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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 12.

EIC spectra calculated with different values of E b . Intrinsic EIC spectra (where the EBL attenuation is not taken into account) are shown at T = 10 2.6 s (thin) and T = 10 3.6 s (thick). The source redshift is set to z = 0.3. For the solid curves, the used parameter set is the same as that in the caption of Figure 3. The dotted curves are for E b = 10 2.5 eV and the dashed curves are for , while the other parameters are the same.

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