Flux upper limits of diffuse TeV gamma rays from the Galactic plane using the effective area of the Tibet-II and -III arrays
文献类型：期刊论文
| 作者 | Amenomori, M.; Ayabe, S.; Cui, S. W.; Danzengluobu; Ding, L. K.; Ding, X. H.; Feng, C. F.; Feng, Z. Y.; Gao, X. Y.; Geng, Q. X. |
| 刊名 | ASTROPHYSICS
 |
| 出版日期 | 2006 |
| 卷号 | 37页码:1932-1937 |
| 关键词 | diffuse TeV gamma rays galactic plane flux upper limits |
| ISSN号 | 0273-1177 |
| DOI | 10.1016/j.asr.2005.08.049 |
| 英文摘要 | We obtained new upper limits on the diffuse gamma rays from the inner Galactic (IG) and outer Galactic (OG) planes in 3-10 TeV region, using the Tibet air shower data and new Monte Carlo simulation results. A difference of the effective area of the air-shower array for observing gamma rays and cosmic rays was carefully taken into account in this analysis, resulting in that the flux upper limits of the diffuse TeV gamma rays were reduced by factors of 4.0-3.7 for 3-10 TeV than those in our previous results (Amenomori, M., Ayabe, S., Cui, S.W., et al. Observation of multi-TeV diffuse gamma rays from the Galactic plane with the Tibet air shower array. Astrophys. J. 580, 887-895, 2002.). This new result suggests that the inverse power index of the energy spectrum of source electrons responsible for generating diffuse TeV gamma rays through inverse Compton effect should be steeper than 2.2 and 2.1 for IG and OG planes, respectively, with 99%C.L. (c) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved. |
| WOS关键词 | AIR SHOWER ARRAY ; EMISSION ; SPECTRUM |
| WOS研究方向 | Engineering ; Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
| 语种 | 英语 |
| WOS记录号 | WOS:000239306500018 |
| 出版者 | ELSEVIER SCIENCE LTD |
| 源URL | [http://119.78.100.186/handle/113462/26511]  |
| 专题 | 中国科学院近代物理研究所 |
| 通讯作者 | Yamamoto, Y. |
| 作者单位 | 1.Konan Univ, Dept Phys, Higashinada Ku, Kobe, Hyogo 6588501, Japan 2.Hirosaki Univ, Dept Phys, Hirosaki, Aomori 0368561, Japan 3.Saitama Univ, Dept Phys, Urawa, Saitama 3388570, Japan 4.Chinese Acad Sci, Inst High Energy Phys, Beijing 100039, Peoples R China 5.Tibet Univ, Dept Math & Phys, Lhasa 850000, Peoples R China 6.Shandong Univ, Dept Phys, Jinan 250100, Peoples R China 7.SW Jiaotong Univ, Inst Modern Phys, Chengdu 610031, Peoples R China 8.Yunnan Univ, Dept Phys, Kunming 650091, Peoples R China 9.Kanagawa Univ, Fac Engn, Yokohama, Kanagawa 2218686, Japan 10.Utsunomiya Univ, Fac Educ, Utsunomiya, Tochigi 3218505, Japan |
| 推荐引用方式 GB/T 7714 | Amenomori, M.,Ayabe, S.,Cui, S. W.,et al. Flux upper limits of diffuse TeV gamma rays from the Galactic plane using the effective area of the Tibet-II and -III arrays[J]. ASTROPHYSICS,2006,37:1932-1937. |
| APA | Amenomori, M..,Ayabe, S..,Cui, S. W..,Danzengluobu.,Ding, L. K..,...&Zhou, X. X..(2006).Flux upper limits of diffuse TeV gamma rays from the Galactic plane using the effective area of the Tibet-II and -III arrays.ASTROPHYSICS,37,1932-1937. |
| MLA | Amenomori, M.,et al."Flux upper limits of diffuse TeV gamma rays from the Galactic plane using the effective area of the Tibet-II and -III arrays".ASTROPHYSICS 37(2006):1932-1937. |
入库方式： OAI收割
来源：近代物理研究所
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