Detrended occultation light curves from the SW photometric channel (2.1 μm, left panel) and white-light light curves from the LW channel (4.5 μm, right panel). Only binned data points are shown here. The darker and lighter shades of the points depict even and odd orbital number parity, respectively. The dates and occultation depth (median and 68-percentile confidence intervals) of the visits are indicated above each plot. The best-fitted models and models computed from randomly selected posteriors to show the model uncertainties are plotted with thick and thin lines.