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Fig. A.1

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Corner plot of the joint white-light fit of the two observations of HD 189733 for M1. The values and errors correspond to the median and the standard deviation of the posterior distributions (assuming they are normal). The subscript numbers in the variables Vsys, ∆ϕ0, mP, and log(si𝑔maW) represent the posterior distribution of the parameters that were independently fitted for the two nights.

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