Fig. 19.
Data and background fits for part of the 21 June 2015, which was during a V404 Cygni outburst for 3 different detectors (n0 (top), n4 (middle), n5 (bottom)) and 2 reconstructed energy ranges (27–50 keV (left) and 50–102 keV (right)). The blue vertical lines indicate GBM trigger times, whereas the red vertical lines indicate possible new emission events that did not trigger GBM.
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