Fig. 1.
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Phased transits observed by LCOGT, TESS (only sectors 46 and 49), and ExTrA, and the posterior model of a planet transiting a star with a polar spot. For clarity, the figure only shows 5-min bins in the phased light curve for TESS and ExTrA. Above the panel: model of the stellar surface and the planet for the median posterior values, as seen by TESS at different times during the transit.
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