activity
20152026
most citedObservation of inverse Compton emission from a long -ray burst

226 citations · 792 across the 30 of their papers we have counts for

collaborators
Showing 2023Show all

6 papers · 1 filter

astro-ph.HE2023★ 47 cited

TeV neutrinos and hard X-rays from relativistic reconnection in the corona of NGC 1068

Damiano F. G. Fiorillo, Maria Petropoulou, Luca Comisso +2

The recent discovery of astrophysical neutrinos from the Seyfert galaxy NGC 1068 suggests the presence of non-thermal protons within a compact "coronal" region close to the central…

astro-ph.HE2023

A Hierarchical Framework for explaining the Cosmic Ray Spectrum using Diffusive Shock Acceleration

Roger Blandford, Paul Simeon, Noémie Globus +3

The hypothesis that the entire cosmic ray spectrum, from to energy, can be accounted for by diffusive shock acceleration on increasin…

astro-ph.HE2023★ 14 cited

Galactic Diffuse Neutrino Emission from Sources beyond the Discovery Horizon

Antonio Ambrosone, Kathrine Mørch Groth, Enrico Peretti +1

The IceCube Neutrino Observatory has recently reported strong evidence for neutrino emission from the Galactic plane. The signal is consistent with model predictions of diffuse emi…

astro-ph.HE2023★ 5 cited

Gamma-ray emission from the Seyfert galaxy NGC 4151: Multi-messenger implications for ultra-fast outflows

Enrico Peretti, Giada Peron, Francesco Tombesi +4

The nuclear activity typical of Seyfert galaxies can drive powerful winds where high-energy phenomena occur. In spite of their high power content, the number of such non-jetted act…

astro-ph.HE2023★ 13 cited

Reacceleration of Galactic Cosmic Rays Beyond the Knee at the Termination Shock of a Cosmic-Ray-Driven Galactic Wind

Payel Mukhopadhyay, Enrico Peretti, Noemie Globus +2

The origin of cosmic rays above the knee in the spectrum is an unsolved problem. We present a wind model in which interstellar gas flows along a non-rotating, expanding flux tube w…

astro-ph.HE2023★ 3 cited

Diffusive shock acceleration at EeV and associated multimessenger flux from ultra-fast outflows driven by Active Galactic Nuclei

Enrico Peretti, Alessandra Lamastra, Francesco Gabriele Saturni +4

Active galactic nuclei (AGN) can launch and sustain powerful winds featuring mildly relativistic velocity and wide opening angle. Such winds, known as ultra-fast outflows (UFOs), c…