Radioastronomical image reconstruction with regularized least squares

S. Naghibzadeh, A. M. Sardarabadi, A. V. D. Veen
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引用次数: 6

Abstract

Image formation using the data from an array of sensors is a familiar problem in many fields such as radio astronomy, biomedical and geodetic imaging. The problem can be formulated as a least squares (LS) estimation problem and becomes ill-posed at high resolutions, i.e. large number of image pixels. In this paper we propose two regularization methods, one based on weighted truncation of the eigenvalue decomposition of the image deconvolution matrix and the other based on the prior knowledge of the "dirty image" using the available data. The methods are evaluated by simulations as well as actual data from a phased-array radio telescope in the Netherlands, the Low Frequency Array Radio Telescope (LOFAR).
正则化最小二乘法重建射电天文图像
在射电天文学、生物医学和大地测量成像等许多领域,利用传感器阵列的数据进行图像生成是一个常见的问题。该问题可以表述为最小二乘(LS)估计问题,并且在高分辨率(即大量图像像素)时变得不适定。本文提出了两种正则化方法,一种是基于图像反卷积矩阵特征值分解的加权截断,另一种是基于使用可用数据的“脏图像”的先验知识。通过模拟和荷兰相控阵射电望远镜(LOFAR)的实际数据对这些方法进行了评估。
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