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  NLTE corrections for Mg and Ca lines (Merle+ 2011)
Post annotation
1.J/MNRAS/418/863/gridGrid of Non-LTE corrections for Mg and Ca lines in the stellar parameter range Teff=[3500, 5250]K, log(g)=[0.5, 2.0], [Fe/H]=[-4.0,0.5] and [α/Fe]=[0.0,0.4] (18012 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)
  Ion (char) Ion (MgI, CaI or CaII) (phys.atmol.element)
  lambda 0.1nm (n)Wavelength (Å) (em.wl;phys.atmol.transition)
  n_lambda (char) * for the blend 8710, 8712 and 8717 MgI lines, a for the CaI 6169.03Å line, b for the CaI 6169.56Å line (meta.note)
  Teff K [3500/5250] Effective temperature (phys.temperature.effective)
  logg [cm/s2] [0.5/2] Surface gravity (phys.gravity)
  [Fe/H] [Sun] [-4/0.5] Metallicity (phys.abund.Z)
  [a/Fe] [Sun] [0/0.4] Enhancement of α elements (Note 1)   (phys.abund)
  W 0.1pm NLTE equivalent width in Angstrom (Note 2)   (spect.line.eqWidth)
  W/W*  NLTE/LTE equivalent width (Note 3)   (meta.note)
  Delta [Sun] (n) NLTE abundance correction (Note 4)   (phys.abund)

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