Table B.1
Sample of M dwarfs from the CARMENES radial velocity survey analysed in this work.
| Karmn | Name | SpT (a) | vr | Ref. (b) | vsini(c) | S/N | Hα flag (d) |
|---|---|---|---|---|---|---|---|
| [km s−1] | [km s−1] | ||||||
| J04167−120 | LP 714-47 | K7.0 V | − 7.45 ± 0.05 | This work | ≤ 2.0 | 258 | 0 |
| J11110+304E | HD 97101 | K7.0 V | − 16.00 ± 0.03 | This work | ≤ 2.0 | 422 | 0 |
| J18198−019 | HD 168442 | K7.0 V | − 14.03 ± 0.03 | Laf20 | ≤ 3.0 | 1447 | 0 |
| J03463+262 | HD 23453 | M0.0 V | 35.59 ± 0.02 | Laf20 | 3.3 ± 4.0 | 728 | 0 |
| J04376+528 | BD+52 857 | M0.0 V | 33.91 ± 0.01 | Laf20 | 3.4 ± 1.5 | 1167 | 0 |
| J04588+498 | BD+49 1280 | M0.0 V | − 34.35 ± 0.02 | Laf20 | ≤ 2.0 | 877 | 0 |
Notes. (a) Spectral types from Carmencita (Alonso-Floriano et al. 2015; Caballero et al. 2016a). (b) Radial velocities from Lafarga et al. (2020, Laf20) if available, or computed using serval (Zechmeister et al. 2018) otherwise. (c) Projected rotational velocities computed as in Reiners et al. (2018). (d) Hα-active stars following Schöfer et al. (2019) (1 if active).
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