Fig. 1.
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Fermi/GBM light curve of GRB 231115A (black), binned at a temporal resolution of counts per 3 ms, with the background model (green). The brown line is the result of the BB analysis of the burst. The pink dots are the time-resolved peak energy values taken from Table 1. At this finer temporal resolution we see a double-peaked structure within the initial burst signal.
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