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Fig. 3


Secondary eclipse of WASP-10b in the Ks-band obtained in the MCMC analysis. The black circles show the data binned every ~8.47 min (127 points per bin). The solid line represents the best model obtained from the MCMC analysis, resulting in an eclipse depth of ΔF = 0.137%, with a baseline level at Fbl = 0.99984. The dotted lines illustrate the ingress and egress positions of the expected eclipse for a circular orbit, and the dashed lines show a phase shift of Δφ = −0.0028, given by the best model. The residuals are presented in the lower panel.

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