The GAPS programme at TNG - LXXI. A sub-Neptune suitable for atmospheric characterization in a multiplanet and mutually inclined system orbiting the bright K dwarf TOI-5789 (HIP 99452)

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Fig. 4

Posterior distribution of the number of planets N_p detected with kima in the HARPS-N radial velocities. The distributions are shown as the number of posterior samples for each value of N_p normalized to the effective sample size (ESS). The orange bar highlights the highest value for N_p =4 corresponding to the most likely 4-planet model.

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