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High-energy Emission Components in the Short GRB 090510

  • Authors: Alessandra Corsi, Dafne Guetta, and Luigi Piro

CORSI, GUETTA, & PIRO 2010 The Astrophysical Journal 720 1008.

  • Provider: AAS Journals

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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