Table 1
Physical and orbital parameters of the investigated planets.
| Planet’s name | Mass, Μ⊕ | Radius, R⊕ | a, AU | e | Teq, K | Stellar mass, M⊕ | References |
|---|---|---|---|---|---|---|---|
| GJ 1061 c* | 1.74 ± 0.1907 | 1.23 ± 0.28 | 0 035 ± 0.001 | <0.29 | 0.12 ± 0.01 | 1 | |
| GJ 1061 d* |  |
1.17 ± 0.25 | 0 052 ± 0.001 | <0.54 | 0.12 ± 0.01 | 1 | |
| GJ 273 b* | 2.193 ± 0.953 | 1.38 ± 0.52 | 0 091 ± 0.01 |  |
0.29 | 2 | |
| GJ 667 C e* |  |
1.57 ± 0.69 | 0 213 ± 0.02 |  |
0.33 | 3 | |
| GJ 667 C f* |  |
1.54 ± 0.66 |  |
 |
0.33 | 3 | |
| K2-288 B b | 5.52 ± 3.58 | 1.906 ± 0.30267 | 0 164 ± 0.03 | 226 ± 22 | 0.33 ± 0.02 | 4 | |
| K2-3 d | 3.76 ± 2.54 | 1.513 ± 0.235 | 0 2086 ± 0.01 | 0.045 ± 0.045 | 282 ± 24 | 0.6 ± 0.09 | 5 |
| K2-72 e | 2.63 ± 1.74 | 1.289 ± 0.1345 |  |
 |
280 |  |
6 |
| Kepler-1229 b | 3.22 ± 1.99 |  |
 |
0.5593 ± 0.0207 | 7 | ||
| Kepler-1649 b | 1.30 ± 0.87 | 1.02 ± 0.056 | 0 0514 ± 0.0028 | 307 ± 26 | 0.2 ± 0.01 | 8 | |
| Kepler-1652 b | 4.20 ± 2.61 | 1.60 ± 0.18 |  |
268 ± 20 |  |
9 | |
| Kepler-186 f | 1.96 ± 1.27 | 1.166 ± 0.078 |  |
 |
0.54 ± 0.02 | 10 | |
| Kepler-296 e | 1.64 ± 1.24 |  |
 |
0.165 ± 0.165 | 337.0 ± 17.5 |  |
7, 19 |
| Kepler-296 f | 2.20 ± 1.51 |  |
 |
0.18 ± 0.15 | 274 ± 15 |  |
7, 19 |
| Kepler-442 b | 3.21 ± 1.95 |  |
 |
 |
0.61 ± 0.03 | 11 | |
| Kepler-452 b | 3.78 ± 2.29 |  |
 |
0.035 ± 0.75 | 265 ± 13 | 1.04 ± 0.05 | 11, 20 |
| Kepler-62 e | 4.36 ± 2.47 | 1 61 ± 0.05 | 0 427 ± 0.004 | 0.13 | 270 ± 15 | 0.69 ± 0.02 | 12 |
| Kepler-62 f | 3.29 ± 1.94 | 1 41 ± 0.07 | 0 718 ± 0.007 | 0.0943 | 208 ± 11 | 0.69 ± 0.02 | 12 |
| Proxima Centauri b* | 1.17 ± 0.086 | 1.07 ± 0.15 | 0 049 ± 0.002 |  |
 |
0.12 ± 0.015 | 13 |
| Ross 128 b* | 1.4 ± 0.21 | 1.13 ± 0.21 | 0 0496 ± 0.0017 | 0.116 ± 0.097 | 256 ± 45 | 0.168 ± 0.017 | 14 |
| Teegarden’s b* | 1.04 ± 0.13 | 1.03 ± 0.13 | 0 0252 ± 0.0009 | 0.0 ± 0.16 | 0.089 ± 0.009 | 15 | |
| Teegarden’s c* | 1.11 ± 0.16 | 1.05 ± 0.14 | 0.0443 ± 0.0015 | 0.0 ± 0.16 | 0.089 ± 0.009 0.416 ± 0.01 | 15 16 | |
| TOI-700 d | 1.84 ± 1.13 |  |
0.163 ± 0.015 |  |
295 ± 55 | 0.416 ± 0.01 | 16 |
| TOI-1452 b | 4.8 ± 1.3 | 1 67 ± 0.07 | 0.061 ± 0.003 | 326 ± 7 | 0.249 ± 0.008 | 17 | |
| TRAPPIST-1 d | 0.388 ± 0.012 |  |
0.02227 ± 0.00019 | 0.00563 ± 0.00172 | 288.0 ± 5.6 | 0.0898 ± 0.0023 | 18, 21 |
| TRAPPIST-1 e | 0.692 ± 0.022 |  |
0.02925 ± 0.00025 | 0.00632 ± 0.0012 | 251.3 ± 4.9 | 0.0898 ± 0.0023 | 18, 21 |
| TRAPPIST-1 f | 1.04 ± 0.03 |  |
0.03849 ± 0.00033 | 0.00842 ± 0.0013 | 219.0 ± 4.2 | 0.0898 ± 0.0023 | 18, 21 |
| TRAPPIST-1 g | 1.32 ± 0.038 |  |
0.04683 ± 0.0004 | 0.00401 ± 0.00109 | 198.6 ± 3.8 | 0.0898 ± 0.0023 | 18, 21 |
Notes. Planets with only m sin i measurements are marked with an asterisk. Values of planetary masses, radii semi-major axes, and eccentricities, along with the mass of the host star and the estimated planetary equilibrium temperature where available. Average masses and radii values with the respective standard deviations predicted by the Forecaster code are shown in italics.
References. 1: Dreizler et al. (2020), 2: Astudillo-Defru et al. (2017), 3: Anglada-Escudé et al. (2013), 4: Feinstein et al. (2019), 5: Sinukoff et al. (2016), 6: Dressing et al. (2017), 7: Morton et al. (2016), 8: Vanderburg et al. (2020), 9: Torres et al. (2017), 10: Torres et al. (2015) 11: Berger et al. (2018), 12: Borucki et al. (2013), 13: Anglada-Escudé et al. (2016), 14: Bonfils et al. (2018), 15: Zechmeister et al. (2019), 16: Rodriguez et al. (2020), 17: Cadieux et al. (2022), 18: Agol et al. (2021), 19: Cartier et al. (2015), 20: Jenkins et al. (2015), 21: Gillon et al. (2017).
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