectrograms "}]}, {"name": "objects", "desc": "Objects ", "columns": [{"name": "RAh", "desc": "Right Ascension J2000 (hours) "}, {"name": "RAm", "desc": "Right Ascension J2000 (minutes) "}, {"name": "RAs", "desc": "Right Ascension J2000 (seconds) "}, {"name": "DE-", "desc": "Declination J2000 (sign) "}, {"name": "DEd", "desc": "Declination J2000 (degrees) "}, {"name": "DEm", "desc": "Declination J2000 (minutes) "}, {"name": "DEs", "desc": "? Declination J2000 (seconds) "}, {"name": "name", "desc": "The name of the planetary nebula "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VII_15"}} {"id": "VII/15", "title_cds": "Galactic Supernova Remnants Catalogue", "title_create": "Ilovaisky+ 1972", "year": "1972", "author": "Ilovaisky S.A., Lequeux J.", "title_pub": "Galactic Supernova Remnants Catalogue", "first_author": "Ilovaisky S.A.", "ref_biblio": [""], "bibcode": ["1972A&A....18..169I"], "see_also": ["VII/14 : Galactic Supernova Remnants Catalogue (Clark+ 1976)", "VII/227 : A Catalogue of Galactic Supernova Remnants (Green 2001)"], "keyword_cds": "Supernova remnants; Radio sources", "description": ["Radio-frequency absorption line observations of 20 sources were used", "to calibrate the relation between radio surface brightness and linear", "diameter. Distances for 116 SNR were derived using the new", "calibration. The catalog lists galactic longitude and latitude in", "decimal degrees, source name, flux density (in 10-26 W m-2 Hz-1) at 1", "GHz, mean angular diameter of the source (arcmin), surface brightness", "at 1 GHz, diameter of the remnant (pc), distance of the remnant (kpc),", "scale height from the galactic plane (pc), radial distance to the", "center (kpc), and references (by number given in the original", "publication)."], "records": ["116 SNRs"], "data": "", "date_update": "25-Jul-2004", "tables": [{"name": "data.dat", "desc": "Galactic SNRs Catalog Data ", "columns": [{"name": "GLON", "desc": "Galactic longitude l(II) "}, {"name": "GLAT", "desc": "?Galactic latitude b(II) "}, {"name": "flag", "desc": "*[* ] \"*\" if not a supernova remnant "}, {"name": "ID", "desc": "Name of source "}, {"name": "S", "desc": "*Flux density at one gigahertz in flux units "}, {"name": "AngDiam", "desc": "Mean angular diameter of source "}, {"name": "B", "desc": "Surface brightness at one gigahertz "}, {"name": "Diam", "desc": "Diameter of the remnant in parsecs "}, {"name": "D", "desc": "Distance of the remnant "}, {"name": "H", "desc": "Scale height from galactic plane "}, {"name": "RadGCen", "desc": "Radial distance from the galactic center "}, {"name": "Ref", "desc": "References "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VII_14"}} {"id": "VII/14", "title_cds": "Galactic Supernova Remnants Catalogue", "title_create": "Clark+ 1976", "year": "1976", "author": "Clark D.H., Caswell J.L.", "title_pub": "Galactic Supernova Remnants Catalogue", "first_author": "Clark D.H.", "ref_biblio": [""], "bibcode": ["1976MNRAS.174..267C"], "see_also": ["VII/15 : Galactic Supernova Remnants Catalog (Ilovaisky+ 1972)", "VII/227 : A Catalogue of Galactic Supernova Remnants (Green 2001)"], "keyword_cds": "Supernova remnants; Radio sources", "description": ["The catalog contains observations for southern galactic supernova", "remnants (SNRs). The observations were made at 408 MHz with the", "one-mile cross-type radio telescope at the Molonglo radio observatory", "between 1969 December and 1971 June and were made at 5000 MHz with the", "Parkes 64-m radio telescope between 1968 May and 1973 April. The", "catalog has two files (two tables in published version). The first", "file lists the 97 known SNRs south of declination +18 degrees (i.e.,", "within the scope of the Molonglo survey and gives Molonglo and Parkes", "observational data where available). For completeness the 23 known", "SNRs north of declination +18 degrees are listed in a second file. The", "catalog includes identifications, the 408-MHz integrated flux", "densities, mean angular diameters, and surface brightnesses of the", "SNRs."], "records": ["120 SNRs"], "doi_pub": ["10.1093/mnras/174.2.267"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "data1.dat", "desc": "Southern (Dec < +18 deg) galactic SNRs ", "columns": [{"name": "SNR", "desc": "Galactic source number "}, {"name": "Alt", "desc": "Other catalogue number or name "}, {"name": "n_S(408)", "desc": "[(*> ] Flux density flag 1 (G1) "}, {"name": "S(408)", "desc": "? Integrated flux density estimate at 408MHz "}, {"name": "n_S(408)b", "desc": "[) *] Flux density flag 2 (G1) "}, {"name": "n_S(5000)", "desc": "[( *] Flux density flag 3 (G1) "}, {"name": "S(5000)", "desc": "?Integrated flux density at 5000MHz "}, {"name": "n_S(5000)b", "desc": "[) *] Flux density flag 4 (G1) "}, {"name": "n_SI", "desc": "[( ] Spectral Index flag 1 (G2) "}, {"name": "SI", "desc": "? Spectral index between 408/5000 MHz (G2) "}, {"name": "n_SIb", "desc": "[ )] Spectral Index flag 2 (G2) "}, {"name": "l_AngDiam", "desc": "*[< >] \" < \" or \" > \" where applicable "}, {"name": "AngDiam", "desc": "?Angular diameter of remnant (arc minutes) "}, {"name": "B(408)", "desc": "?Surface brightness at 408 MHz "}, {"name": "r_S(408)", "desc": "*Original reference to 408 MHz flux density "}, {"name": "r_S(5000)", "desc": "Original reference to 5000 MHz flux density "}, {"name": "MapRef", "desc": "Map reference (where possible Molonglo maps) "}]}, {"name": "data2.dat", "desc": "Northern (Dec > +18 deg) galactic SNRs ", "columns": [{"name": "SNR", "desc": "Galactic source number "}, {"name": "Alt", "desc": "Other catalogue number or name "}, {"name": "n_S(408)", "desc": "[( *] Flux density flag 1 (G1) "}, {"name": "S(408)", "desc": "? Integrated flux density estimate at 408 MHz "}, {"name": "n_S(408)b", "desc": "[* )] Flux density flag 2 (G1) "}, {"name": "n_S(5000)", "desc": "[( *] Flux density flag 3 (G1) "}, {"name": "S(5000)", "desc": "?Integrated flux density at 5000 MHz "}, {"name": "n_S(5000)b", "desc": "[) *] Flux density flag 4 (G1) "}, {"name": "n_SI", "desc": "[( ] Spectral Index flag 1 (G2) "}, {"name": "SI", "desc": "? Spectral index between 408/5000 MHz (G2) "}, {"name": "n_SIb", "desc": "[ )] Spectral Index flag 2 (G2) "}, {"name": "l_AngDiam", "desc": "[< >] \" < \" or \" > \" where applicable "}, {"name": "AngDiam", "desc": "?Angular diameter of remnant (arc minutes) "}, {"name": "B(408)", "desc": "?Surface brightness at 408 MHz "}, {"name": "RefList", "desc": "*List of references to recent data "}, {"name": "r_SI", "desc": "Reference for spectral index information "}, {"name": "MapRef", "desc": "*Map reference of the source "}, {"name": "Sv", "desc": "*Spectral Index defined by S(alpha)v(alpha) "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VII_23"}} {"id": "VII/23", "title_cds": "Absorption Lines in QSO Spectra", "title_create": "Ellis+ 1978", "year": "1978", "author": "Ellis R.S., Phillipps S.", "title_pub": "A Catalogue of Absorption Lines in QSO Spectra", "first_author": "Ellis R.S.", "ref_biblio": [""], "bibcode": ["1978MNRAS.183..271E"], "keyword_cds": "QSOs ; Spectroscopy", "description": ["The catalog is a collection of spectral data for 128 quasi-stellar", "objects (QSO). The data have been assembled from the catalogs of de", "Veny et al. (1971), Smith-Haenni (1977), and Burbidge et al. (1977).", "To ensure every observation is recorded and to search for new or", "omitted results, the entire literature up to 1977 September was", "scanned. The catalog distributed by the ADC is an updated version of", "the original catalog published as microfiche in Ellis and Phillipps", "(1978). The catalog includes object names, positions and", "identifications, V, B-V, U-B, emission redshifts, observation", "references, analyses, and line lists.", "The lists of observed spectral lines come from many observers and", "instruments. References to observations and to analyses are included", "for each QSO, as are alternate names for the QSO, coordinates, and", "magnitude. Each observed line has a reference to the observer, and", "most have the possible line identifications and redshifts listed as", "well. See the original paper for a discussion of the purpose behind", "the compilation of the catalog, in particular, for a discussion of its", "use as a base of raw spectral data that is not tied to any particular", "redshift system."], "records": ["108 records"], "doi_pub": ["10.1093/mnras/183.2.271"], "data": "", "date_update": "19-Jan-2020", "tables": [{"name": "id.dat", "desc": "Identification of each object ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "Ident", "desc": "*Object identifiers "}, {"name": "LineRec", "desc": "*Number of line data records "}]}, {"name": "coord.dat", "desc": "Coordinates ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "RAtag", "desc": "Right Ascension tag, \"RA=\" "}, {"name": "RAh", "desc": "RA hours (B1950) "}, {"name": "RAm", "desc": "RA minutes "}, {"name": "RAs", "desc": "RA seconds "}, {"name": "Dectag", "desc": "Declination tag, \"DEC=\" "}, {"name": "DE-", "desc": "Dec sign "}, {"name": "DEd", "desc": "Dec degrees (B1950) "}, {"name": "DEm", "desc": "Dec arc minutes "}, {"name": "DEs", "desc": "Dec arc seconds "}, {"name": "IDtag", "desc": "*ID reference tag "}, {"name": "IDref", "desc": "*ID reference "}]}, {"name": "mag.dat", "desc": "Magnitudes ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "Magtag", "desc": "Magnitude tag, \"V=\" "}, {"name": "Vmag", "desc": "*Visual magnitude "}, {"name": "Varflag", "desc": "*Variability flag "}, {"name": "B-Vtag", "desc": "B-V color tag, \"B-V=\" "}, {"name": "B-V", "desc": "*B-V color "}, {"name": "U-Btab", "desc": "U-B color tag, \"U-B=\" "}, {"name": "U-B", "desc": "*U-B color "}, {"name": "Ztag", "desc": "Emission redshift tag, \"ZEM=\" "}, {"name": "Z", "desc": "*Emission redshift "}, {"name": "q_Z", "desc": "*Redshift quality flag "}, {"name": "Lflag", "desc": "Left parenthesis "}, {"name": "Nline", "desc": "*? Number of emission lines "}, {"name": "Rflag", "desc": "Right parenthesis "}]}, {"name": "lines.dat", "desc": "line data ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "Lstflag", "desc": "*Last line flag "}, {"name": "ObsWave", "desc": "*? Observed wavelength "}, {"name": "Gsymbol", "desc": "*Group symbols "}, {"name": "RefNum", "desc": "*? Observer reference number "}, {"name": "S-EW", "desc": "*Strength or equivalent width "}, {"name": "Ion", "desc": "*Identified ion "}, {"name": "RestWave", "desc": "? Ion rest wavelength "}, {"name": "Z", "desc": "*? Actual redshift "}, {"name": "SysNum", "desc": "*System numbers "}]}, {"name": "note.dat", "desc": "notes ", "columns": [{"name": "ID", "desc": "Object running number "}, {"name": "note", "desc": "General notes for each object "}]}, {"name": "obs.dat", "desc": "note of observations and analyses ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VII_230"}} {"id": "VII/230", "title_cds": "CfA Redshift Survey, Version Feb. 2000", "title_create": "Huchra+ 2000", "year": "2000", "author": "Huchra J.P., et al.", "title_pub": "The CfA Redshift Survey, Version Feb. 2000", "first_author": "Huchra J.P.", "ref_biblio": [""], "keyword_cds": "Redshifts", "description": ["The CfA Redshift Survey was started in 1977 by Marc Davis, John", "Huchra, Dave Latham and John Tonry. The First CfA Survey, completed in", "1982, (Huchra, Davis, Latham and Tonry, 1983, ApJS 52, 89) had as its", "goal the measurement of radial velocities for all galaxies brighter", "than 14.5 and at high galactic latitude in the merged catalogs of", "Zwicky and Nilson (the UGC). This survey produce the first large area", "and moderately deep maps of large scale structure in the nearby", "universe, as well as the first crude but truly quantitative", "measurements of the 3-D clustering properties of galaxies. The second", "CfA survey (CfA2) was started by John Huchra and Margaret Geller in", "the winter of 1984/5. Between 1985 and 1995, we and our students and", "co-workers measured relative distances via redshifts for about 18,000", "bright galaxies in the northern sky."], "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["zCat", "CfA"], "type": ["CCC"], "records": ["records"], "data": "", "date_update": "05-Oct-2002"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VII_268"}} {"id": "VII/268", "title_cds": "South-Equatorial Galaxy Catalogue", "title_create": "Corwin+ 2010", "year": "2010", "author": "Corwin H.G. Jr, Skiff B.A.", "title_pub": "South-Equatorial Galaxy Catalogue, Version 1.4.3", "first_author": "Corwin H.G. Jr", "ref_biblio": [""], "bibcode": ["2010yCat.7268....0C"], "see_also": ["VII/116 : Southern Galaxy Catalogue (SGC) (Corwin+ 1985)"], "keyword_cds": "Galaxies, optical ; Positional data ; Morphology ;", "description": ["This version (1.4.3) of the South-Equatorial Galaxy Catalogue (SEGC)", "contains accurate positions, diameters, position angles, and de", "Vaucouleurs revised Hubble-Sandage (VRHS) types for 3333 single or", "multiple galaxies in the south-equatorial declination zones between", "+03 and -21{deg}. The data were gleaned from POSS1 103a-O copy plates,", "then checked against the UKST IIIa-J portion of the DSS. The corrected", "position angles and VRHS types are published here in full for the", "first time. Notes on the individual objects are also available. SEGC", "provides a finding list for galaxies generally larger than about 1.8", "arcmin at the 25.0 B-mag.arcsec^-2^ in the south-equatorial zone."], "alias": ["SEGC-1.4.3", "SEGC"], "type": ["CCC"], "records": ["records"], "data": "", "date_update": "05-Oct-2012", "tables": [{"name": "segc143.dat", "desc": " ", "columns": [{"name": "RAh", "desc": "Right Ascension B1950 (hours) "}, {"name": "RAm", "desc": "Right Ascension B1950 (minutes) "}, {"name": "RAs", "desc": "Right Ascension B1950 (seconds) "}, {"name": "DE-", "desc": "Declination B1950 (sign) "}, {"name": "DEd", "desc": "Declination B1950 (degrees) "}, {"name": "DEm", "desc": "Declination B1950 (minutes) "}, {"name": "DEs", "desc": "[0/60] Declination B1950 (seconds) "}, {"name": "Np", "desc": "number of positions used "}, {"name": "Src.pos", "desc": "Position sources "}, {"name": "Names", "desc": "Names of this galaxy found in the literature "}, {"name": "NEDname", "desc": "NED-friendly name "}, {"name": "MType", "desc": "Morphological type on the deVaucouleurs revied Hubble-Sandage system "}, {"name": "n_logD", "desc": "[[] '[' if the diameter applies to more than 1 galaxy "}, {"name": "logD", "desc": "log of major diameter expressed in 0.1arcmin "}, {"name": "u_logD", "desc": "[:? ] Uncertainty flags on logD "}, {"name": "e_logD", "desc": "? standard deviation in logD when 2 or more values were averaged. "}, {"name": "logR", "desc": "Ratio max/min axis "}, {"name": "u_logR", "desc": "[:? ] Uncertainty flags on logR "}, {"name": "e_logR", "desc": "? standard deviation in logR "}, {"name": "---", "desc": "[]] "}, {"name": "Nd", "desc": "Number of diameters and axis rations used "}, {"name": "n_PA", "desc": "[[] '[' if the position angle applies to more than 1 galaxy "}, {"name": "PA", "desc": "?=--- Position angle of major axis "}, {"name": "u_PA", "desc": "[:? ] Uncertainty flags on PA "}, {"name": "---", "desc": "[]] "}, {"name": "e_PA", "desc": "? standard deviation in PA "}, {"name": "Na", "desc": "Number of position angles "}]}, {"name": "notes.dat", "desc": "Notes ", "columns": []}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VII_90A"}} {"id": "VII/90A", "title_cds": "Merged Catalogue of Galaxies", "title_create": "Kogoshvili 1983-1986", "year": "1986", "author": "Kogoshvili N.G.", "title_pub": "Merged Catalogue of Galaxies", "first_author": "Kogoshvili N.G.", "ref_biblio": ["", "", ""], "bibcode": ["1983BICDS..25...63K"], "keyword_cds": "Galaxy catalogs;", "description": ["The catalog has been compiled at Abastumani Astrophysical Observatory.", "It comprises, on the whole, nearly all galaxies in the region between", "+90 degrees and -33 degrees declination and brighter than mag 15.1 as", "well as some fainter ones. The Morphological Catalogue of Galaxies has", "been used as a main source of data for this catalog. The number of", "galaxies in the catalog is 31917. The catalog is kept up to date, and", "this version adds the data published from 1973-1983. The catalog", "includes designations, equatorial coordinates, magnitudes and colors,", "angular diameters, surface brightness, position angles, detailed", "structure descriptions, classifications on several different systems,", "rotation curve data, supernova dates and counts, HII regions, radio", "flux densities, multiple-system membership, and interaction details in", "the first file. The second file lists the full forms of the references", "cited by code numbers in the first file. Also included are brief", "descriptions of the content of second file lists the full forms of the", "references cited by code numbers in the first file. Also included are", "brief descriptions of the content of each reference."], "records": ["31917 galaxies"], "data": "", "date_update": "04-Nov-1999", "tables": [{"name": "adc.doc", "desc": "Documentation from ADC by Anne C. Raugh ", "columns": []}, {"name": "catalog", "desc": "The Merged Catalogue of Galaxies ", "columns": [{"name": "MCG", "desc": "Morphological Catalog of Galaxies (MCG) number "}, {"name": "Name", "desc": "NGC, IC, or Anonymous RC1 number "}, {"name": "Info", "desc": "[*] '*' if additional information is given (It is not clear what \"additional information\" this flag alludes to)"}, {"name": "RAh", "desc": "Hours RA, epoch 1950.0 "}, {"name": "RAm", "desc": "Minutes RA, epoch 1950.0 "}, {"name": "RAs", "desc": "Seconds RA, epoch 1950.0 "}, {"name": "DE-", "desc": "Degrees Dec, epoch 1950.0 "}, {"name": "DEd", "desc": "Degrees Dec, epoch 1950.0 "}, {"name": "DEm", "desc": "Minutes Dec, epoch 1950.0 "}, {"name": "Mag", "desc": "? Integrated magnitude "}, {"name": "q_Mag", "desc": "[0/3]? Magnitude accuracy code (1) "}, {"name": "r_Mag", "desc": "[1/253]? Magnitude reference code (2) "}, {"name": "n_Mag", "desc": "[Z] 'Z' if Mag is from 2 or more galaxies "}, {"name": "MagCnt", "desc": "? Number of galaxies contributing to Mag "}, {"name": "MajDiamIn", "desc": "? Major angular diameter, inner part "}, {"name": "MinDiamIn", "desc": "? Minor angular diameter, inner part "}, {"name": "SurfBrIn", "desc": "[1/6]? Surface brightness of inner part of galaxy as in MCG (3)"}, {"name": "MajDiamWh", "desc": "? Major angular diameter, whole galaxy "}, {"name": "MinDiamWh", "desc": "? Minor angular diameter, whole galaxy "}, {"name": "l_MajDiamWh", "desc": "[>] '>' if [Min,Maj]DiamWh are lower limits "}, {"name": "SurfBr1", "desc": "[1/6]? Surface brightness, first outer region (3)"}, {"name": "SurfBr2", "desc": "[1/6]? Surface Brightness, second outer region (3)"}, {"name": "Incl", "desc": "[1/5]? Estimated inclination to the line of sight as in MCG (4)"}, {"name": "MajDiamB", "desc": "? Major angular diameter from POSS blue print "}, {"name": "MinDiamB", "desc": "? Minor angular diameter from POSS blue print "}, {"name": "MajDiamR", "desc": "? Major angular diameter from POSS red print "}, {"name": "MinDiamR", "desc": "? Minor angular diameter from POSS red print "}, {"name": "POSS_Unc", "desc": "[1/3]? Code for uncertainty in POSS angular diameters (5)"}, {"name": "PosAng", "desc": "? Position angle from UGC (ref.10) "}, {"name": "u_PosAng", "desc": "[1/3]? Code for uncertainty in PosAng (6) "}, {"name": "GenApp", "desc": "[EPLF] General appearance code from MCG "}, {"name": "GenDet1", "desc": "Structural detail 1 (see adc.doc) "}, {"name": "GenDet2", "desc": "Structural detail 2 (see adc.doc) "}, {"name": "fGal/Sup", "desc": "Faint galaxy or superimposed star description (see adc.doc) (7)"}, {"name": "GalStar", "desc": "Structure of the faint galaxy, or inclination, or position of the star (byte 121='*') (see adc.doc)"}, {"name": "NucCnt", "desc": "? Number of nuclei seen in contact "}, {"name": "InnDet", "desc": "Inner region detail (see adc.doc) "}, {"name": "NucInn1", "desc": "Nuclear inner region detail 1 (see adc.doc) "}, {"name": "NucInn2", "desc": "Nuclear inner region detail 2 (see adc.doc) "}, {"name": "Out1Sep", "desc": "Outer region 1 separation symbol (see adc.doc) "}, {"name": "Out1Ndet", "desc": "Outer region 1 number of structural details "}, {"name": "Out1Gen", "desc": "Outer region 1 general description "}, {"name": "Out1Det", "desc": "Outer region 1 structural details "}, {"name": "Out1Unc", "desc": "Outer region 1 structure uncertainty flag "}, {"name": "Out2Sep", "desc": "Outer region 2 separation symbol (see adc.doc) "}, {"name": "Out2Ndet", "desc": "Outer region 2 number of structural details "}, {"name": "Out2Gen", "desc": "Outer region 2 general description "}, {"name": "Out2Det", "desc": "Outer region 2 structural details "}, {"name": "Out2Unc", "desc": "Outer region 2 structure uncertainty flag "}, {"name": "Out3Sep", "desc": "Outer region 3 separation symbol (see adc.doc) "}, {"name": "Out3Ndet", "desc": "Outer region 3 number of structural details "}, {"name": "Out3Gen", "desc": "Outer region 3 general description "}, {"name": "Out3Det", "desc": "Outer region 3 structural details "}, {"name": "Out3Unc", "desc": "Outer region 3 structure uncertainty flag "}, {"name": "Out4Sep", "desc": "Outer region 4 separation symbol (see adc.doc) "}, {"name": "Out4Ndet", "desc": "Outer region 4 number of structural details "}, {"name": "Out4Gen", "desc": "Outer region 4 general description "}, {"name": "Out4Det", "desc": "Outer region 4 structural details "}, {"name": "Out4Unc", "desc": "Outer region 4 structure uncertainty flag "}, {"name": "Out5Sep", "desc": "Outer region 5 separation symbol (see adc.doc) "}, {"name": "Out5Ndet", "desc": "Outer region 5 number of structural details "}, {"name": "Out5Gen", "desc": "Outer region 5 general description "}, {"name": "Out5Det", "desc": "Outer region 5 structural details "}, {"name": "Out5Unc", "desc": "Outer region 5 structure uncertainty flag "}, {"name": "r_Hubble", "desc": "[RPU] Source of revised Hubble class (8) "}, {"name": "HubbleRing", "desc": "Revised Hubble class, outer ring "}, {"name": "Hubble", "desc": "Revised Hubble classification "}, {"name": "HubblePec", "desc": "Revised Hubble class, peculiarities "}, {"name": "Morgan", "desc": "Morgan classification type "}, {"name": "MorganSpc", "desc": "Morgan classification spectral class "}, {"name": "MorganPec", "desc": "Morgan classification peculiarities "}, {"name": "Class", "desc": "Hubble or van den Bergh classification (9) "}, {"name": "r_Class", "desc": "[RU] Source of Hubble or van den Bergh class. "}, {"name": "RV", "desc": "? Heliocentric radial velocity "}, {"name": "r_RV", "desc": "[1/253]? Reference for RV "}, {"name": "RVo", "desc": "? Radial velocity corrected for solar motion "}, {"name": "r_RVo", "desc": "[1/253]? Reference for RVo "}, {"name": "RotVel", "desc": "? Rotational velocity "}, {"name": "R.H", "desc": "? Distance from center of the bending point in the rotational velocity curve; units are arcmin(Ref.11) or kpc(Ref.12)"}, {"name": "l_R.H", "desc": "'>' if R.H is a lower limit "}, {"name": "r_RotVel", "desc": "[1/253]? Reference for RotVel and R.H "}, {"name": "SN_Yr1", "desc": "? Year of first observed supernova "}, {"name": "SN_Yr2", "desc": "? Year of second observed supernova "}, {"name": "SN_Cnt", "desc": "? Number of observed supernovae (Ref.49) "}, {"name": "HII", "desc": "? Number of H II regions "}, {"name": "r_HII", "desc": "[1/253]? H II region reference code "}, {"name": "U-B", "desc": "? Integrated U-B "}, {"name": "r_U-B", "desc": "[1/253]? Integrated U-B reference code "}, {"name": "B-V", "desc": "? Integrated B-V "}, {"name": "r_B-V", "desc": "[1/253]? Integrated B-V reference code "}, {"name": "(U-B)(0)", "desc": "? Integrated face-on U-B, from RC1 or RC2 "}, {"name": "(B-V)(0)", "desc": "? Integrated face-on (B-V)o, from RC1 or RC2 "}, {"name": "Spectrum", "desc": "Integral spectrum "}, {"name": "Flux178", "desc": "? Flux density at 178 MHz "}, {"name": "r_Flux178", "desc": "[1/253]? Reference of Flux178 "}, {"name": "Flux780", "desc": "? Flux density at 780 MHz "}, {"name": "r_Flux780", "desc": "[1/253]? Reference of Flux780 "}, {"name": "Flux1400", "desc": "? Flux density at 1400 MHz (21cm) "}, {"name": "r_Flux1400", "desc": "[1/253]? Reference of Flux1400 "}, {"name": "Flux2700", "desc": "? Flux density at 2700 MHz (11cm) "}, {"name": "r_Flux2700", "desc": "[1/253]? Reference of Flux2700 "}, {"name": "Flux5000", "desc": "? Flux density at 5000 MHz (6cm) "}, {"name": "r_Flux5000", "desc": "[1/253]? Reference of Flux5000 "}, {"name": "CGCG", "desc": "? CGCG (Ref.2) number of nearby cluster "}, {"name": "inCCG", "desc": "[1] '1' if galaxy in CCG (Ref.55) "}, {"name": "inMKN", "desc": "[1] '1' if galaxy in Markarian's (ref.56) "}, {"name": "inIG", "desc": "[1] '1' if galaxy in Isolated Gal. (ref.58) "}, {"name": "inIPG", "desc": "[1] '1' if galaxy in Isolated Pairs (ref.57) "}, {"name": "ByuType", "desc": "Byurakan classification of nucleus "}, {"name": "EmLines", "desc": "[1] '1' if emission lines in spectrum (ref.54) "}, {"name": "CompCode", "desc": "[1/4]? Companion code (10) "}, {"name": "MultCode", "desc": "Multiple-galaxy membership code (see adc.doc) "}, {"name": "CompMCG", "desc": "? MCG number of companion galaxy "}, {"name": "Isolation", "desc": "? Degree of isolation (see adc.doc) "}, {"name": "InterCnt", "desc": "? Number of members observed to be interacting "}, {"name": "u_InterType", "desc": "[BQ] 'B' if interaction is evident, 'Q' if interaction is suspected (11)"}, {"name": "InterType", "desc": "? Interaction type (11) "}, {"name": "Distortion", "desc": "? Type of galaxy distortion (see adc.doc) "}, {"name": "Sep", "desc": "? Angular separation "}, {"name": "FCompCnt", "desc": "? Number of faint components "}, {"name": "FCompCode", "desc": "[1/4]? Code for type of faint component (12) "}, {"name": "FCompMCG", "desc": "? Faint component MCG number or magnitude (13) "}, {"name": "CompDist", "desc": "? Angular distance to the nearest companion "}]}, {"name": "refs", "desc": "References ", "columns": [{"name": "RefNum", "desc": "[1/253]? Reference code number, blank if a continuation of the previous record."}, {"name": "Text", "desc": "Text of reference "}, {"name": "Subject", "desc": "Subject matter of reference "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VIII_93"}} {"id": "VIII/93", "title_cds": "The VLA Low-frequency Sky Survey at 74MHz", "title_create": "Cohen+ 2007-2013", "year": "2013", "author": "Cohen A.S., Lane W.M., Cotton W.D., Kassim N.E., Lazio T.J.W., Perley R.A., Condon J.J., Erickson W.C. < Astron. J. 134, 1245 (2007) >", "title_pub": "The VLA Low-frequency Sky Survey, Version 2013", "first_author": "Cohen A.S.", "ref_biblio": [""], "bibcode": ["2007AJ....134.1245C", "2013yCat.8093....0C"], "keyword_cds": "Radio continuum ; Radio sources ; Surveys", "keyword_pub": "Atmospheric Effects - Catalogs - Radio Continuum: General - Surveys", "abstract": ["The VLA Low-Frequency Sky Survey (VLSS) is a 74MHz (4m) continuum", "survey covering the entire sky north of -30{deg} declination. Using", "the VLA in B- and BnA-configurations, we will map the entire survey", "region at a resolution of 80\" and with an average rms noise of 0.1", "Jy/beam. For a detailed description of the survey and its scientific", "motivations, please see the original proposal to the NRAO skeptical", "review committee.", "The VLSS is being made as a service to the astronomical community,", "and the principal data products are being released to the public as", "soon as they are produced and verified. Details and access to the", "images can be found at http://lwa.nrl.navy.mil/VLSS/"], "object": [], "curator": "Francois Ochsenbein [CDS]", "alias": ["VLSS", "4MASS"], "type": ["OC"], "records": ["records"], "doi_pub": ["10.1086/520719"], "data": "", "date_update": "19-Jan-2020"} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VIII_104"}} {"id": "VIII/104", "title_cds": "SPECFIND V3.0 Catalog of radio continuum spectra", "title_create": "Stein+, 2020", "year": "2020", "author": "Stein Y., Vollmer B., Boch T., Landais G., Vannier P., Brouty M., Allen M.G., Derriere S., Ocvirk P.", "title_pub": "A method for determining radio continuum spectra, and its application to large surveys", "first_author": "Stein Y.", "ref_biblio": [""], "bibcode": ["2020yCat.8104....0S"], "see_also": ["VIII/13 : A new catalog of 53522 4.85GHz sources (BWE) (Becker+ 1991)", "VIII/14 : 87GB Catalog of radio sources (Gregory et al., 1991)", "VIII/15 : Parkes Radio Sources Catalogue (PKS) (Wright+ 1990)", "VIII/16 : Molonglo Reference Catalogue of Radio Sources (MRC) (Large+ 1991)", "VIII/17 : The North 20cm Survey (WB) (White+ 1992)", "VIII/36 : The Second Bologna Survey (B2) (Colla+ 1970-1974)", "VIII/37 : The Third Bologna Survey (B3) (Ficarra+ 1985)", "VIII/38 : The Parkes-MIT-NRAO 4.85GHz (PMN) Surveys (Griffith+ 1993-1996)", "VIII/40 : GB6 catalog of radio sources (Gregory+ 1996)", "VIII/42 : Texas Survey of radio sources at 365MHz (TXS) (Douglas+ 1996)", "VIII/44 : Miyun 232MHz survey (MIYUN) (Zhang+ 1997)", "VIII/52 : The MIT-Green Bank 5GHz Survey (Bennett+, 1986-91)", "VIII/60 : Interferometer phase calibration sources (JVAS) (Patnaik+ 1998)", "VIII/62 : The Westerbork Northern Sky Survey (WENSS) (Leiden, 1998)", "VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)", "VIII/69 : The WISH catalogue at 352 MHz (de Breuck+ 2002)", "VIII/70 : Sydney University Molonglo Sky Survey (SUMSS) (Mauch+ 2003)", "VIII/71 : The FIRST Survey Catalog, Version 03Apr11 (Becker+ 2003)", "J/A+AS/85/805 : 11cm radio continuum survey. IV. (F3R) (Fuerst+ 1990)"], "keyword_cds": "Radio sources ; Galaxies, radio ; Radio continuum", "keyword_pub": "astronomical data bases: miscellaneous - radio continuum: general", "abstract": ["Many radio continuum catalogs with different sensitivity limits and", "spatial resolutions are published via the VizieR database. Because of", "the diversity of spatial resolution, the cross-identification of", "individual sources is complex. By assuming a power-law spectrum, the", "SPECFIND tool is able to handle radio surveys at different frequencies", "from different instruments and different resolutions.", "The SPECFIND V3.0 radio cross-identification catalog uses in its here", "presented latest version, 204 radio continuum catalogs from the VizieR", "database of the Centre de Donnees astronomiques de Strasbourg (CDS) to", "cross-correlate sources and fit their spectral slope. A total of 91", "new catalogs form VizieR were added to the previous version to reach a", "wider frequency range, especially the lower frequency radio regime as", "well as to have better spatial coverage of the entire sky.", "We adapted special selection criteria to all radio tables listed in", "VizieR to define a final sample of new catalogs. We implemented the", "new catalogs into the SPECFIND tool by unifying them and then compare", "the results to the last version. Furthermore we present and", "investigate sources with spectral breaks around 1.4GHz and around", "325MHz.", "By increasing the number of implemented SPECFIND catalogs from 115 to", "204, we improve the number of resulting spectra from 107500 to 340000", "and increase the number of cross-identified sources from 600000 to 1.6", "million. Furthermore, we present two samples of spectral break", "sources. The first sample includes 5515 spectral break sources with", "turnover frequencies around 1.4GHz, the second sample includes 19591", "spectral break sources with turnover frequencies around 325MHz. Both", "samples consist of concave sources, Gigaherz-Peaked Spectrum (GPS) and", "Megaherz-Peaked Spectrum (MPS) sources and genuine GPS/MPS sources.", "SPECFIND V3.0 is a powerful open access tool, reachable via VizieR to", "investigate sources either by looking at the cross-correlated sources", "or to investigate spectral index behaviours. The new version presented", "here brings this tool up to date by implementing the large surveys of", "the last 10 years."], "description": ["We present a new version of SPECFIND. The SPECFIND tool was", "successfully upgraded from 115 catalogs in version 2.0 to version 3.0", "with a final number of 204 processed catalogs. 89 new catalogs were", "ingested and two catalogs were updated. The final number of resulting", "spectra was increased more than a factor of three from 107500 in", "version 2.0 to 340000 in version 3.0. The number of objects with", "cross-identified sources was more than doubled from 600000 in version", "2.0 to 1.6 million in version 3.0.", "The main result is presented in table \"spectra\" with every radio", "continuum source having one entry row. The different objects/spectra", "are named by different sequence numbers (column \"Seq\"). All radio", "continuum sources with the same sequence number belong to the same", "object/spectrum. In the second column, the name of the source is given", "followed by the number of sources within the spectrum (\"N\"). The", "columns \"a\" and \"b\" are the spectral index and the abscissa of the", "spectral fit, respectively. The sixth column contains the frequency of", "the catalog, followed by the flux density, its error and the position", "of the source (Right Ascension and Declination). The column \"SED\" is a", "link to the spectral fit, i.e. the spectrum containing this source.", "The next column \"Aladin\" shows an Aladin Lite6 view of the source. The", "last column gives the beam size of the observation.", "The \"beam\" table contains all 204 tables from the VizieR catalogs", "which were used in SPECFIND V3.0.", "The \"waste\" table has the same general structure as \"spectra\", but", "contains measurements which were cross-identified by position but did", "not match the power-law spectrum. These points are added to the VizieR", "SED plot.", "The spectral break sources are provided in two different tables. The", "first table contains all 5515 spectral break sources including the 210", "concave sources with turnover frequencies around 1.4GHz. The second", "table lists the 19691 spectral break sources including the 900 concave", "sources with turnover frequencies around 325MHz. The structure of the", "tables is similar to the spectra table. The first column gives the", "running number \"Seq\". The sources belonging to the same spectrum have", "the same sequence number. The second column provides the source name;", "the third column the type (spectral break (sb), concave (conc),", "GPS/MPS (gps/mps), GGPS/GMPS (ggps/gmps)), followed by the spectral", "slope and the abscissa associated with the source. In the next column,", "the mean spectral slope of the part of the spectrum (lower or higher", "frequency part) is given. Then the frequency, the flux density and its", "error are listed. Lastly, the position (Right Ascension and", "Declination) and the beam/resolution are specified."], "alias": ["SPECFIND", "SPECFIND3", ""], "type": ["GCC"], "records": ["631736 spectra"], "data": "f", "date_creation": "22-Jan-2020", "date_update": "14-Apr-2021", "tables": [{"name": "spectra.dat", "desc": "The parameters of the radio spectra ", "columns": [{"name": "Seq", "desc": "[1/339592] Sequential number of the spectrum (1) "}, {"name": "Name", "desc": "Main name of the radio source (G1) "}, {"name": "N", "desc": "[2/34] Number of points in spectrum "}, {"name": "a", "desc": "Slope of spectrum (3) "}, {"name": "b", "desc": "Abscissa of spectrum (3) "}, {"name": "nu", "desc": "[16/31000] Frequency "}, {"name": "S(nu)", "desc": "Flux density at frequency nu "}, {"name": "e_S(nu)", "desc": "Mean error on S(nu) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) of source "}, {"name": "DEdeg", "desc": "Declination (J2000) of source "}, {"name": "dFlux", "desc": "Difference with flux expected from NVSS "}, {"name": "dRA", "desc": "Offset in RA from NVSS source "}, {"name": "dDE", "desc": "Offset in DE from NVSS source "}]}, {"name": "waste.dat", "desc": "Source parameters based on positional cross-id ", "columns": [{"name": "Assoc", "desc": "Main name of the radio association (G1) "}, {"name": "Seq", "desc": "[-3326064/339592] Spectrum Sequential number (1) "}, {"name": "nu", "desc": "[16/31000] Frequency "}, {"name": "S(nu)", "desc": "Flux density at frequency nu "}, {"name": "e_S(nu)", "desc": "Mean error on S(nu) "}, {"name": "RAdeg", "desc": "Right ascension (J2000) of source "}, {"name": "DEdeg", "desc": "Declination (J2000) of source "}, {"name": "Name", "desc": "Name of the associated radio source (G1) "}]}, {"name": "beam.dat", "desc": "Characterisation of catalogues in SPECFIND ", "columns": [{"name": "Name", "desc": "Catalog abbreviation used in SPECFIND (G1) "}, {"name": "Abrev", "desc": "Other abbreviation "}, {"name": "I", "desc": "[I&S? -] Interferometer or Single dish "}, {"name": "nu", "desc": "[16,31000] Frequency "}, {"name": "beam", "desc": "Beam size "}, {"name": "Smin", "desc": "? Sensitivity limit "}, {"name": "N", "desc": "Number of sources in catalog "}, {"name": "Cov", "desc": "Coverage "}, {"name": "sp", "desc": "? Percentage of sources having a spectrum "}, {"name": "BibCode", "desc": "Reference's bibcode "}, {"name": "Cat", "desc": "Catalog acronyms in VizieR "}]}, {"name": "ghzbreak_cand.dat", "desc": "Spectral break sources at 1.4 GHz candidates (table A2)", "columns": [{"name": "Seq", "desc": "[1/19691] The sources belonging to the same spectrum have the same sequence number (1)"}, {"name": "Name", "desc": "Source name "}, {"name": "cat", "desc": "Spectral break code (2) "}, {"name": "Resolved", "desc": "[0/1] Resolved (1) flag (3) "}, {"name": "a", "desc": "Spectral slope associated with the source "}, {"name": "b", "desc": "? Abscissa associated with the source "}, {"name": "alow", "desc": "Spectral slope at low frequencies "}, {"name": "e_alow", "desc": "rms uncertainty on spectral slope at low frequencies"}, {"name": "ahigh", "desc": "Spectral slope at high frequencies "}, {"name": "e_ahigh", "desc": "rms uncertainty on spectral slope at high frequencies"}, {"name": "Freq", "desc": "Frequency "}, {"name": "S", "desc": "Flux density at Freq "}, {"name": "e_S", "desc": "rms uncertainty on S "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Beam", "desc": "beam/resolution "}]}, {"name": "mhzbreak_cand.dat", "desc": "Spectral break sources at 325 MHz candidates (table A3)", "columns": [{"name": "Seq", "desc": "[1/19691] The sources belonging to the same spectrum have the same sequence number (1)"}, {"name": "Name", "desc": "Source name "}, {"name": "cat", "desc": "Spectral break code (2) "}, {"name": "Resolved", "desc": "[0/1] Resolved (1) flag (3) "}, {"name": "a", "desc": "Spectral slope associated with the source "}, {"name": "b", "desc": "? Abscissa associated with the source "}, {"name": "alow", "desc": "Spectral slope at low frequencies "}, {"name": "e_alow", "desc": "rms uncertainty on spectral slope at low frequencies"}, {"name": "ahigh", "desc": "Spectral slope at high frequencies "}, {"name": "e_ahigh", "desc": "rms uncertainty on spectral slope at high frequencies"}, {"name": "Freq", "desc": "Frequency "}, {"name": "S", "desc": "Flux density at Freq "}, {"name": "e_S", "desc": "rms uncertainty on S "}, {"name": "RAdeg", "desc": "Right ascension (J2000) "}, {"name": "DEdeg", "desc": "Declination (J2000) "}, {"name": "Beam", "desc": "beam/resolution "}]}]} {"create":{"_index":"private_readme_2021-04-26_19h10m38.001926","_type":"_doc","_id":"VIII_107"}} {"id": "VIII/107", "title_cds": "GLEAM sources ionospheric position shifts", "title_create": "Helmboldt+, 2020", "year": "2020", "author": "Helmboldt J.F., Hurley-Walker N.", "title_pub": "Ionospheric irregularities observed during the Galactic and Extra-galactic All-sky MWA (GLEAM) survey.", "first_author": "Helmboldt J.F.", "ref_biblio": [""], "bibcode": ["2020yCat.8107....0H"], "see_also": ["VIII/16 : Molonglo Reference Catalogue of Radio Sources (Large+ 1991)", "J/ApJS/107/19 : MRC/1Jy Radio source survey. I. (McCarthy+ 1996)", "VIII/100 : GaLactic and Extragalactic All-sky MWA survey", "VIII/102 : GLEAM II. Galactic plane (Hurley-Walker+, 2019)", "VIII/105 : The GLEAM 4-Jy (G4Jy) Sample (White+, 2020)"], "keyword_cds": "Interferometry ; Earth ; Positional data ; Surveys ; Radio sources ; Galaxy catalogs", "keyword_pub": "ionospheric remote sensing - ionospheric disturbances - radio interferometry", "abstract": ["Nearly 200 hours of observing with the Murchison Widefield Array (MWA)", "radio telescope during the Galactic and Extra-galactic All-sky MWA", "(GLEAM) survey were used to assemble images of ionospheric structure.", "These images cover a nearly 50 degree-wide area on the sky at a", "cadence of 10 minutes over many 5-7 hours-long observing runs. They", "are generated by tracking the apparent motions of ~200-800 cosmic", "radio sources caused by changes in the transverse gradient of the", "ionospheric total electron content. Spectral analysis of these images", "revealed that the dataset was dominated by three distinct signatures.", "The first is consistent with field-aligned structures within the", "topside ionosphere/lower plasmasphere previously imaged with the MWA.", "The second are structures that are relatively large and aligned nearly", "east/west. Regional weather data implies that these are preferentially", "detected when there is a noticeable shear within the sub- tropical jet", "stream, which passes near the MWA. This suggests that this signature", "may be related to gravity waves launched by jet stream shear. The", "final signature is consistent with the properties of so-call", "electro-buoyancy waves that are known to occur at midlatitudes at", "night. Detections of these were more common when regional sporadic-E", "was present, supporting a proposed connection between these waves and", "polarization electric fields that may arise within sporadic-E. We", "discuss the implications for future observations with the Square", "Kilometer Array."], "description": ["The expected and measured positions from objects from the Molongo", "Reference Catalog (MRC) within the Murchison Widefield Array (MWA)", "Galactic and Extra-galactic All-sky MWA (GLEAM) survey. The measured", "position offsets are dominated by gradients in ionospheric refraction", "over the MWA field of view."], "alias": [""], "type": ["CCC"], "records": ["447624 sources"], "data": "", "date_update": "18-Aug-2020", "tables": [{"name": "gleamoff.dat", "desc": "Position offsets for GLEAM/MRC objects ", "columns": [{"name": "Time", "desc": "GPS time (seconds since 06-Jan-1980) "}, {"name": "Name", "desc": "Name from the Molongo Reference Catalog, HHMM-DDdA"}, {"name": "RAdeg", "desc": "Right ascension from MRC (J2000.0) "}, {"name": "DEdeg", "desc": "Declination from MRC (J2000.0) "}, {"name": "RAOdeg", "desc": "Observed right ascension (J2000.0) "}, {"name": "e_RAOdeg", "desc": "?=-1 Error in right ascension "}, {"name": "DEOdeg", "desc": "Observed declination (J2000.0) "}, {"name": "e_DEOdeg", "desc": "?=-1 Error in declination "}, {"name": "Flux", "desc": "Peak flux density at 88MHz "}, {"name": "e_Flux", "desc": "?=-1 Error in peak flux density "}, {"name": "A", "desc": "Major axis "}, {"name": "e_A", "desc": "?=-1 Error in major axis "}, {"name": "B", "desc": "Minor axis "}, {"name": "e_B", "desc": "?=-1 Error in minor axis "}, {"name": "PA", "desc": "[] Position angle (clockwise from north) "}, {"name": "e_PA", "desc": "?=-1 Error in position angle "}, {"name": "RMS", "desc": "Local image RMS "}]}]}