Paper
1 December 1991 MARTINI: system operation and astronomical performance
Andrew Peter Doel, Colin N. Dunlop, John Victor Major, Richard M. Myers, Ray M. Sharples
Author Affiliations +
Abstract
The MARTINI adaptive optics system has been engineered for regular astronomical observations on the 4.2 m William Herschel Telescope on La Palma. The design specifications for such a general purpose image-sharpening device are discussed. Examples of the imaging performance achieved during development of MARTINI are presented, together with results from visible-region astronomical imaging programs. The prospects for spectroscopic observations with this class of system are outlined.
© (1991) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Andrew Peter Doel, Colin N. Dunlop, John Victor Major, Richard M. Myers, and Ray M. Sharples "MARTINI: system operation and astronomical performance", Proc. SPIE 1542, Active and Adaptive Optical Systems, (1 December 1991); https://doi.org/10.1117/12.48820
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KEYWORDS
Stars

Mirrors

Astronomy

Telescopes

Wavefront sensors

Adaptive optics

Control systems

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