Fig. 4
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Example of evolution of the angles for a sample of the posterior. The top panel shows the resonant angles ϕ1 = λ1 − 2λ2 + ϖ1 and ϕ2 = λ1 − 2λ2 + ϖ2, where 1 refers to planet b and 2 to planet c, λ is the mean longitude and ϖ the longitude of periastron of the planets. The bottom panel shows the evolution of the longitude of periastron.
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