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Fig. 14


Distributions estimating the posterior densities of orbital periods (Px), eccentricities (ex), and RV amplitudes (Kx) of the five Keplerian signals. The solid curve is a Gaussian density with the same mean (μ) and variance (σ2) as the parameter distribution has. Additional statistics, mode, skewness (μ3) and kurtosis (μ4) of the distributions are also shown.

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