Fig. 5
Follow-up photometry of WASP-42 (left) and WASP-49 (right) together with the respective model and residuals. Each light curve has been divided by the respective photometric baseline model as described in Sect. 3.2. The light curves of WASP-42 are (from top to bottom) EulerCam on March 20 and 25, 2011, and TRAPPIST on March 5, 10, 30 and April 4, 2011 (UT). The light curves of WASP-49 are (from top to bottom) EulerCam on January 19 and March 24, 2011, TRAPPIST on January 19 and 24 October 2011, and FTS on 21 March 2011 (UT).
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