Recent Status Of The Analyses For Stereoscopic Observations With The Cangaroo-Iii Telescopes

T Tanimori,Yoshihiro Adachi,Akihiro Asahara,Geoffrey V Bicknell,R W Clay,Yohei Doi,Philip G Edwards,Ryoji Enomoto,Shuichi Gunji,Shinji Hara,Takefumi Hara,Takashi Hattori,Sei Hayashi,Yukihito Higashi,Rei Inoue,C Itoh,Shigeto Kabuki,F Kajino, H Katagiri,Akiko Kawachi,Saori Kawasaki, R Kifune,R Kiuchi,K Konno, T Ksenofontov,Hidetoshi Kubo, J Kushida,Yukihiro Matsubara,Yoshihiko Mizumoto,Masaki Mori, H Muraishi, Y Maraki,Takashi Naito,T Nakamori,D Nishida, K Nishijimi,Masatoshi Ohishi,John R Patterson,R J Protheroe,Yoshihiro Sakamoto,Makiko Sato,Sachiko Suzuki,Tohru Suzuki, D L Swaby,Hiroshi Tanimura,Greg Thornton,Kunihiko Tsuchiya,Satoshi Watanabe,Tomotaka Yamaoka,M Yamazaki, Shohei Yanagita,Teppei Yoshida,Takanori Yoshikoshi,Makoto Yuasa, Yohei Yukawa

Proceedings of the 29th International Cosmic Ray Conference, Vol 4: OG 2.1, 2.2 & 2.3（2005）

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摘要

CANGAROO-III is an array of four 10m-diameter imaging atmospheric Cherenkov telescopes to search for sub-TeV gamma-rays from celestial objects in collaboration with Japanese and Australian institutions, which is located in southern hemisphere (Woomera, South Australia). Three of four telescopes were made with the same design for stereo observation. We have started observations in stereo mode using those three telescopes since March 2004.We report the recent status of the analyses for stereo observations including several targets of which our previous data are inconsistent with the recent HESS results.

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