Fig. 3
Unbinned phase-folded light curve of KOI-196 with the best-fit model. The inset displays a zoom of the out-of-transit LC binned to 0.02 in phase with the best-fit model of the planet phase variation and occultation (inset, top panel) and its residuals (inset, bottom panel). Out-of-transit residuals binned to 0.02 in phase have a dispersion of 22 ppm.
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