Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/43736
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Type: Journal article
Title: Cangaroo III search for gamma rays from Centaurus A and the ω Centauri region
Other Titles: Cangaroo III search for gamma rays from Centaurus A and the omega Centauri region
Author: Kabuki, S.
Enomoto, R.
Bicknell, G.
Clay, R.
Edwards, P.
Gunji, S.
Hara, S.
Hattori, T.
Hayashi, S.
Higashi, T.
Inoue, R.
Itoh, C.
Kajino, F.
Katagiri, H.
Kawachi, A.
Kawasaki, S.
Kifune, T.
Kiuchi, R.
Konno, K.
Kubo, H.
et al.
Citation: Astrophysical Journal, 2007; 668(2):968-973
Publisher: Univ Chicago Press
Issue Date: 2007
ISSN: 0004-637X
1538-4357
Statement of
Responsibility: 
S.Kabuki, R.Enomoto...R.W. Clay...Y. Yukawa, et al., and the CANGAROO-III collaboration
Abstract: We have observed the giant radio galaxy Centaurus A and the globular cluster ω Centauri in the TeV energy region using the CANGAROO III stereoscopic system. The system has been in operation since 2004 with an array of four Imaging Atmospheric Cerenkov Telescopes (IACT) with 100 m spacings. The observations were carried out in 2004 March and April. In total, approximately 10 hr of data were obtained for each target. No statistically significant gamma-ray signal has been found above 420 GeV over a wide angular region (a 1° radius from the pointing center), and we derive flux upper limits using the wholefield of view. Implications for the total energy of cosmic rays and the density of the cold dark matter are considered.
Rights: Copyright © IOP Publishing 2007. Submitted to Cornell University’s online archive www.arXiv.org in 2007 by Ryoji Enomoto. Post-print sourced from www.arxiv.org.
RMID: 0020073036
DOI: 10.1086/520767
Published version: http://arxiv.org/abs/0706.0367
Appears in Collections:Chemistry and Physics publications

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