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Proceedings Paper

Processing of the astronomical image data obtained from UWFC optical systems
Author(s): Martin Řeřábek; Petr Páta; Pavel Koten
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Paper Abstract

This paper deals with simulation and modeling of the optical systems used in astronomy and their transfer characteristics. It is especially focused to the WFC (Wide-Field Camera) and UWFC (Ultra Wide-Field Camera) SV (Space Variant) optical systems. The properties of UWFC astronomical systems along with specific visual data in astronomical images contribute to complicated evaluation of acquired image data. There is an experiment for estimate the optical aberration of optical systems described in this paper. The results of different deconvolution algorithms, which are used with partially variant model of UWFC optical system, are demonstrated in this paper.

Paper Details

Date Published: 5 September 2008
PDF: 11 pages
Proc. SPIE 7076, Image Reconstruction from Incomplete Data V, 70760L (5 September 2008); doi: 10.1117/12.794858
Show Author Affiliations
Martin Řeřábek, Czech Technical Univ. in Prague (Czech Republic)
Petr Páta, Czech Technical Univ. in Prague (Czech Republic)
Pavel Koten, Astronomical Institute (Czech Republic)

Published in SPIE Proceedings Vol. 7076:
Image Reconstruction from Incomplete Data V
Philip J. Bones; Michael A. Fiddy; Rick P. Millane, Editor(s)

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