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Surface detectors of the TAx4 experiment

https://repo.qst.go.jp/records/85645
https://repo.qst.go.jp/records/85645
33d1989b-aed7-4076-aa99-be6e1fdbb23b
Item type 学術雑誌論文 / Journal Article(1)
公開日 2022-02-16
タイトル
タイトル Surface detectors of the TAx4 experiment
言語
言語 eng
資源タイプ
資源タイプ識別子 http://purl.org/coar/resource_type/c_6501
資源タイプ journal article
アクセス権
アクセス権 metadata only access
アクセス権URI http://purl.org/coar/access_right/c_14cb
著者 Telescope Array Collaboration, The

× Telescope Array Collaboration, The

WEKO 1030961

Telescope Array Collaboration, The

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Yukio, Uchihori

× Yukio, Uchihori

WEKO 1030962

Yukio, Uchihori

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Yukio, Uchihori

× Yukio, Uchihori

WEKO 1030963

en Yukio, Uchihori

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内容記述タイプ Abstract
内容記述 Telescope Array (TA) is the largest ultrahigh energy cosmic-ray (UHECR) observatory in the Northern Hemisphere. It explores the origin of UHECRs by measuring their energy spectrum, arrival-direction distribution, and mass composition using a surface detector (SD) array covering approximately 700 km and fluorescence detector (FD) stations. TA has found evidence for a cluster of cosmic rays with energies greater than 57 EeV. In order to confirm this evidence with more data, it is necessary to increase the data collection rate. We have begun building an expansion of TA that we call TAx4. In this paper, we explain the motivation, design, technical features, and expected performance of the TAx4 SD. We also present TAx4’s current status and examples of the data that have already been collected.
書誌情報 Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment

巻 1019, p. 165726, 発行日 2021-12
出版者
出版者 Elsevier
ISSN
収録物識別子タイプ ISSN
収録物識別子 0168-9002
DOI
識別子タイプ DOI
関連識別子 10.1016/j.nima.2021.165726
関連サイト
識別子タイプ URI
関連識別子 https://www.sciencedirect.com/science/article/pii/S0168900221007117#!
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