Fig. 9
Transit light-curve of a star with a spot anomaly shown as a blue dot and a transiting planet with a radius of Rp/R∗ = 0.1. Overplotted is the best fit allowing transit duration, depth, and time to vary as free parameters (red dotted line), and the best fit obtained by holding the transit duration and depth constant and allowing only the transit timing to vary (green line).
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