Fig. 10
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Results from fits to the TESS light curve, with all the observed transits stacked, with the model taken from the maximum a posteriori point estimation, based on maximizing the posterior probability distributions for each parameter. At this point, T0 = 1791.5206 BTJD, Ρ = 3.1342799 days, a = 21.1 R*, Rp = 0.034 R*, and Ip = 89.4°.
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