31 May 1994 Performance of adaptive optics at Lick Observatory
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Abstract
A prototype adaptive optics system has been developed at Lawrence Livermore National Laboratory for use at Lick Observatory. This system is based on an ITEK 69-actuator continuous-surface deformable mirror, a Kodak fast-framing intensified CCD camera, and a Mercury VME board containing four Intel i860 processors. The system has been tested using natural reference stars on the 40-inch Nickel telescope at Lick Observatory yielding up to a factor of 10 increase in image peak intensity and a factor of 6 reduction in image full width at half maximum. These results are consistent with theoretical expectations.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Scot S. Olivier, Scot S. Olivier, Jong R. An, Jong R. An, Kenneth Avicola, Kenneth Avicola, Horst D. Bissinger, Horst D. Bissinger, James M. Brase, James M. Brase, Herbert W. Friedman, Herbert W. Friedman, Donald T. Gavel, Donald T. Gavel, Erik M. Johansson, Erik M. Johansson, Claire E. Max, Claire E. Max, Kenneth E. Waltjen, Kenneth E. Waltjen, William A. Fisher, William A. Fisher, William C. Bradford, William C. Bradford, } "Performance of adaptive optics at Lick Observatory", Proc. SPIE 2201, Adaptive Optics in Astronomy, (31 May 1994); doi: 10.1117/12.176022; https://doi.org/10.1117/12.176022
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