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Fig. 9


Detrended Spitzer 3.6 μm (left), 4.5 μm (middle), and 8 μm (right) photometry folded on the best-fit transit ephemeris obtained in our analysis per channel for the transits (top, Sect. 3.4.3) and in our global analysis for the occultations (bottom). The best-fit eclipse models are superimposed.

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

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