R. Caputo

TL;DR: In this article, the authors report on γ-ray observations of the Milky-Way satellite galaxies (dSphs) based on six years of Fermi Large Area Telescope data processed with the new Pass8 event-level analysis.

TL;DR: The Fermi Large Area Telescope (LAT) has provided the most detailed view to date of the emission toward the Galactic center (GC) in high-energy gamma-rays as mentioned in this paper.

TL;DR: In this paper, the uncertainty of the Galactic Center (GC) excess spectrum and morphology due to uncertainties in cosmic-ray source distributions and propagation, uncertainties in the distribution of interstellar gas in the Milky Way, and uncertainties due to a potential contribution from the Fermi bubbles.

TL;DR: In this paper, the authors presented a catalog of hard Fermi-LAT sources (2FHLs) in the 50 GeV-2 TeV energy range and found that 86% of the sources can be associated with counterparts at other wavelengths, of which the majority are active galactic nuclei and the rest (11%) are Galactic sources.

TL;DR: In this article, the properties of supernova remnants (SNRs) at high energies were uniformly determined using data from the Fermi Large Area Telescope (LAT), and 30 sources were classified as likely GeV SNRs.