Table 2
Catalogue of v sin i values for 392 M-dwarf stars of the CARMENES sample using VIS spectra a.
| Karmn | Name | Adopted v sin i (km s−1) | v sin i OC (km s−1) | v sin i NI (km s−1) | v sin i literature (km s−1) | Ref. b | veq (km s−1) |
|---|---|---|---|---|---|---|---|
| J00051+457 | BD+44 4548 | <2 | 2 | 2 | 2 | Rein18 | 1.61 ± 0.01 |
| J01019+541 | G 218–020 | 29.3 ± 0.9 | 29.3 ± 0.92 | 29.2 ± 0.9 | 30.6 ± 3.06 | Rein18 | 28.2 ± 0.26 |
| J01056+284 | GJ 1029 | <2 | 2 | 2 | 4.1 ± 0.41 | Jen09 | 0.65 ± 0.02 |
| J02002+130 | TZ Ari | <2 | 2 | 2 | 2 | Rein18 | 4.04 ± 0.08 |
| J02164+135 | LP 469–206 | 13.4 ± 0.7 | 13.4 ± 0.7 | 13.4 ± 0.7 | 12.4 ± 1.24 | Barn14 | ... |
Notes. (a) Only five rows are shown as an example, the complete table is available in the GitHub repository. Listed are: star’s Karmn identifier, most common or discovery name, adopted v sin i, v sin i obtained using oversampled convolution (OC), numerical integration (NI), the value from the literature and reference to the work, and the equatorial rotation velocity. (b) Jen09: Jenkins et al. (2009), Barn14: Barnes et al. (2014), Rein18: Reiners et al. (2018).
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