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J/A+A/397/257
  Chemical compositions of four barium stars (Liang+, 2003)
Post annotation
  
1.J/A+A/397/257/table3Atomic data and EWs of lines in four stars (134 rows)
2.J/A+A/397/257/table5Abundance uncertainties (73 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)
  (1)lambda 0.1nm Wavelengths of line (em.wl)
   (ALL)Ion (char) Atomic element of line (phys.atmol.element)
  (1)chi eV Excitation potential of line (phys.energy;phys.atmol.excitation)
  (1)loggf  Oscillator strengths of line (phys.atmol.wOscStrength)
  (1)r_loggf (char) The reference sources of n-capture elements (Note 1)   (meta.ref)
  (1)EWs(1) pm (n) Equivalent widths of lines in star HD 26886 (spect.line.eqWidth)
  (1)EWs(2) pm (n) Equivalent widths of lines in star HD 27271 (spect.line.eqWidth)
  (1)EWs(3) pm (n) Equivalent widths of lines in star HD 50082 (spect.line.eqWidth)
  (1)EWs(4) pm (n) Equivalent widths of lines in star HD 98839 (spect.line.eqWidth)
  (2)Star (char) Star name (meta.id;meta.main)
  (2)sigma(EW/sqrt(N))  Abundance errors caused by EWs values (stat.error)
  (2)Delta(Teff)  Abundance errors caused by increasing 100K in effective temperature (stat.error)
  (2)Delta(logg)  Abundance errors caused by increasing in surface gravity (Note 1)   (stat.error)
  (2)Delta(xit)  Abundance errors caused by increasing 0.3km/s in microturbulent velocity (stat.error)
  (2)sigma(tot)  Total abundance errors caused by the combined uncertainties in gf-values, EWs and stellar atmospheric parameters (stat.error)

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