Follow-up, high-precision, time-series photometry of the WASP-65b during the transit (see Table 4). The observations are shown as black points and are phase folded on the ephemeris shown in Table 7. The superimposed, solid, red line is our best-fit transit model (Sect. 3.3) using the formalism of Mandel & Agol (2002). The residuals from the fit and the individual data points photometric uncertainties are displayed directly under each light curve. The light curves and residuals are displaced from zero for clarity.
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