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Fig. 1

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Left: new transit light curves for TrES-5 b, sorted by the observation date and, if observed simultaneously, by the telescope’s aperture size. The best-fitting model is drawn with red lines. A signature of starspot occultation identified in the light curve acquired on 2019 November 30 is marked with grey points. These measurements were masked out in transit modelling. Right: photometric residuals from the transit model.

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