activity
20002021
most citedParametrization of gamma-ray production cross-sections for pp interactions in a broad proton energy range from the kinematic threshold to PeV energies

354 citations · 2.8k across the 54 of their papers we have counts for

collaborators

57 papers

astro-ph.HE2021★ 24 cited

Evidence of 100 TeV -ray emission from HESS J1702-420: A new PeVatron candidate

H. Abdalla, F. Aharonian, F. Ait Benkhali +232

The identification of PeVatrons, hadronic particle accelerators reaching the knee of the cosmic ray spectrum (few eV), is crucial to understand the origin of cosmic rays…

astro-ph.HE2021★ 20 cited

Extragalactic magnetic field constraints from ultra-high-energy cosmic rays from local galaxies

Arjen van Vliet, Andrea Palladino, Andrew Taylor +1

We interpret the correlation between local star-forming galaxy positions and ultra-high-energy cosmic ray (UHECR) directions, recently detected by the Pierre Auger Observatory (PAO…

astro-ph.HE2021★ 18 cited

Particle acceleration in radio galaxies with flickering jets: GeV electrons to ultrahigh energy cosmic rays

James H. Matthews, Andrew M. Taylor

Variability is a general property of accretion discs and their associated jets. We introduce a semi-analytic model for particle acceleration and radio jet/lobe evolution and explor…

astro-ph.HE2020★ 8 cited

Ultrahigh-energy dipole and beyond

Rodrigo Guedes Lang, Andrew M. Taylor, Vitor de Souza

Recent data from the Pierre Auger Observatory has revealed the presence of a large-scale dipole in the arrival direction distribution of ultra-high energy cosmic rays (UHECR). In t…

astro-ph.HE2020★ 26 cited

Revisiting the distance to the nearest UHECR source: Effects of extra-galactic magnetic fields

Rodrigo Guedes Lang, Andrew M. Taylor, Markus Ahlers +1

We update the constraints on the location of the nearest UHECR source. By analyzing recent data from the Pierre Auger Observatory using state-of-the-art CR propagation models, we r…

astro-ph.HE2020★ 11 cited

Extension of the synchrotron radiation of electrons to very high energies in clumpy environments

Dmitry Khangulyan, Felix Aharonian, Carlo Romoli +1

The synchrotron cooling of relativistic electrons is one of the most effective radiation mechanisms in astrophysics. It not only accompanies the process of particle acceleration bu…