Table B.3
Eccentricity constrained by secondary eclipses.
| Planet | e cos ωα | e sin ωα | e | Ref. occ.b |
|---|---|---|---|---|
| GJ 1214 b | −0.00094 ± 0.00018 | −0.0005 ± 0.0029 | 0.0011 ± 0.0014 | Kem23 |
| GJ 1252 b | −0.0027 ± 0.0058 | −0.012 ± 0.012 | 0.012 ± 0.012 | Cro22 |
| GJ 3470 b | −0.019 ± 0.007 | 0.001 ± 0.178 | 0.019 ± 0.014 | Ben19 |
| HAT-P-20 b | −0.01352 ± 0.00060 | 0.0170 ± 0.0034 | 0.0217 ± 0.0027 | Dem15 |
| TOI-824 b | 0.0001 ± 0.0083 | −0.0003 ± 0.0083 | 0.0003 ± 0.0042 | Roy22 |
| WASP-43 b | −0.049 ± 0.011 | −0.03 ± 0.14 | 0.057 ± 0.076 | Ble14 |
| WASP-80 b | −0.023 ± 0.001 | −0.007 ± 0.014 | 0.024 ± 0.004 | Tri15 |
Notes. (a)Orbital parameters referred to the planet frame (transit at a true anomaly ν = −90°).(b) Ben19: Benneke et al. (2019); Ble14: Blecic et al. (2014); Cro22: Crossfield et al. (2022); Dem15: Deming et al. (2015); Kem23: Kempton et al. (2023); Roy22: Roy et al. (2022); Tri15: Triaud et al. (2015)
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