Table B.1
Properties and results of the interior structure modeling for the planets in our sample.
| Planet | Period [d] | Rp [R⊕] | Mp [M⊕] | Age [Gyr] | Teq [K] | fenv, low Fe/H | fenv, medium Fe/H | fenv, high Fe/H | References |
|---|---|---|---|---|---|---|---|---|---|
| EPIC 211945201 b | 19.49213 | 6.12 ± 0.1 | ![]() |
![]() |
882 ± 15 | 0.21 ± 0.02 | ![]() |
0.38 ± 0.03 | 1 |
| K2-24 b | 20.88257 | 5.64 ± 0.07 | ![]() |
![]() |
769 ± 37 | 0.2 ± 0.01 | 0.27 ± 0.03 | 0.34 ± 0.02 | 2 |
| K2-24 c | 42.3773 | ![]() |
![]() |
![]() |
607 ± 30 | 0.48 ± 0.03 | 0.59+0.07 | ![]() |
2 |
| K2-280 b | 19.89526 | 7.5 ± 0.5 | 37 ± 6 | ![]() |
788 ± 26 | 0.46 ± 0.07 | ![]() |
0.74 ± 0.1 | 3 |
| KOI-1783.01 | 134.4629 | ![]() |
![]() |
3.4 ± 0.7 | 421 ± 7 | 0.72 ± 0.05 | ![]() |
![]() |
4 |
| KOI-1783.02 | 284.2162 | ![]() |
![]() |
3.4 ± 0.7 | 328 ± 6 | ![]() |
![]() |
![]() |
4 |
| KOI-94 e | 54.3261 | ![]() |
19 ± 3 | ![]() |
654 ± 30 | 0.2 ± 0.02 | ![]() |
0.39 ± 0.04 | 4 |
| Kepler-103 c | 179.60978 | 5.45 ± 0.18 | 58 ± 12 | ![]() |
437 ± 5 | 0.15 ± 0.03 | ![]() |
0.27 ± 0.05 | 5 |
| Kepler-111 c | 224.77833 | 7.08 ± 0.33 | ![]() |
|
352 ± 9 | ![]() |
|
|
6 |
| Kepler-117 b | 18.7959228 | 8.1 ± 0.3 | 30 ± 11 | ![]() |
990 ± 30 | 0.46 ± 0.05 | ![]() |
![]() |
7 |
| Kepler-1513 b | 160.8842 | ![]() |
![]() |
4.1 ± 1.9 | 343 ± 16 | ![]() |
![]() |
0.98 ± 0.02 | 8 |
| Kepler-450 b | 28.4548844 | 6.083 ± 0.003 | ![]() |
![]() |
863 ± 35 | 0.21 ± 0.01 | ![]() |
![]() |
9 |
| Kepler-849 b | 394.62508 | 8.1 ± 0.4 | 299 ± 70 | ![]() |
363 ± 12 | 0.46 ± 0.07 | ![]() |
![]() |
6 |
| Kepler-9 b | 19.23891 |
|
![]() |
![]() |
724 ± 11 |
|
0.69 ± 0.1 | ![]() |
10 |
| Kepler-9 c | 38.9853 | ![]() |
![]() |
![]() |
572 ± 9 | ![]() |
![]() |
![]() |
10 |
| TIC 139270665 b | 23.624 | 9.8 ± 0.5 | 164 ± 17 | 3.8 ± 0.5 | 834 ± 22 | 0.32 ± 0.04 | ![]() |
![]() |
11 |
| TOI-1386 b | 25.83839 | ![]() |
47.0 ± 6.3 | ![]() |
676 ± 14 | 0.22 ± 0.03 | ![]() |
![]() |
12 |
| TOI-1439 b | 27.644 | ![]() |
![]() |
![]() |
819 ± 13 | ![]() |
0.03 ± 0.02 | 0.06 ± 0.03 | 13 |
| TOI-1836 b | 20.38085 | 8.38 ± 0.19 | 28.4 ± 4.3 | ![]() |
999 ± 21 | 0.53 ± 0.04 | ![]() |
![]() |
14 |
| TOI-2019 b | 15.3444 | 5.66 ± 0.28 | 34.6 ± 4.2 | ![]() |
989 ± 29 | 0.16 ± 0.03 | ![]() |
![]() |
14 |
| TOI-2134 c | 95.5 | 7.27 ± 0.42 | 42 ± 8 | ![]() |
308 ± 7 | ![]() |
![]() |
![]() |
15 |
| TOI-2525 b | 23.2856 | 8.67 ± 0.12 | 27 ± 2 | ![]() |
560 ± 16 | 0.67 ± 0.03 | ![]() |
![]() |
16 |
| TOI-4994 b | 21.491984 | ![]() |
89 ± 13 | ![]() |
718 ± 21 | 0.63 ± 0.06 | ![]() |
![]() |
17 |
| TOI-5678 b | 47.73022 | 4.91 ± 0.08 | 20.0 ± 4.0 | ![]() |
513 ± 7 | 0.13 ± 0.01 | 0.16 ± 0.02 | 0.23 ± 0.02 | 18 |
| HD 332231 b | 18.71204 | ![]() |
77.6 ± 6.7 | 3.0 ± 0.5 | 876 ± 22 | ![]() |
0.89 ± 0.07 | ![]() |
19 |
| PH2 b | 282.5254 | 9.49 ± 0.16 | ![]() |
5.0 ± 1.5 | 295 ± 5 | ![]() |
![]() |
![]() |
5 |
| TOI-1898 b | 45.522149 | 9.74 ± 0.22 | 127.5 ± 6.6 | 3.5+0.3−1.1 | 741 ± 13 | 0.77 ± 0.04 | ![]() |
![]() |
14 |
| TOI-2328 b | 17.10197 | 9.97 ± 0.45 | 51.0 ± 6.4 | ![]() |
707 ± 31 | 0.87 ± 0.08 | ![]() |
![]() |
20 |
References: 1 Chakraborty et al. (2018); 2 Nascimbeni et al. (2024); 3 Nowak et al. (2020); 4 Jontof-Hutter et al. (2022); 5 Dubber et al. (2019); 6 Dalba et al. (2024); 7 Bruno et al. (2015); 8 Yahalomi et al. (2024); 9 Yoffe et al. (2021); 10 Borsato et al. (2019); 11 (Dalba & Peluso, private communication); 12 Hill et al. (2024); 13 Polanski et al. (2024); 14 Chontos et al. (2024); 15 Rescigno et al. (2024); 16 Trifonov et al. (2023); 17 Rodríguez Martínez et al. (2025); 18 Ulmer-Moll et al. (2023); 19 Dalba et al. (2020); 20 Tala Pinto et al. (2025).
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