Large-scale Cosmic-ray Anisotropies with 19yr of Data from the Pierre Auger Observatory

Authors

A. Abdul Halim, The University of Adelaide
P. Abreu, Instituto Superior Técnico
M. Aglietta, Istituto Nazionale Di Astrofisica, Rome
I. Allekotte, Centro Atomico Bariloche
K. Almeida Cheminant, FOM-Institute of Subatomic Physics - NIKHEF
A. Almela, Comision Nacional de Energia Atomica Argentina
R. Aloisio, Gran Sasso Science Institute
J. Alvarez-Muñiz, Instituto Galego de Física de Altas Enerxías (IGFAE)
A. Ambrosone, Gran Sasso Science Institute
J. Ammerman Yebra, Instituto Galego de Física de Altas Enerxías (IGFAE)
G. A. Anastasi, Università degli Studi di Catania
L. Anchordoqui, Lehman College
B. Andrada, Comision Nacional de Energia Atomica Argentina
L. Andrade Dourado, Gran Sasso Science Institute
S. Andringa, Instituto Superior Técnico
L. Apollonio, Università degli Studi di Milano
C. Aramo, Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
P. R. Araújo Ferreira, Rheinisch-Westfälische Technische Hochschule Aachen
E. Arnone, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
J. C. Arteaga Velázquez, Universidad Michoacana de San Nicolás de Hidalgo
P. Assis, Instituto Superior Técnico
G. Avila, Comision Nacional de Energia Atomica Argentina
E. Avocone, Laboratori Nazionali del Gran Sasso
A. Bakalova, Institute of Physics of the Czech Academy of Sciences
F. Barbato, Gran Sasso Science Institute
A. Bartz Mocellin, Colorado School of Mines
J. A. Bellido, The University of Adelaide
C. Berat, Université Grenoble Alpes
M. E. Bertaina, Istituto Nazionale di Fisica Nucleare, Sezione di Torino
G. Bhatta, Henryk Niewodniczanski Institute of Nuclear Physics of the Polish Academy of Sciences
M. Bianciotto, Istituto Nazionale di Fisica Nucleare, Sezione di Torino

Document Type

Article

Publication Date

11-1-2024

Abstract

Results are presented for the measurement of large-scale anisotropies in the arrival directions of ultra–high-energy cosmic rays detected at the Pierre Auger Observatory during 19 yr of operation, prior to AugerPrime, the upgrade of the observatory. The 3D dipole amplitude and direction are reconstructed above 4 EeV in four energy bins. Besides the established dipolar anisotropy in R.A. above 8 EeV, the Fourier amplitude of the 8–16 EeV energy bin is now also above the 5σ discovery level. No time variation of the dipole moment above 8 EeV is found, setting an upper limit to the rate of change of such variations of 0.3% yr−1 at the 95% confidence level. Additionally, the results for the angular power spectrum are shown, demonstrating no other statistically significant multipoles. The results for the equatorial dipole component down to 0.03 EeV are presented, using for the first time a data set obtained with a trigger that has been optimized for lower energies. Finally, model predictions are discussed and compared with observations, based on two source emission scenarios obtained in the combined fit of spectrum and composition above 0.6 EeV.

Publication Title

Astrophysical Journal

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