Paper
1 August 1990 Adaptive optics prototype system for IR astronomy II: first observing results
Fritz Merkle, Pierre Y. Kern, Francois J. Rigaut, Pierre J. Lena, Gerard Rousset
Author Affiliations +
Proceedings Volume 1271, Adaptive Optics and Optical Structures; (1990) https://doi.org/10.1117/12.20410
Event: The International Congress on Optical Science and Engineering, 1990, The Hague, Netherlands
Abstract
For the first time in ground-based astronomy, diffraction-limited imaging through atmospheric turbulence has been achieved in real time by adaptive optics in the infrared wavelengths range. This paper presents the first results and a short analysis, which demonstrate the considerable gain in resolution and sensitivity by the application of this technique. Single stars, close binary stars, and a satellite have been resolved. In one cases an other star several arcseconds apart has been used as reference for the wavefront sensing.
© (1990) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Fritz Merkle, Pierre Y. Kern, Francois J. Rigaut, Pierre J. Lena, and Gerard Rousset "Adaptive optics prototype system for IR astronomy II: first observing results", Proc. SPIE 1271, Adaptive Optics and Optical Structures, (1 August 1990); https://doi.org/10.1117/12.20410
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KEYWORDS
Adaptive optics

Stars

Wavefront sensors

Prototyping

Telescopes

Astronomy

Infrared radiation

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