Characterization of dark-matter-induced anisotropies in the diffuse gamma-ray background

@article{Fornasa2013CharacterizationOD,
  title={Characterization of dark-matter-induced anisotropies in the diffuse gamma-ray background},
  author={Mattia Fornasa and Jes{\'u}s Zavala and Miguel Sanchez-conde and Jennifer M. Siegal-Gaskins and Timur Delahaye and Francisco Prada and Mark Vogelsberger and Fabio Zandanel and Carlos S. Frenk},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2013},
  volume={429},
  pages={1529-1553}
}
The Fermi-LAT collaboration has recently reported the detection of angular power above the photon noise level in the diffuse gamma-ray background between 1 and 50 GeV. Such signal can be used to constrain a possible contribution from dark matter (DM) induced photons. We estimate the intensity and features of the angular power spectrum (APS) of this potential DM signal, for both decaying and annihilating DM candidates, by constructing template all-sky gamma-ray maps for the emission produced in… 
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