Fig. 2
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Occultation light curve analysis. Top panel: phase-folded Kepler occultation light curve of HAT-P-11 b binned by 1 min, based on 196 occultations (see text). Our best-fitting model of the occultation in the Kepler bandpass is overplotted with a black solid line. The data have been binned for clarity (black dots with error bars). Bottom panel: residuals of the fit.
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