The Blazar Spectral Energy Distribution Sequence Model of the Diffuse Gamma-Ray Background and its Implications for Dark Matter Detection | Instituto de Física Teórica UAM/CSIC (Webpage 2008-2015)

The Blazar Spectral Energy Distribution Sequence Model of the Diffuse Gamma-Ray Background and its Implications for Dark Matter Detection

Submitted on: Sáb, 11/12/2010 - 12:49 — tomas

Preprint info

IFT Number:

IFT-UAM/CSIC-10-97

Publication Type:

Preprint

Authors:

Kevork N. Abazajian; Steve Blanchet; J.Patrick Harding

Source:

(Submitted)

URL:

http://arxiv.org/abs/1012.1247

ISI Journal:

Non-ISI or not yet published