Fig. 13
Pairwise marginal posteriors of the MCMC analysis for the 55 Cnc e planet and the phase variation modeled as described in Eq. (1). For visibility, we plot T0 − 4417 and fold the Φ11 parameter over ± π. We found a double maxima for the Φ15 parameter around 0 [mod 2π] and π, which is meaningless as the corresponding modulation amplitude α15 is roughly null.
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