Table 1.
Summary of the rotation and flare analysis of the 45 M dwarfs from Lépine & Gaidos (2011) that were also observed as part of the TESS prime mission.
| EPIC id | Campaign | Prot, K2 [d] | Nflare/dayK2 | TIC id | Sector |
|---|---|---|---|---|---|
| 202059198 | C0 | 27.307 ± 0.465 | 0.030 | 385812015 | 6 |
| 202059199 | C0 | – | 0.121 | 385811983 | 6 |
| 202059222 | C0 | 72.160 ( * ) ± | – | 438489075 | 6 |
| 202059223 | C0 | – | – | 438496720 | 6 |
| 202059229 | C0 | 5.006 ± 0.025 | 0.121 | 372611670 | 6 |
| 201909533 | C1 | 2.294 ± 0.003 | 0.200 | 291074569 | 22 |
| 202571062 | C2 | 3.988 ± 0.017 | 0.077 | 392323519 | 12 |
| 202748218 | C2 | 120.610 ( * ) ± | – | 68559790 | 12 |
| 206007536 | C3 | 16.095 ± 0.503 | 0.030 | 188578639 | 2 |
| 206019392 | C3 | 75.440 ( * ) ± | 0.225 | 188580272 | 2 |
| 210317378 | C4 | 26.909 ± 0.202 | 0.058 | 345454031 | 5 |
| 210340480 | C4 | – | 0.015 | 311128611 | 5 |
| 210360545 | C4 | – | – | 242985446 | 5 |
| 210393283 | C4 | 16.626 ± 0.093 | – | 434135656 | 5 |
| 210408563 | C4 | 17.080 ± 0.648 | 0.073 | 435881860 | 5 |
| 210434433 | C4 | 23.278 ± 0.638 | 0.044 | 348663808 | 5 |
| 210434769 | C4 | – | – | 348663813 | 5 |
| 212323908 | C6 | – | – | 335010451 | 10 |
| 213817346 | C7 | 0.812 ± 0.004 | 0.184 | 169148174 | 13 |
| 220215093 | C8 | 57.550 ± 0.254 | 0.104 | 399702696 | 3 |
| 228711280 | C10 | 60.700 ± 6.070 | – | 110996526 | 10 |
| 229149393 | C10 | 8.389 ± 0.083 | – | 291109924 | 23 |
| 242219524 | C11 | 23.946 ± 0.221 | 0.014 | 105559958 | 12 |
| 245919787 | C12 | 5.649 ± 0.016 | 0.076 | 434101713 | 2 |
| 245983914 | C12 | 10.792 ± 0.366 | 0.076 | 9051707 | 2 |
| 246043232 | C12 | 90.667 ( * ) ± | 0.038 | 9633428 | 2 |
| 246048874 | C12 | 19.272 ± 0.029 | 0.038 | 9062134 | 2 |
| 210491860 | C13 | 15.031 ± 0.158 | – | 456892725 | 5 |
| 246625561 | C13 | 2.215 ± 0.041 | 0.063 | 436584697 | 5 |
| 246732310 | C13 | 12.933 ± 0.047 | 0.352 | 436655312 | 5 |
| 246807434 | C13 | 107.122 ( * ) ± | – | 436678563 | 5 |
| 246862801 | C13 | 15.992 ± 0.080 | 0.038 | 436635454 | 5 |
| 201497396 | C14 | 13.590 ± 0.173 | 0.180 | 281746741 | 9 |
| 201501470 | C14 | 1.304 ± 0.045 | 0.090 | 281731214 | 9 |
| 248425357 | C14 | 108.485 ( * ) ± | 0.026 | 277811911 | 8 |
| 248453031 | C14 | 34.232 ± 0.895 | 0.077 | 374312723 | 9 |
| 249101965 | C15 | 66.301 ± 1.081 | 0.012 | 185856339 | 11 |
| 249186244 | C15 | – | – | 186072161 | 11 |
| 249338840 | C15 | 22.354 ± 0.081 | 0.069 | 70111746 | 11 |
| 251550724 | C17 | 46.965 ± 0.134 | 0.107 | 115070878 | 23 |
| 251567386 | C17 | – | – | 130718008 | 23 |
| 251583820 | C17 | 52.926 ± 0.256 | – | 66765158 | 23 |
| 251584738 | C17 | 41.648 ± 1.080 | 0.015 | 66766055 | 23 |
| 211385897 | C5,C18 | 11.508 ± 0.298 | 0.211 | 366499976 | 7 |
| 211498244 | C5,C18 | – | 0.008 | 27654301 | 7 |
Notes. The results from the K2 mission are adopted from Raetz et al. (2020b). ( * )The period exceeds the duration of the K2 observation and is therefore not reliable. No uncertainties are given.
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