Translator Disclaimer
10 July 2008 The PALM-3000 high-order adaptive optics system for Palomar Observatory
Author Affiliations +
Abstract
Deployed as a multi-user shared facility on the 5.1 meter Hale Telescope at Palomar Observatory, the PALM-3000 highorder upgrade to the successful Palomar Adaptive Optics System will deliver extreme AO correction in the near-infrared, and diffraction-limited images down to visible wavelengths, using both natural and sodium laser guide stars. Wavefront control will be provided by two deformable mirrors, a 3368 active actuator woofer and 349 active actuator tweeter, controlled at up to 3 kHz using an innovative wavefront processor based on a cluster of 17 graphics processing units. A Shack-Hartmann wavefront sensor with selectable pupil sampling will provide high-order wavefront sensing, while an infrared tip/tilt sensor and visible truth wavefront sensor will provide low-order LGS control. Four back-end instruments are planned at first light: the PHARO near-infrared camera/spectrograph, the SWIFT visible light integral field spectrograph, Project 1640, a near-infrared coronagraphic integral field spectrograph, and 888Cam, a high-resolution visible light imager.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Antonin H. Bouchez, Richard G. Dekany, John R. Angione, Christoph Baranec, Matthew C. Britton, Khanh Bui, Rick S. Burruss, John L. Cromer, Stephen R. Guiwits, John R. Henning, Jeff Hickey, Daniel L. McKenna, Anna M. Moore, Jennifer E. Roberts, Thang Q. Trinh, Mitchell Troy, Tuan N. Truong, and Viswa Velur "The PALM-3000 high-order adaptive optics system for Palomar Observatory", Proc. SPIE 7015, Adaptive Optics Systems, 70150Z (10 July 2008); doi: 10.1117/12.789777; https://doi.org/10.1117/12.789777
PROCEEDINGS
7 PAGES


SHARE
Advertisement
Advertisement
RELATED CONTENT

Coupling a low order curvature wavefront sensor with a high...
Proceedings of SPIE (September 10 1998)
A compact design of a WFS for a natural guide...
Proceedings of SPIE (July 28 2010)
Exoplanet imaging with the Giant Magellan Telescope
Proceedings of SPIE (June 22 2006)
Instrumental Limitations In Adaptive Optics For Astronomy
Proceedings of SPIE (September 19 1989)

Back to Top