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EBL Inhomogeneity and Hard-Spectrum Gamma-Ray Sources

Authors: Hassan Abdalla, and Markus Böttcher

2017 The Astrophysical Journal 835 237.

Provider: AAS Journals

Caption: Figure 1.

Illustration of an underdense region between the observer at redshift z and the source at redshift z_s. We assume that the underdense region has a radius R and the redshift at the center of the underdense region is z_v.

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