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Table A.6
Estimates of planetary masses, densities, and RV semi-amplitudes according to our atmospheric evolution modelling framework and system parameters.
| Parameters | This work | D20 | |
|---|---|---|---|
| HD 108236 b | Mp [M⊕] |  |
5 ± 2 |
| ρp [ρ⊕] | 1.00 ± 0.10 | 1.25 ± 0.40 | |
| K [m s−1] | 1.91 ± 0.19 | ||
| HD 108236 c | Mp [M⊕] |  |
7 ± 2 |
| ρp [ρ⊕] | 1.00 ± 0.08 | 0.79 ± 0.29 | |
| K [m s−1] | 3.41 ± 0.28 | ||
| HD 108236 d | Mp [M⊕] |  |
10 ± 2 |
| ρp [ρ⊕] |  |
0.50 ± 0.20 | |
| K [m s−1] | 2.25 ± 0.24 | ||
| HD 108236 e | Mp [M⊕] |  |
13 ± 2 |
| ρp [ρ⊕] |  |
0.43 ± 0.16 | |
| K [m s−1] | 2.14 ± 0.66 | ||
| HD 108236 f | Mp [M⊕] |  |
not discovered |
| ρp [ρ⊕] |  |
||
| K [m s−1] | 0.90 ± 0.10 | ||
Notes. Planetary masses and density values are compared with the predictions reported by D20, who used the probabilistic mass-radius relation of Chen & Kipping (2017).
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