Fig. 4
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Secondary eclipse depths estimated for each individual epoch from the light curves reduced by the DRP (blue) and PIPE (orange, with a slight offset along the x-axis for visibility), along with the calculated mean secondary eclipse depths (blue and orange dotted lines for the light curves reduced by DRP and PIPE respectively; the shaded regions show the uncertainties). We note that the eclipse depths estimated from the two sets of light curve data reduced by independent pipelines (i.e., DRP and PIPE) are in close statistical agreement with each other.
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