Fig. 4
Bayesian Block light curves of Obs1 and Obs2. The eclipses are clearly defined, except for the third eclipse of Obs2, which is affected by data gaps. The gaps are plainly visible, beginning around phase 2.1. A few noisy blocks of implausible count rate are also visible (see Worpel & Schwope 2015) but do not affect the eclipse timings.
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