pith. sign in

arxiv: 1201.4964 · v3 · pith:OKPXQLSNnew · submitted 2012-01-24 · 🌌 astro-ph.IM

The surface detector array of the Telescope Array experiment

T. Abu-Zayyad , R. Aida , M. Allen , R. Anderson , R. Azuma , E. Barcikowski , J. W. Belz , D. R. Bergman
show 129 more authors
S. A. Blake R. Cady B. G. Cheon J. Chiba M. Chikawa E. J. Cho W. R. Cho H. Fujii T. Fujii T. Fukuda M. Fukushima D. Gorbunov W. Hanlon K. Hayashi Y. Hayashi N. Hayashida K. Hibino K. Hiyama K. Honda T. Iguchi D. Ikeda K. Ikuta N. Inoue T. Ishii R. Ishimori D. Ivanov S. Iwamoto C. C. H. Jui K. Kadota F. Kakimoto O. Kalashev T. Kanbe K. Kasahara H. Kawai S. Kawakami S. Kawana E. Kido H. B. Kim H. K. Kim J. H. Kim K. Kitamoto K. Kobayashi Y. Kobayashi Y. Kondo K. Kuramoto V. Kuzmin Y. J. Kwon S. I. Lim S. Machida K. Martens J. Martineau T. Matsuda T. Matsuura T. Matsuyama J. N. Matthews I. Myers M. Minamino K. Miyata H. Miyauchi Y. Murano T. Nakamura S. W. Nam T. Nonaka S. Ogio M. Ohnishi H. Ohoka K. Oki D. Oku T. Okuda A. Oshima S. Ozawa I. H. Park M. S. Pshirkov D. Rodriguez S. Y. Roh G. Rubtsov D. Ryu H. Sagawa N. Sakurai A. L. Sampson L. M. Scott P. D. Shah F. Shibata T. Shibata H. Shimodaira B. K. Shin J. I. Shin T. Shirahama J. D. Smith P. Sokolsky T. J. Sonley R. W. Springer B. T. Stokes S. R. Stratton T. A. Stroman S. Suzuki Y. Takahashi M. Takeda A. Taketa M. Takita Y. Tameda H. Tanaka K. Tanaka M. Tanaka S. B. Thomas G. B. Thomson P. Tinyakov I. Tkachev H. Tokuno T. Tomida S. Troitsky Y. Tsunesada K. Tsutsumi Y. Tsuyuguchi Y. Uchihori S. Udo H. Ukai G. Vasiloff Y. Wada T. Wong M. Wood Y. Yamakawa H. Yamaoka K. Yamazaki J. Yang S. Yoshida H. Yoshii R. Zollinger Z. Zundel
This is my paper
classification 🌌 astro-ph.IM
keywords arraysurfacedetectordetectorsexperimentfluorescenceobservationshower
0
0 comments X
read the original abstract

The Telescope Array (TA) experiment, located in the western desert of Utah,USA, is designed for observation of extensive air showers from extremely high energy cosmic rays. The experiment has a surface detector array surrounded by three fluorescence detectors to enable simultaneous detection of shower particles at ground level and fluorescence photons along the shower track. The TA surface detectors and fluorescence detectors started full hybrid observation in March, 2008. In this article we describe the design and technical features of the TA surface detector.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Ultraheavy Ultrahigh-Energy Cosmic Rays

    astro-ph.HE 2024-05 unverdicted novelty 7.0

    Ultraheavy nuclei have longer energy loss lengths at ≲300 EeV than lighter nuclei, allowing them to explain UHECRs above 100 EeV from sources like collapsars and neutron star mergers while predicting distinct shower maxima.

  2. Ultra-high energy event KM3-230213A as a cosmogenic neutrino in light of minimal UHECR flux models

    astro-ph.HE 2025-09 unverdicted novelty 4.0

    Minimal UHECR flux models from the Telescope Array predict cosmogenic neutrino fluxes consistent with the KM3-230213A event at the 2σ level.

  3. POEMMA (Probe of Extreme Multi-Messenger Astrophysics) design

    astro-ph.HE 2019-07 unverdicted novelty 3.0

    POEMMA is a proposed NASA probe-class mission designed to observe ultra-high energy cosmic rays and cosmic neutrinos from space.