Figure 2 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 2.

Same as Figure 1, but at T = 10 ^3.6 s and z = 0.3.