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Zero distortion three mirror telescope designed for the Dark Universe Explorer (DUNE) space mission

机译:零失真三镜望远镜专为暗宇探险家(沙丘)空间任务设计

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A feasibility study is presently led by CNES for the Dark UNiverse Explorer (DUNE), a space mission designed to provide unprecedented constraints on dark matter and dark energy using weak gravitational lensing measurements over a very large region of the sky (20 000 square degrees). To achieve this scientific goal, the instrument requires a stable 0.23 arc second FWHM PSF with very low ellipticity (6%) over a field of view of 0.55 square degree. To perform the survey we adopted the drift scan mode which brings many advantages in this type of mission but adds the unusual requirement of a zero distortion optical design. We will present the optical performances of a 1.2 meters Korsch three mirror telescope concept (called NODI for NO Distortion) where the third mirror works with an atypical large magnification and a slightly curved focal surface to obtain zero distortion over an annular 1.7 degrees field of view. A mosaic of 64 CCD detectors of 8 Mega pixels each is shown to pave the curved focal surface without significant degradation of the distortion.
机译:可行性研究目前由国家空间研究中心为黑暗的宇宙探测器(DUNE),太空任务旨在提供使用过的天空非常大的区域的弱引力透镜测量暗物质和暗能量前所未有的限制导致(20 000平方度) 。为了实现这一科学目标,仪器需要稳定的0.23弧电弧第二FWHM PSF,在0.55平方度的视野上具有非常低的椭圆度(6%)。为了执行调查,我们采用了漂移扫描模式,这在这种类型的任务中带来了许多优点,但增加了零失真光学设计的不寻常要求。我们将介绍一个1.2米的korsch三镜望远镜概念的光学性能(称为Nodi,没有失真),其中第三镜具有非典型大放大率和略微弯曲的焦点表面,以通过环形1.7度的视野获得零失真。每个8兆像素的64个CCD探测器的马赛克各自被显示为铺设弯曲的焦点,而不会显着降低变形。

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