VizieR

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

VizieR

Simple TargetList Of TargetsFast Xmatch with large catalogs or Simbad
Target Name (resolved by Sesame) or Position:
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NB: The epoch used for the query is the original epoch of the table(s)Radius Box size

  
J/MNRAS/495/1016
  Spectra quality impact on nebular abundances (Rodriguez, 2020)
ReadMe+ftp
2020MNRAS.495.1016R
Similar Catalogs
Post annotation 		img(gal)
1.J/MNRAS/495/1016/tableb1(c)Physical conditions of the sample PNe (179 rows)
2.J/MNRAS/495/1016/tableb2Ionic abundances derived from collisionally excited lines (179 rows)
3.J/MNRAS/495/1016/tableb3Ionic and total abundances of helium (179 rows)
4.J/MNRAS/495/1016/tableb4Total abundances (179 rows)
5.J/MNRAS/495/1016/tableb5Partial and final scores for the sample spectra (179 rows)
6.J/MNRAS/495/1016/refsReferences for tables B1-B5 (69 rows)

Simple ConstraintList Of Constraints
 
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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)
  (1+2+3+4+5)Name (char) Planetary nebula name ((unassigned);phys.veloc.orbital;arith.diff;spect.line.veloc;arith)
   (ALL)Ref (char) Reference ((unassigned);phys.veloc.orbital;arith.diff;phys.veloc.dispersion;(unassigned))
  (1+2+3+4+5)f_Ref (char) Flag on Ref (Note G1)   ((unassigned);(unassigned);(unassigned);pos.eq.dec)
  (1)ne[SII] cm-3 (n) Electron density derived from the [SII]{lambda}6716/{lambda}6731 diagnosis ((unassigned);(unassigned);(unassigned);(unassigned);(unassigned))
  (1)ne[OII] cm-3 (n) Electron density derived from the [OII]{lambda}3726/{lambda}3729 diagnosis ((unassigned);(unassigned);(unassigned);(unassigned);(unassigned))
  (1)ne[ClIII] cm-3 (n) Electron density derived from the [ClIII]{lambda}5518/{lambda}5538 diagnosis ((unassigned);(unassigned);(unassigned);(unassigned);(unassigned))
  (1)ne[ArIV] cm-3 (n) Electron density derived from the [ArIV]{lambda}4711/{lambda}4740 diagnosis ((unassigned);(unassigned);(unassigned);(unassigned);(unassigned))
  (1)ne cm-3 Geometric mean of the electron density (Note 1)   ((unassigned);(unassigned);(unassigned);(unassigned);spect.dopplerVeloc.radio;meta.main)
  (1)Te[NII] K Electron temperature obtained from the diagnostics [NII]{lambda}5755/ ({lambda}6548+{lambda}6583) ((unassigned);(unassigned);(unassigned);em.radio.400-750MHz;(unassigned))
  (1)Te[OIII] K Electron temperature obtained from the diagnostics [OIII]{lambda}4363/ ({lambda}4959+{lambda}5007) ((unassigned);(unassigned);(unassigned);em.radio.400-750MHz;(unassigned))

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (1+2+3+4+5)ptot  Final score of the spectrum (see Section 6.9) ((unassigned);phys.veloc.orbital;arith.diff;pos.cartesian)
  (1)SimbadName (char) (n)Designation understandable by the Simbad data-base ((unassigned);phys.veloc.orbital;arith.diff;spect.line.veloc)
  (1)_RA deg Right Ascension (J2000) from SIMBAD (not part of the original data) ((unassigned);(unassigned);(unassigned);(unassigned);arith)
  (1)_DE deg Declination (J2000) from SIMBAD (not part of the original data) ((unassigned);(unassigned);(unassigned);(unassigned);arith)
  (2)O+(b)  12+log(O+/H+) abundance calculated using the blue [OII] lines ((unassigned);phys.luminosity.fun;arith.grad;phys.polarization.stokes.Q)
  (2)O+(r)  (n) 12+log(O+/H+) abundance calculated using the red [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (2)O++  12+log(O++/H+) abundance ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (2)N+  12+log(N+/H+) abundance ((unassigned);phys.veloc.orbital;arith.diff;phys.polarization.stokes.Q)
  (2)Ne++  (n) 12+log(Ne++/H+) abundance ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (2)S+  12+log(S+/H+) abundance ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (2)S++  (n) 12+log(S++/H+) abundance ((unassigned);phys.veloc.orbital;arith.diff;phys.polarization.stokes.Q)
  (2)Ar++  (n) 12+log(Ar++/H+) abundance ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (2)Cl++  (n) 12+log(Cl++/H+) abundance ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (3)He+4026  (n) 12+log(He+/H) abundance derived from the {lambda}4026 line ((unassigned);(unassigned);(unassigned);pos.cylindrical)
  (3)He+4388  (n) 12+log(He+/H) abundance derived from the {lambda}4388 line ((unassigned);(unassigned);(unassigned);pos.cylindrical)
  (3)He+4922  (n) 12+log(He+/H) abundance derived from the {lambda}4922 line ((unassigned);(unassigned);(unassigned);pos.cylindrical)
  (3)He+4471  (n) 12+log(He+/H) abundance derived from the {lambda}4471 line ((unassigned);(unassigned);(unassigned);pos.cylindrical)
  (3)He+5876  12+log(He+/H) abundance derived from the {lambda}5876 line ((unassigned);(unassigned);(unassigned);pos.cylindrical)
  (3)He+6678  (n) 12+log(He+/H) abundance derived from the {lambda}6678 line ((unassigned);(unassigned);(unassigned);pos.cylindrical)
  (3)He+  12+log(He+/H) abundance ((unassigned);(unassigned);(unassigned);pos.cylindrical)
  (3)He++  (n) 12+log(He++/H) abundance ((unassigned);(unassigned);(unassigned);pos.cylindrical)
  (3)He  12+log(He/H) abundance ((unassigned);(unassigned);(unassigned);pos.cylindrical)
  (4)O(b)  12+log(O/H) abundance calculated using the blue [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)N(b)  12+log(N/H) abundance calculated using the blue [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)Ne(b)  (n) 12+log(Ne/H) abundance calculated using the blue [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)S(b)  (n) 12+log(S/H) abundance calculated using the blue [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (4)Ar(b)  (n) 12+log(Ar/H) abundance calculated using the blue [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)Cl(b)  (n) 12+log(Cl/H) abundance calculated using the blue [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)O(r)  (n) 12+log(O/H) abundance calculated using the red [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)N(r)  (n) 12+log(N/H) abundance calculated using the red [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)Ne(r)  (n) 12+log(Ne/H) abundance calculated using the red [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)S(r)  (n) 12+log(S/H) abundance calculated using the red [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)Ar(r)  (n) 12+log(Ar/H) abundance calculated using the red [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (4)Cl(r)  (n) 12+log(Cl/H) abundance calculated using the red [OII] lines ((unassigned);(unassigned);(unassigned);phys.polarization.stokes.Q)
  (5)p0   [0/10] Score indicating whether the spectra was obtained with a CCD (p0=10) or not (p0=0) ((unassigned);(unassigned);(unassigned);pos.cartesian)
  (5)p1   [20] Score related to the available temperature diagnostics ((unassigned);(unassigned);(unassigned);pos.cartesian)
  (5)N  Number of density diagnostics ((unassigned);(unassigned);(unassigned);src.var)
  (5)p2  Score related to the density diagnosis (p2=9-15 for 1-4 working density diagnostics) ((unassigned);(unassigned);(unassigned);pos.cartesian)
  (5)[NII]  (n) [NII] {lambda}6584/{lambda}6548 line ratio ((unassigned);(unassigned);(unassigned);phys.atmol.qn.I;instr.param)

ALL cols		    
(n) indicates a possible blank or NULL column(i)indexed column
  (5)p3   [0/10] Score associated to [NII] ((unassigned);(unassigned);(unassigned);pos.cartesian)
  (5)[OIII]  (n) [OIII] {lambda}5007/{lambda}4959 line ratio ((unassigned);(unassigned);(unassigned);phys.atmol.qn.I;instr.param)
  (5)p4   [0/10] Score associated to [OIII] ((unassigned);(unassigned);(unassigned);pos.cartesian)
  (5)NHeI  Number of HeI lines unaffected by optical depth effects available in the spectra ((unassigned);(unassigned);(unassigned);src.var)
  (5)p5   [2/20] Score assigned to NHeI (Note 1)   ((unassigned);(unassigned);(unassigned);pos.cartesian)
  (5)NBL  Number of balmer lines (out of H{alpha}, H{gamma} and H{delta}) whose intensities are listed in the spectra ((unassigned);(unassigned);(unassigned);src.var)
  (5)P-B  (n) Difference between the median deviations of the Paschen and Balmer lines from their expected values (see Section 6.7) ((unassigned);(unassigned);(unassigned);pos.bodyrc.lon;meta.main)
  (5)p6   [0/15] Score assigned using the behaviour of all these lines ((unassigned);(unassigned);(unassigned);pos.cartesian)
  (6)BibCode (char) BibCode ((unassigned);(unassigned);(unassigned);pos.angDistance)
  (6)Aut (char) Author's name ((unassigned);(unassigned);(unassigned);phys.temperature)
  (6)Com (char) Comments ((unassigned);(unassigned);(unassigned);phys.veloc.orbital)

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