Fig. A.2.
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Combined background-subtracted EPIC light curves in different energy bands, binned at 500 s, and normalised to the fitted value of the peaks. The envelopes correspond to the 16th and 84th percentiles of the posteriors, similarly to what is shown in Fig. 5. This shows the energy dependence of the start of the burst. This is similar to Fig. 2 of Miniutti et al. (2019), for instance.
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