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An Overview of The VERITAS Prototype Telescope And Camera

机译:VERITAS原型望远镜和照相机概述

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摘要

VERITAS (the Very Energetic Radiation Imaging Telescope Array System) is the next generation ground-based gamma-ray observatory that is being built in southern Arizona by a collaboration of ten institutions in Canada, Ireland, the U.K. and the U.S.A. VERITAS is designed to operate in the range from 50 GeV to 50 TeV with optimal sensitivity near 200 GeV; it will effectively overlap with the next generation of space-based gamma-ray telescopes. The first phase of VERITAS, consisting of four telescopes of 12 m aperture, will be operational by the time of the GLAST launch in 2007. Eventually the array will be expanded to include the full array of seven telescopes on a filled hexagonal grid of side 80 m. A prototype VERITAS telescope with a reduced number of mirrors and signal channels has been built. Its design and performance is described here. The prototype is scheduled to be upgraded to a full 499 pixel camera with 350 mirrors during the autumn of 2004.
机译:VERITAS(高能辐射成像望远镜阵列系统)是由加拿大,爱尔兰,英国和美国的十个机构合作在亚利桑那州南部建造的下一代地面伽玛射线观测站。在50 GeV至50 TeV范围内,最佳灵敏度接近200 GeV;它将与下一代天基伽玛射线望远镜有效重叠。 VERITAS的第一阶段由四个12 m孔径的望远镜组成,将于2007年GLAST发射时投入使用。最终,该阵列将扩展到包括在80边的填充六边形网格上的全部七个阵列的望远镜米VERITAS原型望远镜的镜面和信号通道数量减少了。它的设计和性能在这里描述。该原型机计划于2004年秋季升级为带350个镜子的完整499像素相机。

著录项

  • 作者

    Cogan, P;

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  • 年度 2004
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  • 原文格式 PDF
  • 正文语种 eng
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