Fig. 5
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Residuals (black) from the subtraction of noiseless, spotted transit light curves from noise-added, spotted light curves for four combinations of stellar radius, planetary radius, and stellar apparent magnitude. Red curves represent the residuals after three-point smoothing. Horizontal blue lines are the 3 × σ75s noise level, while vertical green lines mark the umbra-penumbra boundaries. Detectable penumbral have residuals above 3 × σ75 s.
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