Status of the Ashra project

M. Sasaki; Y. Aita; Y. Arai; Y. Asaoka; T. Chonan; S. Dye; R. Fox; S. Fukagawa; G. Guillian; J. Hamilton; Y. Hsiung; M. Huang; M. Jobashi; T. Kimura; H. Kuze; J. Learned; N. Manago; S. Matsuno; K. Noda; Y. Ogawa; A. Okumura; N. Sugiyama; M. Wang; Y. Watanabe; M. Yasuda

Status of the Ashra project

M. Sasaki, Y. Aita, Y. Arai, Y. Asaoka, T. Chonan, S. Dye, R. Fox, S. Fukagawa, G. Guillian, J. Hamilton, Y. Hsiung, M. Huang, M. Jobashi, T. Kimura, H. Kuze, J. Learned, N. Manago, S. Matsuno, K. Noda, Y. OgawaA. Okumura, N. Sugiyama, M. Wang, Y. Watanabe, M. Yasuda

研究成果: Paper › 査読

1 被引用数 (Scopus)

抄録

The All-sky Survey High Resolution Air shower detector (Ashra) is primarily designed to elucidate transient objects such as Gamma Ray Bursts not only detecting optical lights but also simultaneously TeV, PeV neutrinos, and EeV cosmic rays. Ashra records images in unprecedented arc-minute detail of high-energy cosmic particle interactions in the atmosphere using new wide angle high resolution optics, Image Intensifier and CMOS technology. A first run of data taking with prototype versions of the optical and the trigger systems took place in 2004-2005, allowing us to evaluate the performance of the systems and to approach an analysis strategy. Full configuration of the Mauna Loa site will be reached by 2006. We will illustrate the summary of the Ashra project and the pilot data with the analysis for optical transient and TeV-ray search.

本文言語	English
ページ	197-200
ページ数	4
出版ステータス	Published - 2005 1月 1
外部発表	はい
イベント	29th International Cosmic Ray Conference, ICRC 2005 - Pune, India 継続期間: 2005 8月 3 → 2005 8月 10

Other

Other	29th International Cosmic Ray Conference, ICRC 2005
国/地域	India
City	Pune
Period	05/8/3 → 05/8/10

ASJC Scopus subject areas

核物理学および高エネルギー物理学

他のファイルとリンク

引用スタイル

Sasaki, M, Aita, Y, Arai, Y, Asaoka, Y, Chonan, T, Dye, S, Fox, R, Fukagawa, S, Guillian, G, Hamilton, J, Hsiung, Y, Huang, M, Jobashi, M, Kimura, T, Kuze, H, Learned, J, Manago, N, Matsuno, S, Noda, K, Ogawa, Y, Okumura, A, Sugiyama, N, Wang, M, Watanabe, Y & Yasuda, M 2005, 'Status of the Ashra project', Paper presented at 29th International Cosmic Ray Conference, ICRC 2005, Pune, India, 05/8/3 - 05/8/10 pp. 197-200.

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abstract = "The All-sky Survey High Resolution Air shower detector (Ashra) is primarily designed to elucidate transient objects such as Gamma Ray Bursts not only detecting optical lights but also simultaneously TeV, PeV neutrinos, and EeV cosmic rays. Ashra records images in unprecedented arc-minute detail of high-energy cosmic particle interactions in the atmosphere using new wide angle high resolution optics, Image Intensifier and CMOS technology. A first run of data taking with prototype versions of the optical and the trigger systems took place in 2004-2005, allowing us to evaluate the performance of the systems and to approach an analysis strategy. Full configuration of the Mauna Loa site will be reached by 2006. We will illustrate the summary of the Ashra project and the pilot data with the analysis for optical transient and TeV-ray search.",

author = "M. Sasaki and Y. Aita and Y. Arai and Y. Asaoka and T. Chonan and S. Dye and R. Fox and S. Fukagawa and G. Guillian and J. Hamilton and Y. Hsiung and M. Huang and M. Jobashi and T. Kimura and H. Kuze and J. Learned and N. Manago and S. Matsuno and K. Noda and Y. Ogawa and A. Okumura and N. Sugiyama and M. Wang and Y. Watanabe and M. Yasuda",

year = "2005",

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AU - Sasaki, M.

AU - Aita, Y.

AU - Arai, Y.

AU - Asaoka, Y.

AU - Chonan, T.

AU - Dye, S.

AU - Fox, R.

AU - Fukagawa, S.

AU - Guillian, G.

AU - Hamilton, J.

AU - Hsiung, Y.

AU - Huang, M.

AU - Jobashi, M.

AU - Kimura, T.

AU - Kuze, H.

AU - Learned, J.

AU - Manago, N.

AU - Matsuno, S.

AU - Noda, K.

AU - Ogawa, Y.

AU - Okumura, A.

AU - Sugiyama, N.

AU - Wang, M.

AU - Watanabe, Y.

AU - Yasuda, M.

PY - 2005/1/1

Y1 - 2005/1/1

N2 - The All-sky Survey High Resolution Air shower detector (Ashra) is primarily designed to elucidate transient objects such as Gamma Ray Bursts not only detecting optical lights but also simultaneously TeV, PeV neutrinos, and EeV cosmic rays. Ashra records images in unprecedented arc-minute detail of high-energy cosmic particle interactions in the atmosphere using new wide angle high resolution optics, Image Intensifier and CMOS technology. A first run of data taking with prototype versions of the optical and the trigger systems took place in 2004-2005, allowing us to evaluate the performance of the systems and to approach an analysis strategy. Full configuration of the Mauna Loa site will be reached by 2006. We will illustrate the summary of the Ashra project and the pilot data with the analysis for optical transient and TeV-ray search.

AB - The All-sky Survey High Resolution Air shower detector (Ashra) is primarily designed to elucidate transient objects such as Gamma Ray Bursts not only detecting optical lights but also simultaneously TeV, PeV neutrinos, and EeV cosmic rays. Ashra records images in unprecedented arc-minute detail of high-energy cosmic particle interactions in the atmosphere using new wide angle high resolution optics, Image Intensifier and CMOS technology. A first run of data taking with prototype versions of the optical and the trigger systems took place in 2004-2005, allowing us to evaluate the performance of the systems and to approach an analysis strategy. Full configuration of the Mauna Loa site will be reached by 2006. We will illustrate the summary of the Ashra project and the pilot data with the analysis for optical transient and TeV-ray search.

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T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -

Status of the Ashra project

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ASJC Scopus subject areas

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