activity
20212025
most citedArrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

86 citations · 134 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.HE2025

First Array-Wide Search for Diffuse UHE Neutrinos with the Askaryan Radio Array

Marco Stein Muzio

The Askaryan Radio Array (ARA) is an ultrahigh energy (UHE) neutrino detector at the South Pole, designed to search for radio pulses emitted by neutrino-initiated particle showers…

astro-ph.HE2023★ 9 cited

Science with the Global Cosmic-ray Observatory (GCOS)

Rafael Alves Batista

The Global Cosmic-ray Observatory (GCOS) is a proposed large-scale observatory for studying ultra-high-energy cosmic particles, including ultra-high-energy cosmic rays (UHECRs), ph…

astro-ph.HE2023

Progress Towards a Diffuse Neutrino Search in the Full Livetime of the Askaryan Radio Array

Paramita Dasgupta, Marco Stein Muzio

The Askaryan Radio Array (ARA) is an in-ice ultrahigh energy (UHE, PeV) neutrino experiment at the South Pole that aims to detect radio emissions from neutrino-induced partic…

astro-ph.HE2022★ 86 cited

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

The Pierre Auger Collaboration, P. Abreu, M. Aglietta +372

A promising energy range to look for angular correlation between cosmic rays of extragalactic origin and their sources is at the highest energies, above few tens of EeV ($1\:{\rm E…

astro-ph.HE2021★ 17 cited

The UHECR dipole and quadrupole in the latest data from the original Auger and TA surface detectors

Peter Tinyakov, Luis Anchordoqui, Teresa Bister +13

The sources of ultra-high-energy cosmic rays are still unknown, but assuming standard physics, they are expected to lie within a few hundred megaparsecs from us. Indeed, over cosmo…

astro-ph.HE2021★ 22 cited

UHECR arrival directions in the latest data from the original Auger and TA surface detectors and nearby galaxies

Armando di Matteo, Luis Anchordoqui, Teresa Bister +13

The distribution of ultra-high-energy cosmic-ray arrival directions appears to be nearly isotropic except for a dipole moment of order per cent. None…