Fe I lines used in the A1 analysis to determine iron abundances for Star 3.
|λ||log (gf)||Sourcea||E low||Abundance|
|(nm)||[cm-1]||[log (NH) = 12.00]|
Notes. For each line, the wavelength λ, the gf value, the lower level excitation potential Elow, and the line abundance are given.
References as listed in Kurucz & Bell (1995): http://kurucz.harvard.edu/LINELISTS/LINES/gfall.ref.
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