Figure 7 from On the Implications of Late Internal Dissipation for Shallow-decay Afterglow Emission and Associated High-energy Gamma-ray Signals

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On the Implications of Late Internal Dissipation for Shallow-decay Afterglow Emission and Associated High-energy Gamma-ray Signals

Murase et al. 2011 The Astrophysical Journal 732 77.

Caption: Figure 7.

Same as Figure 6, but at 100 GeV. The CTA sensitivity (with the duty factor of 30%) is overlaid instead of the Fermi one (CTA Consortium 2010).