Fig. A.4

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Eclipse observed in the QLP data for TIC 91145541. The top panel shows the combined data of Sectors 44, 45, 71, and 72, providing a lower limit for the orbital period of the binary system of ≥ 41.5 days. In the middle and bottom panels are zoom-ins of different regions of the eclipse. The bottom panel reveals an increase in brightness immediately before the eclipse, consistent across Sectors 44 and 71.
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