Fig. 3
High-S/N transit light curves. The upper observations (blue circles) were obtained by FTN, using a Pan-STARRS z filter, on 2010 Feb. 26. The lower observations (red diamonds), offset in relative flux by 0.026 for display, were obtained by Euler, using a Gunn r filter, on 2010 Apr. 15. The best-fitting transit models generated from the parameters of Table 4 are overplotted.
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