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Fig. 12

Simulated time-integrated (t0 + 58, t0 + 66 s) count spectrum (8–440 keV) of the extended afterglow of GRB 090618 (upper panel), count spectrum (8 keV–10 MeV) of the main pulse emission (t0 + 58, t0 + 66), and best fit with a blackbody + power-law model (middle panel) and a simple power-law model (lower panel).
This figure is made of several images, please see below:
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