Open Access
Table C.4
Main planetary parameters of the Msample.
Planet | P [d] | Rp[R⊕] | Mp [M⊕] | ρp[ρ⊕] | Rp-location | Reference |
---|---|---|---|---|---|---|
TOI-732 b | 2.46 ± 0.19 | below | This work | |||
TOI-732 c | 12.252284 ± 0.000013 | above | This work | |||
GJ 1132 b | 1.628931 ± 0.000027 | 1.13 ± 0.056 | 1 66 ± 0 23 | 1.15 ± 0.23 | below | Bonfils et al. (2018) |
GJ 1214 b | 1.58040433 ± 0.00000013 | 8.17 ± 0.43 | 0.396 ± 0.031 | above | Cloutier et al. (2021a) | |
GJ 1252 b | 0.51824160 ± 0.00000069 | 1.180 ± 0.078 | 1.32 ± 0.28 | 0.80 ± 0.23 | below | Crossfield et al. (2022) |
GJ 3090 b | 2.13 ± 0.11 | 3.34 ± 0.72 | 0.346 ± 0.092 | above | Almenara et al. (2022) | |
GJ 3473 b | 1.86 ± 0.30 | 0.92 ± 0.18 | below | Kemmer et al. (2020) | ||
GJ 357 b | 1.84 ± 0.31 | 1.02 ± 0.27 | below | Luque et al. (2019) | ||
GJ 367 b | 0.718 ± 0.054 | 0.546 ± 0.078 | 1.48 ± 0.39 | below | Lam et al. (2021) | |
GJ 486 b | 1.27 ± 0.20 | below | Trifonov et al. (2021) | |||
HD 260655 b | 2.76953 ± 0.00003 | 1.24 ± 0.023 | 2.14 ± 0.34 | 1.12 ± 0.19 | below | Luque et al. (2022) |
HD 260655 c | 5.70588 ± 0.00007 | 3.09 ± 0.48 | 0.86 ± 0.16 | below | Luque et al. (2022) | |
K2-146 b | 2.6698 ± 0.0001 | 2.25 ± 0.10 | 5.6 ± 0.7 | 0.492 ± 0.090 | above | Lam et al. (2020) |
K2-18 b | 32.940045 ± 0.000010 | 2.61 ± 0.087 | 8.63 ± 1.35 | 0.485 ± 0.090 | above | Benneke et al. (2019) |
K2-25 b | 3.44 ± 0.12 | 0.60 ± 0.15 | above | Stefansson et al. (2020) | ||
K2-3 b | 0.569 ± 0.093 | above | Diamond-Lowe et al. (2022) | |||
Kepler-138 c | 1.51 ± 0.04 | 0.67 ± 0.17 | below | Piaulet et al. (2023) | ||
L 168-9 b | 1.40150 ± 0.00018 | 1.39 ± 0.09 | 4.6 ± 0.56 | 1.71 ± 0.39 | below | Astudillo-Defru et al. (2020) |
L 98-59 c | 3.6904 ± 0.0003 | 1.35 ± 0.07 | 0.98 ± 0.21 | below | Cloutier et al. (2019) | |
L 98-59 d | 1.94 ± 0.28 | 0.55 ± 0.14 | below | Demangeon et al. (2021) | ||
LHS 1140 b | 1.635 ± 0.046 | 1.46 ± 0.16 | below | Lillo-Box et al. (2020) | ||
LHS 1140 c | 3.77792 ± 0.00003 | 1.10 ± 0.15 | below | Lillo-Box et al. (2020) | ||
LHS 1478 b | 2.33 ± 0.20 | 1.22 ± 0.18 | below | Soto et al. (2021) | ||
LP 791-18 c | 2.438 ± 0.096 | 7.1 ± 0.7 | 0.490 ± 0.075 | above | Peterson et al. (2023) | |
LTT 1445 A b | 1.29 ± 0.22 | below | Winters et al. (2022) | |||
LTT 1445 A c | 1.02 ± 0.19 | below | Winters et al. (2022) | |||
TOI-1075 b | 0.6047328 ± 0.0000032 | 1.73 ± 0.37 | below | Essack et al. (2023) | ||
TOI-1201 b | 0.446 ± 0.079 | above | Kossakowski et al. (2021) | |||
TOI-1231 b | 15.4 ± 3.3 | 0.317 ± 0.079 | above | Burt et al. (2021) | ||
TOI-1235 b | 1.21 ± 0.21 | below | Bluhm et al. (2020) | |||
TOI-1634 b | 0.9893436 ± 0.0000020 | 1.749 ± 0.079 | 10.14 ± 0.95 | 1.90 ± 0.31 | below | Hirano et al. (2021) |
TOI-1695 b | 6.36 ± 1.0 | 0.93 ± 0.26 | below | Cherubim et al. (2023) | ||
TOI-244 b | 1.52 ± 0.12 | 2.68 ± 0.3 | 0.76 ± 0.20 | below | Castro-González et al. (2023) | |
TOI-269 b | 3.6977104 ± 0.0000037 | 2.77 ± 0.12 | 8.8 ± 1.4 | 0.414 ± 0.085 | above | Cointepas et al. (2021) |
TOI-270 b | 3.3601538 ± 0.0000048 | 1.206 ± 0.039 | 1.58 ± 0.26 | 0.901 ± 0.172 | below | Van Eylen et al. (2021) |
TOI-270 c | 5.6605731 ± 0.0000031 | 2.355 ± 0.064 | 6.15 ± 0.37 | 0.471 ± 0.048 | above | Van Eylen et al. (2021) |
TOI-270 d | 11.379573 ± 0.000013 | 2.133 ± 0.058 | 4.78 ± 0.43 | 0.493 ± 0.060 | above | Van Eylen et al. (2021) |
TOI-776 b | 1.85 ± 0.13 | 4.0 ± 0.9 | 0.63 ± 0.19 | below | Luque et al. (2021) | |
TRAPPIST-1 b | 1.510826 ± 0.000006 | 1.374 ± 0.069 | 0.989 ± 0.060 | below | Agol et al. (2021) | |
TRAPPIST-1 c | 2.421937 ± 0.000018 | 1.308 ± 0.056 | 0.991 ± 0.055 | below | Agol et al. (2021) | |
TRAPPIST-1 d | 4.049219 ± 0.000026 | 0.388 ± 0.012 | 0.793 ± 0.040 | below | Agol et al. (2021) | |
TRAPPIST-1 e | 6.101013 ± 0.000035 | 0.692 ± 0.022 | 0.889 ± 0.046 | below | Agol et al. (2021) | |
TRAPPIST-1 f | 9.20754 ± 0.000032 | 1.039 ± 0.031 | 0.910 ± 0.042 | below | Agol et al. (2021) | |
TRAPPIST-1 g | 12.352446 ± 0.000054 | 1.321 ± 0.038 | 0.920 ± 0.043 | below | Agol et al. (2021) | |
TRAPPIST-1 h | 18. 772866 ± 0.000021 | 0.755 ± 0.014 | 0.326 ± 0.020 | 0.757 ± 0.063 | below | Agol et al. (2021) |
Notes. Rp-location refers to the location of the exoplanets with respect to the radius valley as derived by the SVM algorithm described in Sect. 6.
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