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Table 3
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 |
| [nm] | [dex] | [dex] | [dex] | [pm] |
| (50 G – HD) | (100 G – HD) | (200 G – HD) | ||
|
|
||||
| 1558.826 | 0.00 | 0.00 | +0.01 | 11.63 |
| 1564.851 | −0.05 | −0.07 | −0.08 | 9.57 |
| 1565.287 | −0.03 | −0.05 | −0.06 | 7.18 |
| 1566.202 | −0.02 | −0.02 | −0.03 | 19.88 |
| 1566.524 | −0.01 | −0.01 | −0.02 | 7.67 |
|
|
||||
| ⟨ ⟩ | −0.022 | −0.030 | −0.036 | |
| ±0.017 | ±0.026 | ±0.031 | ||
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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