Design study of CANGAROO-III, stereoscopic imaging atmospheric Cherenkov telescopes for sub-TeV γ-ray detection

R. Enomoto*, S. Hara, A. Asahara, G. V. Bicknell, P. G. Edwards, S. Gunji, T. Hara, J. Jimbo, F. Kajino, H. Katagiri, J. Kataoka, A. Kawachi, T. Kifune, H. Kubo, J. Kushida, Y. Matsubara, Y. Mizumoto, M. Mori, M. Moriya, H. MuraishiY. Muraki, T. Naito, T. Nakase, K. Nishijima, K. Okumura, J. R. Patterson, K. Sakurazawa, D. L. Swaby, K. Takano, T. Tanimori, T. Tamura, K. Tsuchiya, K. Uruma, S. Yanagita, T. Yoshida, T. Yoshikoshi, A. Yuki

*この研究の対応する著者

研究成果査読

52 被引用数 (Scopus)

抄録

CANGAROO-III is an imaging atmospheric Cherenkov telescope array of four 10-m telescopes for very high energy (sub-TeV) γ-ray astronomy. A design study of the CANGAROO-III telescope system was carried out using the Monte Carlo technique in order to optimize the pixel size and the telescope spacing. Studies were also made of observations at low elevation angles.

本文言語English
ページ(範囲)235-244
ページ数10
ジャーナルAstroparticle Physics
16
3
DOI
出版ステータスPublished - 2002 1
外部発表はい

ASJC Scopus subject areas

  • 天文学と天体物理学

フィンガープリント

「Design study of CANGAROO-III, stereoscopic imaging atmospheric Cherenkov telescopes for sub-TeV γ-ray detection」の研究トピックを掘り下げます。これらがまとまってユニークなフィンガープリントを構成します。

引用スタイル