Table 2
Stellar parameters and their uncertainties derived in this work.
| Star | Teff/K |  |
log g/cm s−2 | u log g | [Fe/H] | u[Fe/H] |
|---|---|---|---|---|---|---|
| BD+00549B | 3726 | 60 | 4.931 | 0.029 | –0.66 | 0.07 |
| BD-064756B | 3442 | 33 | 4.814 | 0.006 | –0.02 | 0.06 |
| GJ105A | 4607 | 93 | 4.960 | 0.150 | 0.02 | 0.06 |
| GJ105B | 3483 | 69 | 4.994 | 0.017 | –0.31 | 0.05 |
| GJ15A | 3609 | 73 | 4.883 | 0.023 | –0.30 | 0.16 |
| GJ205 | 3941 | 26 | 4.727 | 0.008 | 0.19 | 0.06 |
| GJ212 | 3838 | 35 | 4.734 | 0.015 | 0.09 | 0.10 |
| GJ297.2B | 3597 | 52 | 4.801 | 0.004 | –0.08 | 0.08 |
| GJ3195 | 3571 | 52 | 4.863 | 0.014 | –0.10 | 0.11 |
| GJ324B | 3262 | 76 | 5.000 | 0.003 | 0.24 | 0.11 |
| GJ338A | 4000 | 19 | 4.690 | 0.012 | –0.11 | 0.05 |
| GJ338B | 4029 | 19 | 4.711 | 0.013 | –0.13 | 0.05 |
| GJ393 | 3586 | 47 | 4.847 | 0.018 | –0.15 | 0.06 |
| GJ412A | 3593 | 96 | 4.900 | 0.020 | –0.31 | 0.12 |
| GJ447 | 3243 | 101 | 5.066 | 0.015 | –0.13 | 0.05 |
| GJ526 | 3729 | 38 | 4.792 | 0.018 | –0.32 | 0.08 |
| GJ687 | 3539 | 69 | 4.875 | 0.063 | –0.02 | 0.12 |
| GJ725A | 3584 | 51 | 4.925 | 0.025 | –0.34 | 0.05 |
| GJ725B | 3556 | 61 | 4.984 | 0.032 | –0.38 | 0.06 |
| GJ752A | 3684 | 38 | 4.819 | 0.035 | –0.09 | 0.08 |
| GJ777B | 3251 | 152 | 5.043 | 0.038 | –0.08 | 0.04 |
| GJ809 | 3839 | 41 | 4.741 | 0.054 | –0.12 | 0.11 |
| GJ880 | 3649 | 83 | 4.754 | 0.009 | 0.25 | 0.12 |
| LSPMJ0355+5214 | 3481 | 61 | 4.986 | 0.014 | –0.19 | 0.02 |
| Ross799 | 3686 | 29 | 4.790 | 0.007 | –0.04 | 0.05 |
Notes. The M dwarf LSPM J1204+1728S is not included (see text). GJ 105A and GJ 338A are K dwarfs but are included since they are within the parameter range of the model grid used to train The Payne and have APOGEE spectra. The uncertainties are derived as described in Sect. 3.4.
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