Fig. 3: Effect of EBL attenuation on the gamma-ray flux for two redshift intervals and three different EBL models20,21,22. | Nature Communications

Fig. 3: Effect of EBL attenuation on the gamma-ray flux for two redshift intervals and three different EBL models20,21,22.

From: The diffuse gamma-ray flux from clusters of galaxies

Fig. 3

This figure indicates that the EBL flux attenuation is more prominent at high redshifts and sensitive to the adopted EBL model. The flux is plotted for α = 2.3 and \({E}_{\max }=1{0}^{17}\) eV.

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