Table A.1
Small transiting planets with precise masses around M dwarfs.
Name | Alternative name | Radius | Mass | Reference | ||||
---|---|---|---|---|---|---|---|---|
[R⊕] | [M⊕] | |||||||
GJ 3473 b (a,b) | G 50–16 b | 1.264 | ± | 0.050 | 1.86 | ± | 0.30 | This work |
LP 729–54 b (a,b) | LTT 3780 b | 1.35 | ± | 0.06 | 2.34 | ± | 0.24 | Nowak et al. (2020); Cloutier et al. (2020a) |
TOI-1235 b (a,b) | TYC 4384–1735–1 b | 1.69 | ± | 0.08 | 5.9 | ± | 0.6 | Bluhm et al. (2020); Cloutier et al. (2020b) |
GJ 357 b (a,b) | LHS 2157 b | 1.217 | ± | 0.084 | 1.84 | ± | 0.31 | Luque et al. (2019); Jenkins et al. (2019) |
GJ 1252 b (a) | L 210–70 b | 1.193 | ± | 0.074 | 2.10 | ± | 0.58 | Shporer et al. (2020) |
L 98–59 c (a) | TOI-175.01 | 1.35 | ± | 0.07 | 2.42 | ± | 0.35 | Cloutier et al. (2019); Kostov et al. (2019) |
L 98–59 d (a) | TOI-175.01 | 1.57 | ± | 0.14 | 2.31 | ± | 0.46 | Cloutier et al. (2019); Kostov et al. (2019) |
L 168–9 b (a) | CD–60 8051 b | 1.39 | ± | 0.09 | 4.60 | ± | 0.58 | Astudillo-Defru et al. (2020) |
Kepler-138 c | KOI-314.2 | 1.67 | ± | 0.15 | 5.2 | ± | 1.3 | Almenara et al. (2018); Kipping et al. (2014); Mann et al. (2017) |
Kepler-138 d | KOI-314.3 | 1.68 | ± | 0.15 | 1.17 | ± | 0.30 | Almenara et al. (2018); Kipping et al. (2014); Mann et al. (2017) |
GJ 1132 b | LTT 3758 b | 1.130 | ± | 0.057 | 1.66 | ± | 0.23 | Bonfils et al. (2018); Berta-Thompson et al. (2015) |
LHS 1140 b | GJ 3053 b | 1.727 | ± | 0.033 | 6.99 | ± | 0.89 | Ment et al. (2019); Dittmann et al. (2017) |
LHS 1140 c | GJ 3053 c | 1.282 | ± | 0.024 | 1.81 | ± | 0.39 | Ment et al. (2019) |
TRAPPIST-1 b | 2MUCD 12 171 b | 1.121 | ± | 0.033 | 1.017 | ± | 0.16 | Grimm et al. (2018); Delrez et al. (2018); Gillon et al. (2016) |
TRAPPIST-1 c | 2MUCD 12 171 c | 1.095 | ± | 0.031 | 1.156 | ± | 0.15 | Grimm et al. (2018); Delrez et al. (2018); Gillon et al. (2016) |
TRAPPIST-1 d | 2MUCD 12 171 d | 0.784 | ± | 0.023 | 0.297 | ± | 0.039 | Grimm et al. (2018); Delrez et al. (2018); Gillon et al. (2017) |
TRAPPIST-1 e | 2MUCD 12 171 e | 0.910 | ± | 0.027 | 0.772 | ± | 0.079 | Grimm et al. (2018); Delrez et al. (2018); Gillon et al. (2017) |
TRAPPIST-1 f | 2MUCD 12 171 f | 1.046 | ± | 0.030 | 0.934 | ± | 0.095 | Grimm et al. (2018); Delrez et al. (2018); Gillon et al. (2017) |
TRAPPIST-1 g | 2MUCD 12 171 g | 1.148 | ± | 0.033 | 1.148 | ± | 0.098 | Grimm et al. (2018); Delrez et al. (2018); Gillon et al. (2017) |
TRAPPIST-1 h | 2MUCD 12 171 h | 0.773 | ± | 0.027 | 0.331 | ± | 0.056 | Grimm et al. (2018); Delrez et al. (2018); Luger et al. (2017) |
Notes. (a) Planets discovered by TESS. (b)Target stars in the CARMENES guaranteed time observations survey (Quirrenbach et al. 2014; Reiners et al. 2018). The table is based on TEPCat (Southworth 2011, visited on 15 July 2020) and shows the known transiting planets with radii smaller than 2 R⊕ and mass determinations to a precision better than 30% in orbits around stars with temperatures lower than 4000 K. The first reference always denotes the source of the properties.
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