Please use this identifier to cite or link to this item: https://hdl.handle.net/2440/47638
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Type: Journal article
Title: Observation of very high energy gamma rays from HESS J1804-216 with CANGAROO-III telescopes
Author: Higashi, Y.
Kubo, H.
Yoshida, T.
Enomoto, R.
Tanimori, T.
Edwards, P.
Naito, T.
Bicknell, G.
Clay, R.
Gunji, S.
Hara, S.
Hara, T.
Hattori, T.
Hayashi, S.
Hirai, Y.
Inoue, K.
Kabuki, S.
Kajino, F.
Katagiri, H.
Kawachi, A.
et al.
Citation: The Astrophysical Journal: an international review of astronomy and astronomical physics, 2008; 683(2):957-966
Publisher: Univ Chicago Press
Issue Date: 2008
ISSN: 0004-637X
1538-4357
Statement of
Responsibility: 
Y. Higashi, H. Kubo, T. Yoshida, R. Enomoto, T. Tanimori, P. G. Edwards, T. Naito, G. V. Bicknell, R. W. Clay, S. Gunji, S. Hara, T. Hara, T. Hattori, S. Hayashi, Y. Hirai, K. Inoue, S. Kabuki, F. Kajino, H. Katagiri, A. Kawachi, T. Kifune, R. Kiuchi, J. Kushida, Y. Matsubara, T. Mizukami, Y. Mizumoto, R. Mizuniwa, M. Mori, H. Muraishi, Y. Muraki, T. Nakamori, S. Nakano, D. Nishida, K. Nishijima, M. Ohishi, Y. Sakamoto, A. Seki, V. Stamatescu, T. Suzuki, D. L. Swaby, G. Thornton, F. Tokanai, K. Tsuchiya, S. Watanabe, Y. Yamada, E. Yamazaki, S. Yanagita, . Yoshikoshi and Y. Yukawa
Abstract: We observed the unidentified TeV gamma-ray source HESS J1804-216 with the CANGAROO-III atmospheric Cerenkov telescopes from 2006 May to July. We detected very high energy gamma rays above 600 GeV at the 10 σ level in an effective exposure of 76 hr. We obtained a differential flux of (5.0 ± 1.5stat ± 1.6sys) × 10-12 (E/1 TeV)-α cm-2 s-1 TeV-1 with a photon index a of 2.69 ± 0.30stat ± 0.34sys, which is consistent with that of the H.E.S.S. observation in 2004. We also confirm the extended morphology of the source. By combining our result with multiwavelength observations, we discuss the possible counterparts of HESS J1804-216 and the radiation mechanism based on leptonic and hadronic processes for a supernova remnant and a pulsar wind nebula. © 2008. The American Astronomical Society.All rights reserved.
Description: Copyright © 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A.
DOI: 10.1086/589877
Grant ID: ARC
Published version: http://dx.doi.org/10.1086/589877
Appears in Collections:Aurora harvest 6
Chemistry and Physics publications

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