Galaxy evolution is an important topic, and our physical understanding must be complete to
establish a correct picture. This includes a thorough treatment of feedback. The effects of …

Based on the expected population of core collapse supernova remnants and the huge
number of detected pulsars in the Galaxy, still representing only a fraction of the real …

High-energy diffuse gamma-ray and neutrino emission are expected from the Galactic
plane, generated by hadronuclear interactions between cosmic rays and the interstellar …

The γ-ray emission from the W51 complex is widely acknowledged to be attributed to the
interaction between the cosmic rays (CRs) accelerated by the shock of supernova remnant …

The KM2A is the largest sub-array of the Large High Altitude Air Shower Observatory
(LHAASO). It consists of 5216 electromagnetic particle detectors (EDs) and 1188 muon …

Ultra-high energy cosmic rays (UHECRs) beyond the Greisen-Zatsepin-Kuzmin (GZK) cut-off
provide us with a unique opportunity to understand the universe at extreme energies …

Although celestial sources emitting in the few tens of GeV up to a few TeV are being
investigated by imaging atmospheric Čerenkov telescope arrays such as HESS, MAGIC …

In this Letter we try to search for signals generated by ultraheavy dark matter at the Large
High Altitude Air Shower Observatory (LHAASO) data. We look for possible γ rays by dark …

Ultrarelativistic particles called cosmic rays permeate the Milky Way, propagating through
the turbulent Galactic magnetic fields. The mechanisms under which these particles …

HEX-P is a probe-class mission concept that will combine high spatial resolution X-ray
imaging (< 1 0 ″FWHM) and broad spectral coverage (0.2–80 keV) with an effective area …