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Contribution Poster
Observation of VHE gamma rays from HESS J1804-216 with CANGAROO-III Telescopes
Speakers
- Mr. Yusuke HIGASHI
Primary authors
- Mr. Yusuke HIGASHI (Kyoto University)
Co-authors
- Geoffry V BICKNELL (Australian National University)
- Roger W CLAY (University of Adelaide)
- Philip G EDWARDS (Australia Telescope National Facility, CSIRO)
- Ryoji ENOMOTO (Institute for Cosmic Ray Research, University of Tokyo)
- Shuichi GUNJI (Yamagata University)
- Satoshi HARA (Ibaraki Prefectural University of Health Sciences)
- Tadao HARA (Yamanashi Gakuin University)
- Takahiro HATTORI (Tokai University)
- Sei'ichi HAYASHI (Konan University)
- Yasufumi HIRAI (Ibaraki University)
- Kenji INOUE (Yamagata University)
- Chie ITOH (Ibaraki Prefectural University of Health Sciences)
- Shigeto KABUKI (Kyoto University)
- Fumiyoshi KAJINO (Konan University)
- Hidetoshi KATAGIRI (Hiroshima University)
- Akiko KAWACHI (Tokai University)
- Tadashi KIFUNE (Institute for Cosmic Ray Research, University of Tokyo)
- Ryuta KIUCHI (Institute for Cosmic Ray Research, UniveInstitute for Cosmic Ray Research, Univercity of Tokyo)
- Hidetoshi KUBO (Kyoto University)
- Junko KUSHIDA (Tokai University)
- Yutaka MATSUBARA (Solar-Terrestrial Environment Laboratory)
- Taku MIZUKAMI (Kyoto University)
- Yoshihiko MIZUMOTO (Dept. of Optical and Infrared Astronomy, National Astronomical Observatory, National Institutes of Natural Sciences)
- Ryoji MIZUNIWA (Tokai University)
- Masaki MORI (Institute for Cosmic Ray Research, University of Tokyo)
- Hiroshi MURAISHI (Kitasato University)
- Yasushi MURAKI (Solar-Terrestrial Environment Laboratory, Nagoya University)
- Tsuguya NAITO (Yamanashi Gakuin University)
- Takeshi NAKAMORI (Kyoto University)
- Shintaro NAKANO (Kyoto University)
- Daisuke NISHIDA (Kyoto University)
- Kyoshi NISHIJIMA (Tokai University)
- Michiko OHISHI (Institute for Cosmic Ray Research, University of Tokyo)
- Yukiko SAKAMOTO (Tokai University)
- Atsushi SEKI (Tokai University)
- Victor STAMATESCU (University of Adelaide)
- Toshitaka SUZUKI (Ibaraki University)
- David L SWABY (University of Adelaide)
- Toru TANIMORI (Kyoto University)
- Greg THORNTON (University of Adelaide)
- Fuyuki TOKANAI (Yamagata University)
- Ken'ichi TSUCHIYA (Kyoto University)
- Shio WATANABE (Kyoto University)
- Yosuke YAMADA (Konan University)
- Eiichi YAMAZAKI (Tokai University)
- Shohei YANAGITA (Ibarki University)
- Tatsuo YOSHIDA (Ibaraki University)
- Takanori YOSHIKOSHI (Institute for Cosmic Ray Research, University of Tokyo)
- Yohei YUKAWA (Institute for Cosmic Ray Research, University of Tokyo)
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Abstract content
The H.E.S.S. collaboration has reported the detection of gamma-ray emission from eight new sources located in the Galactic Plane. HESS J1804-216 is one of the brightest of them, and its size and photon index make it one of the largest and softest sources. The H.E.S.S. collaboration proposed two possible counter parts, young Vela-like pulsar B1800-21 and the SNR G8.7-0.1, but it does not perfectly line up with them. Recently, the discovery of new supernova remnant, G8.31-0.09, with radio observation was reported,which located within the error circle of H.E.S.S., but more compact in size. Suzaku deep observations discovered new two X-ray sources, centered on the HESS J1804-216.Using SWIFT data found three faint X-ray sources in the region of HESS J1804-216, one of them near its center.
We observed HESS J1804-216 with CANGAROO-III telescopes from May to July in 2006.We detected gamma-ray signals with more than 5 sigma level during an effective exposure of 74.8 hours. The differential flux is consistent with that of H.E.S.S.. Its morphology is under study, but it seems extended compared to our PSF.
If this papers is presented for a collaboration, please specify the collaboration
CANGAROO-III
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 2 (OG part 1), pages 645-648