Orateur
Kazumasa Kawata
(ICRR, University of Tokyo)
Description
The Telescope Array (TA) is the largest ultra-high-energy cosmic-ray (UHECR) detector in the northern hemisphere, which consists of 507 surface detector (SD) covering a total 700 km^2 and three fluorescence detector stations. In this presentation, we will summarize recent results on the search for directional anisotropy of UHECRs using the latest data set collected by the TA SD array.
Auteur principal
Kazumasa Kawata
(ICRR, University of Tokyo)
