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Fig. A.1


Bayesian evidence of different models and datasets (from top to bottom: HARPS-only, ESPRESSO-only, and HARPS+ESPRESSO). Each panel contains 15 different models that include a different number of planets: no planets (GP-only, yellow), one-planet models (pink), two-planet models (red), and three-planet model (green). Each has different orbital configuration assumptions (planets with either circular or eccentric orbits). As an example, model 3p1c2c corresponds to a three-planet model in which planets 1 (LHS 1140 b) and 2 (LHS 1140 c) have assumed circular orbits, but planet 3 (LHS 1140 d) has free eccentricity. The bars corresponding to each model include this information at the bottom of the bar. At the top of each bar we show the Bayes factor of each model compared to the stronggest evidence model for each dataset. The highest bar corresponds to the strongest evidence model.

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