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  Comparative modelling of cool giants spectra (Lebzelter+, 2012)
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1.J/A+A/547/A108/table8Fe lines used in the A1 analysis to determine abundances for Star 3 (artificial star) (5 rows)

Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  lambda nm Wavelength (em.wl)
  log(gf)  gf value (stat.value;phys.absorption.coeff)
  Source (char) Line data source (Note 1)   (meta.bib)
  Elow cm-1 Lower level excitation potential (phys.atmol.excitation;phys.atmol.level)
  abund  Abundance (log(NH)=12.00) (phys.abund)

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