Update on the large-scale cosmic-ray anisotropy search at the highest energies by the Telescope Array Experiment

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  • uploaded June 25, 2021

Discussion timeslot (ZOOM-Meeting): 15. July 2021 - 12:00
ZOOM-Meeting URL: https://desy.zoom.us/j/92210078166
ZOOM-Meeting ID: 92210078166
ZOOM-Meeting Passcode: ICRC2021
Corresponding Session: https://icrc2021-venue.desy.de/channel/06-CR-Anisotropies-CRI/118
Live-Stream URL: https://icrc2021-venue.desy.de/livestream/Discussion-03/4

Abstract:
'Large-scale anisotropy at the highest energies is essential for the understanding the transition from cosmic rays of galactic origin to those of extra-galactic origin, along with the magnetic fields in the galaxy and those beyond. Motivated by a significant detection of the large-scale anisotropy above 8 EeV by the Pierre Auger Observatory (Auger), we have previously reported, using 11 years of Telescope Array (TA) surface array data, a result compatible with both that of Auger, and with a isotropic source distribution [ApJL, 898:L28, (2020)]. In this contribution, we will show latest results to search for the large-scale anisotropy at the highest energies.'

Authors: Toshihiro Fujii | for the Telescope Array Collaboration
Collaboration: Telescope Array

Indico-ID: 145
Proceeding URL: https://pos.sissa.it/395/291

Tags:
Presenter: Toshihiro Fujii

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