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Fig. E.3

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Prior and posterior distributions of the period and semi-amplitude from the global analysis of FWHM and RV measurements of the blind search of the candidate planet system using ESPRESSO data. We use a normal prior on orbital period N$\[\mathcal{N}\]$(3.15, 0.3) d for the confirmed planet b (left), and an uniform prior U$\[\mathcal{U}\]$(2, 7) d for planet c (center-left), planet d (center-right), and planet e (right). For all planets we use an uniform prior U$\[\mathcal{U}\]$(0, 5) m s−1 on semi-amplitude velocity.

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