Table 1
Stars with planets in the sample.
Star | Teff [K] | Spectral type | R* [R⊙] | V | M* [M⊙] | References | Tmag | Tess sectors |
---|---|---|---|---|---|---|---|---|
61 Vir | 5577 | G5 V | 0.963 | 4.69 | 0.942 | 1 | 4.09 | 10 |
BD-06 1339 | 4324 | K7/M0 V | 0.602 | 9.7 | 0.7 | 2 | 8.29 | 6 |
BD-08 2823 | 4746 | K3 V | 0.710 | 9.86 | 0.74 | 3 | 8.86 | 8, 35 |
DMPP-1 | 6196 | F8 V | 1.260 | 7.98 | 1.21 | 4 | 7.47 | 6, 33 |
GJ 1061 | 2953 | M5.5 V | 0.156 | 12.7 | 0.12 | 5 | 9.47 | 3, 4, 30, 31 |
GJ 1132 | 3270 | M4.5 V | 0.207 | 13.68 | 0.181 | 6 | 12.14 | 9, 10, 36 |
GJ 15 A | 3607 | M1 V | 0.380 | 7.22 | 0.38 | 7 | 6.23 | 17 |
GJ 163 | 3500 | M3.5 V | 0.425 | 11.79 | 0.38 | 8 | 9.47 | 3–5, 30, 31 |
GJ 180 | 3562 | M3 | 0.420 | 10.914 | 0.39 | 8 | 8.82 | 5, 32 |
GJ 273 | 3382 | M3.5 V | 0.293 | 9.84 | 0.29 | 9 | 7.31 | 7 |
GJ 3138 | 3717 | M0 V | 0.50 | 10.83 | 0.681 | 9 | 10.19 | 3, 30 |
GJ 3293 | 3466 | M2.5 | 0.404 | 11.945 | 0.42 | 9 | 9.82 | 5, 31, 32 |
GJ 3323 | 3159 | M4 | 0.119 | 12.57 | 0.164 | 9 | 9.43 | 5, 32 |
GJ 3473 | 3347 | M4 | 0.364 | 13.74 | 0.36 | 10,11 | 11.20 | 7, 34 |
GJ 357 | 3505 | M2.5 V | 0.337 | 10.91 | 0.342 | 12 | 8.74 | 8, 35 |
GJ 433 | 3472 | M1.5 V | 0.500 | 9.81 | 0.48 | 13,14 | 7.81 | 10, 36 |
GJ 676 A | 3734 | M0 | 0.690 | 9.58 | 0.73 | 11,14 | 7.90 | 12 |
GJ 682 | 3172 | M4 | 0.340 | 10.94 | 0.31 | 8 | 8.25 | 12 |
GJ 876 | 3227 | M2.5 V | 0.400 | 10.16 | 0.34 | 8 | 7.57 | 2, 29 |
GJ 887 | 3688 | M1 V | 0.471 | 7.39 | 0.489 | 15 | 5.48 | 2, 28 |
HD 10180 | 5911 | G1 V | 1.109 | 7.33 | 1.06 | 16,17 | 6.75 | 1, 2, 28, 29 |
HD 109271 | 5783 | G5 V | 1.258 | 8.04 | 1.047 | 2 | 7.44 | 10 |
HD 136352 | 5664 | G4 V | 1.010 | 5.65 | 0.81 | 18 | 5.05 | 12 |
HD 1461 | 5765 | G5 V | 1.110 | 6.479 | 1.03 | 8 | 5.86 | 3 |
HD 158259 | 5834 | G0 | 1.290 | 6.479 | 1.15 | 8 | 5.90 | 17, 20, 24–26 |
HD 181433 | 4900 | K2 IV/ V | 0.830 | 8.4 | 0.77 | 8 | 7.49 | 27 |
HD 20003 | 5494 | G8 V | 0.922 | 8.39 | 0.875 | 18 | 7.71 | 1, 2, 6, 13, 27, 29 |
HD 20781 | 5256 | K0 V | 0.834 | 8.48 | 0.7 | 18 | 7.72 | 4, 31 |
HD 20794 | 5401 | G8 V | 0.920 | 4.26 | 0.85 | 8 | 3.58 | 3, 4, 30, 31 |
HD 213885 | 5978 | G0 V | 1.068 | 7.95 | 1.068 | 19 | 7.38 | 1, 27, 28 |
HD 215497 | 5113 | K3 V | 0.850 | 8.96 | 0.86 | 14 | 8.11 | 1, 28 |
HD 21693 | 5430 | G8 V | 0.914 | 7.95 | 0.8 | 18 | 7.27 | 2–4, 29–31 |
HD 219134 | 4966 | K3 V | 0.778 | 5.569 | 0.78 | 20 | 4.63 | 17, 24 |
HD 31527 | 5898 | G2 V | 1.074 | 7.49 | 0.96 | 18 | 6.93 | 5, 32 |
HD 40307 | 4827 | K3 V | 0.720 | 7.17 | 0.74 | 8 | 6.25 | 1–8, 10–13, 27–36 |
HD 45184 | 5869 | G1.5 V | 1.080 | 6.38 | 1.03 | 18 | 5.79 | 6, 33 |
HD 51608 | 5358 | G7 V | 0.916 | 8.17 | 0.8 | 18 | 7.46 | 2, 3, 5–9, 12, 13, 29, 32, 33, 35, 36 |
HD 69830 | 5361 | K0 V | 0.850 | 5.96 | 0.9 | 8 | 5.26 | 7, 34 |
HD 7924 | 5177 | K0 V | 0.780 | 7.17 | 0.65 | 14 | 6.39 | 18, 19 |
HIP 54373 | 3848 | K5 | 0.500 | 10.38 | 0.57 | 8 | 8.67 | 9, 36 |
HIP 57274 | 4510 | 0.780 | 8.97 | 0.29 | 8 | 7.90 | 22 | |
YZ Cet | 3056 | M4 V | 0.168 | 12.04 | 0.13 | 21 | 12.29 | 3, 30 |
τ Cet | 5283 | G8.5 | 0.830 | 3.496 | 0.8 | 8 | 2.75 | 3, 30 |
55 Cnc | 5235 | G8 V | 0.930 | 5.95 | 0.96 | 8 | 5.20 | 21 |
References. (1) Vogt et al. (2010); (2) Lo Curto et al. (2013); (3) Hébrard et al. (2010); (4) Staab et al. (2020); (5) Dreizler et al. (2020); (6) (Berta-Thompson et al. 2015); (7) Pinamonti et al. (2018); (8) Turnbull (2015); (9) Astudillo-Defru et al. (2017b); (10) Kemmer et al. (2020); (11) Hawley et al. (1996); (12) Luque et al. (2019); (13) Tuomi et al. (2014); (14) Stassun et al. (2017); (15) Jeffers et al. (2020); (16) Kane & Gelino (2014); (17) Lovis et al. (2011); (18) Udry et al. (2019); (19) Espinoza et al. (2020); (20) Motalebi et al. (2015); (21) Astudillo-Defru et al. (2017a).
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