Present status of the 7–10 m telescope of CANGAROO II

Autor:	Shohei Yanagita, H. Muraishi, Yasushi Muraki, J. R. Patterson, M. Moriya, A. Yuki, Takanori Yoshikoshi, A. Kawachi, Kyoshi Nishijima, R. Susukita, Yoshihiko Mizumoto, S. Le Bohec, Masaki Mori, Tsuguya Naito, Jamie Holder, Tadashi Kifune, J. Jimbo, T. Hara, T. Tamura, Hidetoshi Kubo, Shuichi Gunji, Yutaka Matsubara, Gavin Rowell, Shinji Hara, Toru Tanimori, Tatsuo Yoshida, S. A. Dazeley, M. D. Roberts, J. Kushida, K. Sakurazawa
Rok vydání:	1999
Předmět:	Physics Aperture Astrophysics::High Energy Astrophysical Phenomena media_common.quotation_subject Astrophysics::Instrumentation and Methods for Astrophysics Astronomy Astronomy and Astrophysics Astrophysics::Cosmology and Extragalactic Astrophysics Astrophysics law.invention Telescope law Sky Astrophysics::Galaxy Astrophysics Cherenkov radiation media_common
Zdroj:	Scopus-Elsevier
ISSN:	0927-6505
DOI:	10.1016/s0927-6505(99)00063-8
Popis:	The Cherenkov telescope of the CANGAROO II project will start operation in 1999 in Woomera, South Australia, with a 7 m aperture using 60 plastic mirrors. The telescope, which can potentially be extended to a 10 m aperture, will be used to observe gamma-ray sources with an energy threshold of the order of 100 GeV in the southern sky.
Databáze:	OpenAIRE
Externí odkaz:	https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3de0aa58ee94ac9d2a64b74438411b10 https://doi.org/10.1016/s0927-6505(99)00063-8 Zobrazit plný text záznamu Full Text from ScienceDirect