Table 6
Mdwarfs with interferometric angular diameter measurements in common with the CARMENES GTO survey.
| Name | Karmn | SpT | R | Teff | Lbol | M | Ref. (a) | Teff (b) | logg(b) | [Fe/H]corr (b) |
|---|---|---|---|---|---|---|---|---|---|---|
| [R⊙] | [K] | [10−4L⊙] | [M⊙] | [K] | [dex] | [dex] | ||||
| HD 79210 | J09143+526 | M0.0 V | 0.5773 ± 0.0131 | 3907 ± 35 | 697 ± 21 | 0.622 | B12 | 4015 ± 16 | 4.91 ± 0.08 | − 0.12 ± 0.05 |
| HD 79211 | J09144+526 | M0.0 V | 0.5673 ± 0.0137 | 3867 ± 37 | 647 ± 19 | 0.600 | B12 | 3983 ± 17 | 5.17 ± 0.07 | − 0.03 ± 0.04 |
| GX And | J00183+440 | M1.0 V | 0.3874 ± 0.0023 | 3563 ± 11 | 217.3 ± 2.1 | 0.423 | B12 | 3603 ± 24 | 4.99 ± 0.14 | − 0.52 ± 0.11 |
| BD+44 2051 A | J11054+435 | M1.0 V | 0.3982 ± 0.0091 | 3497 ± 39 | 212.9 ± 2.6 | 0.403 | B12 | 3628 ± 19 | 5.01 ± 0.13 | − 0.56 ± 0.09 |
| BD+25 3173 | J16581+257 | M1.0 V | 0.5387 ± 0.0157 | 3590 ± 45 | 432 ± 13 | 0.54 | v14 | 3782 ± 17 | 4.87 ± 0.09 | − 0.05 ± 0.05 |
| HD 199305 | J20533+621 | M1.0 V | 0.5472 ± 0.0067 | 3692 ± 22 | 499.0 ± 6.2 | 0.573 | B12 | 3815 ± 16 | 4.83 ± 0.14 | − 0.10 ± 0.08 |
| HD 36395 | J05314−036 | M1.5 V | 0.5735 ± 0.0044 | 3801 ± 9 | 616.3 ± 8.8 | 0.615 | B12 | 3850 ± 27 | 4.71 ± 0.18 | 0.05 ± 0.08 |
| Lalande 21185 | J11033+359 | M1.5 V | 0.3921 ± 0.0037 | 3465 ± 17 | 198.9 ± 1.2 | 0.403 | B12 | 3557 ± 26 | 4.95 ± 0.14 | − 0.49 ± 0.10 |
| HD 119850 | J13457+148 | M1.5 V | 0.4840 ± 0.0084 | 3618 ± 31 | 360 ± 5 | 0.520 | B12 | 3620 ± 24 | 4.93 ± 0.12 | − 0.34 ± 0.07 |
| HD 216899 | J22565+165 | M1.5 V | 0.5477 ± 0.0048 | 3713 ± 11 | 511.2 ± 7.4 | 0.569 | B12 | 3798 ± 21 | 4.80 ± 0.12 | 0.03 ± 0.06 |
| HD 285968 | J04429+189 | M2.0 V | 0.4525 ± 0.0221 | 3679 ± 77 | 337 ± 18 | 0.45 | v14 | 3678 ± 16 | 5.13 ± 0.08 | 0.00 ± 0.03 |
| Ross 905 | J11421+267 | M2.5 V | 0.4546 ± 0.0182 | 3416 ± 53 | 252.5 ± 1.2 | 0.472 | B12 | 3533 ± 26 | 4.83 ± 0.11 | − 0.12 ± 0.10 |
| HO Lib | J15194−077 | M3.0 V | 0.2990 ± 0.0100 | 3442 ± 54 | 113 ± 8 | 0.297 | B12 | 3500 ± 26 | 4.97 ± 0.11 | − 0.08 ± 0.07 |
| BD+68 946 | J17364+683 | M3.0 V | 0.4183 ± 0.0070 | 3413 ± 28 | 212.8 ± 2.3 | 0.413 | B12 | 3389 ± 81 | 4.89 ± 0.15 | − 0.06 ± 0.13 |
| HD 173739 | J18427+526N | M3.0 V | 0.3561 ± 0.0039 | 3407 ± 15 | 153.1 ± 1.8 | 0.318 | B12 | 3473 ± 34 | 4.90 ± 0.11 | − 0.31 ± 0.12 |
| Barnard’s star | J17578+046 | M3.5 V | 0.1867 ± 0.0012 | 3224 ± 10 | 33.8 ± 0.2 | 0.150 | B12 | 3254 ± 32 | 5.13 ± 0.12 | − 0.57 ± 0.10 |
| HD 173740 | J18427+596S | M3.5 V | 0.3232 ± 0.0061 | 3104 ± 28 | 87.1 ± 1.2 | 0.235 | B12 | 3393 ± 48 | 4.98 ± 0.12 | − 0.38 ± 0.18 |
| IL Aqr | J22532−142 | M4.0 V | 0.3761 ± 0.0059 | 3129 ± 19 | 122 ± 2 | 0.37 | v14 | 3421 ± 40 | 4.83 ± 0.10 | − 0.06 ± 0.10 |
Notes. (a) Stellar radii, effective temperatures, luminosities, and stellar masses from Boyajian et al. (2012, B12) and von Braun et al. (2014, v14). The estimates of the stellar mass from these works conservatively assume 10 and 5% uncertainties, respectively. (b) This work.
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