Fig. 1.
Swift/XRT (0.3−10 keV) light curve of IGR J11215−5952 to monitor the onset of the 2017 outburst (upper panel), compared with the times of the NuSTAR observation (lower panel, 3−78 keV). A time binning of 187 s has been assumed. We note that, since there are gaps in both observations (by Swift and NuSTAR), unfortunately they were never simultaneous. The down arrows in the upper panel indicate upper limits.
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