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CHOUGH: Spatially filtered Shack-Hartmann wave-front sensor for HOAO

机译:Chough:包浩浩的空间过滤的棚屋挥杆波前传感器

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The CANARY-Hosted Upgrade for High-Order Adaptive Optics (CHOUGH), is a narrow-field of view High-Order Single Conjugate on-sky AO demonstrator to be placed on the 4.2m WHT telescope. It aims to produce a Strehl ratio greater than 0.5 in the visible region of the spectrum (> 640nm). A High-Order wave-front sensor (HOWFS) is a central piece of the experiment; it is a Shack-Hartmann with a sampling of 31x31 subapertures across the pupil. A variable aperture spatial filter designed to reduce aliasing for high-spatial frequencies, located at a focal plane preceding the lenslet array. The HOWFS has a quad-cell configuration on the detector with a one-pixel guard ring and 48μm subaperture. The detector is a NüVü EMCCD camera, 24μm pixel size, operating at>500Hz. The lenslet array, collimator and relay are commercial off-the-shelf. This was technically challenging due to the small size of the pupil, 2.3mm, and the small optics involved in the design.
机译:本金丝雀终端升级为高阶自适应光学(Chough),是一个狭窄的观看高阶单缀合物上的天空AO演示,可以放在4.2M WHT望远镜上。它旨在在光谱(> 640nm)的可见区域中产生大于0.5的斯特勒比比。高阶波前传感器(Howws)是实验的中心部件;它是一名棚屋,坐在瞳孔上有31x31亚峰的采样。可变孔隙空间滤波器,设计用于减少位于透镜阵列前面的焦平面的高空间频率的混叠。 Howfs在探测器上具有四个单元配置,具有单像素的防护环和48μm子孔节。探测器是NüvüEMCCD相机,24μm像素尺寸,操作> 500Hz。 Lenslet阵列,准直器和继电器是商业现成的。这是由于瞳孔大小,2.3mm和设计中涉及的小型光学器件导致的技术上挑战。

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