EPJ Web of Conferences (Jan 2019)

TA Anisotropy Summary

  • Kawata K.,
  • di Matteo A.,
  • Fujii T.,
  • Ivanov D.,
  • Jui C.C.H.,
  • Lundquist J.P.,
  • Matthews J.N.,
  • Ogio S.,
  • Sagawa H.,
  • Thomson G.B.,
  • Tinyakov P.,
  • Tkachev I.,
  • Troitsky S.

DOI
https://doi.org/10.1051/epjconf/201921001004
Journal volume & issue
Vol. 210
p. 01004

Abstract

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The Telescope Array (TA) is the largest ultra-high-energy cosmic-ray (UHECR) detector in the northern hemisphere. It consists of an array of 507 surface detectors (SD) covering a total 700 km2 and three fluorescence detector stations overlooking the SD array. In this proceedings, we summarize recent results on the search for directional anisotropy of UHECRs using the latest dataset collected by the TA SD array. We obtained hints of the anisotropy of the UHECRs in the northern sky from the various analyses.