Bayesian image reconstruction with space-variant noise suppression

被引:10
作者
Nunez, J
Llacer, J
机构
[1] Univ Barcelona, Dept Astron & Meteorol, E-08028 Barcelona, Spain
[2] Observ Fabra, Barcelona, Spain
[3] Univ Calif Berkeley, Lawrence Berkeley Lab, Div Engn, Berkeley, CA 94720 USA
来源
ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES | 1998年 / 131卷 / 01期
关键词
techniques : image processing; methods : data analysis;
D O I
10.1051/aas:1998259
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In this paper we present. a Bayesian image reconstruction algorithm with entropy prior (FMAPE) that uses a space-variant hyperparameter. The spatial variation of the hyperparameter allows different degrees of resolution in areas of different statistical characteristics, thus avoiding the large residuals resulting from algorithms that use a constant hyperparameter. In the first implementation of the algorithm, we begin by segmenting a Maximum Likelihood Estimator (MLE) reconstruction. The segmentation method is based on using a wavelet decomposition and a self-organizing neural network. The result is a predetermined number of extended regions plus a small region for each star or bright object. To assign a different value of the hyperparameter to each extended region and star, we use either feasibility tests or cross-validation methods. Once the set of hyperparameters is obtained, we carried out the final Bayesian reconstruction, leading to a reconstruction with decreased bias and excellent visual characteristics. The method has been applied to data from the Iron-refurbished Hubble Space Telescope. The method can be also applied to ground-based images.
引用
收藏
页码:167 / 180
页数:14
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