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Home All issues Volume 693 (January 2025) A&A, 693 (2025) L7 Full HTML
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Table A.1.

Our sample of exoplanets.

# Name Mass [MJup] Radius [RJup] Age [Gyr] Teq [K] Stellar met [dex]
1fm‡ Kepler-75 b 9.9 ± 0.5 1.03 ± 0.06 6 ± 3 850 -0.07 ± 0.15
2fm TOI-2373 b 9.3 ± 0.2 0.93 ± 0.02 5.9 ± 1.7 860 0.3 ± 0.05
3 TOI-2338 b 5.98 ± 0.20 1 ± 0.02 7 ± 2 799 0.22 ± 0.04
4 WASP-162 b 5.2 ± 0.2 1 ± 0.05 * 12 . 97 − 2.35 + 0.83 $ ^{\ast}12.97_{-2.35}^{+0.83} $ 910 0.28 ± 0.13
5‡ Kepler-1704 b 4.16 ± 0.29 1 . 066 − 0.042 + 0.044 $ 1.066_{-0.042}^{+0.044} $ 7 . 4 − 1.0 + 1.5 $ 7.4_{-1.0}^{+1.5} $ 253.8 0.196 ± 0.058
6‡ TOI-2589 b 3.5 ± 0.1 1.08 ± 0.03 11 ± 2 592 0.12 ± 0.04
7 TOI-5153 b 3.26 ± 0.18 1.06 ± 0.04 5.4 ± 1 906 0.12 ± 0.08
8† NGTS-20 b 2.98 ± 0.16 1.07 ± 0.04 4.1 ± 2.7 688 0.15 ± 0.08
9 TOI-2180 b 2.755 ± 0.087 1 . 01 − 0.019 + 0.022 $ 1.01_{-0.019}^{+0.022} $ 8 . 1 − 1.3 + 1.5 $ 8.1_{-1.3}^{+1.5} $ 348 0.253 ± 0.057
10‡ HATS-76 b 2.629 ± 0.089 1.079 ± 0.031 4 . 6 − 4.0 + 8.7 $ 4.6_{-4.0}^{+8.7} $ 939.8 0 . 322 − 0.049 + 0.065 $ 0.322_{-0.049}^{+0.065} $
11‡ TOI-4127 b 2.30 ± 0.11 1 . 096 − 0.032 + 0.039 $ 1.096_{-0.032}^{+0.039} $ 4.8 ± 2.1 605.1 0.14 ± 0.12
12 K2-114 b 2.01 ± 0.12 0.932 ± 0.031 7 . 2 − 4.5 + 4.3 $ 7.2_{-4.5}^{+4.3} $ 701 0.41 ± 0.037
13 TOI-4515 b 2.005 ± 0.052 1.086 ± 0.039 1.2 ± 0.2 705 0.05 ± 0.03
14‡ HAT-P-15 b 1.946 ± 0.066 1.072 ± 0.043 6 . 8 − 1.6 + 2.5 $ 6.8_{-1.6}^{+2.5} $ 904 0.22 ± 0.08
15‡ TIC237913194 b 1.942 ± 0.092 1 . 117 − 0.047 + 0.054 $ 1.117_{-0.047}^{+0.054} $ 5.7 ± 1.7 974 0.14 ± 0.05
16‡ Kepler-117 c 1.84 ± 0.18 1.101 ± 0.035 5.3 ± 1.4 704 -0.04 ± 0.1
17 HATS-74A b 1.46 ± 0.14 1.032 ± 0.021 * 11 − 5.1 + 2.8 $ ^{\ast}11_{-5.1}^{+2.8} $ 895.1 0 . 514 − 0.021 + 0.033 $ 0.514_{-0.021}^{+0.033} $
18 HATS-77 b 1.374 ± 0.1 1.165 ± 0.021 12.1 ± 5 828.3 0.253 ± 0.039
19 HATS-17 b 1.338 ± 0.065 0.777 ± 0.056 2.1 ± 1.3 814 0.3 ± 0.03
20 TOI-5542 b 1.32 ± 0.1 1.009 ± 0.036 10 . 8 − 3.6 + 2.1 $ 10.8_{-3.6}^{+2.1} $ 441 -0.21 ± 0.08
21† TOI-2010 b 1.286 ± 0.057 1.054 ± 0.027 1 . 9 − 1.3 + 2.2 $ 1.9_{-1.3}^{+2.2} $ 400.2 0.168 ± 0.055
22 WASP-130 b 1.23 ± 0.04 0.89 ± 0.03 2 − 1.6 + 5.9 $ 2_{-1.6}^{+5.9} $ 833 0.26 ± 0.1
23 Kepler-87 b 1.02 ± 0.028 1.204 ± 0.049 7.5 ± 0.5 478 -0.17 ± 0.03
24 TOI-1811 b 0.972 ± 0.078 0.994 ± 0.025 5 . 9 − 4.0 + 4.9 $ 5.9_{-4.0}^{+4.9} $ 962.2 0.306 ± 0.077
25 K2-140 b 0.93 ± 0.04 1.21 ± 0.09 9 . 8 − 4.6 + 3.4 $ 9.8_{-4.6}^{+3.4} $ 962 0.1 ± 0.1
26‡ TOI-1478 b 0.851 ± 0.052 1.06 ± 0.04 9 . 1 − 3.9 + 3.1 $ 9.1_{-3.9}^{+3.1} $ 918 0 . 078 − 0.066 + 0.072 $ 0.078_{-0.066}^{+0.072} $
27† K2-290 c 0.774 ± 0.047 1.006 ± 0.05 4 − 0.8 + 1.6 $ 4_{-0.8}^{+1.6} $ 676 -0.06 ± 0.1
28 HAT-P-54 b 0.76 ± 0.032 0.944 ± 0.028 3 . 9 − 2.1 + 4.3 $ 3.9_{-2.1}^{+4.3} $ 818 -0.127 ± 0.08
29† TOI-3714 b 0.689 ± 0.03 0.944 ± 0.02 * 12 . 5 − 6.5 + 1.3 $ ^{\ast}12.5_{-6.5}^{+1.3} $ 764 0.39 ± 0.086
30 WASP-84 b 0.687 ± 0.033 0.976 ± 0.025 2.1 ± 1.6 833 0.09 ± 0.12
31† HAT-P-17 b 0.534 ± 0.018 1.01 ± 0.029 7.8 ± 3.3 792 0 ± 0.08
32 HATS-75 b 0.491 ± 0.039 0.884 ± 0.013 * 13 . 8 − 3.2 + 0.0 $ ^{\ast}13.8_{-3.2}^{+0.0} $ 772.3 0 . 522 − 0.028 + 0.051 $ 0.522_{-0.028}^{+0.051} $
33 TOI-201 b 0.42 ± 0.05 1 . 008 − 0.015 + 0.012 $ 1.008_{-0.015}^{+0.012} $ 0 . 87 − 0.49 + 0.46 $ 0.87_{-0.49}^{+0.46} $ 759 0.24 ± 0.036
34 TOI-5344 b 0.412 ± 0.04 0.946 ± 0.021 * 10 . 9 − 5.8 + 2.9 $ ^{\ast}10.9_{-5.8}^{+2.9} $ 689 0.425 ± 0.088
35 WASP-132 b 0.41 ± 0.03 0.87 ± 0.03 0 . 5 − 0.0 + 2.0 $ 0.5_{-0.0}^{+2.0} $ 763 0.22 ± 0.13
36 HATS-47 b 0 . 369 − 0.021 + 0.031 $ 0.369_{-0.021}^{+0.031} $ 1.117 ± 0.014 8.1 852.9 -0.113 ± 0.035
37 HATS-49 b 0 . 353 − 0.027 + 0.038 $ 0.353_{-0.027}^{+0.038} $ 0.765 ± 0.013 10 . 5 − 2.0 + 1.4 $ 10.5_{-2.0}^{+1.4} $ 834.8 0.208 ± 0.053
38 K2-287 b 0.315 ± 0.027 0.847 ± 0.013 4.7 ± 1.0 804 0.2 ± 0.04
39 TOI-1268 b 0.30331 ± 0.026 0.812 ± 0.054 0.245 ± 0.135 918.9 0.36 ± 0.06
40† TOI-4406 b 0.3 ± 0.03 1 ± 0.02 2.9 ± 0.7 904 0.1 ± 0.05
41† HAT-P-19 b 0.277 ± 0.017 1.008 ± 0.014 7.2 ± 4 981.2 0.166 ± 0.07
42† WASP-69 b 0.26 ± 0.017 1.057 ± 0.047 2 − 1.5 + 1.0 $ 2_{-1.5}^{+1.0} $ 963 0.144 ± 0.077
43 K2-329 b 0.26 ± 0.022 0.774 ± 0.026 1 . 8 − 1.3 + 2.2 $ 1.8_{-1.3}^{+2.2} $ 650 0 . 098 − 0.07 + 0.065 $ 0.098_{-0.07}^{+0.065} $
44 HD332231 b 0.244 ± 0.021 0.867 ± 0.027 4 . 3 − 1.9 + 2.5 $ 4.3_{-1.9}^{+2.5} $ 876 0.036 ± 0.059
45 TOI-3629 b 0.243 ± 0.02 0.74 ± 0.014 * 9 . 8 − 4.8 + 4.0 $ ^{\ast}9.8_{-4.8}^{+4.0} $ 711 0.549 ± 0.093
46 HAT-P-12 b 0.211 ± 0.012 0 . 959 − 0.021 + 0.029 $ 0.959_{-0.021}^{+0.029} $ 2.5 ± 2.0 963 -0.29 ± 0.05
47 WASP-156 b 0.128 ± 0.01 0.51 ± 0.02 6.4 ± 4 970 0.24 ± 0.12
48 HATS-72 b 0.1254 ± 0.004 0.722 ± 0.003 12 . 17 − 0.45 + 0.24 $ 12.17_{-0.45}^{+0.24} $ 739.3 0.099 ± 0.014
49ce TOI-4010 d 0.12003 ± 0.01 0 . 551 − 0.013 + 0.012 $ 0.551_{-0.013}^{+0.012} $ 6.1 ± 3.1 650 0.37 ± 0.07

Notes. ‡ indicates planets for which a model fully made of H–He cannot match the upper bound of the measured radius, for both EOSs. † is similar but when only CMS19+HG23 does not match the upper bound. fm indicates planets for which solutions have been found only with the fully mixed case. ce indicates planets for which solutions have been found only with the core+envelope case. * indicates that the age was adapted so that the upper bound does not exceed the age of the galaxy. Planets shown in bold have not been considered in our analysis since the lower bound of their high measured radius could not be matched even when assuming a zero metallicity (pure H–He).

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