课题基金 / 基金详情

University of Utah - Operation of the Telescope Array, TALE, and the TAx4 Expansion

University of Utah - Operation of the Telescope Array, TALE, and the TAx4 Expansion
犹他大学 - 望远镜阵列、TALE 和 TAx4 扩展的操作
批准号:
1712517
负责人:
Charles Jui
金额:
$242.41万
依托单位:
依托单位国家:
美国
项目类别:
Continuing Grant
财政年份:
2017
资助国家:
美国
项目状态:
已结题
起止时间:
2017-08-01 至 2020-07-31

项目摘要

项目成果

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中文摘要
翻译
宇宙射线是来自太空的高能亚原子粒子,以接近光速的速度传播。宇宙射线的起源及其加速机制尚不清楚,但它们可能起源于银河系内外的极端天体物理现象。望远镜阵列(TA)是北半球最大的宇宙射线天文台。TA位于犹他州德尔塔外,代表了美日联合努力,旨在研究宇宙中最高能量粒子的性质和起源。这笔授予犹他大学的奖金将支持TA的持续运行、TA低能量扩展(TALE)和扩展后的天文台(TAx4)上线。犹他大学是TA的主办机构,因此在TA的日常运作中起着关键作用。该奖项还将支持犹他大学小组参与天体物理科学项目整合研究和教育(ASPIRE)计划,该计划通过交互式教育材料网站和访问当地学校吸引地区教师、学生和公众。该小组还将在受益于TA位置和基础设施的其他领域主持相关实验。TA实验的主要目的是测量最高能量宇宙射线的能量和空间分布以及化学成分,以解决超高能量宇宙射线的性质和起源问题。犹他大学的宇宙射线物理小组在TA的设计、集成、部署、操作和管理方面发挥着关键作用。这些努力包括设施和探测器的维护,观察班次的人员配备,数据处理,模拟和分析,以及遵守土地管理局的规定。
英文摘要
Cosmic rays are highly energetic sub-atomic particles from space that travel at velocities near the speed of light. The origin of cosmic rays and their acceleration mechanisms are unknown, but they likely originate in extreme astrophysical phenomena both within and beyond our galaxy. The Telescope Array (TA) is the largest cosmic ray observatory in the northern hemisphere. Located outside Delta, Utah, and representing a joint US-Japanese effort, TA was designed to study the nature and origin of the highest energy particles in the Universe. This award to the University of Utah supports the continued operation of TA, the TA Low Energy extension (TALE), and the expanded observatory (TAx4) as it comes online. The University of Utah is the host institution for TA and therefore plays a critical role in its daily operation. This award will also support the University of Utah group's involvement in the Astrophysics Science Project Integrating Research and Education (ASPIRE) program, which engages area teachers, students, and the public through a web site of interactive educational materials and visits to local schools. The group will also host associated experiments in other fields that benefit from the TA location and infrastructure.The primary objectives of the TA experiment are to measure the energy and spatial distributions, and the chemical composition of the highest energy cosmic rays in order to address the nature and origin of ultra-high energy cosmic rays. The cosmic ray physics group at the University of Utah plays critical roles in the design, integration, deployment, operation, and management of TA. These efforts include facility and detector maintenance, staffing for observing shifts, data handling, simulation and analysis, and maintaining compliance with the Bureau of Land Management regulations.
期刊论文(20)
专著(0)
科研奖励(0)
会议论文
DOI: 10.1093/mnras/stz3618
发表时间: 2019-03
期刊: Monthly Notices of the Royal Astronomical Society
影响因子: 4.8
作者: [R. Abbasi;M. Abe;T. Abu-Zayyad;M. Allen;R. Azuma;E. Barcikowski;J. Belz;D. Bergman;S. Blake;R. Cady;B. Cheon;J. Chiba;M. Chikawa;A.diMatteo;T. Fujii;K. Fujita;R. Fujiwara;M. Fukushima;G. Furlich;W. Hanlon;M. Hayashi;Y. Hayashi;N. Hayashida;K. Hibino;K. Honda;D. Ikeda;N. Inoue;T. Ishii;R. Ishimori;H. Ito;D. Ivanov;H. Jeong;S. Jeong;C. Jui;K. Kadota;F. Kakimoto;O. Kalashev;K. Kasahara;H. Kawai;S. Kawakami;S. Kawana;K. Kawata;E. Kido;H. Kim;J. H. Kim;S. Kishigami;S. Kitamura;Y. Kitamura;V. Kuzmin;Mikhail V. Kuznetsov;Y. Kwon;K. H. Lee;B. Lubsandorzhiev;J. Lundquist;K. Machida;K. Martens;T. Matsuyama;J. Matthews;R. Mayta;M. Minamino;K. Mukai;I. Myers;K. Nagasawa;S. Nagataki;K. Nakai;R. Nakamura;T. Nakamura;T. Nonaka;H. Oda;S. Ogio;J. Ogura;M. Ohnishi;H. Ohoka;T. Okuda;Y. Omura;M. Ono;R. Onogi;A. Oshima;S. Ozawa;I. H. Park;M. Pshirkov;J. Remington;D. Rodriguez;G. Rubtsov;D. Ryu;H. Sagawa;R. Sahara;K. Saito;Y. Saito;N. Sakaki;T. Sako;N. Sakurai;L. Scott;T. Seki;K. Sekino;P. Shah;F. Shibata;T. Shibata;H. Shimodaira;B. Shin;H. Shin;J. Smith;P. Sokolsky;B. Stokes;S. Stratton;T. Stroman;T. Suzawa;Y. Takagi;Y. Takahashi;M. Takamura;M. Takeda;R. Takeishi;A. Taketa;M. Takita;Y. Tameda;H. Tanaka;Kiyoshi Tanaka;M. Tanaka;Y. Tanoue;S. Thomas;G. Thomson;P. Tinyakov;I. Tkachev;H. Tokuno;T. Tomida;S. Troitsky;Y. Tsunesada;K. Tsutsumi;Y. Uchihori;S. Udo;F. Urban;T. Wong;K. Yada;M. Yamamoto;H. Yamaoka;K. Yamazaki;J. Yang;K. Yashiro;H. Yoshii;Y. Zhezher;Z. Zundel]
通讯作者: R. Abbasi;M. Abe;T. Abu-Zayyad;M. Allen;R. Azuma;E. Barcikowski;J. Belz;D. Bergman;S. Blake;R. Cady;B. Cheon;J. Chiba;M. Chikawa;A.diMatteo;T. Fujii;K. Fujita;R. Fujiwara;M. Fukushima;G. Furlich;W. Hanlon;M. Hayashi;Y. Hayashi;N. Hayashida;K. Hibino;K. Honda;D. Ikeda;N. Inoue;T. Ishii;R. Ishimori;H. Ito;D. Ivanov;H. Jeong;S. Jeong;C. Jui;K. Kadota;F. Kakimoto;O. Kalashev;K. Kasahara;H. Kawai;S. Kawakami;S. Kawana;K. Kawata;E. Kido;H. Kim;J. H. Kim;S. Kishigami;S. Kitamura;Y. Kitamura;V. Kuzmin;Mikhail V. Kuznetsov;Y. Kwon;K. H. Lee;B. Lubsandorzhiev;J. Lundquist;K. Machida;K. Martens;T. Matsuyama;J. Matthews;R. Mayta;M. Minamino;K. Mukai;I. Myers;K. Nagasawa;S. Nagataki;K. Nakai;R. Nakamura;T. Nakamura;T. Nonaka;H. Oda;S. Ogio;J. Ogura;M. Ohnishi;H. Ohoka;T. Okuda;Y. Omura;M. Ono;R. Onogi;A. Oshima;S. Ozawa;I. H. Park;M. Pshirkov;J. Remington;D. Rodriguez;G. Rubtsov;D. Ryu;H. Sagawa;R. Sahara;K. Saito;Y. Saito;N. Sakaki;T. Sako;N. Sakurai;L. Scott;T. Seki;K. Sekino;P. Shah;F. Shibata;T. Shibata;H. Shimodaira;B. Shin;H. Shin;J. Smith;P. Sokolsky;B. Stokes;S. Stratton;T. Stroman;T. Suzawa;Y. Takagi;Y. Takahashi;M. Takamura;M. Takeda;R. Takeishi;A. Taketa;M. Takita;Y. Tameda;H. Tanaka;Kiyoshi Tanaka;M. Tanaka;Y. Tanoue;S. Thomas;G. Thomson;P. Tinyakov;I. Tkachev;H. Tokuno;T. Tomida;S. Troitsky;Y. Tsunesada;K. Tsutsumi;Y. Uchihori;S. Udo;F. Urban;T. Wong;K. Yada;M. Yamamoto;H. Yamaoka;K. Yamazaki;J. Yang;K. Yashiro;H. Yoshii;Y. Zhezher;Z. Zundel
DOI: 10.1103/physrevd.98.022002
发表时间: 2018-04
期刊: EPJ Web of Conferences
影响因子: --
作者: [Telescope Array Collaboration R.U. Abbasi;M. Abe;T. Abu-Zayyad;M. Allen;R. Azuma;E. Barcikowski;J. Belz;D. Bergman;S. Blake;R. Cady;B. Cheon;J. Chiba;M. Chikawa;A. Matteo;T. Fujii;K. Fujita;M. Fukushima;G. Furlich;T. Goto;W. Hanlon;M. Hayashi;Y. Hayashi;N. Hayashida;K. Hibino;K. Honda;D. Ikeda;N. Inoue;T. Ishii;R. Ishimori;H. Ito;D. Ivanov;H. Jeong;S. Jeong;C. Jui;K. Kadota;F. Kakimoto;O. Kalashev;K. Kasahara;H. Kawai;S. Kawakami;S. Kawana;K. Kawata;E. Kido;H. Kim;J. Kim;S. Kishigami;S. Kitamura;Y. Kitamura;V. Kuzmin;M. Kuznetsov;Y. Kwon;K. H. Lee;B. Lubsandorzhiev;J. Lundquist;K. Machida;K. Martens;T. Matsuyama;J. Matthews;R. Mayta;M. Minamino;K. Mukai;I. Myers;K. Nagasawa;S. Nagataki;R. Nakamura;T. Nakamura;T. Nonaka;H. Oda;S. Ogio;J. Ogura;M. Ohnishi;H. Ohoka;T. Okuda;Y. Omura;M. Ono;R. Onogi;A. Oshima;S. Ozawa;I. Park;M. Pshirkov;J. Remington;D. Rodriguez;G. Rubtsov;D. Ryu;H. Sagawa;R. Sahara;K. Saito;Y. Saito;N. Sakaki;N. Sakurai;L. Scott;T. Seki;K. Sekino;P. Shah;F. Shibata;T. Shibata;H. Shimodaira;B. Shin;H. Shin;J. Smith;P. Sokolsky;B. Stokes;S. Stratton;T. Stroman;T. Suzawa;Y. Takagi;Y. Takahashi;M. Takamura;M. Takeda;R. Takeishi;A. Taketa;M. Takita;Y. Tameda;H. Tanaka;K. Tanaka;M. Tanaka;S. Thomas;G. Thomson;P. Tinyakov;I. Tkachev;H. Tokuno;T. Tomida;S. Troitsky;Y. Tsunesada;K. Tsutsumi;Y. Uchihori;S. Udo;F. Urban;T. Wong;M. Yamamoto;R. Yamane;H. Yamaoka;K. Yamazaki;J. Yang;K. Yashiro;Y. Yoneda;S. Yoshida;H. Yoshii;Y. Zhezher;Z. Institute;D. Physics;Astronomy;U. Utah;Salt lake City;Utah.;Usa;T. Z. F. O. Science;Engineering;Saitama University;Saitama;Japan.;Graduate School of Science;Tokyo Institute of Technology;Meguro;Tokyo;T. Z. F. O. Science;Hanyang University;Seongdong-gu;Seoul.;J Korea;Tokyo University of Science;Noda;Chiba;K. University;Higashi Osaka;Osaka;Service de Physique Th'eorique;Universit́e Libre de Bruxelles;Brussels;Belgium;Inst. for Nucl. Research;U. Tokyo;Kashiwa;O. University;K. I. F. T. Physics;Mathematics of the Universe;Todai Institutes for Advanced Study;Information Science;Technology;Shinshu University;Nagano;Faculty of Electrical Engineering;Kanagawa University;Yokohama;Kanagawa;Interdisciplinary Graduate School of Medicine;University of Yamanashi;Kofu;Yamanashi;Astrophysical Big Bang Laboratory;Riken;Wako;S. University;Jang-an-gu;Suwon;T. University;Setagaya-ku;Institute for Nuclear Research of the Russian Academy of Sciences-Institute-for-Nuclear-Research-of-the-Russian-of-1381645366;Moscow;Russia.;Advanced Research Institute for Science;W. University;Shinjuku-ku;C. University;School of Physical Sciences;Ulsan National Institute of Science;UNIST-gil;Ulsan;Y. University;Seodaemun-gu;A. G. S. O. Science;Technology Institute of Engineering;Faculty of Computer Science;K. University;Kochi;D. Sciences;R. University;Kusatsu;Shiga;Sternberg Astronomical Institute;M. University;Rutgers University - The State University of New Jersey-Rutgers-University-The-State-University-of-New-1388356903;Piscataway;N. Jersey.;E. R. Institute;Bunkyo-ku;Department of Materials Science;O. University;Neyagawa-shi;G. S. O. Sciences;H. University;Hiroshima;Institute of Particle;Nuclear Studies;Kek;Tsukuba;Ibaraki;National Institute of Advanced Industrial Science;Ceico;I. Physics;Czech Academy of Sciences;Prague;Czech Republic;Institute for Fundamental Physics of the Universe;Ewha Womans University;Seodaaemun-gu;E. University;Matsuyama;Ehime]
通讯作者: Telescope Array Collaboration R.U. Abbasi;M. Abe;T. Abu-Zayyad;M. Allen;R. Azuma;E. Barcikowski;J. Belz;D. Bergman;S. Blake;R. Cady;B. Cheon;J. Chiba;M. Chikawa;A. Matteo;T. Fujii;K. Fujita;M. Fukushima;G. Furlich;T. Goto;W. Hanlon;M. Hayashi;Y. Hayashi;N. Hayashida;K. Hibino;K. Honda;D. Ikeda;N. Inoue;T. Ishii;R. Ishimori;H. Ito;D. Ivanov;H. Jeong;S. Jeong;C. Jui;K. Kadota;F. Kakimoto;O. Kalashev;K. Kasahara;H. Kawai;S. Kawakami;S. Kawana;K. Kawata;E. Kido;H. Kim;J. Kim;S. Kishigami;S. Kitamura;Y. Kitamura;V. Kuzmin;M. Kuznetsov;Y. Kwon;K. H. Lee;B. Lubsandorzhiev;J. Lundquist;K. Machida;K. Martens;T. Matsuyama;J. Matthews;R. Mayta;M. Minamino;K. Mukai;I. Myers;K. Nagasawa;S. Nagataki;R. Nakamura;T. Nakamura;T. Nonaka;H. Oda;S. Ogio;J. Ogura;M. Ohnishi;H. Ohoka;T. Okuda;Y. Omura;M. Ono;R. Onogi;A. Oshima;S. Ozawa;I. Park;M. Pshirkov;J. Remington;D. Rodriguez;G. Rubtsov;D. Ryu;H. Sagawa;R. Sahara;K. Saito;Y. Saito;N. Sakaki;N. Sakurai;L. Scott;T. Seki;K. Sekino;P. Shah;F. Shibata;T. Shibata;H. Shimodaira;B. Shin;H. Shin;J. Smith;P. Sokolsky;B. Stokes;S. Stratton;T. Stroman;T. Suzawa;Y. Takagi;Y. Takahashi;M. Takamura;M. Takeda;R. Takeishi;A. Taketa;M. Takita;Y. Tameda;H. Tanaka;K. Tanaka;M. Tanaka;S. Thomas;G. Thomson;P. Tinyakov;I. Tkachev;H. Tokuno;T. Tomida;S. Troitsky;Y. Tsunesada;K. Tsutsumi;Y. Uchihori;S. Udo;F. Urban;T. Wong;M. Yamamoto;R. Yamane;H. Yamaoka;K. Yamazaki;J. Yang;K. Yashiro;Y. Yoneda;S. Yoshida;H. Yoshii;Y. Zhezher;Z. Institute;D. Physics;Astronomy;U. Utah;Salt lake City;Utah.;Usa;T. Z. F. O. Science;Engineering;Saitama University;Saitama;Japan.;Graduate School of Science;Tokyo Institute of Technology;Meguro;Tokyo;T. Z. F. O. Science;Hanyang University;Seongdong-gu;Seoul.;J Korea;Tokyo University of Science;Noda;Chiba;K. University;Higashi Osaka;Osaka;Service de Physique Th'eorique;Universit́e Libre de Bruxelles;Brussels;Belgium;Inst. for Nucl. Research;U. Tokyo;Kashiwa;O. University;K. I. F. T. Physics;Mathematics of the Universe;Todai Institutes for Advanced Study;Information Science;Technology;Shinshu University;Nagano;Faculty of Electrical Engineering;Kanagawa University;Yokohama;Kanagawa;Interdisciplinary Graduate School of Medicine;University of Yamanashi;Kofu;Yamanashi;Astrophysical Big Bang Laboratory;Riken;Wako;S. University;Jang-an-gu;Suwon;T. University;Setagaya-ku;Institute for Nuclear Research of the Russian Academy of Sciences-Institute-for-Nuclear-Research-of-the-Russian-of-1381645366;Moscow;Russia.;Advanced Research Institute for Science;W. University;Shinjuku-ku;C. University;School of Physical Sciences;Ulsan National Institute of Science;UNIST-gil;Ulsan;Y. University;Seodaemun-gu;A. G. S. O. Science;Technology Institute of Engineering;Faculty of Computer Science;K. University;Kochi;D. Sciences;R. University;Kusatsu;Shiga;Sternberg Astronomical Institute;M. University;Rutgers University - The State University of New Jersey-Rutgers-University-The-State-University-of-New-1388356903;Piscataway;N. Jersey.;E. R. Institute;Bunkyo-ku;Department of Materials Science;O. University;Neyagawa-shi;G. S. O. Sciences;H. University;Hiroshima;Institute of Particle;Nuclear Studies;Kek;Tsukuba;Ibaraki;National Institute of Advanced Industrial Science;Ceico;I. Physics;Czech Academy of Sciences;Prague;Czech Republic;Institute for Fundamental Physics of the Universe;Ewha Womans University;Seodaaemun-gu;E. University;Matsuyama;Ehime
Testing a Reported Correlation between Arrival Directions of Ultra-high-energy Cosmic Rays and a Flux Pattern from nearby Starburst Galaxies using Telescope Array Data
使用望远镜阵列数据测试超高能宇宙射线到达方向与附近星爆星系通量模式之间的相关性
DOI: 10.3847/2041-8213/aaebf9
发表时间: 2018
期刊: The astrophysical journal
影响因子: --
作者: [Abbasi RU]
通讯作者: Abbasi RU
Constraints on the diffuse photon flux with energies above 10^18 eV using the surface detector of the Telescope Array experiment
使用望远镜阵列实验的表面探测器对能量高于10^18 eV的漫射光子通量的约束
DOI: 10.1016/j.astropartphys.2019.03.003
发表时间: 2019
期刊: Astroparticle physics
影响因子: 3.5
作者: [Abbasi RU]
通讯作者: Abbasi RU
18
    Analysis of Data from the Telescope Array Observatory
    • 批准号:
      2310163
    • 项目类别:
      Standard Grant
    • 资助金额:
      $40.0万
    • 财政年份:
      2023
    • 负责人:
      Charles Jui
    • 依托单位:
    Operation of the Telescope Array Observatory
    • 批准号:
      2209583
    • 项目类别:
      Continuing Grant
    • 资助金额:
      $230.0万
    • 财政年份:
      2022
    • 负责人:
      Charles Jui
    • 依托单位:
    Analysis of Data from the Telescope Array Observatory
    • 批准号:
      2209584
    • 项目类别:
      Standard Grant
    • 资助金额:
      $31.0万
    • 财政年份:
      2022
    • 负责人:
      Charles Jui
    • 依托单位:
    Operation of the Telescope Array Observatory
    • 批准号:
      2112904
    • 项目类别:
      Standard Grant
    • 资助金额:
      $86.5万
    • 财政年份:
      2021
    • 负责人:
      Charles Jui
    • 依托单位:
    海外基金