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.
Authors
- D. Ivanov (ORCID: https://orcid.org/0000-0002-4420-2830)
- H. Sagawa (ORCID: https://orcid.org/0000-0002-6900-7855)
- K. Kawata (ORCID: https://orcid.org/0000-0001-6332-2005)
- Jihyun Kim (ORCID: https://orcid.org/0000-0002-8814-031X)
- Gordon Thomson
Publication Details
- Published
- 2025-09-23
- DOI
- https://doi.org/10.22323/1.501.0302
- Primary Topic
- Adaptive optics and wavefront sensing
- Type
- article
- Field-Weighted Citation Impact
- 0.00