Paper
1 January 1993 Wavefront sensor optimization in astronomical applications
Gerard Lelievre, J. Sebag, D. Bauduin, F. Fidouh, J. L. Lebrun, B. S. Servan
Author Affiliations +
Abstract
Microlens arrays made by engraving photoresist coatings are suitable for astronomical applications, especially in the Shack-Hartmann type of wavefront sensor. Their characteristics have to be carefully chosen to fit the turbulence strength. Our instrument, composed of a photon-counting device and a Shack-Hartmann sensor, allows synchronous recordings of short-exposure images and their corresponding wavefronts. In post-processing, the point spread functions (PSF) are calculated and used to deconvolve the direct images. A new real- time centroiding device transforms this experiment into a quasi real-time imaging corrective system.
© (1993) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gerard Lelievre, J. Sebag, D. Bauduin, F. Fidouh, J. L. Lebrun, and B. S. Servan "Wavefront sensor optimization in astronomical applications", Proc. SPIE 1781, Specification and Measurement of Optical Systems, (1 January 1993); https://doi.org/10.1117/12.140973
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CITATIONS
Cited by 2 scholarly publications.
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KEYWORDS
Wavefront sensors

Wavefronts

Microlens array

Telescopes

Sensors

Astronomy

Optical testing

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