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An overview and status of GMT active and adaptive optics
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Paper Abstract

The Giant Magellan Telescope (GMT) wavefront control system will provide active optics control and optimized atmospheric turbulence correction to every instrument on the 25.4 m diameter GMT. All subsystems of the GMT wavefront control system have passed their preliminary design reviews, and several are now in the detailed design and prototyping phases. Significant progress has been made developing optimized control algorithms, and simulating observatory performance over a wide range of environmental conditions. We review the wavefront control strategy in each observing mode, and the associated image quality error budgets. We also describe recent d and prototyping progress, and our plans to complete the wavefront control system development and prepare for first light.

Paper Details

Date Published: 10 July 2018
PDF: 16 pages
Proc. SPIE 10703, Adaptive Optics Systems VI, 107030W (10 July 2018); doi: 10.1117/12.2314255
Show Author Affiliations
Antonin H. Bouchez, GMTO Corp. (United States)
George Z. Angeli, GMTO Corp. (United States)
David S. Ashby, GMTO Corp. (United States)
Large Binocular Telescope Observatory (United States)
Robert Bernier, GMTO Corp. (United States)
Rodolphe Conan, GMTO Corp. (United States)
Brian A. McLeod, Smithsonian Astrophysical Observatory (United States)
Fernando Quirós-Pacheco, GMTO Corp. (United States)
Marcos A. van Dam, Flat Wavefronts (New Zealand)


Published in SPIE Proceedings Vol. 10703:
Adaptive Optics Systems VI
Laird M. Close; Laura Schreiber; Dirk Schmidt, Editor(s)

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