Chinese Physics C > 1997, Vol. 21 > Issue(7): 583-590

Atmospheric Cherenkov Telescope

Institute of High Energy Physics,The Chinese Academy of Sciences,Beijing 100039

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Abstract：
Two tracking atmospheric Cherenkov telescopes have been operated at Xing Long Station,Beijing Astronomical Observatory,on the basis of atmospheric Cherenkov radiation produced by extensive air shower.They are used to search for point sources of very high energy gamma ray and to study their emission characteristics as well as to detect the spatial distribution of very high energy gamma ray intensity.The construction and the performance of the telescopes as well as the testing results under observation conditions are presented in this paper.

References

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Jiang Yinlin, Chen Yongzhong, Xu Chunxian, He Huilin, He Huihai, Li Huidong and Huo Anxiang. Atmospheric Cherenkov Telescope[J]. Chinese Physics C, 1997, 21(7): 583-590.

Jiang Yinlin, Chen Yongzhong, Xu Chunxian, He Huilin, He Huihai, Li Huidong and Huo Anxiang. Atmospheric Cherenkov Telescope[J]. Chinese Physics C, 1997, 21(7): 583-590. shu

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Received: 1900-01-01
Revised: 1900-01-01

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通讯作者:陈斌, bchen63@163.com

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沈阳化工大学材料科学与工程学院沈阳 110142

Atmospheric Cherenkov Telescope

Corresponding author:Jiang Yinlin,

Institute of High Energy Physics,The Chinese Academy of Sciences,Beijing 100039

Received Date:1900-01-01

Accepted Date:1900-01-01

Available Online:1997-07-05

Abstract:Two tracking atmospheric Cherenkov telescopes have been operated at Xing Long Station,Beijing Astronomical Observatory,on the basis of atmospheric Cherenkov radiation produced by extensive air shower.They are used to search for point sources of very high energy gamma ray and to study their emission characteristics as well as to detect the spatial distribution of very high energy gamma ray intensity.The construction and the performance of the telescopes as well as the testing results under observation conditions are presented in this paper.

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Atmospheric Cherenkov Telescope

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