activity
20152023
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV

409 citations · 2.1k across the 23 of their papers we have counts for

collaborators
Showing 2016Show all

5 papers · 1 filter

hep-ex2016★ 236 cited

Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +435

Ultrahigh energy cosmic ray air showers probe particle physics at energies beyond the reach of accelerators. Here we introduce a new method to test hadronic interaction models with…

astro-ph.HE2016★ 51 cited

Ultrahigh-energy neutrino follow-up of Gravitational Wave events GW150914 and GW151226 with the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +410

On September 14, 2015 the Advanced LIGO detectors observed their first gravitational-wave (GW) transient GW150914. This was followed by a second GW event observed on December 26, 2…

astro-ph.CO2016★ 55 cited

Propagation of Ultra High Energy Cosmic Rays in Extragalactic Magnetic Fields: A view from cosmological simulations

Stefan Hackstein, Franco Vazza, Marcus Brueggen +2

We use the CRPropa code to simulate the propagation of ultra high energy cosmic rays (with energy and pure proton composition) through extragalactic magnetic…

astro-ph.HE2016★ 28 cited

Azimuthal asymmetry in the risetime of the surface detector signals of the Pierre Auger Observatory

The Pierre Auger Collaboration, A. Aab, P. Abreu +436

The azimuthal asymmetry in the risetime of signals in Auger surface detector stations is a source of information on shower development. The azimuthal asymmetry is due to a combinat…

astro-ph.IM2016★ 322 cited

CRPropa 3 - a Public Astrophysical Simulation Framework for Propagating Extraterrestrial Ultra-High Energy Particles

Rafael Alves Batista, Andrej Dundovic, Martin Erdmann +7

We present the simulation framework CRPropa version 3 designed for efficient development of astrophysical predictions for ultra-high energy particles. Users can assemble modules of…