15 July 2008 High-order wavefront sensing system for PALM-3000
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PALM-3000 is an upgrade to the current PALM-241 adaptive optics system at the 5.1 m Hale telescope which will allow diffraction-limited science in visible wavelengths using bright natural guide stars, have more modest performance with an upgraded Sodium laser guide star, and allow for guiding on faint natural guide stars. A key sub-system of the upgrade is a new high-order Shack-Hartmann wavefront sensor with selectable pupil sampling, up to 64 subapertures across the telescope aperture, to minimize wavefront reconstruction error for varying brightness of guide source with a frame rate up to 3 kHz. The design and current status of the high-order wavefront sensing system is presented.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Christoph Baranec, Christoph Baranec, } "High-order wavefront sensing system for PALM-3000", Proc. SPIE 7015, Adaptive Optics Systems, 70155M (15 July 2008); doi: 10.1117/12.788460; https://doi.org/10.1117/12.788460


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