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Proceedings Paper

Adaptive optics performance analysis for the Gemini 8-m Telescopes Project
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Paper Abstract

This paper summarizes adaptive optics performance estimates obtained for the Gemini 8-m telescopes, with an emphasis on relatively low order systems employing Shack-Hartmann wavefront sensors, continuous facesheet deformable mirrors with zonal actuators, and either a natural guide star or a laser guide star in the mesospheric sodium layer. Adaptive optics performance is characterized in terms of the fractional encircled energy within a 0.1 arc sec detector at 2.2 microns under average seeing conditions at Mauna Kea. The increased sky coverage achieved using laser guide stars according to this definition of performance is significant, even for a relatively low order adaptive optics system designed for turbulence compensation at 2.2 microns at a good astronomical site.

Paper Details

Date Published: 31 May 1994
PDF: 16 pages
Proc. SPIE 2201, Adaptive Optics in Astronomy, (31 May 1994); doi: 10.1117/12.176076
Show Author Affiliations
Brent L. Ellerbroek, Air Force Phillips Lab. (United States)
Stephen M. Pompea, S.M. Pompea and Associates (United States)
David J. Robertson, Aura, Inc. (United States)
C. Matt Mountain, Gemini 8-m Telescopes Project (United States)


Published in SPIE Proceedings Vol. 2201:
Adaptive Optics in Astronomy
Mark A. Ealey; Fritz Merkle, Editor(s)

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