Fig. E.1
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Phase-folded TESS LC assuming the best model ephemerides of planet e (a) and planetary candidate 5 (b). The black points are the TESS data points at the original cadence. The red line is the data binned in phase using bins of 15 min. The dashed pink and brown lines are the expected transit signal assuming that the planets have the same radius as planet d (see Table H.1).
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