Fig. F.1
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Rotation period analysis from the SAP TESS light curve, after masking transits of TOI-6041 b. Top: Lomb-Scargle periodogram showing a broad, significant peak between 20–30 d, under the 0.001% FAP. Bottom: Light curve phase-folded on the best-fit period (∼23 d), with the model overplotted in red. This analysis was performed using the <mono>Astropy</mono> library.
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