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Fig. 3

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Detrended photometry period-folded on the best-fit transit ephemeris obtained in our global analysis (Sect. 3.2) after zoom on the transit (left) and occultation (right) phases. For the transit and occultation phases, the measurements were binned per interval of 2 min and 7.2 min, respectively. For both panels, the best-fit eclipse models are superimposed.

This figure is made of several images, please see below:

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