Fig. C.1
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MCMC posterior distributions for the main fitted transit parameters (see Sect. 5.1.1): the log of the orbital period (log P), the mid-transit time (T0), the transit depth (dF), and the cosine of the orbital inclination (cos ip) for each of the two planets; and the log of the stellar density (log ρ★). This plot was made using the corner python package (Foreman-Mackey 2016).
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