Jun 23 – 28, 2014
Europe/Zurich timezone

An explanation to the diffuse gamma-ray emission.

Jun 26, 2014, 5:10 PM
Room 4 (Tuschinski Theatre)

Room 4

Tuschinski Theatre

Presentation Cosmic Rays Cosmic Rays


Fiorenza Donato


We evaluate the contribution to the high latitude gamma-ray emission in the GeV-TeV energy range as due to various AGN populations. We give an estimation of the unresolved energy spectrum and compare our results to the data collected by the Fermi-LAT. We also briefly discuss the relevant anisotropy in the IGRB. Finally, we give some hints to the possibility left to dark matter searches in the high latitude gamma-ray sky.

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