Fig. 10
Photometry follow-up of WASP-138 observed from EulerCam (red). The data are phase-folded with the ephemeris from our analysis. The EulerCAM light curve is assigned an arbitrary offset from the zero magnitute for clarity. The best-fit transit model from Mandel & Agol (2002) is plotted as a black solid line, and the residuals of the fit are plotted directly below the light curves.
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