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Table 6.
Comparison of the rotation periods given in the literature with our measured values for the mid-M stars.
| Reference | Category | Gl 752A | Gl 48 | Gl 15A | Gl 849 | Gl 411 | Gl 687 | Gl 251 | GJ 4333 | Gl 876 | GJ 3378 |
|---|---|---|---|---|---|---|---|---|---|---|---|
| This work | Bℓ | 53 ± 4 | 51.2 ± 1.4 | 44.3 ± 2.0 | 41.4 ± 0.4 | 470 ± 40 | 56.5 ± 0.9 | 99 ± 8 | 72.0 ± 1.0 | 82.8 ± 1.4 | 92 ± 5 |
| Rivera et al. (2005) | phm | 96.7 ± 1.0 | |||||||||
| Bonfils et al. (2013) | act | 2000 ? | 61.0, 30.1 | ||||||||
| Burt et al. (2014) | phm | 61.8 ± 1.0 | |||||||||
| Howard et al. (2014) | phm | 43.82 ± 0.56 | |||||||||
| Suárez Mascareño et al. (2015) | act | 46.5 ± 0.3 | 39.2 ± 6.3 | 87.3 ± 5.7 | |||||||
| Nelson et al. (2016) | act | 95 ± 1 | |||||||||
| Suárez Mascareño et al. (2016) | phm | 46.0 ± 0.2 | |||||||||
| Moutou et al. (2017) | ZDI | 90 ± 10 | |||||||||
| Suárez Mascareño et al. (2017) | act | 90.9 ± 16.5 | |||||||||
| Suárez Mascareño et al. (2018) | act | 45.0 ± 4.4 | |||||||||
| Díaz et al. (2019) | phm | 56.15 ± 0.27 | |||||||||
| Díez Alonso et al. (2019) | phm | 46.0 ± 0.2 | 51.5 ± 2.6 | 18.1 ± 0.3 | 74.7 ± 0.7 | 81.0 ± 0.8 | |||||
| Reinhold & Hekker (2020) | phm | 31.31 ± 8.15 | |||||||||
| Stock et al. (2020) | phm | 122.1 ± 2.2 | |||||||||
| Sabotta et al. (2021) | act | 174.48 | 43.39 | 67.59, 119.48 | 83.39 |
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