Table 5.
Fe I lines used for deriving ν sin i and the iron abundance correction Δ[Fe/H].
| Spectral line parameters | Sun | HD 207129 | HD 95456 | |||||||
|---|---|---|---|---|---|---|---|---|---|---|
| Chemical Species | Wavelength λ (Å) | EP (eV) | log ℊ f (dex) | Source | Vmacro (km s−1) | Δ[Fe/H] (dex) | ν sin i (km s−1) | Δ[Fe/H] (dex) | ν sin i (km s−1) | Δ[Fe/H] (dex) |
| Fe I | 6094.3800 | 4.650 | −1.566 | T13 | 2.14 | −0.088 | 2.53 | −0.088 | 1.58 | −0.118 |
| Fe I | 6200.3190 | 2.609 | −2.437 | Do14 | 2.06 | −0.019 | 1.97 | −0.022 | 0.00 | −0.091 |
| Fe I | 6481.8800 | 2.280 | −2.929 | T13 | 1.94 | −0.078 | 1.95 | −0.074 | 0.00 | −0.130 |
| Fe I | 6593.8800 | 2.430 | −2.384 | T13 | 2.05 | −0.049 | 1.94 | −0.055 | 0.00 | −0.134 |
| Fe I | 6699.1408 | 4.593 | −2.101 | Vald3 | 2.23 | −0.078 | 2.14 | −0.119 | 1.59 | −0.112 |
| Fe I | 6703.5655 | 2.759 | −3.160 | Vald3 | 2.00 | 0.068 | 2.04 | 0.069 | 0.61 | 0.0419 |
| Fe I | 6725.3553 | 4.103 | −2.300 | Vald3 | 2.23 | 0.051 | 2.41 | 0.052 | 1.12 | 0.0288 |
| Fe I | 6726.6658 | 4.607 | −1.094 | Vald3 | 2.19 | 0.021 | 2.39 | 0.016 | 1.40 | −0.037 |
| Fe I | 6810.2570 | 4.607 | −0.986 | Do14 | 2.15 | −0.044 | 2.24 | −0.049 | 0.98 | −0.111 |
| Fe I | 6857.2490 | 4.076 | −2.150 | Do14 | 2.17 | 0.010 | 2.53 | 0.019 | 1.51 | −0.015 |
| Average Std. dev. | 2.12 ±0.10 | −0.021 ±0.056 | 2.21 ±0.24 | −0.025 ±0.063 | 0.88 ±0.68 | −0.068 ±0.067 | ||||
Notes. The lines and their parameters are adopted from the VALD-v3 database Kupka et al. (2011; Vald3), Tsantaki et al. (2013; T13) or Doyle et al. (2014; Do14), as indicated in the fifth column. For the Sun, we used a fixed ν sin i of 1.9 km s−1in order to derive its Vmacro, whereas for HD 207129 and HD 95456 we proceeded the other way round, fixing the Vmacro values at 2.33 and 3.33 km s−1, respectively, in finding their ν sin i (see Sect. 3.2).
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