Fig. 1
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Simulated local stellar surface velocity below the planet along the transit chord as a function of the phase (bottom) and stellar radius (top) for a given star–planet orientation (λ = 0°; i* = 150°; b = 0.2; V = 10). The best-fit DR model is shown in blue, and the best-fit SB model is plotted in orange; a positive BIC indicates a preference for the more complex DR model.
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