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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/table9Equivalent widths of Fe lines used for deriving atmospheric parameters (52 rows)

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  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  lambda 0.1nm [4132.9/6430.9] Wavelength, Angstroms (em.wl)
  El (char) Element (phys.atmol.element)
  Elow eV [0.087/4.6] Energy, lower level (phys.energy;phys.atmol.level)
  loggf [-] [-4.95/-0.02] Log, statistical weight*oscillator strength (stat.weight;phys.atmol.oscStrength)
  EW-HE0457 0.1pm (n) [55/145.6] Equivalent width of line, HE0457-1805 (spect.line.eqWidth)
  Ab-HE0457 [-] (n) [5.3/5.7] Derived absolute abundance for line, HE 0457-1805 (phys.abund)
  EW-HE0920 0.1pm (n) [27.4/92] Equivalent width of line, HE0920-0506 (spect.line.eqWidth)
  Ab-HE0920 [-] (n) [6.6/6.9] Derived absolute abundance for line, HE 0920-0506 (phys.abund)
  EW-HE1241 0.1pm (n) [20.5/151] Equivalent width of line, HE1241-0337 (spect.line.eqWidth)
  Ab-HE1241 [-] (n) [4.8/5.3] Derived absolute abundance for line, HE 1241-0337 (phys.abund)
  EW-HE1327 0.1pm (n) [20/83.4] Equivalent width of line, HE1327-2116 (spect.line.eqWidth)
  Ab-HE1327 [-] (n) [4.5/4.8] Derived absolute abundance for line, HE 1327-2116 (phys.abund)

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