Fig. 3
Left, from top to bottom: period-folded TRAPPIST transit light curves of WASP-50 for 2010 December 23, 25, and 27, and Euler transit light curve. These light curves are divided by the best-fitting baseline models (see details in Sect. 4), and the best-fitting transit models are superimposed. Three light curves and models are shifted in the y-axis for the sake of clarity. Right: the residuals to the fit for each light curve.
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