Fig. 1
Left: full PDCSAP light curve from TESS after removing the smoothing model described in Sect. 3.2. The grey points represent the raw measurements, while the blue dots are the same data binned over 10 min. The model showing the best fit to the light curve with two planets corresponding to TOI-402.01 and TOI-402.02 is shown as the black curve. Middle: light curve phase-folded in phase to highlight the transit of TOI-402.01 and the best-fit model. Right: as in the middle plot, but for TOI-402.02.
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