Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/12413
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Type: Journal article
Title: Present status of the 7-10 m telescope of CANGAROO II
Author: Yoshikoshi, T.
Dazeley, S.
Gunji, S.
Hara, S.
Hara, T.
Holder, J.
Jimbo, J.
Kawachi, A.
Kifune, T.
Kubo, H.
Kushida, J.
Bohec, S.
Matsubara, Y.
Mizumoto, Y.
Mori, M.
Moriya, M.
Muraishi, H.
Muraki, Y.
Naito, T.
Nishijima, K.
et al.
Citation: Astroparticle Physics, 1999; 11(1-2):267-269
Publisher: ELSEVIER SCIENCE BV
Issue Date: 1999
ISSN: 0927-6505
1873-2852
Abstract: 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.
DOI: 10.1016/S0927-6505(99)00063-8
Description (link): http://www.elsevier.com/wps/find/journaldescription.cws_home/523319/description#description
Published version: http://dx.doi.org/10.1016/s0927-6505(99)00063-8
Appears in Collections:Aurora harvest 7
Physics publications

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