Table A.3.
Stellar atmospheric parameters derived with STEPARSYN (Teff, log g, [Fe/H], and Vbroad), trigonometric gravities (log gtrig), mass (M*), and radius (R*) for the stars analysed in this work.
| Name | Teff | log g | [Fe/H] | Vbroad | log gtrig | M* | R* |
|---|---|---|---|---|---|---|---|
| [K] | [dex] | [dex] | [km s−1] | [dex] | [M⊙] | [R⊙] | |
| Sun | 5775 ± 13 | 4.41 ± 0.02 | −0.04 ± 0.01 | 3.71 ± 0.03 | … | 1 | 1 |
| HD 4628 | 4969 ± 37 | 4.57 ± 0.05 | −0.33 ± 0.02 | 2a | 4.59 ± 0.02 | 0.720 ± 0.014 | 0.691 ± 0.007 |
| η Cas A | 5874 ± 34 | 4.30 ± 0.06 | −0.33 ± 0.02 | 4.00 ± 0.07 | 4.30 ± 0.02 | 0.881 ± 0.014 | 1.062 ± 0.022 |
| μ Cas | 5370 ± 35 | 4.58 ± 0.05 | −0.87 ± 0.02 | 1.1a | 4.50 ± 0.01 | 0.747 ±0.008 | 0.781 ± 0.018 |
| τ Cet | 5400 ± 60 | 4.58 ± 0.05 | −0.53 ± 0.04 | 1.6a | 4.54 ± 0.02 | 0.760 ± 0.017 | 0.750 ± 0.015 |
| HD 16160 | 4900 ± 45 | 4.65 ± 0.07 | −0.19 ± 0.02 | 1.3a | 4.60 ± 0.02 | 0.741 ± 0.015 | 0.691 ± 0.006 |
| θ Per A | 6302 ± 20 | 4.25 ± 0.03 | −0.02 ± 0.01 | 9.39 ± 0.04 | 4.30 ± 0.01 | 1.201 ± 0.010 | 1.250 ± 0.020 |
| α Cet | 3883 ± 41 | 1.56 ± 0.17 | −0.01 ± 0.09 | 6.30 ± 0.23 | 1.08 ± 0.06 | 2.803 ± 0.219 | 77.347 ± 5.120 |
| ϵ Eri | 5086 ± 33 | 4.62 ± 0.06 | −0.08 ± 0.02 | 3.11 ± 0.14 | 4.58 ± 0.02 | 0.806 ± 0.019 | 0.734 ± 0.015 |
| HD 22879 | 5763 ± 30 | 4.13 ± 0.05 | −0.91 ± 0.02 | 3.97 ± 0.08 | 4.29 ± 0.01 | 0.977 ± 0.015 | 1.135 ± 0.023 |
| δ Eri | 4934 ± 41 | 3.62 ± 0.09 | 0.04 ± 0.02 | 3.27 ± 0.11 | 3.67 ± 0.04 | 1.094 ± 0.047 | 2.450 ± 0.070 |
| Aldebaran | 3858 ± 21 | 0.99 ± 0.10 | −0.36 ± 0.07 | 4.93 ± 0.13 | 1.02 ± 0.04 | 0.912 ± 0.063 | 47.535 ± 1.427 |
| π3 Ori | 6358 ± 34 | 4.04 ± 0.08 | −0.02 ± 0.02 | 18.20 ± 0.14 | 4.25 ± 0.01 | 1.230 ± 0.012 | 1.339 ± 0.029 |
| HD 49933 | 6725 ± 26 | 4.20 ± 0.05 | −0.39 ± 0.02 | 11.10 ± 0.08 | 4.21 ± 0.01 | 1.188 ± 0.014 | 1.379 ± 0.009 |
| Procyon | 6631 ± 34 | 3.97 ± 0.05 | −0.02 ± 0.02 | 6.18 ± 0.03 | 4.00 ± 0.01 | 1.480 ± 0.010 | 1.965 ± 0.043 |
| β Gem | 4756 ± 23 | 2.76 ± 0.07 | 0.02 ± 0.03 | 4.08 ± 0.07 | 2.73 ± 0.03 | 1.819 ± 0.075 | 9.324 ± 0.215 |
| μ Leo | 4480 ± 43 | 2.07 ± 0.13 | 0.21 ± 0.07 | 4.32 ± 0.12 | 2.41 ± 0.07 | 1.311 ± 0.161 | 11.503 ± 0.360 |
| 20 LMi | 5691 ± 32 | 4.27 ± 0.06 | 0.13 ± 0.02 | 4.04 ± 0.07 | 4.29 ± 0.02 | 1.010 ± 0.016 | 1.158 ± 0.021 |
| 36 UMa | 6102 ± 43 | 4.29 ± 0.08 | −0.15 ± 0.03 | 4.19 ± 0.09 | 4.29 ± 0.02 | 1.049 ± 0.021 | 1.180 ± 0.027 |
| β Vir | 6024 ± 28 | 3.88 ± 0.04 | 0.04 ± 0.02 | 5.24 ± 0.05 | 4.03 ± 0.02 | 1.226 ± 0.041 | 1.722 ± 0.032 |
| Gmb 1830 | 4997 ± 18 | 4.60 ± 0.03 | −1.41 ± 0.02 | 0a | 4.60 ± 0.01 | 0.616 ± 0.001 | 0.631 ± 0.003 |
| HD 107328 | 4427 ± 20 | 1.62 ± 0.06 | −0.51 ± 0.16 | 5.00 ± 0.07 | 1.81 ± 0.08 | 1.049 ± 0.180 | 20.428 ± 0.540 |
| ϵ Vir | 5019 ± 23 | 2.73 ± 0.05 | 0.08 ± 0.03 | 5.16 ± 0.06 | 2.72 ± 0.01 | 2.878 ± 0.020 | 11.939 ± 0.206 |
| β Com | 6000 ± 22 | 4.40 ± 0.04 | 0.10 ± 0.04 | 5.56 ± 0.05 | 4.40 ± 0.02 | 1.130 ± 0.024 | 1.075 ± 0.025 |
| η Boo | 5956 ± 18 | 3.64 ± 0.04 | 0.15 ± 0.01 | 13.55 ± 0.05 | 3.73 ± 0.01 | 1.587 ± 0.022 | 2.762 ± 0.042 |
| Arcturus | 4294 ± 24 | 1.49 ± 0.04 | −0.59 ± 0.02 | 4.98 ± 0.07 | 1.58 ± 0.04 | 0.887 ± 0.043 | 24.457 ± 0.606 |
| θ Boo A | 6300 ± 23 | 3.93 ± 0.04 | −0.09 ± 0.01 | 29.50 ± 0.12 | 4.06 ± 0.01 | 1.255 ± 0.039 | 1.661 ± 0.010 |
| 18 Sco | 5763 ± 18 | 4.42 ± 0.03 | -0.02 ± 0.01 | 3.80 ± 0.03 | 4.39 ± 0.02 | 0.977 ± 0.012 | 1.017 ± 0.023 |
| γ Sge | 3943 ± 25 | 1.27 ± 0.10 | 0.00 ± 0.15 | 5.35 ± 0.14 | 1.23 ± 0.08 | 1.446 ± 0.263 | 46.623 ± 2.241 |
| HD 189733 | 4995 ± 32 | 4.51 ± 0.06 | −0.01 ± 0.01 | 4.08 ± 0.09 | 4.55 ± 0.02 | 0.800 ± 0.018 | 0.758 ± 0.003 |
| 61 Cyg A | 4576 ± 36 | 4.69 ± 0.06 | −0.37 ± 0.02 | 1.9a | 4.69 ± 0.02 | 0.624 ± 0.010 | 0.574 ± 0.005 |
| 61 Cyg B | 4088 ± 26 | 4.61 ± 0.07 | −0.44 ± 0.04 | 0.7a | 4.57 ± 0.04 | 0.451 ± 0.024 | 0.562 ± 0.015 |
| HD 209458 | 6028 ± 24 | 4.21 ± 0.04 | −0.07 ± 0.01 | 5.55 ± 0.05 | 4.29 ± 0.01 | 1.054 ± 0.012 | 1.178 ± 0.027 |
| ξ Peg | 6091 ± 18 | 3.73 ± 0.03 | −0.40 ± 0.01 | 9.02 ± 0.05 | 3.89 ± 0.01 | 1.096 ± 0.001 | 1.909 ± 0.016 |
| HD 220009 | 4260 ± 26 | 1.57 ± 0.05 | −0.79 ± 0.03 | 4.42 ± 0.07 | 1.58 ± 0.01 | 0.777 ± 0.003 | 22.920 ± 0.111 |
Notes.
We fixed Vbroad to the values of v sin i reported in the literature. These were taken from Hale (1994) for μ Cas, Jenkins et al. (2011) for τ Cet, Latham et al. (2002) for Gmb 1830, Marsden et al. (2014) for HD 4628, and Queloz et al. (1998) for both the 61 Cyg system and HD 16160.
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