Table 3
Adopted parameters for metal-poor benchmark candidates.
| Star | θLD | σ θLD | Fbol | σ Fbol | Teff | σ Teff | log g | σ log g | vmic | vsini | σ vsini |
| (mas) | (mas) | (10-11 Wm-2) | (10-11 Wm-2) | (K) | (K) | (dex) | (dex) | (km s-1) | (km s-1) | (km s-1) | |
|
|
|||||||||||
| *BD+264251 | 0.077 | 0.001 | 0.2759 | 0.0059 | 6129 | 80 | 4.41 | 0.16 | 1.40 | 2.81 | 2.10 |
| HD 102200 | 0.138 | 0.002 | 0.9062 | 0.0041 | 6155 | 80 | 4.22 | 0.07 | 1.43 | 1.90 | 4.59 |
| HD 106038 | 0.073 | 0.001 | 0.2477 | 0.0026 | 6121 | 80 | 4.55 | 0.14 | 1.39 | 0.00 | 0.00 |
| *HD 126681 | 0.128 | 0.002 | 0.5543 | 0.0050 | 5640 | 80 | 4.64 | 0.07 | 1.16 | 0.00 | 0.00 |
| HD 175305 | 0.447 | 0.006 | 4.3520 | 0.6752 | 5059 | 80 | 2.53 | 0.14 | 1.54 | 5.01 | 1.92 |
| *HD 196892 | 0.178 | 0.002 | 1.4130 | 0.0233 | 6053 | 80 | 4.19 | 0.06 | 1.36 | 0.00 | 0.00 |
| HD 201891 | 0.273 | 0.004 | 3.1154 | 0.0517 | 5948 | 80 | 4.30 | 0.04 | 1.29 | 2.93 | 5.31 |
| *HD 218857 | 0.194 | 0.003 | 0.8841 | 0.1625 | 5162 | 80 | 2.66 | 0.32 | 1.58 | 3.14 | 6.80 |
| *HD 241253 | 0.091 | 0.001 | 0.3642 | 0.0013 | 6023 | 80 | 4.22 | 0.18 | 1.34 | 1.89 | 4.50 |
| HD 298986 | 0.073 | 0.001 | 0.2691 | 0.0067 | 6223 | 100 | 4.19 | 0.19 | 1.48 | 4.07 | 5.98 |
Notes. The θLD were computed as a part of the IRFM. In addition, the Teff and Fbol in this table represents the adopted Teff and bolometric flux from the IRFM, respectively. We estimated vmic using the GES relationship of Bergemann and Hill. The uncertainty in vmic was conservatively assumed to be 0.20 km s-1 for all stars. 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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