Open Access
Table A.1
Parameters of the 48 host stars.
| Hostname | [Si/H] | Ref. | [Mg/H] | Ref. | [Fe/H] | Ref. | Festar% |
|---|---|---|---|---|---|---|---|
| EPIC 220674823 | 0.05 ± 0.03 | (1) | 0.07 ± 0.05 | (1) | 0.1 ± 0.03 | (1) | 0.3535 ± 0.0217 |
| EPIC 249893012 | 0.17 ± 0.03 | (1) | 0.21 ± 0.05 | (1) | 0.15 ± 0.02 | (1) | 0.3129 ± 0.0172 |
| GJ 1132 | −0.12 ± 0.15 | Berta-Thompson et al. (2015) | |||||
| GJ 1252 | 0.1 ± 0.1 | Shporer et al. (2020) | |||||
| GJ 3473 | 0.11 ± 0.19 | Kemmer et al. (2020) | |||||
| GJ 357 | −0.12 ± 0.16 | Luque et al. (2019) | |||||
| GJ 367 | −0.01 ± 0.12 | Lam et al. (2021) | |||||
| GJ 486 | 0.07 0.16 | Trifonov et al. (2021) | |||||
| GJ 9827 | −0.28 ± 0.12 | Dai et al. (2019) | |||||
| HD 136352 | −0.17 ± 0.029 | (2) | −0.05 ± 0.104 | (2) | −0.26 ± 0.083 | (2) | 0.2612 ± 0.0445 |
| HD 137496 | −0.03 ± 0.04 | Azevedo Silva et al. (2022) | |||||
| HD 15337 | 0.06 ± 0.05 | (1) | 0.09 0.04 | (1) | 0.03 0.03 | (1) | 0.3103 ± 0.0218 |
| HD 213885 | −0.01 ± 0.03 | (1) | −0.01 ± 0.04 | (1) | 0.0 ± 0.01 | (1) | 0.3374 ± 0.0136 |
| HD 219134 | 0.0 0.06 | (1) | 0.03 0.06 | (1) | 0.03 0.03 | (1) | 0.3238 ± 0.0263 |
| HD 3167 | 0.03 ± 0.04 | (1) | 0.1 ± 0.04 | (1) | 0.04 ± 0.02 | (1) | 0.3206 ± 0.0174 |
| K2-131 | −0.02 ± 0.08 | Dai et al. (2019) | |||||
| K2-141 | −0.03 ± 0.12 | (1) | −0.16 ± 0.11 | (1) | −0.06 ± 0.05 | (1) | 0.3447 ± 0.0514 |
| K2-216 | −0.15 ± 0.16 | (1) | −0.23 ± 0.15 | (1) | −0.15 ±0.09 | (1) | 0.35 ± 0.0756 |
| K2-229 | −0.06 ± 0.05 | (1) | −0.07 ± 0.03 | (1) | −0.06 ± 0.02 | (1) | 0.3346 ± 0.0188 |
| K2-265 | 0.05 ± 0.04 | (1) | 0.11 ± 0.03 | (1) | 0.09 ± 0.02 | (1) | 0.3383 ± 0.0166 |
| K2-291 | 0.04 ± 0.04 | (1) | 0.1 ± 0.03 | (1) | 0.09 ± 0.02 | (1) | 0.3435 ± 0.0167 |
| K2-36 | 0.05 ± 0.025 | (3) | −0.03 ± 0.025 | (3) | 0.0 ± 0.025 | (3) | 0.3243 ± 0.0155 |
| KOI-1599 | 0.06 ± 0.2 | Mullally et al. (2015) | |||||
| Kepler-10 | −0.1 ± 0.03 | (1) | −0.01 ± 0.03 | (1) | −0.14 ± 0.01 | (1) | 0.2913 ± 0.0111 |
| Kepler-105 | −0.06 ± 0.025 | (4) | −0.09 ± 0.025 | (4) | −0.11 ± 0.025 | (4) | 0.3138 ± 0.0152 |
| Kepler-107 | 0.37 ± 0.04 | (1) | 0.41 ± 0.11 | (1) | 0.42 ± 0.03 | (1) | 0.3485 ± 0.0334 |
| Kepler-138 | −0.28 ± 0.099 | Jontof-Hutter et al. (2015) | |||||
| Kepler-20 | 0.06 ± 0.03 | (1) | 0.07 ± 0.04 | (1) | 0.05 ± 0.03 | (1) | 0.3249 ± 0.0196 |
| Kepler-36 | −0.15 ± 0.025 | (3) | −0.17 ± 0.025 | (3) | −0.16 ± 0.025 | (3) | 0.3317 ± 0.0157 |
| Kepler-406 | 0.25 ± 0.04 | (1) | 0.23 ± 0.05 | (1) | 0.24 ± 0.02 | (1) | 0.3317 ± 0.019 |
| Kepler-65 | 0.17 ± 0.025 | (3) | 0.11 ± 0.025 | (3) | 0.19 ± 0.025 | (3) | 0.3562 ± 0.0162 |
| Kepler-78 | −0.09 ± 0.07 | (1) | −0.15 ± 0.1 | (1) | −0.14 ± 0.04 | (1) | 0.3202 ± 0.0355 |
| Kepler-80 | 0.04 ± 0.08 | MacDonald et al. (2016) | |||||
| Kepler-93 | −0.16 ± 0.02 | (1) | −0.14 ± 0.04 | (1) | −0.14 ± 0.01 | (1) | 0.3378 ± 0.0122 |
| Kepler-99 | 0.27 ± 0.025 | (3) | 0.23 ± 0.025 | (3) | 0.27 ± 0.025 | (3) | 0.3413 ± 0.0159 |
| L168-9 | 0.04 ± 0.17 | Astudillo-Defru et al. (2020) | |||||
| L 98-59 | −0.46 ± 0.26 | Demangeon et al. (2021) | |||||
| LHS 1140 | −0.24 ± 0.1 | Ment et al. (2019) | |||||
| LHS 1478 | −0.13 ± 0.19 | Soto et al. (2021) | |||||
| LTT 3780 | 0.09 ± 0.16 | Nowak et al. (2020) | |||||
| TOI-1235 | 0.33 ± 0.16 | Bluhm et al. (2020) | |||||
| TOI-1444 | 0.13 ± 0.06 | Dai et al. (2021) | |||||
| TOI-178 | −0.23 ± 0.05 | Leleu et al. (2021) | |||||
| TOI-270 | −0.2 ± 0.12 | Van Eylen et al. (2021) | |||||
| TOI-431 | 0.053 ± 0.111 | (5) | 0.02 ± 0.137 | (5) | 0.02 ± 0.08 | Sousa et al. (2011) | 0.3229 ± 0.0593 |
| TRAPPIST-1 | 0.04 ± 0.08 | Gillon et al. (2017b) | |||||
| Kepler-30 | 0.21 ± 0.11 | Rowe et al. (2015) | |||||
| WASP-47 | 0.43 ± 0.05 | (1) | 0.46 ± 0.06 | (1) | 0.4 ± 0.04 | (1) | 0.3103 ± 0.0274 |
References. (1) Adibekyan et al. (2021); (2) Soto & Jenkins (2018); (3) Brewer et al. (2016); (4) Brewer & Fischer (2018); (5) Adibekyan et al. (2012)
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