Table E.1.
Parameters assumed for the planets in the HDO and CH3D detection studies (Sects. 4 and 5).
| Name | T* (K) | R* (R⊙) | TP (K) | RP (R♃) | a (au) | d (pc) |
|---|---|---|---|---|---|---|
| 51 Eri b | 7331a | 1.45a | 760b | 1.1b | 13b | 29.4 |
| HR 8799 cde | 7193 | 1.44 | 1200 | 1.05c | 17-43 | 39.4 |
| GJ 504 b | 5978 | 1.36 | 544 | 0.96 | >27.8f | 17.56 |
| GJ 1214 b-liked | 3250 | 0.22 | 604 | 0.25 | 0.0149 | 7.28d |
| 51 Peg b | 5793 | 1.27 | 1260 | 1.4e | 0.0520 | 14.7 |
Notes. If not otherwise stated, the data shown here have been culled from http://www.openexoplanetcatalogue.com. (a) Rajan et al. (2017). (b) Samland et al. (2017). (c)The radii of HR 8799 cde are a mean value for the three planets, the radii of which vary between 1 and 1.1 R♃. (d) Here we assume a planet and star similar in size and temperature to GJ 1214 b, but twice as close to the Solar System as the GJ 1214 system: for every transiting GJ 1214 b-like planet, one may expect up to 10 non-transiting ones, hence at least one at half the distance of the GJ 1214 system. (e)This planet is non-transiting, hence its true radius is unknown. We assumed 1.4 R♃ here. (f) Bonnefoy et al. (2018).
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