Operating performance of the gamma-ray Cherenkov telescope: An end-to-end Schwarzschild-Couder telescope prototype for the Cherenkov Telescope Array
Operating performance of the gamma-ray Cherenkov telescope: An end-to-end Schwarzschild-Couder telescope prototype for the Cherenkov Telescope Array
复制标题
伽马射线切伦科夫望远镜的运行性能：切伦科夫望远镜阵列的端到端史瓦西-库德望远镜原型
DOI：
10.1016/j.nima.2016.05.059
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发表时间：
2017
期刊：
影响因子：
--
通讯作者：
Dournaux J
中科院分区：
文献类型：
--
作者：
Dournaux J
切伦科夫望远镜阵列（CTA）联盟的目标是建立下一代地基甚高能伽马射线天文台。该阵列将配备不同尺寸的望远镜，使其能够覆盖从约20 GeV到100 TeV以上的宽伽马射线能带。超过5 TeV的最高能量将由大量视场约为9°的小型望远镜（SST）覆盖。基于Schwarzschild-Couder双镜光学系统的伽玛射线切伦科夫望远镜（GCT）是三种建议的SST设计之一。GCT在这方面的贡献和切伦科夫阵雨获得的第一个图像的望远镜和它的相机。2015年11月在法国默东获得。
The Cherenkov Telescope Array (CTA) consortium aims to build the next-generation ground-based very-high-energy gamma-ray observatory. The array will feature different sizes of telescopes allowing it to cover a wide gamma-ray energy band from about 20 GeV to above 100 TeV. The highest energies, above 5 TeV, will be covered by a large number of Small-Sized Telescopes (SSTs) with a field-of-view of around 9°. The Gamma-ray Cherenkov Telescope (GCT), based on Schwarzschild–Couder dual-mirror optics, is one of the three proposed SST designs. The GCT is described in this contribution and the first images of Cherenkov showers obtained using the telescope and its camera are presented. These were obtained in November 2015 in Meudon, France.
用于切伦科夫望远镜阵列的 SST 双镜望远镜：创新的镜面制造工艺
影响因子：
1.1
作者：
D. Dumas;J. Huet;J. Dournaux;P. Laporte;C. Rulten;J. Schmoll;H. Sol;F. Sayede;P. Micolon;J. Glicenstein;B. Peyaud
通讯作者：
B. Peyaud