Fig. 10
Secondary eclipse light curve of Kepler-423, phase-folded to the orbital period of the planet. Kepler data are median-binned in intervals of 0.015 cycles in phase (~1 h). The 1σ error bars are the median absolute deviations of the data points inside the bin, divided by the square root of the number of points. The best fitting transit model is overplotted with a red line.
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