Table 6
Mass estimations of the planets of HD 108236.
| This work | Literature | ||||||
|---|---|---|---|---|---|---|---|
| CK17 | RVs | T21(a) (RVs) | B21(b) | D21(c) (CK17) | |||
| Planet | Mass [M⊕] | K [m s−1] | Mass [M⊕] | Density [gr cm−3 ] | Mass [M⊕] | ||
| b |  |
 |
 |
5.0 ± 2.0 | 4.33 ± 1.54 | 4.23 ± 0.40 | 5 ± 2 |
| c |  |
 |
 |
3.0 ± 1.0 | 3.97 ± 1.77 | 8.90 ± 0.66 | 7 ± 2 |
| d |  |
 |
 |
0.5 ± 0.5 | <7.75 | 7.75 ± 0.80 | 10 ± 2 |
| e |  |
 |
 |
3.0 ± 1.0 | 19.10 ± 3.91 |  |
13 ± 2 |
| f |  |
 |
 |
15.0 ± 6.0 | 10.85 ± 5.55 | 3.95 ± 0.4 | – |
Notes. The masses from the radial velocities (RVs) and from the probabilistic method based on the M-R relations of Chen & Kipping (2017; CK17) (Sect. 7.1) are shown. The fitted RV semi-amplitudes, K, and the derived planet densities are also shown. We recall in the last 3 columns the values from the literature: (a)Teske et al. (2021),(b)Bonfanti et al. (2021), and (c)Daylan et al. (2021).
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