Main Image
Volume 312 - 7th International Fermi Symposium (IFS2017) - Session Central Galaxy
Diffuse gamma-ray emission modeling and the Galactic center GeV excess
D. Malyshev* on behalf of the Fermi-LAT Collaboration
*corresponding author
Full text: pdf
Published on: 2017 December 12
Abstract
The Galactic center is one of the most important regions to search for a gamma-ray signal from a possible annihilation of dark matter due to its proximity and high dark matter density. In the past years, several groups have reported an excess of gamma rays in the Fermi Large Area Telescope data with an approximately spherical morphology around the Galactic center. In this contribution, we will overview the current observational status of the excess and the difficulties in the gamma-ray analysis near the Galactic center.
DOI: https://doi.org/10.22323/1.312.0052
Open Access
Creative Commons LicenseCopyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.