Fig. 3
The twelve WASP-48b Ks-band occultation lightcurves that show the lowest RMS × β2, created by different combinations of reference stars and aperture sizes. The data are binned in intervals of 10 min, with the orange model indicating the MCMC fitted solution for that particular aperture and reference star combination. The caption within the figure lists the number of reference stars and aperture size, respectively.
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