中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
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. ; Guo, H. W. ; He, H. H. ; He, M. ; Hibino, K. ; Hotta, N. ; Hu, H. B. ; Huang, J. ; Huang, Q. ; Izumi, M ; Jia, H. Y. ; Kajino, F. ; Kasahara, K. ; Katayose, Y. ; Kato, C. ; Kawata, K. ; Labaciren, ; Le, G. M. ; Li, J.Y. ; Lu, H. ; Lu, S. L. ; Meng, X. R. ; Mizutani, K. ; Mu, J. ; Munakata, K. ; Nagai, A. ; Nanjo, H. ; Nishizawa, M. ; Ohnishi, M. ; Ohta, I. ; Onuma, H. ; Ouchi, T. ; Ozawa, S. ; Ren, J. R. ; Saito, T. ; Saito, T. Y. ; Sakata, M. ; Sasaki, T. ; Shibata, M. ; Shiomi, A. ; Shirai, T. ; Sugimoto, H. ; Takita, M. ; Tan, Y. H. ; Tateyama, N. ; Torii, S. ; Tsuchlya, H. ; Udo, S. ; Utsugi, T ; Wang, B.S. ; Wang, H. ; Wang, X. ; Wang, Y. G. ; Wu, H. R. ; Xue, L. ; Yamamoto, Y. ; Yan, C. T. ; Yang, X. C. ; Yasue, S. ; Ye, Z. H. ; Yu, G. C. ; Yuan, A. F. ; Yuda, T. ; Zhang, H. M. ; Zhang, J. L. ; Zhang, N. J. ; Zhang, X. Y. ; Zhang, Y. ; Zhaxisangzhu, ; Zhou, X. X. ; Tibet, ASgamma Collaboration
刊名Astrophysics
出版日期2006
卷号37期号:10页码:1932-1937
关键词diffuse TeV gamma rays galactic plane flux upper limits air shower array emission spectrum
ISSN号0273-1177
通讯作者北京8701信箱
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.
收录类别SCI
原文出处http://www.sciencedirect.com/science?_ob=MImg&_imagekey=B6V3S-4H9996M-4-N&_cdi=5738&_user=1999492&_pii=S0273117705010859&_orig=search&_coverDate=12%2F31%2F2006&_sk=999629989&view=c&wchp=dGLbVzb-zSkzk&md5=a0787e1d0b6e71f93fa89846326223f2&ie=/sdarticle.pdf
语种英语
源URL[http://ir.cssar.ac.cn/handle/122/1709]  
专题国家空间科学中心_其他部室
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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(10):1932-1937.
APA Amenomori, M..,Ayabe, S..,Cui, S. W..,Danzengluobu,.,Ding, L. K..,...&Tibet, ASgamma Collaboration.(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(10),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 37.10(2006):1932-1937.

入库方式: OAI收割

来源:国家空间科学中心

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