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

  • Authors: Kohta Murase, Kenji Toma, Ryo Yamazaki, and Peter Mészáros

Murase et al. 2011 The Astrophysical Journal 732 77.

  • Provider: AAS Journals

Caption: Figure 9.

Gamma-ray spectra of EIC and SSC emission in the late internal dissipation emission model at T = 10 2.6 s (thin) and T = 10 3.6 s (thick), but the source redshift is taken as z = 1. Source parameters are the same as that used in the caption of Figure 3. The EBL attenuation is included in EIC and SSC, but not included in EIC (intrinsic) and SSC (intrinsic). One can see that it is crucial for detections by Cherenkov telescopes.

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