Strehl-constrained iterative blind deconvolution for post-adaptive-optics data

被引:22
|
作者
Desidera, G. [1 ,2 ]
Carbillet, M. [2 ]
机构
[1] Univ Genoa, DISI, I-16146 Genoa, Italy
[2] Univ Nice Sophia Antipolis, Observ Cote Azur, CNRS, UMR H Fizeau 6525, F-06108 Nice 2, France
关键词
methods: data analysis; methods: numerical; techniques: image processing; INTERFEROMETRIC IMAGES; ASTRONOMICAL IMAGES; RESTORATION; RECONSTRUCTION;
D O I
10.1051/0004-6361/200912913
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Aims. We aim to improve blind deconvolution applied to post-adaptive-optics (AO) data by taking into account one of their basic characteristics, resulting from the necessarily partial AO correction: the Strehl ratio. Methods. We apply a Strehl constraint in the framework of iterative blind deconvolution (IBD) of post-AO near-infrared images simulated in a detailed end-to-end manner and considering a case that is as realistic as possible. Results. The results obtained clearly show the advantage of using such a constraint, from the point of view of both performance and stability, especially for poorly AO-corrected data. The proposed algorithm has been implemented in the freely-distributed and CAOS-based Software Package AIRY.
引用
收藏
页码:1759 / 1762
页数:4
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