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

被引:56
作者
Enomoto, R
Hara, S
Asahara, A
Bicknell, GV
Edwards, PG
Gunji, S
Hara, T
Jimbo, J
Kajino, F
Katagiri, H
Kataoka, J
Kawachi, A
Kifune, T
Kubo, H
Kushida, J
Matsubara, Y
Mizumoto, Y
Mori, M
Moriya, M
Muraishi, H
Muraki, Y
Naito, T
Nakase, T
Nishijima, K
Okumura, K
Patterson, JR
Sakurazawa, K
Swaby, DL
Takano, K
Tanimori, T
Tamura, T
Tsuchiya, K
Uruma, K
Yanagita, S
Yoshida, T
Yoshikoshi, T
Yuki, A
机构
[1] Univ Tokyo, ICRR, Chiba 2778582, Japan
[2] Tokyo Inst Technol, Meguro Ku, Tokyo 1528551, Japan
[3] Australian Natl Univ, Weston, ACT 2611, Australia
[4] ISAS, Sagamihara, Kanagawa 2298510, Japan
[5] Yamagata Univ, Dept Phys, Yamagata 9908560, Japan
[6] Yamanashi Gakuin Univ, Kofu, Yamanashi 4008575, Japan
[7] Tokai Univ, Hiratsuka, Kanagawa, Japan
[8] Konan Univ, Dept Phys, Kobe, Hyogo 6588501, Japan
[9] Kyoto Univ, Dept Phys, Sakyo ku, Kyoto 6068502, Japan
[10] Nagoya Univ, STE Lab, Nagoya, Aichi 4648602, Japan
[11] Natl Astronom Observ, Mitaka, Tokyo 1818588, Japan
[12] IPU, Ami, Ibaraki 3000394, Japan
[13] Univ Adelaide, Dept Phys & Math Phys, Adelaide, SA 5005, Australia
[14] Kanagawa Univ, Kanagawa 2218686, Japan
[15] Ibaraki Univ, Mito, Ibaraki 3108512, Japan
[16] OCU, Dept Phys, Osaka 5588585, Japan
关键词
imaging atmospheric Cherenkov telescope; stereoscopic observation; simulation; design study;
D O I
10.1016/S0927-6505(01)00112-8
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
CANGAROO-III is an imaging atmospheric Cherenkov telescope array of four 10-m telescopes for very high energy (sub-TeV) gamma-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. (C) 2002 Elsevier Science B.V. All rights reserved.
引用
收藏
页码:235 / 244
页数:10
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