Abundance corrections for the five IR spectral lines of Fe i included in this study.
|λ||Δlog ϵ(Fe)⊙||Δlog ϵ(Fe)⊙||Δlog ϵ(Fe)⊙||W HD|
|(50 G – HD)||(100 G – HD)||(200 G – HD)|
Notes. Same order as per Cols. 1–5 of Table 2. In the bottom row, we provide the (unweighted) mean of the abundance corrections and corresponding rms.
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