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Fig. 3

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All occultation lightcurves obtained in the z′-band. The upper six lightcurves were obtained with EulerCam and are unbinned, while the lower four lightcurves were obtained with TRAPPIST and binned in two-minute intervals. Left panel: the raw lightcurves, together with the occultation and photometric models. Right panel: the lightcurves and the occultation model, divided by the photometric model. The lower panel shows all data, corrected for the photometric model and binned in four-minute intervals. Data and model are shown on the left, while the residuals are shown on the right.

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