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Fig. 1.
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XRISM Resolve and NuSTAR light curves in the 2−10 keV and 4−30 keV energy range, respectively, for observations 1 (top) and 2 (bottom) showing absorption dips at the start and end of the observations. The binning is 25 s in each panel. The thick tick marks at the top axis mark the start and end of phase-resolved intervals.
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