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Fig. 3


Comparing the photometric results of SOAP-T and the theoretical model of a transiting planet over an unspotted star (Mandel & Agol 2002). The cyan, red, and yellow lines show SOAP-T’s results for a star without limb darkening, a star with linear limb darkening (γ1 = 0.6), and a star with quadratic limb darkening (γ1 = 0.29 and γ2 = 0.34), respectively. The dash-dotted, dashed, and the dotted lines show the corresponding results using the mechanism by Mandel & Agol (2002).

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