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

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 NuVu 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.

[1]  Eric Gendron,et al.  CANARY: the on-sky NGS/LGS MOAO demonstrator for EAGLE , 2008, Astronomical Telescopes + Instrumentation.

[2]  Tim Morris,et al.  CHOUGH, the Canary Hosted-Upgrade for High-Order Adaptive Optics , 2014, Astronomical Telescopes and Instrumentation.

[3]  B. Macintosh,et al.  Spatially filtered wave-front sensor for high-order adaptive optics. , 2004, Journal of the Optical Society of America. A, Optics, image science, and vision.

[4]  Richard Myers,et al.  Durham adaptive optics real-time controller. , 2010, Applied optics.