Cangaroo-III search for gamma rays from Kepler's supernova remnant

被引：2

作者：

Enomoto, R. ^{[1
]}

Higashi, Y. ^{[2
]}

Yoshida, T. ^{[3
]}

Tanimori, T. ^{[2
]}

Bicknell, G. V. ^{[4
]}

Clay, R. W. ^{[5
]}

Edwards, P. G. ^{[6
]}

Gunji, S. ^{[7
]}

Hara, S. ^{[8
]}

Hara, T. ^{[9
]}

Hattori, T. ^{[10
]}

Hayashi, S. ^{[11
]}

Hirai, Y.

Inoue, K. ^{[7
]}

Kabuki, S. ^{[2
]}

Kajino, F. ^{[11
]}

Katagiri, H. ^{[12
]}

Kawachi, A. ^{[10
]}

Kifune, T. ^{[1
]}

Kiuchi, R. ^{[1
]}

Kubo, H. ^{[2
]}

Kushida, J. ^{[10
]}

Matsubara, Y. ^{[13
]}

Mizukami, T.

Mizumoto, Y. ^{[14
]}

Mizuniwa, R. ^{[10
]}

Mori, M. ^{[1
]}

Muraishi, H. ^{[15
]}

Muraki, Y.

Naito, T. ^{[9
]}

Nakamori, T.

Nakano, S. ^{[2
]}

Nishida, D. ^{[2
]}

Nishijima, K. ^{[10
]}

Ohishi, M. ^{[1
]}

Sakamoto, Y. ^{[10
]}

Seki, A. ^{[10
]}

Stamatescu, V.

Suzuki, T. ^{[3
]}

Swaby, D. L. ^{[5
]}

Thornton, G. ^{[5
]}

Tokanai, F. ^{[7
]}

Tsuchiya, K. ^{[16
]}

Watanabe, S. ^{[2
]}

Yamada, Y. ^{[11
]}

Yamazaki, E. ^{[10
]}

Yanagita, S.

Yoshikoshi, T. ^{[1
]}

Yukawa, Y. ^{[1
]}

机构：

[1] Univ Tokyo, Inst Cosm Ray Res, Chiba 2778582, Japan

[2] Kyoto Univ, Dept Phys, Sakyo Ku, Kyoto 6068502, Japan

[3] Ibaraki Univ, Fac Sci, Mito, Ibaraki 3108512, Japan

[4] Australian Natl Univ, Res Sch Astron & Astrophys, Weston, ACT 2611, Australia

[5] Univ Adelaide, Sch Chem & Phys, Adelaide, SA 5005, Australia

[6] CSIRO, Australia Telescope Natl Facil, Narrabri, NSW 2390, Australia

[7] Yamagata Univ, Dept Phys, Yamagata 9908560, Japan

[8] Ibaraki Prefectural Univ Hlth Sci, Ami, Ibaraki 3000394, Japan

[9] Yamanashi Gakuin Univ, Fac Management Informat, Yamanashi 4008575, Japan

[10] Tokai Univ, Dept Phys, Kanagawa 2591292, Japan

[11] Konan Univ, Dept Phys, Kobe, Hyogo 6588501, Japan

[12] Hiroshima Univ, Dept Phys Sci, Hiroshima 7398526, Japan

[13] Nagoya Univ, Solar Terr Environm Lab, Aichi 4648602, Japan

[14] Natl Inst Nat Sci, Natl Astron Observ Japan, Mitaka, Tokyo 1818588, Japan

[15] Kitasato Univ, Sch Allied Hlth Sci, Kanagawa 2288555, Japan

[16] Natl Res Inst Police Sci, Kashiwa, Chiba 2770882, Japan

来源：

ASTROPHYSICAL JOURNAL | 2008年 / 683卷 / 01期

关键词：

gamma rays : observations; supernovae : individual (Kepler's SNR);

D O I：

10.1086/589912

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Kepler's supernova, discovered in 1604 October, produced a remnant that has been well studied observationally in the radio, infrared, optical, and X-ray bands, and theoretically. Some models have predicted a TeV gamma-ray flux that is detectable with current Imaging Cerenkov Atmospheric Telescopes. We report on observations carried out in 2005 April with the CANGAROO-III Telescope. No statistically significant excess was observed, and limitations on the allowed parameter range in the model are discussed.

引用

页码：383 / 388

页数：6

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