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  Abundances in dwarfs, subgiants, and giants (da Silva+, 2015)
Post annotation
1.J/A+A/580/A24/table2Atomic line parameters and solar EWs (178 rows)

Query by Constraints constraints help applied on Columns (Output Order: + - )
ShowSortColumn  Constraint Explain   (UCD)
  recno  Record number assigned by the VizieR team. Should Not be used for identification. (meta.record)
  lambda0 0.1nm [4518/6753] Spectral line central wavelength (em.wl.central)
  Line (char) Atomic line identification (;spect.line)
  chi eV [0/5.7] Lower-level excitation potential χ (phys.atmol.excitation)
  loggf  (n) Logarithmic statistical weight of the lower level multiplied by the oscillator strength (stat.weight;phys.atmol.oscStrength;phys.atmol.level)
  EW 0.1pm [5/122] Solar equivalent width (mÅ) (spect.line.eqWidth)

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(n) indicates a possible blank or NULL column(i)indexed column
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