Fig. H.1

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Prior and posterior distributions of the orbital periods (left panels) and RV semi-amplitudes (right panels) for the seven planets. The priors are shown as grey distributions. The dashed orange lines indicate the posterior distributions obtained from the RV analysis using the HARPS, HARPS-N, and HIRES instruments. The dashed blue lines correspond to the posterior distributions derived from the ESPRESSO data alone. The pink distributions represent the posterior results from the combined analysis of all four instruments.
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