Fig. 7
Left: NuSTAR count rate in band 3–10 keV during the whole pointing spanning ~2.5 orbits. The orbital phase is labeled on top of the panels. This spectral band consists almost solely of the blackbody emission. Right: NuSTAR count rate in the band 20–60 keV. This spectral band consists of only the power law emission. The dashed lines demarcate the ~1 ksec NuSTAR spectra that are shown in Fig. 8.
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