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Table 5
Results of the MC analysis performed on the RVs extracted with the DRS and TERRA recipes using a sum of three sinusoids to model the stellar activity component.
Jump parameter | Prior | Best-fit value | |
---|---|---|---|
DRS | TERRA | ||
γ (m s−1) | ![]() |
13643.6![]() |
−0.09![]() |
![]() |
|||
σjit (m s−1) | ![]() |
6.4![]() |
6.8![]() |
Stellar activity signal | |||
Prot (days) | ![]() |
16.65 ± 0.02 | 16.68 ± 0.02 |
Prot/2 (days) | ![]() |
8.499![]() |
8.507 ± 0.005 |
Prot/3 (days) | ![]() |
5.754 ± 0.003 | 5.755![]() |
![]() |
![]() |
7.8 ± 1.2 | 7.9 ± 1.2 |
![]() |
![]() |
7811.5 ± 0,4 | 7811.9![]() |
![]() |
![]() |
14.6 ± 1.1 | 14.5 ± 1.1 |
![]() |
![]() |
7809.4 ± 0.2 | 7809.1 ± 0.2 |
![]() |
![]() |
7.4 ± 1.4 | 6.7 ± 1.3 |
![]() |
![]() |
7802.9 ± 0.2 | 7802.8![]() |
Planetary signals | |||
Kb (m s−1) | ![]() |
2.8 ± 1.3 | 2.4 ± 1.2 |
Kc (m s−1) | ![]() |
5.0 ± 1.4 | 4.9 ± 1.4 |
mb (M⊕) | derived | 4.2 ± 1.8 | 3.7![]() |
mc (M⊕) | derived | 11.7![]() |
11.5 ± 3.2 |
Bayesian evidence ln(![]() |
−310.5 ± 0.06 | −310.14 ± 0.04 |
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