Table 5
Adopted [Fe/H] for metal-poor benchmark candidates.
Star | [Fe/H] | σFeI | Δ(Teff) | Δ(log g) | Δ(vmic) | Δ(LTE) | Δ(ion) | σFeII | NFeI | NFeII | ||
|
||||||||||||
*BD+264251 | −1.23 | 0.07 | 0.09 | 0.02 | 0.02 | 0.03 | −0.05 | 0.05 | 63 | 8 | ||
HD 102200 | −1.12 | 0.07 | 0.08 | 0.01 | 0.01 | 0.04 | 0.02 | 0.07 | 58 | 8 | ||
HD 106038 | −1.25 | 0.08 | 0.08 | 0.01 | 0.01 | 0.02 | −0.03 | 0.05 | 66 | 7 | ||
*HD 126681 | −1.07 | 0.06 | 0.05 | 0.01 | 0.01 | 0.01 | 0.02 | 0.05 | 61 | 7 | ||
HD 175305 | −1.29 | 0.06 | 0.06 | −0.01 | −0.01 | 0.06 | 0.08 | 0.04 | 56 | 8 | ||
*HD 196892 | −0.93 | 0.05 | 0.05 | 0.01 | 0.01 | 0.04 | 0.03 | 0.05 | 68 | 8 | ||
HD 201891 | −0.97 | 0.06 | 0.06 | 0.00 | 0.00 | 0.03 | 0.07 | 0.02 | 68 | 8 | ||
*HD 218857 | −1.78 | 0.07 | 0.11 | 0.04 | 0.04 | 0.06 | 0.01 | 0.05 | 56 | 8 | ||
*HD 241253 | −0.99 | 0.06 | 0.09 | 0.01 | 0.01 | 0.03 | 0.09 | 0.03 | 66 | 7 | ||
HD 298986 | −1.26 | 0.07 | 0.09 | 0.01 | 0.02 | 0.05 | 0.04 | 0.05 | 66 | 6 |
Notes. The [Fe/H] is the NLTE-corrected and is the recommended value for each star. The Δ(Teff) is the uncertainty in the [Fe/H] due to the uncertainty in Teff, Δ(log g) is the uncertainty in the [Fe/H] due to the uncertainty in log g, and Δ(vmic) is the uncertainty in the [Fe/H] due to the uncertainty in vmic. Δ(LTE) is the NLTE-corrected [Fe/H] minus the LTE [Fe/H]. Δ(ion) = [Fe i /H] – [Fe iiH]. The line-to-line dispersion of Fe i and Fe ii are σFe ii and σFe ii, respectively. Finally NFeI and NFeII are the number of Fe i and Fe ii lines used for the analysis, respectively. Stars with an asterisk (*) in Col. 1 are currently not recommended (see Sect. 6.1 for a star-by-star discussion on the recommendations).
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