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Автор Wang Yue
Автор Bi Xiao-Jun
Автор Cui Shu-Wang
Автор Ding Lin-Kai
Автор Dan Zeng-Luo-Bu
Автор Ding Xiao-Hong
Автор Fan Chao
Автор Feng Cun-Feng
Автор Feng Zhao-Yang
Автор Feng Zhen-Yong
Автор Gao Xiao-Yu
Автор Geng Qing-Xi
Автор Guo Hong-Wei
Автор He Hui-Hai
Автор He Mao
Автор Hu Hai-Bing
Автор Hu Hong-Bo
Автор Huang Qing
Автор Jia Huan-Yu
Автор La Ba-Ci-Ren
Автор Le Gui-Ming
Автор Li Ai-Feng
Автор Li Jin-Yu
Автор Lou Yu-Qing
Автор Lu Hong
Автор Lu Sui-Ling
Автор Meng Xian-Ru
Автор Mu Jun
Автор Ren Jing-Ru
Автор Tan You-Heng
Автор Wang Bo
Автор Wang Hui
Автор Wang Yong-Gang
Автор Wu Han-Rong
Автор Xue Liang
Автор Yang Xian-Chu
Автор Ye Zong-Hai
Автор Yuan Ai-Fang
Автор Zhang Hui-Min
Автор Zhang Ji-Long
Автор Zhang Nai-Jian
Автор Zhang Xue-Yao
Автор Zhang Yong
Автор Zhang Yi
Автор Zha Xi-Sang-Zhu
Автор Zhou Xun-Xiu
Автор Yuan Qiang
Дата выпуска 2008-11-01
dc.description Using the data taken from Tibet II High Density (HD) Array (1997 February–1999 September) and Tibet-III array (1999 November–2005 November), our previous northern sky survey for TeV γ-ray point sources has now been updated by a factor of 2.8 improved statistics. From 0.0° to 60.0° in declination (Dec) range, no new TeV γ-ray point sources with sufficiently high significance were identified while the well-known Crab Nebula and Mrk421 remain to be the brightest TeV γ-ray sources within the field of view of the Tibet air shower array. Based on the currently available data and at the 90% confidence level (C.L.), the flux upper limits for different power law index assumption are re-derived, which are approximately improved by 1.7 times as compared with our previous reported limits.
Формат application.pdf
Издатель Institute of Physics Publishing
Копирайт 2008 Chinese Physical Society and the Institute of High Energy Physics of the Chinese Academy of Sciences and the Institute of Modern Physics of the Chinese Academy of Sciences
Название An updated search of steady TeV γ-ray point sources in northern hemisphere using the Tibet air shower arraySupported by Grants-in-Aid for Scientific Research on Priority Areas (712) (MEXT), Japan Society for Promotion of Science (JSPS), National Natural Science Foundation of China (10675134, 10533020) and Chinese Academy of Sciences
Тип paper
DOI 10.1088/1674-1137/32/11/004
Electronic ISSN 2058-6132
Print ISSN 1674-1137
Журнал Chinese Physics C
Том 32
Первая страница 868
Последняя страница 872
Выпуск 11

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