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Characteristics and performance of GAW, Gamma Air Watch – a path-finder of a new generation of Imaging Atmospheric ˇ Cerenkov Telescope with large field of view

机译:GAW的特点和性能,伽马空气腕表 - 具有大视野的新一代成像大气Cerenkov望远镜的路径查找器

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GAW, acronym for Gamma Air Watch, is a path-finder experiment designed to test the feasibility of a different technological approach for Imaging Atmospheric ⅶ Cerenkov Telescopes. GAW differentiates from the existing and presently planned telescopes for two main features: the adoption of a refractive optics system as light collector and the use of single photoelectron counting as detector working mode. The optics of GAW, composed by a custom-made 2.13 diameter single-sided Fresnel lens, will allow to achieve large field of view capability (8 】 8). The focal surface consists of a matrix of multianode photomultipliers. The large number of active channels (of the order of 105) makes it basically a large UV sensitive digital camera with high resolution imaging capability. GAWis being mounted at the Calar Alto observatory, Spain, 2150 m a.s.l., and its calibration phase is planned to start in 2012. GAW is a collaboration effort of several Research Institutes in Italy, Portugal and Spain. Keywords: ⅶ Cerenkov Telescopes; TeV astronomyAbstract: GAW, acronym for Gamma Air Watch, is a path-finder experiment designed to test the feasibility of a different technological approach for Imaging Atmospheric ⅶ Cerenkov Telescopes. GAW differentiates from the existing and presently planned telescopes for two main features: the adoption of a refractive optics system as light collector and the use of single photoelectron counting as detector working mode. The optics of GAW, composed by a custom-made 2.13 diameter single-sided Fresnel lens, will allow to achieve large field of view capability (8 】 8). The focal surface consists of a matrix of multianode photomultipliers. The large number of active channels (of the order of 105) makes it basically a large UV sensitive digital camera with high resolution imaging capability. GAWis being mounted at the Calar Alto observatory, Spain, 2150 m a.s.l., and its calibration phase is planned to start in 2012. GAW is a collaboration effort of several Research Institutes in Italy, Portugal and Spain.
机译:全球大气监测网,缩写伽玛空气观察,是一个路径查找器实验旨在测试成像大气ⅶ切伦科夫望远镜不同的技术方法的可行性。 GAW从两个主要特点的现有的和目前计划望远镜区分:通过折射光学系统的光收集器和使用单光电子计数的作为检测器的工作模式。 GAW的光学,通过定制的2.13直径单面菲涅耳透镜构成,将允许实现视图能力(8】8)的大视场。焦面由多阳极光电倍增管的矩阵。大量的活动通道(的105级)的使得它基本上是一个大的UV敏感的数字摄像机具有高分辨率的成像能力。 GAWis被安装在卡拉阿托天文台,西班牙,2150米a.s.l.,其标定阶段,计划于2012年开始GAW是多家科研院所的在意大利,葡萄牙和西班牙的合作努力。关键词:ⅶ切伦科夫望远镜; TeV的astronomyAbstract:全球大气监测网,缩写伽玛空气观察,是一个路径查找器实验旨在测试成像大气ⅶ切伦科夫望远镜不同的技术方法的可行性。 GAW从两个主要特点的现有的和目前计划望远镜区分:通过折射光学系统的光收集器和使用单光电子计数的作为检测器的工作模式。 GAW的光学,通过定制的2.13直径单面菲涅耳透镜构成,将允许实现视图能力(8】8)的大视场。焦面由多阳极光电倍增管的矩阵。大量的活动通道(的105级)的使得它基本上是一个大的UV敏感的数字摄像机具有高分辨率的成像能力。 GAWis被安装在卡拉阿托天文台,西班牙,2150米a.s.l.,其标定阶段,计划于2012年开始GAW是多家科研院所的在意大利,葡萄牙和西班牙的合作努力。

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