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Table B.4

Results for water-rich rocky planets observed by TESS after 30,000 runs (Monte Carlo method).

Exoplanet Mp Rp S:O Prot a D2 D3 Seff Prob. CMF MMF IMF Roℓ Regime ℳ/ℳ⊕
GJ 143 b 22.884 ±1.186 2.615 ±0.095 1:1 35.613 0.191 0.433 0.823 5.6 1.00 0.11 ±0.02 0.63 ±0.10 0.26 ±0.12 5.18 ±0.47 Multip. 0.04 ± 0.01
HD 108236 b 3.290 ±0.190* 1.615 ±0.029 1:1 3.796 0.045 0.792 1.429 345.3 0.99 0.11 ±0.01 0.65 ±0.06 0.24 ± 0.07 0.48 ± 0.05 Multip. 0.04 ± 0.01
HD 108236 c 5.020 ±0.288* 2.071 ± 0.030 1:1 6.203 0.063 0.780 1.429 179.3 0.99 0.03 ±0.01 0.20 ±0.08 0.77 ± 0.09 0.70 ±0.07 Multip. 0.01 ± 0.002
HD 110113 b 4.630 ±0.346 2.026 ± 0.060 1:1 2.541 0.036 0.881 1.606 690.0 0.76 0.03 ± 0.02 0.20 ±0.11 0.77 ±0.13 0.25 ± 0.03 Multip. 0.02 ±0.003
HD 15337 c 8.522 ±0.903 2.371 ±0.065 1:1 17.178 0.126 0.644 1.201 29.0 0.75 0.03 ± 0.02 0.20 ±0.11 0.77 ±0.13 2.39 ± 0.24 Multip. 0.01 ± 0.002
HD 207897 b 14.396 ± 0.925 2.503 ±0.046 1:1 16.202 0.117 0.573 1.071 26.6 1.00 0.08 ±0.01 0.45 ±0.08 0.47 ± 0.09 2.56 ±0.26 Multip. 0.03 ± 0.01
HD 23472 c 10.315 ±3.781 2.203 ± 0.182 1:1 29.652 0.171 0.469 0.891 8.0 0.59 0.10 ±0.04 0.59 ±0.22 0.31 ± 0.25 5.42 ±0.54 Multip. 0.02 ±0.003
HD 63433 b 5.413 ±0.300* 2.130 ±0.050 1:1 7.108 0.072 0.802 1.470 144.6 0.77 0.03 ± 0.02 0.16 ±0.09 0.81 ±0.11 0.76 ± 0.08 Multip. 0.01 ± 0.002
HD 86226 c 7.285 ± 0.666 2.160 ±0.046 1:1 3.984 0.049 0.986 1.798 480.4 1.00 0.07 ± 0.02 0.39 ±0.11 0.54 ±0.13 0.50 ±0.05 Multip. 0.04 ± 0.01
HIP 97166 b 19.996 ±0.868 2.740 ±0.075 1:1 10.289 0.089 0.644 1.199 58.6 1.00 0.07 ± 0.02 0.40 ±0.10 0.53 ±0.12 1.42 ± 0.14 Multip. 0.05 ± 0.01
HR 858 b 5.094 ±0.286* 2.085 ± 0.037 3:2 2.391 0.048 1.350 2.440 1037 0.95 0.03 ±0.01 0.18 ±0.08 0.79 ±0.10 0.23 ± 0.02 Multip. 0.02 ±0.003
HR 858 c 4.484 ±0.259* 1.939 ± 0.040 1:1 5.973 0.067 1.354 2.440 510.3 1.00 0.06 ± 0.02 0.33 ±0.09 0.61 ±0.10 0.75 ± 0.08 Multip. 0.02 ±0.003
HR 858 d 5.482 ±0.298* 2.149 ± 0.043 3:2 7.487 0.103 1.348 2.440 224.9 0.76 0.02 ±0.01 0.14 ±0.08 0.84 ±0.09 0.76 ± 0.08 Multip. 0.01 ± 0.002
L 98-59 b 0.371 ± 0.076 0.864 ±0.030 1:1 2.253 0.022 0.115 0.215 24.4 0.74 0.12 ±0.02 0.68 ±0.15 0.20 ±0.17 0.20 ±0.02 Multip. 0.01 ± 0.002
L 98-59 c 2.204 ±0.144 1.407 ± 0.044 1:1 3.691 0.030 0.109 0.215 12.6 0.85 0.12 ±0.01 0.72 ± 0.07 0.16 ±0.08 0.44 ± 0.04 Multip. 0.03 ± 0.01
L 98-59 d 1.942 ±0.161 1.531 ±0.062 1:1 7.451 0.048 0.110 0.215 4.9 0.99 0.06 ± 0.03 0.38 ±0.16 0.56 ±0.18 1.10 ±0.11 Multip. 0.01 ± 0.002
LTT 1445A b 1.835 ±0.588 1.399 ±0.071 3:2 3.573 0.038 0.097 0.190 6.4 0.42 0.10 ±0.04 0.61 ± 0.23 0.29 ± 0.26 0.52 ±0.05 Multip. 0.02 ±0.003
LTT 3780 c 8.787 ±0.822 2.302 ±0.088 1:1 12.252 0.077 0.123 0.250 2.6 0.97 0.06 ± 0.03 0.33 ±0.15 0.61 ±0.18 1.83 ±0.18 Multip. 0.02 ±0.003
TOI-1062 b 10.139 ± 0.478 2.268 ± 0.054 1:1 4.113 0.049 0.672 1.245 214.9 1.00 0.08 ±0.01 0.49 ± 0.08 0.43 ± 0.09 0.50 ±0.05 Multip. 0.08 ± 0.01
TOI-1260 b 8.618 ±0.813 2.346 ± 0.056 1:1 3.127 0.036 0.343 0.665 91.1 0.95 0.04 ± 0.02 0.25 ±0.12 0.71 ±0.13 0.35 ± 0.05 Multip. 0.04 ± 0.01
TOI-1266 b 14.874 ±4.645 2.397 ± 0.079 1:1 10.895 0.074 0.163 0.326 4.9 0.74 0.10 ±0.04 0.60 ±0.22 0.31 ± 0.26 1.61 ± 0.16 Multip. 0.06 ± 0.01
TOI-1266 c 2.695 ±0.756 1.575 ± 0.078 1:1 18.801 0.106 0.167 0.326 2.4 0.65 0.10 ±0.04 0.57 ±022 0.33 ± 0.26 3.03 ± 0.30 Multip. 0.01 ± 0.002
TOI-1634 b 4.899 ±0.397 1.790 ± 0.046 1:1 0.989 0.015 0.170 0.341 122.9 1.00 0.11 ±0.01 0.65 ±0.09 0.24 ± 0.10 0.10 ±0.01 Dipolar 2.54 ±0.51
TOI-1685 b 3.782 ±0.364 1.700 ±0.041 1:1 0.669 0.012 0.175 0.349 214.9 1.00 0.10 ±0.02 0.61 ±0.10 0.29 ±0.11 0.06 ± 0.003 Dipolar 1.67 ±0.33
TOI-1749 b 2.536 ±0.146* 1.492 ± 0.064 1:1 2.388 0.029 0.265 0.509 81.3 0.53 0.11 ±0.02 0.67 ± 0.10 0.22 ±0.12 0.28 ± 0.03 Multip. 0.04 ± 0.01
TOI-1749 d 15.00 ±0.00 2.520 ±0.086 1:1 9.051 0.071 0.259 0.509 13.7 1.00 0.08 ±0.02 0.46 ±0.11 0.46 ± 0.13 1.29 ±0.13 Multip. 0.05 ± 0.01
TOI-178 c 4.634 ±0.348 1.703 ±0.050 1:1 3.238 0.037 0.358 0.689 95.5 0.73 0.12 ±0.01 0.74 ± 0.07 0.14 ±0.08 0.41 ± 0.04 Multip. 0.07 ± 0.01
TOI-1807 b 4.138 ±0.239* 1.849 ±0.025 1:1 0.549 0.012 0.450 0.845 1486 1.00 0.07 ± 0.01 0.42 ±0.06 0.51 ±0.08 0.05 ± 0.01 Dipolar 1.20 ± 0.24
TOI-2257 b 5.614 ±0.308* 2.159 ±0.048 5:2 14.076 0.145 0.109 0.221 0.68 0.64 0.02 ±0.01 0.15 ± 0.09 0.83 ±0.10 1.60 ±0.40 Multip. 0.01 ± 0.002
TOI-237 b 2.686 ±0.156* 1.483 ± 0.046 1:1 5.436 0.034 0.066 0.133 3.6 0.62 0.12 ±0.01 0.72 ± 0.07 0.16 ±0.08 0.71 ± 0.07 Multip. 0.03 ± 0.01
TOI-431 c 2.831 ±0.215 1.526 ±0.060 1:1 4.849 0.052 0.505 0.935 99.5 0.66 0.12 ±0.02 0.69 ±0.10 0.19 ±0.11 0.64 ± 0.06 Multip. 0.03 ± 0.01
TOI-451 b 4.374 ± 0.252* 1.910 ±0.070 1:1 1.859 0.029 0.759 1.388 778.9 1.00 0.06 ± 0.02 0.36 ±0.14 0.58 ±0.16 0.19 ±0.02 Multip. 0.04 ± 0.01
TOI-561 b 1.590 ±0.208 1.423 ±0.038 1:1 0.447 0.011 0.732 1.309 5167 1.00 0.07 ± 0.03 0.44 ±0.15 0.49 ±0.17 0.04 ± 0.002 Dipolar 0.41 ± 0.08
TOI-561 d 11.962 ±0.735 2.529 ± 0.075 1:1 25.620 0.157 0.710 1.309 23.4 0.99 0.05 ±0.02 0.27 ±0.12 0.68 ±0.14 4.44 ± 0.44 Multip. 0.01 ± 0.002
TOI-561 e 16.003 ± 1.327 2.670 ±0.064 1:1 77.229 0.328 0.710 1.309 5.4 1.00 0.05 ±0.02 0.31 ±0.11 0.64 ±0.13 15.27 ±1.53 Multip. 0.01 ± 0.002
TOI-763 b 9.793 ±0.452 2.280 ± 0.064 1:1 5.606 0.060 0.748 1.380 177.8 1.00 0.08 ±0.02 0.45 ±0.10 0.47 ±0.11 0.79 ± 0.08 Multip. 0.05 ± 0.01
TOI-776 b 4.021 ±0.511 1.847 ±0.074 1:1 8.247 0.065 0.224 0.442 11.7 0.97 0.07 ± 0.03 0.40 ±0.17 0.53 ±0.20 1.12 + 0.11 Multip. 0.01 ± 0.002
TOI-776 c 5.489 ±0.966 2.008 ± 0.078 1:1 15.665 0.100 0.222 0.442 5.0 0.88 0.07 ± 0.03 0.39 ±0.18 0.54 ±0.21 2.40 ±0.24 Multip. 0.01 ± 0.002
TOI-824 b 18.608 ± 1.062 2.865 ±0.078 1:1 1.393 0.022 0.427 0.813 405.1 0.65 0.03 ± 0.02 0.18 ±0.10 0.79 ±0.12 0.12 ±0.01 Dipolar 1.68 ±0.34
TOI-849 b 39.409 ± 1.473 3.406 ±0.047 1:1 0.766 0.016 0.751 1.389 2503 0.55 0.02 ±0.01 0.09 ± 0.05 0.89 ±0.06 0.04 ± 0.01 Dipolar 1.29 ±0.52
pi Men c 4.855 ±0.471 2.040 ±0.028 1:1 6.268 0.068 1.087 1.968 307.3 0.94 0.04 ± 0.02 0.22 ±0.10 0.74 ±0.12 0.73 ± 0.07 Multip. 0.01 ± 0.002

Notes. Mp is the planetary mass normalized to the Earth mass. Those values highlighted with an asterisk have been estimated following (Chen & Kipping 2017). Rp is the planetary radius normalized to the Earth radius. S:O shows the Spin:Orbit resonance. Prot is the planetary rotational period in days, a, D2 and D3 are respectively are the semi-major axis, inner and outer boundaries of the HZ expressed in A.U. Seff is normalized mean effective flux considering orbital eccentricity. Prob. It is the probability of being water-rich rocky planet. All the planets are tidally locked. Errors in the rotational period have not been included because they are so small that they have no impact on the magnetic properties of exoplanets.

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