Medium-scale anisotropies measured by Telescope Array surface detectors

The Telescope Array (TA) experiment, the largest observatory for ultra-high energy cosmic rays in the Northern Hemisphere, has identified two medium-scale anisotropies: the TA Hotspot near the constellation Ursa Major and an excess in the direction of the Perseus-Pisces supercluster. Studying these medium-scale anisotropies may provide insights into the origins of ultra-high energy cosmic rays. This presentation will explore an oversampling analysis of TA surface detector data to evaluate these medium-scale event excesses and will present the latest findings on the TA Hotspot and the Perseus-Pisces supercluster excess.

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Publication Details

Published
2025-09-23
DOI
https://doi.org/10.22323/1.501.0302
Primary Topic
Adaptive optics and wavefront sensing
Type
article
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Medium-scale anisotropies measured by Telescope Array surface detectors

D. Ivanov, H. Sagawa, K. Kawata, Jihyun Kim et al.
Adaptive optics and wavefront sensing
article

Medium-scale anisotropies measured by Telescope Array surface detectors

D. Ivanov, H. Sagawa, K. Kawata, Jihyun Kim, Gordon Thomson
article en

Abstract

The Telescope Array (TA) experiment, the largest observatory for ultra-high energy cosmic rays in the Northern Hemisphere, has identified two medium-scale anisotropies: the TA Hotspot near the constellation Ursa Major and an excess in the direction of the Perseus-Pisces supercluster. Studying these medium-scale anisotropies may provide insights into the origins of ultra-high energy cosmic rays. This presentation will explore an oversampling analysis of TA surface detector data to evaluate these medium-scale event excesses and will present the latest findings on the TA Hotspot and the Perseus-Pisces supercluster excess.

Openalex Percentile: Top 79%
Adaptive optics and wavefront sensing
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