Fig. 4

Left-hand panel: light curves of the WASP-67 eclipses observed in Gunn-r with the Euler telescope (Hellier et al. 2012), in Bessell-R with the Danish telescope (this work) and with an I + z filter with the TRAPPIST telescope (Hellier et al. 2012). The filters and the name of each telescope are labelled on the figure. The jktebop best fits are shown as solid lines for each optical dataset. Right-hand panel: residuals of each fit.
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