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Table A.3
Results from SPECIES for the GBS samples, for the stellar parameters.
| Starname | Sp Type | [Fe∕H] | T(K) | log g | ξt (km s−1) | vsini (km s−1) | M (M⊙) |
|---|---|---|---|---|---|---|---|
| 18Sco | G V | 0.11 ± 0.04 | 5872 ± 20 | 4.53 ± 0.15 | 0.87 ± 0.02 | 1.35 ± 0.16 | 1.1 ± 0.0 |
| 61CygB | K V | −0.48 ± 0.37 | 4989 ± 171 | 3.28 ± 2.67 | 0.95 ± 0.18 | 2.61 ± 2.43 | 2.7 ± 1.3 |
| Arcturus | FGK III | −0.20 ± 0.37 | 4752 ± 354 | 2.90 ± 1.90 | 1.73 ± 0.04 | 3.29 ± 1.66 | 3.5 ± 0.2 |
| Gmb1830 | K V | −1.17 ± 0.10 | 5368 ± 61 | 4.66 ± 1.08 | 1.41 ± 0.08 | 0.00 ± 0.00 | 0.1 ± 0.0 |
| HD107328 | FGK III | −0.41 ± 0.09 | 4526 ± 47 | 2.02 ± 0.46 | 1.70 ± 0.03 | 2.30 ± 0.47 | 3.2 ± 0.0 |
| HD220009 | FGK III | −0.86 ± 0.41 | 4120 ± 354 | 1.06 ± 2.78 | 1.34 ± 0.04 | −0.07 ± 3.60 | 3.7 ± 0.1 |
| HD22879 | G V | −0.85 ± 0.13 | 5858 ± 80 | 4.37 ± 0.28 | 0.68 ± 0.06 | 0.00 ± 0.00 | 0.8 ± 0.0 |
| HD49933 | F V | −0.48 ± 0.25 | 6732 ± 137 | 4.33 ± 1.44 | 2.24 ± 0.26 | 4.04 ± 1.90 | 1.3 ± 0.0 |
| Procyon | F V | 0.14 ± 0.26 | 6744 ± 137 | 4.06 ± 1.71 | 1.59 ± 0.18 | 0.00 ± 0.00 | 1.6 ± 0.1 |
| Sun | G V | 0.00 ± 0.05 | 5799 ± 25 | 4.46 ± 0.19 | 0.90 ± 0.02 | 1.56 ± 0.21 | 1.0 ± 0.0 |
| alfCenA | G V | 0.26 ± 0.09 | 5831 ± 42 | 4.34 ± 0.16 | 0.98 ± 0.03 | 1.78 ± 0.34 | 1.1 ± 0.0 |
| betAra | M III | −0.35 ± 0.69 | 4116 ± 500 | 0.59 ± 5.05 | 3.10 ± 0.10 | 6.88 ± 4.08 | 14.3 ± 0.6 |
| betGem | FGK III | 0.18 ± 0.08 | 5010 ± 38 | 3.17 ± 0.24 | 1.30 ± 0.03 | 2.16 ± 0.24 | 3.2 ± 0.2 |
| betHyi | FGK IV | −0.05 ± 0.08 | 5874 ± 38 | 4.04 ± 0.19 | 1.21 ± 0.04 | 3.05 ± 0.28 | 1.2 ± 0.0 |
| betVir | G V | 0.21 ± 0.06 | 6223 ± 28 | 4.21 ± 0.21 | 1.24 ± 0.03 | 1.66 ± 0.34 | 1.4 ± 0.0 |
| delEri | FGK IV | 0.16 ± 0.07 | 5133 ± 35 | 3.87 ± 0.23 | 0.93 ± 0.03 | 1.87 ± 0.24 | 0.9 ± 0.0 |
| epsEri | K V | −0.07 ± 0.13 | 5276 ± 35 | 4.46 ± 1.74 | 1.13 ± 0.04 | 2.53 ± 2.23 | 0.8 ± 0.0 |
| epsFor | FGK IV | −0.39 ± 0.07 | 5370 ± 4 | 4.26 ± 0.42 | 0.69 ± 0.03 | 2.15 ± 0.38 | 1.9 ± 0.1 |
| epsVir | FGK III | −0.06 ± 0.12 | 4830 ± 1 | 2.15 ± 0.24 | 1.48 ± 0.05 | 2.16 ± 0.32 | 4.5 ± 0.1 |
| etaBoo | FGK IV | −0.07 ± 0.26 | 5670 ± 1 | 3.03 ± 0.50 | 1.71 ± 0.13 | 11.96 ± 0.43 | 2.1 ± 0.0 |
| gamSge | M III | 0.14 ± 0.26 | 4481 ± 158 | 2.63 ± 0.92 | 1.98 ± 0.12 | 4.10 ± 0.79 | 4.5 ± 0.0 |
| ksiHya | FGK III | 0.21 ± 0.08 | 5186 ± 36 | 3.16 ± 0.21 | 1.35 ± 0.03 | 4.04 ± 0.21 | 0.1 ± 0.0 |
| muAra | G V | 0.38 ± 0.21 | 5967 ± 106 | 4.62 ± 0.48 | 1.10 ± 0.08 | 1.99 ± 0.44 | 1.3 ± 0.2 |
| muLeo | FGK III | 0.21 ± 0.15 | 4458 ± 1 | 2.23 ± 0.39 | 1.60 ± 0.07 | 1.21 ± 0.37 | 2.3 ± 0.0 |
Notes. The spectral types were drawn from Heiter et al. (2015), and denote the temperature classification, plus the luminosity class (V: dwarf, IV: subgiant, III: giant).
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