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Home All issues Volume 706 (February 2026) A&A, 706 (2026) A50 Full HTML
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Table A.1

Exoplanet data used in this study.

Planet M (MJ) R (RJ) Age (Myr) Zst T (K) ZCE ZFM
TOI-4010d 0.12 ± 0.01 0.551 ± 0.013 3000–9200 0.036 ± 0.07 650 0.724 ± 0.011 0.672 ± 0.026
HATS-72b 0.125 ± 0.004 0.722 ± 0.003 11710–12410 0.019 ± 0.014 739 0.4 ± 0.008 0.423 ± 0.004
WASP-156b 0.128 ± 0.01 0.51 ± 0.02 2400–10400 0.027 ± 0.12 970 0.736 ± 0.01 0.767 ± 0.045
HAT-P-12b* 0.211 ± 0.057 0.959 ± 0.025 500–4500 0.008 ± 0.05 963 0.129 ± 0.05 0.294 ± 0.073
TOI-3629b* 0.243 ± 0.082 0.74 ± 0.014 5000–13800 0.055 ± 0.093 711 0.397 ± 0.026 0.427 ± 0.025
HD332231b* 0.244 ± 0.086 0.867 ± 0.027 2400–6800 0.017 ± 0.059 876 0.222 ± 0.048 0.311 ± 0.045
K2-329b 0.26 ± 0.022 0.774 ± 0.026 500–4000 0.019 ± 0.068 650 0.318 ± 0.024 0.45 ± 0.044
WASP-69b 0.26 ± 0.017 1.057 ± 0.047 500–3000 0.021 ± 0.077 963 0.06 ± 0.044 0.199 ± 0.057
HAT-P-19b* 0.277 ± 0.06 1.008 ± 0.014 3200–11200 0.023 ± 0.07 981 0.021 ± 0.014 0.112 ± 0.025
TOI-4406b* 0.3 ± 0.1 1.0 ± 0.02 2200–3600 0.019 ± 0.05 904 0.044 ± 0.025 0.152 ± 0.034
TOI-1268b 0.303 ± 0.026 0.812 ± 0.054 110–380 0.035 ± 0.06 919 0.311 ± 0.029 0.511 ± 0.026
K2-287b* 0.315 ± 0.086 0.847 ± 0.013 3700–5700 0.024 ± 0.04 804 0.255 ± 0.024 0.328 ± 0.02
HATS-49b* 0.353 ± 0.092 0.765 ± 0.013 8500–11900 0.025 ± 0.053 835 0.392 ± 0.025 0.416 ± 0.018
WASP-132b 0.41 ± 0.03 0.87 ± 0.03 500–2500 0.026 ± 0.13 763 0.268 ± 0.046 0.376 ± 0.044
TOI-5344b* 0.412 ± 0.097 0.946 ± 0.021 5100–13800 0.041 ± 0.088 689 0.067 ± 0.035 0.134 ± 0.04
TOI-201b* 0.42 ± 0.095 1.008 ± 0.014 380–1330 0.027 ± 0.036 759 0.086 ± 0.03 0.209 ± 0.037
HATS-75b* 0.491 ± 0.079 0.884 ± 0.013 10600–13800 0.051 ± 0.4 772 0.188 ± 0.025 0.288 ± 0.019
HAT-P-17b* 0.534 ± 0.034 1.01 ± 0.029 4500–11100 0.015 ± 0.08 792 0.04 ± 0.029 0.108 ± 0.039
WASP-84b* 0.687 ± 0.048 0.976 ± 0.025 500–3700 0.019 ± 0.12 833 0.142 ± 0.047 0.222 ± 0.064
TOI-3714b* 0.689 ± 0.044 0.944 ± 0.02 6000–13800 0.038 ± 0.086 764 0.124 ± 0.035 0.155 ± 0.051
HAT-P-54b* 0.76 ± 0.042 0.944 ± 0.028 1800–8200 0.011 ± 0.08 818 0.168 ± 0.05 0.217 ± 0.054
K2-290c 0.774 ± 0.047 1.006 ± 0.05 3200–5600 0.013 ± 0.1 676 0.093 ± 0.06 0.159 ± 0.063
TOI-1478b 0.851 ± 0.052 1.06 ± 0.04 5200–12200 0.018 ± 0.069 918 0.048 ± 0.034 0.111 ± 0.051
K2-140b 0.93 ± 0.04 1.21 ± 0.09 5300–13200 0.019 ± 0.1 962 0.058 ± 0.045 0.112 ± 0.06
TOI-1811b* 0.972 ± 0.079 0.994 ± 0.025 1900–10800 0.031 ± 77.0 962 0.112 ± 0.044 0.194 ± 0.049
WASP-130b 1.23 ± 0.04 0.89 ± 0.03 400–7900 0.028 ± 0.1 833 0.291 ± 0.039 0.362 ± 0.052
TOI-2010b* 1.286 ± 0.044 1.054 ± 0.027 600–4200 0.023 ± 0.055 400 0.096 ± 0.064 0.144 ± 0.067
TOI-5542b 1.32 ± 0.1 1.009 ± 0.036 7200–12900 0.009 ± 0.08 441 0.087 ± 0.068 0.135 ± 0.08
HATS-17b 1.338 ± 0.065 0.777 ± 0.056 800–3400 0.031 ± 0.03 814 0.318 ± 0.025 0.482 ± 0.047
HATS-74Ab* 1.46 ± 0.096 1.032 ± 0.021 5900–13800 0.05 ± 0.027 895 0.063 ± 0.031 0.172 ± 0.034
Kepler-117c 1.84 ± 0.18 1.101 ± 0.035 3900–6700 0.014 ± 0.1 704 0.035 ± 0.028 0.082 ± 0.04
TIC237913194b 1.942 ± 0.092 1.117 ± 0.051 4000–7400 0.021 ± 0.05 974 0.056 ± 0.045 0.105 ± 0.051
HAT-P-15b 1.946 ± 0.066 1.072 ± 0.043 5200–9300 0.026 ± 0.08 904 0.066 ± 0.05 0.115 ± 0.053
TOI-4515b 2.005 ± 0.052 1.086 ± 0.039 1000–1400 0.017 ± 0.03 705 0.067 ± 0.057 0.153 ± 0.058
K2-114b 2.1 ± 0.12 0.932 ± 0.031 2700–11700 0.04 ± 0.037 701 0.256 ± 0.052 0.285 ± 0.045
TOI-4127b 2.3 ± 0.11 1.096 ± 0.036 2700–6900 0.021 ± 0.12 605 0.044 ± 0.036 0.091 ± 0.043
HATS-76b* 2.629 ± 0.034 1.079 ± 0.031 600–13300 0.032 ± 0.057 940 0.066 ± 0.044 0.116 ± 0.053
TOI-2180b* 2.755 ± 0.03 1.01 ± 0.021 6800–9600 0.028 ± 0.057 348 0.132 ± 0.036 0.163 ± 0.043
NGTS-20b 2.98 ± 0.16 1.07 ± 0.04 1400–6800 0.022 ± 0.08 688 0.079 ± 0.059 0.137 ± 0.103
TOI-5153b* 3.26 ± 0.05 1.06 ± 0.04 4400–6400 0.02 ± 0.08 906 0.103 ± 0.063 0.155 ± 0.044
TOI-2589b* 3.5 ± 0.029 1.08 ± 0.03 9000–13000 0.02 ± 0.04 582 0.047 ± 0.035 0.069 ± 0.038
WASP-162b 5.2 ± 0.2 1.0 ± 0.05 10620–13800 0.029 ± 0.13 910 0.186 ± 0.094 0.187 ± 0.048
TOI-2338b 5.98 ± 0.2 1.0 ± 0.02 5000–9000 0.026 ± 0.04 799 0.149 ± 0.055 0.182 ± 0.014

Notes. Planetary parameters are taken from Howard et al. (2025b) and are available on dace.unige.ch. In addition to the planetary parameters, the retrieved bulk metallicity means and standard deviation for the CE and FM are reported on the rightmost columns. Planet names with the asterisk (*) are making up the initial 21 planets that have been tested with tighter constraints on the radius uncertainties (smaller than 3% [σR < 3%] instead of 5% used for the full dataset.

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