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Proceedings Paper

Design and expected performance of an MCAO system for the Giant Magellan Telescope
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Paper Abstract

Adaptive optics will play a crucial role in achieving the full potential of the next generation of large diameter telescopes. In this paper, we present an optical design for a multi-conjugate adaptive optics system for the Giant Magellan Telescope, a 25.7 m telescope with a primary mirror consisting of seven 8.4 m segments. The tri-conjugate MCAO optics is based on adaptive secondary technology developed for the MMT telescope and incorporates dynamic refocus optics for the laser guide star wavefront sensors. We use the results of analytic (non-Monte-Carlo) numerical simulations to determine the optimal configuration of deformable mirrors as well as laser and natural guide stars. The simulation results are extended to include and quantify the effects of wavefront sensor and control loop delay noise as well as dynamic refocus and fitting error on the expected system performance and sky coverage.

Paper Details

Date Published: 24 December 2003
PDF: 12 pages
Proc. SPIE 5169, Astronomical Adaptive Optics Systems and Applications, (24 December 2003); doi: 10.1117/12.511742
Show Author Affiliations
N. Mark Milton, Univ. of Arizona (United States)
Michael Lloyd-Hart, Univ. of Arizona (United States)
Andrew Cheng, Univ. of Arizona (United States)
James A. Georges III, Univ. of Arizona (United States)
James Roger P. Angel, Univ. of Arizona (United States)


Published in SPIE Proceedings Vol. 5169:
Astronomical Adaptive Optics Systems and Applications
Robert K. Tyson; Michael Lloyd-Hart, Editor(s)

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