Top: out-of-eclipse 2011/2012 CoRoT light curve (black) with the two-spot model (cyan) and individual light curve draws from the converged MCMC walkers (grey). Data masked in in the fit are shown by orange points. Vertically offset are the individual spot models for the primary and secondary stars (red dashed and blue dot-dashed, respectively) and the residuals (grey). Middle and bottom: as above for Spitzer 3.6 and 4.5 μm, respectively. All plots share common axes.