Deconvolution of adaptive optics images: from theory to practice

被引：16

作者：

Conan, JM ^{[1
]}

Fusco, T ^{[1
]}

Mugnier, LM ^{[1
]}

Marchis, F ^{[1
]}

Roddier, C ^{[1
]}

Roddier, F ^{[1
]}

机构：

[1] Off Natl Etud & Rech Aerosp, DOTA, F-92322 Chatillon, France

来源：

ADAPTIVE OPTICAL SYSTEMS TECHNOLOGY, PTS 1 AND 2 | 2000年 / 4007卷

关键词：

adaptive optics; atmospheric turbulence; deconvolution; image restoration; inverse problems; astronomy;

D O I：

10.1117/12.390374

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Practical guidelines are proposed for deconvolution of partially adaptive optics corrected images: from raw data to high photometric precision object restoration. Preliminary processing is discussed (detector calibration, background subtraction...). The deconvolution scheme itself is then presented. It takes into account the noise statistics in the image, the imprecise knowledge of the point spread function (PSF), and the available a priori information on the object (spatial structure, positivity...). This deconvolution scheme is first validated on simulated images of NAGS, the AO system of the VLT and then applied to astronomical images. In particular, an edge preserving regularization is tested on several solar system objects: Io, Uranus and Neptune.

引用

页码：913 / 924

页数：12

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