VizieR

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VizieR

  
J/A+A/592/A70
  Gaia FGK stars: low-metallicities candidates (Hawkins+, 2016)
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img(gal)
1.J/A+A/592/A70/tablea10HD 298986 Fe abundance measurements for each line and node (72 rows)

 
Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  Element (char) Element and Ion state (phys.atmol.element)
  lambda 0.1nm Wavelength of line used in the abundance determination (em.wl;spect.line)
  <EW> 0.1pm Mean Equivalent width from all nodes (spect.line.eqWidth;stat.mean)
  <A>  Mean Fe abundance derived for that line across all nodes (phys.abund.Fe;stat.mean)
  NLTE  (n) NLTE correction for that line (Note 1)   (arith.factor)
  EW(EPI) 0.1pm (n) Equivalent width obtained by the EPINARBO method (Note 2)   (spect.line.eqWidth;meta.modelled)
  EW(BOL) 0.1pm (n) Equivalent width obtained by the Bologna method (Note 2)   (spect.line.eqWidth;meta.modelled)
  EW(ULB) 0.1pm (n) Equivalent width obtained by the ULB method (Note 2)   (spect.line.eqWidth;meta.modelled)
  EW(iSPEC) 0.1pm (n) Equivalent width obtained by the iSPEC method (Note 2)   (spect.line.eqWidth;meta.modelled)
  A(EPI)  (n) abundance obtained by the EPINARBO method (Note 2)   (phys.abund.Fe)
  A(BOL)  (n) abundance obtained by the Bologna method (Note 2)   (phys.abund.Fe)
  A(ULB)  (n) abundance obtained by the ULB method (Note 2)   (phys.abund.Fe)
  A(iSPEC)  (n) abundance obtained by the iSPEC method (Note 2)   (phys.abund.Fe)

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