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18 November 2008 PSF model of wide-field optical system for restoration of space (in)variant astronomical image data
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Proceedings Volume 7138, Photonics, Devices, and Systems IV; 713821 (2008) https://doi.org/10.1117/12.818066
Event: Photonics, Devices, and Systems IV, 2008, Prague, Czech Republic
Abstract
The third order optical aberrations models for LSI/LSV (Linear Space Invariant/Variant) systems is described in this paper. These models are based on Seidel and Zernike approximating polynomials. Optical aberrations effect to the PSF (Point Sread Function) of optical imaging systems is described as well. Higher quality and precision of image data can be obtained with deconvolution of the acquired images and system point spread function. The PSF can be modelled as a space variant function from the estimation of optical system wavefront aberrations.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Martin Rerábek and Petr Páta "PSF model of wide-field optical system for restoration of space (in)variant astronomical image data", Proc. SPIE 7138, Photonics, Devices, and Systems IV, 713821 (18 November 2008); https://doi.org/10.1117/12.818066
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