Detrended individual (light blue, without uncertainties) and binned (blue, binned over 7.2 min intervals) secondary eclipse light curves corresponding to epochs 971 and 1889, reduced by using the DRP (top) and PIPE (bottom). The best-fit transit models are shown as brown lines (the green portions show the disruptions in the light curves), and the residuals from the best-fit models in the bottom panels. The light curves reduced by the DRP and PIPE are in statistical agreement with each other.