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J/ApJ/934/110
  Abundance analysis of 4 HES metal-poor stars (Shejeelammal+, 2022)
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2022ApJ...934..110S
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1.J/ApJ/934/110/table10Equivalent widths of lines used for deriving elemental abundances (172 rows)

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  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  lambda 0.1nm [4161.5/6643.7] Wavelength, Angstroms (em.wl)
  El (char) Element (phys.atmol.element)
  Elow eV [0.0/5.8] Energy, lower level (phys.energy;phys.atmol.level)
  loggf [-] [-3.5/0.6] Log, statistical weight*oscillator strength (stat.weight;phys.atmol.oscStrength)
  EW-HE0457 0.1pm (n) [21.8/150] Equivalent width of line, HE0457-1805 (spect.line.eqWidth)
  Ab-HE0457 [-] (n) [1.2/7.1] Derived absolute abundance for line, HE 0457-1805 (phys.abund)
  EW-HE0920 0.1pm (n) [12.1/173] Equivalent width of line, HE0920-0506 (spect.line.eqWidth)
  Ab-HE0920 [-] (n) [1.1/7.6] Derived absolute abundance for line, HE 0920-0506 (phys.abund)
  EW-HE1241 0.1pm (n) [9.2/166] Equivalent width of line, HE1241-0337 (spect.line.eqWidth)
  Ab-HE1241 [-] (n) [-0.6/6] Derived absolute abundance for line, HE 1241-0337 (phys.abund)
  EW-HE1327 0.1pm (n) [10/98] Equivalent width of line, HE1327-2116 (spect.line.eqWidth)
  Ab-HE1327 [-] (n) [-0.24/5.5] Derived absolute abundance for line, HE 1327-2116 (phys.abund)

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