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Search for Cosmic-Ray Electron and Positron Anisotropies with Seven Years of Fermi Large Area Telescope Data

  • (Fermi-LAT Collaboration)
  • Hiroshima University
  • c/o DESY
  • Clemson University
  • MST-8, Los Alamos National Laboratory
  • University of California at Santa Cruz
  • University of Pisa
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • INFN Sezione di Trieste
  • University of Trieste
  • Politecnico di Bari
  • INFN Sezione di Bari
  • Stanford Linear Accelerator Center
  • INFN Sezione di Torino
  • University of Turin
  • NASA Goddard Space Flight Center
  • Science and Research Directorate
  • George Mason University
  • Naval Research Laboratory
  • INFN Sezione di Perugia
  • RWTH Aachen University
  • INAF Istituto di Radioastronomia
  • University of Bologna
  • Università Telematica Pegaso
  • and Physics University of Udine
  • INFN
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • University of Maryland
  • University of Iceland
  • University of Tokyo
  • KTH Royal Institute of Technology
  • Oskar Klein Centre
  • University of Sheffield
  • University of Wisconsin-Madison
  • Faculty of Science, Mahidol University
  • Sezione di Roma
  • Laboratoire Univers et Particules de Montpellier
  • Max-Planck-Institut für Physik
  • University of Padova
  • Medical University of Innsbruck
  • NYCB Real-Time Computing Inc.
  • Max Planck Institut für Extraterrestrische Physik
  • Nagoya University
  • Pompeu Fabra University (UPF)
  • University of Nova Gorica
  • University of Geneva

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

68 Citations (Scopus)

Résumé

The Large Area Telescope on board the Fermi Gamma-ray Space Telescope has collected the largest ever sample of high-energy cosmic-ray electron and positron events since the beginning of its operation. Potential anisotropies in the arrival directions of cosmic-ray electrons or positrons could be a signature of the presence of nearby sources. We use almost seven years of data with energies above 42 GeV processed with the Pass 8 reconstruction. The present data sample can probe dipole anisotropies down to a level of 10-3. We take into account systematic effects that could mimic true anisotropies at this level. We present a detailed study of the event selection optimization of the cosmic-ray electrons and positrons to be used for anisotropy searches. Since no significant anisotropies have been detected on any angular scale, we present upper limits on the dipole anisotropy. The present constraints are among the strongest to date probing the presence of nearby young and middle-aged sources.

langue originaleAnglais
Numéro d'article091103
journalPhysical Review Letters
Volume118
Numéro de publication9
Les DOIs
étatPublié - 1 mars 2017

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