Comment on "Joint Anisotropy and Source Count Constraints on the Contribution of Blazars to the Diffuse Gamma-Ray Background"
J. Patrick Harding, Kevork N. Abazajian

TL;DR
This paper critiques a previous study on blazars' contribution to the gamma-ray background, showing that more realistic models suggest blazars account for a larger fraction of the background than previously claimed.
Contribution
It demonstrates that previous assumptions oversimplify blazar populations, and provides a more accurate estimate of their contribution to the gamma-ray background based on physical models.
Findings
Physical models can explain up to 60% of the gamma-ray background.
Simplified assumptions underestimate blazar contribution to the background.
Spectral information significantly impacts anisotropy calculations.
Abstract
We show the conclusions claimed in the manuscript arXiv:1202.5309v1 by Cuoco, Komatsu and Siegal-Gaskins (CKS) are not generally valid. The results in CKS are based on a number of simplifying assumptions regarding the source population below the detection threshold and the threshold flux itself, and do not apply to many physical models of the blazar population. Physical blazar population models that match the measured source counts above the observational threshold can account for 60% of the diffuse gamma-ray background intensity between 1-10 GeV, while the assumptions in CKS limit the intensity to <30%. The shortcomings of the model considered in CKS arise from an over-simplified blazar source model. A number of the simplifying assumptions are unjustified, including: first, the adoption of an assumed power-law source-count distribution, dN/dS, to arbitrary low source fluxes, which is…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle physics theoretical and experimental studies · Dark Matter and Cosmic Phenomena
