Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory

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Main Author: Bianciotto, Marta
Format: Preprint
Published: 2025
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author Bianciotto, Marta
author_facet Bianciotto, Marta
contents Measurements of anisotropies in the arrival directions of ultra-high-energy cosmic rays are crucial to pinpoint their sources, which are yet to be discovered. A dipolar anisotropy in right ascension above 8~EeV has been detected by the Pierre Auger Observatory with a significance of $6.8 σ$. The direction of the dipole suggests an extragalactic origin of ultra-high-energy cosmic rays above those energies. In this contribution, we provide an overview of the studies on large-scale anisotropies in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory with energy thresholds from $\sim 0.03$~EeV up to $32$~EeV and we present and discuss the recent results achieved with the latest available dataset, which includes 19 years of operations -- resulting in a total exposure of 123,000~km$^2$~sr~yr and nearly 50,000 events above 8~EeV.
format Preprint
id arxiv_https___arxiv_org_abs_2507_19243
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
Bianciotto, Marta
High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
Measurements of anisotropies in the arrival directions of ultra-high-energy cosmic rays are crucial to pinpoint their sources, which are yet to be discovered. A dipolar anisotropy in right ascension above 8~EeV has been detected by the Pierre Auger Observatory with a significance of $6.8 σ$. The direction of the dipole suggests an extragalactic origin of ultra-high-energy cosmic rays above those energies. In this contribution, we provide an overview of the studies on large-scale anisotropies in the arrival directions of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory with energy thresholds from $\sim 0.03$~EeV up to $32$~EeV and we present and discuss the recent results achieved with the latest available dataset, which includes 19 years of operations -- resulting in a total exposure of 123,000~km$^2$~sr~yr and nearly 50,000 events above 8~EeV.
title Large-scale anisotropies of ultra-high-energy cosmic rays measured at the Pierre Auger Observatory
topic High Energy Astrophysical Phenomena
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2507.19243