Paper
7 July 2000 Adaptive optics for the 6.5-m MMT
Michael Lloyd-Hart, Francois P. Wildi, Buddy Martin, Patrick C. McGuire, Matthew A. Kenworthy, Robert L. Johnson, Bruce C. Fitz-Patrick, George Z. Angeli, Stephen M. Miller III, James Roger P. Angel
Author Affiliations +
Abstract
The adaptive optics system for the 6.5 m MMT conversion telescope will be the first to compensate the aberrated wavefront at the telescope's secondary mirror. This approach has unique advantages in terms of optical simplicity, high throughput and low emissivity. We report here the present state of construction, and the results of static and dynamic performance tests of the Cassegrain optical package.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael Lloyd-Hart, Francois P. Wildi, Buddy Martin, Patrick C. McGuire, Matthew A. Kenworthy, Robert L. Johnson, Bruce C. Fitz-Patrick, George Z. Angeli, Stephen M. Miller III, and James Roger P. Angel "Adaptive optics for the 6.5-m MMT", Proc. SPIE 4007, Adaptive Optical Systems Technology, (7 July 2000); https://doi.org/10.1117/12.390307
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CITATIONS
Cited by 13 scholarly publications.
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KEYWORDS
Telescopes

Mirrors

Adaptive optics

Wavefronts

Actuators

Wavefront sensors

Turbulence

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