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SST dual-mirror telescope for Cherenkov Telescope Array: an innovative mirror manufacturing process

机译:用于Cherenkov望远镜阵列的SST双镜望远镜:创新的镜制造工艺

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The Observatoire de Paris is constructing a prototype Small-Sized Telescope (SST) for the Cherenkov Telescope Array (CTA), named SST-GATE, based on the dual-mirror Schwarzschild-Couder optical design. Considering the mirrors size and its specific curvature and the optical requirements for the Cherenkov imaging telescope, a non-conventional process has been used for designing and manufacturing the mirrors of the SST-GATE prototype. Based on machining, polishing and coating of aluminium bulk samples, this process has been validated by simulation and tests that will be detailed in this paper after a discussion on the Schwarzschild-Couder optical design which so far has never been used to design ground based telescopes. Even if the SST-GATE is a prototype for small size telescopes of the CTA array, the primary mirror of the telescope is 4 meters diameter, and it has to be segmented. Due to the dual-mirror configuration, the alignment is a complex task that needs a well defined and precise process that will be discussed in this paper.
机译:巴黎天文台正在基于双镜Schwarzschild-Couder光学设计,为Cherenkov望远镜阵列(CTA)建造一个原型小型望远镜(SST),名为SST-GATE。考虑到镜子的尺寸及其比曲率以及切伦科夫成像望远镜的光学要求,已使用非常规方法来设计和制造SST-GATE原型的镜子。在对铝块状样品进行机械加工,抛光和涂层处理的基础上,该过程已通过仿真和测试验证,在对Schwarzschild-Couder光学设计进行讨论后,本文将对此进行详细介绍,到目前为止,该光学设计从未用于设计地面望远镜。 。即使SST-GATE是用于CTA阵列小型望远镜的原型,望远镜的主镜直径为4米,也必须进行分段。由于采用了双镜配置,因此对齐是一项复杂的任务,需要一个定义明确且精确的过程,本文将对此进行讨论。

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