The region around the Galactic Center (GC) is now well established to be brighter at
energies of a few GeV than what is expected from conventional models of diffuse gamma …

Most of the celestial γ rays detected by the Large Area Telescope (LAT) on board the Fermi
Gamma-ray Space Telescope originate from the interstellar medium when energetic cosmic …

ABSTRACT 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 γ-rays. This paper …

The possible gamma-ray excess in the inner Galaxy and the Galactic center (GC) suggested
by Fermi-LAT observations has triggered a large number of studies. It has been interpreted …

The excess of γ rays in the data measured by the Fermi Large Area Telescope from the
galactic center region is one of the most intriguing mysteries in astroparticle physics. This …

The γ-ray sky> 100 MeV is dominated by the diffuse emissions from interactions of cosmic
rays with the interstellar gas and radiation fields of the Milky Way. Observations of these …

Using the latest AMS-02 cosmic-ray antiproton flux data, we search for a potential dark
matter annihilation signal. The background parameters about the propagation, source …

We present version 2 of the DRAGON code designed for computing realistic predictions of
the CR densities in the Galaxy. The code numerically solves the interstellar CR transport …

We investigate the birth and evolution of Galactic isolated radio pulsars. We begin by
estimating their birth space velocity distribution from proper-motion measurements of …

We report on the discovery of eight repeating fast radio burst (FRB) sources found using the
Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope. These sources span …