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  Abundance Analyses of RV Tauri Variables (Gonzalez+ 1997)
Post annotation
1.J/ApJ/479/427/table6Individual abundance results for R Sge (112 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)
  Ion (char) Atomic species (phys.atmol.element)
  log(Eps0)  Solar abundance for the ion (phys.abund)
  lambda 0.1nm Wavelength (em.wl)
  EP eV Low energy potential (;phys.atmol.level)
  log(gf)  log of oscillator strength (phys.atmol.wOscStrength)
  EW1 10-4nm Equivalent width, 1992 May 22 (spect.line.eqWidth)
  log(Eps1)   Abundance at lambda, 1992 May 22 (phys.abund)
  EW2 10-4nm Equivalent width, 1994 June 24 (spect.line.eqWidth)
  log(Eps2)   Abundance at lambda, 1994 June 24 (phys.abund)
  EW3 10-4nm Equivalent width, 1994 July 29 (spect.line.eqWidth)
  log(Eps3)   Abundance at lambda, 1994 July 29 (phys.abund)
  EW4 10-4nm Equivalent width, 1995 June 12 (spect.line.eqWidth)
  log(Eps4)   Abundance at lambda, 1995 June 12 (phys.abund)

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