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Multi-resolution anisotropy studies of ultrahigh-energy cosmic rays detected at the Pierre Auger Observatory

Journal Article · · Journal of Cosmology and Astroparticle Physics
 [1]; ;  [2];  [3];  [4];  [5];  [6]; ;  [7];  [8];  [9];  [10];
  1. Institute for Mathematics, Astrophysics and Particle Physics (IMAPP), Radboud Universiteit, Nijmegen (Netherlands)
  2. Laboratório de Instrumentação e Física Experimental de Partículas—LIP and Instituto Superior Técnico—IST, Universidade de Lisboa—UL (Portugal)
  3. Osservatorio Astrofisico di Torino (INAF), Torino (Italy)
  4. Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), Universités Paris 6 et Paris 7, CNRS-IN2P3 (France)
  5. Universidade de São Paulo, Inst. de Física, São Paulo (Brazil)
  6. Centro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET) (Argentina)
  7. Instituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Centro Atómico Constituyentes, Comisión Nacional de Energía Atómica (Argentina)
  8. Universidad Nacional Autónoma de México, México (Mexico)
  9. Universidad de Santiago de Compostela (Spain)
  10. Gran Sasso Science Institute (INFN), L'Aquila (Italy)
We report a multi-resolution search for anisotropies in the arrival directions of cosmic rays detected at the Pierre Auger Observatory with local zenith angles up to 80{sup o} and energies in excess of 4 EeV (4 × 10{sup 18} eV). This search is conducted by measuring the angular power spectrum and performing a needlet wavelet analysis in two independent energy ranges. Both analyses are complementary since the angular power spectrum achieves a better performance in identifying large-scale patterns while the needlet wavelet analysis, considering the parameters used in this work, presents a higher efficiency in detecting smaller-scale anisotropies, potentially providing directional information on any observed anisotropies. No deviation from isotropy is observed on any angular scale in the energy range between 4 and 8 EeV. Above 8 EeV, an indication for a dipole moment is captured; while no other deviation from isotropy is observed for moments beyond the dipole one. The corresponding p -values obtained after accounting for searches blindly performed at several angular scales, are 1.3 × 10{sup −5} in the case of the angular power spectrum, and 2.5 × 10{sup −3} in the case of the needlet analysis. While these results are consistent with previous reports making use of the same data set, they provide extensions of the previous works through the thorough scans of the angular scales.
OSTI ID:
22676159
Journal Information:
Journal of Cosmology and Astroparticle Physics, Journal Name: Journal of Cosmology and Astroparticle Physics Journal Issue: 06 Vol. 2017; ISSN 1475-7516
Country of Publication:
United States
Language:
English

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Using spherical wavelets to search for magnetically-induced alignment in the arrival directions of ultra-high energy cosmic rays text January 2013
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Full sky harmonic analysis hints at large ultra-high energy cosmic ray deflections journal March 2015
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Effects of the galactic magnetic field upon large scale anisotropies of extragalactic cosmic rays journal November 2010
Integrated Sachs-Wolfe effect from the cross correlation of WMAP3 year and the NRAO VLA sky survey data: New results and constraints on dark energy text January 2006
Anisotropies of ultrahigh energy cosmic rays diffusing from extragalactic sources journal June 2014
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Cited By (6)

Observation of Anisotropy of TeV Cosmic Rays with Two Years of HAWC journal September 2018
Probing large-scale magnetism with the Cosmic Microwave Background text January 2017
The Giant Radio Array for Neutrino Detection (GRAND): Science and Design text January 2018
Probing large-scale magnetism with the cosmic microwave background journal March 2018
The Giant Radio Array for Neutrino Detection (GRAND): Science and design journal August 2019
Performance and science reach of the Probe of Extreme Multimessenger Astrophysics for ultrahigh-energy particles journal January 2020

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