Fig. 1
Energy-resolved light curves of GRB 120711A. The top panel shows the 20−200 keV IBIS light curve that is severely affected by telemetry gaps. The lower panels show the SPI light curves in five energy bands. In all cases, the light curves are binned over 1 s. The vertical dashed line at T0 + 115 s represents the end of the T90 duration.
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