CHOUGH: implementation and performance of a high-order 4m AO demonstrator
2016
CHOUGHis a small, fast project to provide an experimental on-sky high-order SCAO capability to the 4.2m WHT telescope. The basic goal has r 0 -sized sub- apertures with the aim of achieving high-
Strehl ratios(> 0:5) in the visible (> 650 nm). It achieves this by including itself into the CANARY experiment:
CHOUGHis mounted as a
breadboardand intercepts the beam within CANARY via a
periscope. In doing so, it takes advantage of the mature CANARY infrastructure, but add new AO capabilities. The key instruments that
CHOUGHbrings to CANARY are: an atmospheric dispersion compensator; a 32 × 32 (1000 actuator) MEMS
deformable mirror; 31 × 31
wavefront sensor; and a complementary (narrow-field) imager. CANARY provides a 241-actuator DM, tip/tilt mirror, and comprehensive off-sky alignment facility together with a RTC. In this work, we describe the
CHOUGHsub-systems: backbone, ADC, MEMS-DM, HOWFS, CAWS, and NFSI.
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