Understanding the physical mechanisms that control galaxy formation is a fundamental
challenge in contemporary astrophysics. Recent advances in the field of astrophysical …

CO line emission represents the most accessible and widely used tracer of the molecular
ISM. This renders the translation of observed CO intensity into total H2 gas mass critical to …

The origin of high-energy cosmic rays, atomic nuclei that continuously impact Earth's
atmosphere, is unknown. Because of deflection by interstellar magnetic fields, cosmic rays …

We present an incremental version (4FGL-DR3, for Data Release 3) of the fourth Fermi
Large Area Telescope (LAT) catalog of γ-ray sources. Based on the first 12 years of science …

The IceCube Neutrino Observatory has established the existence of a high-energy all-sky
neutrino flux of astrophysical origin. This discovery was made using events interacting within …

Fermi Large Area Telescope Fourth Source Catalog - IOPscience Skip to content IOP
Science home Accessibility Help Search all IOPscience content Search Article Lookup …

We report, for the first time, the long-awaited detection of diffuse gamma rays with energies
between 100 TeV and 1 PeV in the Galactic disk. Particularly, all gamma rays above 398 …

The diffuse Galactic γ-ray emission, mainly produced via interactions between cosmic rays
and the interstellar medium and/or radiation field, is a very important probe of the …

Astrophysical neutrinos are excellent probes of astroparticle physics and high-energy
physics. With energies far beyond solar, supernovae, atmospheric, and accelerator …

The main objectives of the KM3NeT Collaboration are (i) the discovery and subsequent
observation of high-energy neutrino sources in the Universe and (ii) the determination of the …