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Fig. A.1

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Posterior distributions and joint correlations between all free parameters in the joint fit to the In-Orbit Commissioning transit and phase curve observations sampled with the No U-Turn Sampler. The parameters include: the mid-transit time t0, limb-darkening parameters u0, u1, the ratio of planetary to stellar radius RpR, the impact parameter b, the eclipse depth δecl; two sets of detrending vector weights for the following vectors, one per visit: the ThermFront 2 temperature sensor reading, thecosine and sine of the roll angle, and a unit vector; the amplitude of the piecewise-Lambertian variations A; and the startand stop longitudes of the lower-reflectivity region ξ1 and ξ2. The last parameter, log σ is the natural logarithm of the flux uncertainty for each measurement.

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