VizieR

CfA VizieR . ADAC VizieR . Cambridge (UK) VizieR . IUCAA VizieR . INASAN VizieR .

VizieR

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J/MNRAS/511/6179
  Low-mass cool dwarfs of NYMGs from Gaia EDR3 (Lee+, 2022)
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img(gal)
1.J/MNRAS/511/6179/group(c)NYMG groups in our sample (7 rows)
2.J/MNRAS/511/6179/table4(c)The new highly likely members of NYMGs identified having Gaia EDR3 RVs (139 rows)
3.J/MNRAS/511/6179/tableb1(c)The new highly likely members of NYMGs identified without Gaia EDR3 RV measurements (1863 rows)
4.J/MNRAS/511/6179/table6(c)The newly suggested ultracool dwarf candidate members of NYMGs (231 rows)
5.J/MNRAS/511/6179/table7(c)Newly confirmed NYMG members after obtaining WiFeS optical spectra (35 rows)
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Column  Constraint Explain   (UCD)
  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc)
   (ALL)Group (char) Nearby young stellar moving group NYMG (Group) ((unassigned);phys.veloc.orbital;arith.diff;spect.line.veloc)
  (1)Ntab4  Relative number of group members in the table4.dat ((unassigned);(unassigned);(unassigned);src.var)
  (1)Ntabb1  Relative number of group members in the tableb1.dat ((unassigned);(unassigned);(unassigned);src.var)
  (1)Ntab6  Relative number of group members in the table6.dat ((unassigned);phys.veloc.orbital;arith.diff;src.var)
  (1)Ntab7  Relative number of group members in the table4.dat ((unassigned);(unassigned);(unassigned);src.var)
  (1)Ntot  Total number of group members ((unassigned);(unassigned);(unassigned);src.var)
  (1)SimbadName (char) (n)Designation understandable by the Simbad data-base ((unassigned);(unassigned);(unassigned);spect.line.veloc)
  (1)_RA deg (n)Right Ascension (J2000) from SIMBAD (not part of the original data) ((unassigned);phys.veloc.orbital;arith.diff;(unassigned);arith)
  (1)_DE deg (n)Declination (J2000) from SIMBAD (not part of the original data) ((unassigned);(unassigned);(unassigned);(unassigned);arith)
  (2+3+4)ID  Identifier number (ID) ((unassigned);(unassigned);(unassigned);spect.line.veloc)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3+4+5)GaiaEDR3  Gaia EDR3 source identifier unique number (GaiaEDR3source_id) ((unassigned);(unassigned);(unassigned);spect.line.veloc;arith)
  (2+3+4+5)RAJ2000 "h:m:s" Right Ascension (J2000) ((unassigned);phys.veloc.orbital;arith.diff;(unassigned);arith)
  (2+3+4+5)DEJ2000 "d:m:s" Declination (J2000) ((unassigned);phys.veloc.orbital;arith.diff;(unassigned);arith)
  (2+3+4+5)pmRA mas/yr Proper motion in right ascension pmRA*cosDE of the source in ICRS at Ep=2016.0 (pmra) ((unassigned);(unassigned);(unassigned);instr.offset;(unassigned))
  (2+3+4+5)pmDE mas/yr Proper motion in declination direction of the source in ICRS at Ep=2016.0 (pmdec) ((unassigned);(unassigned);(unassigned);instr.offset;(unassigned))
  (2+3+4+5)Plx mas Absolute stellar parallax of the source at the Ep=2016.0 (plx) ((unassigned);phys.veloc.orbital;arith.diff;em.wl.effective;meta.main)
  (2+5)RV km/s Gaia EDR3 radial velocity (rv) (obs.param;stat.covariance;arith.grad;spect.index;arith.diff;meta.main)
  (2+3+4+5)Gmag mag G-band mean magnitude (Vega) (g) ((unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned))
  (2+3)BP-RP mag BP-RP colour (bp_rp) ((unassigned);phys.veloc.orbital;arith.diff;pos.healpix;(unassigned);(unassigned);(unassigned))
  (2+3+4)SPkin % The sum of Pkin across multiple groups denoted {Sigma} Pkin ({Sigma}Pkin) (Note G1)   ((unassigned);(unassigned);(unassigned);pos.parallax;(unassigned);meta.main)
  (2+3+4+5)Pkin % The Pkin spatio-kinematic membership probability for a single group is computed with BAMG code (Pkin) (Note G2)   ((unassigned);phys.veloc.orbital;arith.diff;pos.parallax;(unassigned);meta.main)
  (2+3+5)YouthCMD  The Youth(CMD) parameter (YouthCMD) (Note G3)   ((unassigned);(unassigned);(unassigned);pos.bodyrc.lon;(unassigned);(unassigned))
  (2+3+4+5)NUVmag mag (n) NUV magnitudes (AB mag) from GALEX DR5 Bianchi et al. 2011MNRAS.411.2770B, Cat. J/MNRAS/411/2770 (NUV) ((unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned))

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (2+3+4+5)YouthNUV  The Youth(NUV) parameter (YouthNUV) (Note 1)   ((unassigned);(unassigned);(unassigned);pos.bodyrc.lon;(unassigned);(unassigned))
  (2+3+4+5)Simbad (char) ask the Simbad data-base about this object ((unassigned);phys.veloc.orbital;arith.diff;pos.geocentric)
  (4)Jmag mag J-band at 1.25 µm apparent magnitude (Vega) from the 2MASS catalogue Cutri et al. 2003, Cat. II/246 (j) ((unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned))
  (4)Hmag mag H-band at 1.65 µm apparent magnitude (Vega) from the 2MASS catalogue Cutri et al. 2003, Cat. II/246 (h) ((unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned))
  (4)Kmag mag Ks-band at 1.85 µm apparent magnitude (Vega) from the 2MASS catalogue Cutri et al. 2003, Cat. II/246 (k) ((unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned))
  (4)W1mag mag W1-band at 3.35 µm apparent magnitude (Vega) from the ALLWISE catalogue Cutri et al. 2014, Cat. II/328 (w1) ((unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned))
  (4)W2mag mag W2-band at 4.6 µm apparent magnitude (Vega) from the ALLWISE catalogue Cutri et al. 2014, Cat. II/328 (w2) ((unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned))
  (5)SpType (char) Spectral type from observations detailed in the section 3.2 Pilot spectroscopic observations (SpT) ((unassigned);(unassigned);(unassigned);pos.posAng;meta.main)
  (5)e_RV km/s Uncertainty of RV measurements (errRV) ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (5)BPmag mag Integrated BP mean magnitude (Vega) (BPmag) ((unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned))
  (5)RPmag mag Integrated RP mean magnitude (Vega) (RPmag) ((unassigned);(unassigned);(unassigned);stat.filling;(unassigned);(unassigned))
  (5)EWHa 0.1nm Equivalent width of H{alpha} emission line are measured with the splot task in IRAF (EWH{alpha}) ((unassigned);(unassigned);(unassigned);phys.at.moment.magnetic;(unassigned);(unassigned))
  (5)e_EWHa 0.1nm EWHa uncertainties are calculated using equation 6 of Cayrel 1988IAUS..132..345C (errEWH{alpha}) ((unassigned);(unassigned);(unassigned);time.age;meta.main)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
  (5)l_EWLi (char) Upper limit flag of EWLi values in the case of non-detection, upper limits are provided ((unassigned);(unassigned);(unassigned);pos.galactic.lon)
  (5)EWLi 10-4nm Equivalent width of Li 6708 Å emission line measured with the splot task in IRAF (EWLi) ((unassigned);(unassigned);(unassigned);phys.at.moment.magnetic;meta.main)
  (5)e_EWLi 10-4nm (n) EWLi uncertainties are calculated using equation 6 of Cayrel 1988IAUS..132..345C (errEWLi) ((unassigned);(unassigned);(unassigned);time.age;meta.main)
  (5)f_Pkin (char) Flag indicating with Pkin of a single group is less than 90 per cent and {Sigma}Pkin => 90 per cent (Note G2)   ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (5)Obs "Y:M:D" (n)Observation date WiFeS spectrograph (Obs.date) ((unassigned);(unassigned);(unassigned);pos.centroid;stat.param)

ALL cols
    
(n) indicates a possible blank or NULL column(i)indexed column
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