西藏ASgamma实验伽玛射线观测亮点。

M. Takita
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引用次数: 0

摘要

西藏ASgamma实验位于海拔4300米的中国西藏。实验由65,700平方米的地面风淋阵和3,400平方米的地下水切伦科夫μ子探测器组成。地面空气阵雨阵列用于重建主粒子能量和方向,地下μ子探测器用于区分伽玛射线诱导的弱μ子空气阵雨和宇宙射线(质子、氦、…)诱导的富μ子空气阵雨。最近,西藏ASgamma实验成功地观测到了来自某些点/扩展源的100 TeV区域的伽马射线,以及沿银河系盘的亚pev漫射伽马射线。在这次演讲中,将介绍观测结果及其解释,并对未来进行展望。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Highlights from gamma-ray observation by the Tibet ASgamma experiment.
The Tibet ASgamma experiment is located at 4,300m above sea level, in Tibet, China.The experiment is composed of a 65,700 m2 surface air shower array and 3,400 m2 underground water Cherenkov muon detectors. The surface air shower array is used for reconstructing the primary particle energy and direction, while the underground muon detectors are used for discriminating gamma-ray induced muon-poor air showers from cosmic-ray (proton, helium,...) induced muon-rich air showers.Recently,the Tibet ASgamma experiment successfully observed gamma rays in the 100 TeV region from some point/extended sources as well as sub-PeV diffuse gamma rays along the Galactic disk.In this talk, The observational results as well as their interpretations will be presented, followed by some future prospect.
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