Fig. C.2.

Marginalized posterior of the Np parameter in the Kima fit to the RV measurements of λ2 For. The number of samples in each bin corresponds to the likelihood, while the ratio of the height of each bin indicates the Bayes factor of one configuration over another. Comparing the cases of Np = 0 and Np = 1 the Bayes factor is effectively infinite, indicating that there is at least one planet in the system. In contrast, the ratio between Np = 2 and Np = 1 is low, with a Bayes factor of 1.67, suggesting that there is little evidence to support a two-planet configuration.
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