Fig. 3
Phased light curves of WASP-18Ab, WASP-19b, and WASP-77Ab transits. The three data set of light curves are fitted simultaneously with RV archival data using EXOFASTv2 in order to estimate the orbital and physical parameters of the system. Top panel: the light blue solid line shows the best-fit model for WASP-18Ab, and below are the residuals in gray. Thesame is shown for WASP-19b in orange (center panel), and for WASP-77Ab in pink (bottom panel).
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