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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)recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
   (ALL)Ion (char) Atomic species (phys.atmol.element)
   (ALL)log(Eps0)  Solar abundance for the ion (phys.abund)
   (ALL)lambda 0.1nm Wavelength (em.wl)
   (ALL)EP eV Low energy potential (;phys.atmol.level)
   (ALL)log(gf)  log of oscillator strength (phys.atmol.wOscStrength)
   (ALL)EW1 10-4nm Equivalent width, 1994 June 25-27 (spect.line.eqWidth)
   (ALL)log(Eps1)   Abundance at lambda, 1994 June 25-27 (phys.abund)
   (ALL)EW2 10-4nm Equivalent width, 1995 June 10&12 (spect.line.eqWidth)
   (ALL)log(Eps2)   Abundance at lambda, 1995 June 10&12 (phys.abund)
   (ALL)EW3 10-4nm Equivalent width, 1996 Mar 3 (spect.line.eqWidth)

ALL cols
 (i)indexed column
   (ALL)log(Eps3)   Abundance at lambda, 1996 Mar 3 (phys.abund)
  (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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