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  Li abundances in solar-analog stars (Takeda+, 2007)
Post annotation
1.J/A+A/468/663/table3EWs of Fe I/Fe II lines and resulting Fe abundances (18445 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)
  Star (char) Star name (Sun/Moon or HIP NNNNNN) (;meta.main)
  Line  Line No. (cf. Takeda et al. 2005, Cat. J/PASJ/57/27) (;spect.line)
  Elem  26.00 for Fe I, 26.01 for Fe II (meta.note)
  lambda 0.1nm Line wavelength (em.wl;spect.line)
  EP(low) eV Excitation potential of the lower level (phys.atmol.excitation;phys.atmol.level)
  loggf  log(gf) value (stat.value;arith.zp)
  EW 0.1pm (n) Fe line equivalent width (spect.line.eqWidth)
  A(Fe)  (n) Line-by-line Fe abundance (phys.abund.Fe)

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