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  Abundance Analyses of RV Tauri Variables (Gonzalez+ 1997)
Post annotation
1.J/ApJ/479/427/table3Individual abundance results for EP Lyr (211 rows)
2.J/ApJ/479/427/table6Individual abundance results for R Sge (112 rows)

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Column  Constraint Explain   (UCD)
   (ALL)EP eV Low energy potential (;phys.atmol.level)
   (ALL)EW1 10-4nm Equivalent width, 1994 June 25-27 (spect.line.eqWidth)
   (ALL)EW2 10-4nm Equivalent width, 1995 June 10&12 (spect.line.eqWidth)
   (ALL)EW3 10-4nm Equivalent width, 1996 Mar 3 (spect.line.eqWidth)
   (ALL)Ion (char) Atomic species (phys.atmol.element)
   (ALL)lambda 0.1nm Wavelength (em.wl)
   (ALL)log(Eps0)  Solar abundance for the ion (phys.abund)
   (ALL)log(Eps1)   Abundance at lambda, 1994 June 25-27 (phys.abund)
   (ALL)log(Eps2)   Abundance at lambda, 1995 June 10&12 (phys.abund)
   (ALL)log(Eps3)   Abundance at lambda, 1996 Mar 3 (phys.abund)
   (ALL)log(gf)  log of oscillator strength (phys.atmol.wOscStrength)

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  (ALL)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  (2)EW4 10-4nm Equivalent width, 1995 June 12 (spect.line.eqWidth)
  (2)log(Eps4)   Abundance at lambda, 1995 June 12 (phys.abund)

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