Paper
11 September 1998 Estimation of the point spread function for the adaptive optics system ADONIS
Stephan Harder, Alain Chelli
Author Affiliations +
Abstract
The wavefront correction by an adaptive optics (AO) system is never perfect, but images obtained with AO can be restored by deconvolution methods, if the point spread function is known. We present the first result of PSF reconstruction from the wavefront sensor measurements applied to the AO system ADONIS installed at the 3.6m ESO telescope at La Silla.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephan Harder and Alain Chelli "Estimation of the point spread function for the adaptive optics system ADONIS", Proc. SPIE 3353, Adaptive Optical System Technologies, (11 September 1998); https://doi.org/10.1117/12.321647
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Cited by 1 scholarly publication.
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KEYWORDS
Point spread functions

Adaptive optics

Mirrors

Optical transfer functions

Turbulence

Telescopes

Wavefronts

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