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  Pal1-I elemental equivalent widths and abundances (Monaco+, 2011)
Post annotation
1.J/A+A/525/A124/tablea1Adopted line atomic parameters and elemental abundances and equivalent widths measured for Pal1-I and the Sun (205 rows)

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ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  El (char) Element (phys.atmol.element)
  Ion  (n)Ionization degree (phys.atmol.ionStage)
  lambda 0.1nm Wavelength of the line (Å) (em.wl;spect.line)
  loggf  (n) Oscillator strength of the line (spect.line.intensity)
  n_loggf (char) [H] H for HFS (Note 1)   (meta.note)
  chi eV (n) Lower excitation potential of the transition (phys.atmol.excitation;stat.min)
  n_chi (char) [H] H for HFS (Note 1)   (meta.note)
  WPal1-I 0.1pm Line equivalent width for Pal1-I (spect.line.eqWidth)
  epsPal1-I  Abundance (eps=log(X/H)+12) obtained from this line for Pal1-I (phys.abund)
  WSun 0.1pm (n) Line equivalent width for the Sun (spect.line.eqWidth)
  epsSun  (n) Abundance (eps=log(X/H)+12) obtained from this line for the Sun (phys.abund)

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