activity
20132026
most citedEvidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector

1.6k citations · 12.8k across the 95 of their papers we have counts for

collaborators

96 papers

astro-ph.HE2026

Bayesian parameter study of the Seyfert-starburst composite galaxies NGC 1068 and NGC 7469

Björn Eichmann, Silvia Salvatore, Santiago del Palacio +4

Multimessenger observation of the Seyfert-starburst composite galaxies NGC 1068 and NGC 7469 indicate a characteristic feature in the radio band (the so-called mm-bump) as well as…

astro-ph.HE2025

Monte Carlo parameter study for Seyfert AGN-starburst composite galaxies NGC1068 and NGC7469

Silvia Salvatore, Björn Eichmann, Giacomo Sommani +3

Seyfert-starburst composite galaxies host two promising phenomena of non-thermal high-energy radiation. In this regard the IceCube observation of high-energy neutrinos from the dir…

astro-ph.HE2024★ 1 cited

High-energy neutrinos from the vicinity of the supermassive black hole in NGC 1068

P. Padovani, E. Resconi, M. Ajello +12

We present a comprehensive multi-messenger study of NGC 1068, the prototype Seyfert II galaxy recently associated with high-energy IceCube neutrinos. Various aspects of the source,…

astro-ph.HE2023★ 10 cited

On the possible jet contribution to the -ray luminosity in NGC 1068

S. Salvatore, B. Eichmann, X. Rodrigues +2

NGC 1068 is a nearby widely studied Seyfert II galaxy presenting radio, infrared, X- and -ray emission as well as strong evidence for high-energy neutrino emission. Recently, th…

astro-ph.HE2023★ 1 cited

Modified temperature redshift relation and UHECR propagation

Janning Meinert, Leonel Morejón, Alexander Sandrock +3

We re-examine the interactions of ultra-high energy cosmic rays (UHECRs) with photons from the cosmic microwave background (CMB) under a changed, locally non-linear temperature red…

astro-ph.HE2023★ 1 cited

CRPropa 3.2: a public framework for high-energy astroparticle simulations

Sophie Aerdker, Rafael Alves Batista, Julia Becker Tjus +16

CRPropa is a Monte Carlo framework for simulating the propagation of (ultra-) high-energy particles in the Universe, including cosmic rays, gamma rays, electrons, and neutrinos. It…