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Table 3

Best-fit values obtained for the star-planet model when using the full dataset of RVs, and the data corresponding to the different seasons analysed in this work.

Parameter Full dataset Season 1 Season 2 Season 3 Full dataset (QPC) kernel
Pb (d)
           
T0,b (d)
           
Kb (m s−1)
           
eb
           
ωb (deg)

Notes. The best-fit values obtained using the full dataset of RVs and the QPC kernel are also given. Parameters e and ω were derived from the posterior distribution of and .

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