Image Details
Caption: Figure 1.
Modeling of the high-energy emission during interval II in the IS scenario (Guetta & Granot 2003). The red arrow marks the level of BAT upper-limits (see, e.g., De Pasquale et al. 2010) while the green diamond marks the level of the flux observed by the LAT around 1 GeV (see Figure 2 in Abdo et al. 2009b).
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