Orateur
Jennifer Siegal-Gaskins
(CCAPP, Ohio State University)
Description
The contribution of unresolved sources to the diffuse gamma-ray background could produce anisotropies in this emission on small angular scales. Recent studies have considered the angular power spectrum and other anisotropy metrics as tools for identifying the contributions to the diffuse emission from unresolved source classes, such as extragalactic and Galactic dark matter as well as various astrophysical gamma-ray source populations. I will present the results of an anisotropy analysis of the diffuse emission measured by the Fermi-LAT.
Author
Jennifer Siegal-Gaskins
(CCAPP, Ohio State University)
