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The design of an adaptive optics telescope : the case of DAG

机译:自适应光学望远镜的设计:DAG的情况

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In this paper, we describe in detail the optical design of DAG, a new 4 m telescope for Turkey. DAG is an "adaptive optics friendly" telescope, in a sense that each design decision is taken considering the potential impact on the AO performance (vibrations, static aberrations etc.) The objective is to make this telescope fully ready for AO at first light. It is designed as a Ritchey-Chrétien combination, 56 m focal length, with Nasmyth foci only, and active optics. Its total RMS error is expected to be 45 nm up to Zernike mode 78, and 26 nm for the higher, non AO corrected modes. A final design optimization has been done by the telescope manufacturers, demonstrating that our AO-based requirements can be satisfied, without much diffculty.
机译:在本文中,我们详细描述了DAG的光学设计,是火鸡的新的4米望远镜。 DAG是一个“自适应光学友好的”望远镜,以至于考虑到对AO性能的潜在影响(振动,静态像差等)来说,目的是使这种望远镜在第一灯上完全准备好AO。它被设计为Ritchey-Chrétien组合,56米的焦距,仅用NASMYTH Foci,以及主动光学器件。它的总rms误差预计为45 nm,最高可达Zernike模式78,并且对于较高的非AO校正模式为26nm。望远镜制造商已经完成了最终的设计优化,证明我们可以满足我们的AO - 基于AO的要求,而无需太多。

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