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Fig. A.1

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Posterior distributions and joint correlations between all free parameters in the transit model fit. The parameters are: orbital period P, mid-transit time t0, impact parameter b, quadratic limb-darkening coefficients u0 and u1, stellar radius R and mass M, planet-to-star radius ratio Rp/Rs, and transit depth δt, with a numeric subscript corresponding to the sector. We note that log(s) is the natural logarithm of the flux uncertainty for each measurement.

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