Fig. 4.
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Light curves of the events GRB 180128A, GRB 200415A, and GRB 150101B, binned to a temporal resolution of 1 ms for energies from 10–500 keV. The black lines represent the raw data. The gray line shows the energy-integrated background. The red lines show the significance of the pulses above the background (gray line) using a BB algorithm. At this temporal resolution, GRB 180128A displays two distinct millisecond peaks.
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