Fig. 1
1-s light curve of GRB 000226 detected with GRBM unit 2 in the 40–700 keV band shown as an example. The dashed horizontal line shows the parabolic fit to the background. The vertical lines mark the time intervals corresponding to the 128-s spectra continuously acquired. Spectra “A” and “B” include the GRB, while the adjacent intervals are used to interpolate the background in each channel.
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