Optical measurements with cooled CCD cameras for CANGAROO-III

Kiuchi, R.; Mori, M.; Kawachi, A.; Adachi, Y.; Asahara, A.; Bicknell, G. V.; Clay, R. W.; Doi, Y.; Edwards, P. G.; Enomoto, R.; Gunji, S.; Hara, S.; Hara, T.; Hattori, T.; Hayashi, S.; Higashi, Y.; Inoue, R.; Itoh, C.; Kabuki, S.; Kajino, F.; Katagiri, H.; Kawasaki, S.; Kifune, T.; Konno, K.; Ksenofontov, L. T.; Kubo, H.; Kushida, J.; Matsubara, Y.; Mizumoto, Y.; Muraishi, H.; Muraki, Y.; Naito, T.; Nakamori, T.; Nishida, D.; Nishijima, K.; Ohishi, M.; Patterson, J. R.; Protheroe, R. J.; Sakamoto, Y.; Sato, M.; Suzuki, S.; Suzuki, T.; Swaby, D. L.; Tanimori, T.; Tanimura, H.; Thornton, G.; Tsuchiya, K.; Watanabe, S.; Yamaoka, T.; Yamazaki, M.; Yanagita, S.; Yoshida, T.; Yoshikoshi, T.; Yuasa, M.; Yukawa, Y.

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Optical measurements with cooled CCD cameras for CANGAROO-III

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2005

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CANGAROO-III consists of four telescopes installed in Woomera, South Australia to observe celestial γ-ray sources by detecting Cherenkov light from air showers. Stereo observations have been performed since March 2004 with an improved angular resolution and a lower energy threshold. In this paper, we present some preliminary results of optical measurements by cooled CCD cameras.

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https://dspace-test.anu.edu.au/handle/1885/733743347

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Optical measurements with cooled CCD cameras for CANGAROO-III

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