Performance of adaptive optics at Lick Observatory

Scot S. Olivier; Jong R. An; Kenneth Avicola; Horst D. Bissinger; James M. Brase; Herbert W. Friedman; Donald T. Gavel; Erik M. Johansson; Claire E. Max; Kenneth E. Waltjen; William A. Fisher; William C. Bradford

doi:10.1117/12.176022

31 May 1994 Performance of adaptive optics at Lick Observatory

Scot S. Olivier, Jong R. An, Kenneth Avicola, Horst D. Bissinger, James M. Brase, Herbert W. Friedman, Donald T. Gavel, Erik M. Johansson, Claire E. Max, Kenneth E. Waltjen, William A. Fisher, William C. Bradford

Author Affiliations +

Proceedings Volume 2201, Adaptive Optics in Astronomy; (1994) https://doi.org/10.1117/12.176022
Event: 1994 Symposium on Astronomical Telescopes and Instrumentation for the 21st Century, 1994, Kailua, Kona, HI, United States

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.

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Scot S. Olivier, Jong R. An, Kenneth Avicola, Horst D. Bissinger, James M. Brase, Herbert W. Friedman, Donald T. Gavel, Erik M. Johansson, Claire E. Max, Kenneth E. Waltjen, William A. Fisher, and William C. Bradford "Performance of adaptive optics at Lick Observatory", Proc. SPIE 2201, Adaptive Optics in Astronomy, (31 May 1994); https://doi.org/10.1117/12.176022

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