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A Boosting Approach for the Detection of Faint Compact Sources in Wide Field Aperture Synthesis Radio Images

机译:一种促进宽场孔径合成无线图像中微小紧凑源的促进方法

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Several thresholding techniques have been proposed so far in order to perform faint compact source detection in wide field interferometric radio images. Due to their low intensity/noise ratio, some objects can be easily missed by these automatic detection methods. In this paper we present a novel approach to overcome this problem. Our proposal is based on using local features extracted from a bank of filters. These features provide a description of different types of faint source structures. Our approach performs an initial training step in order to automatically learn and select the most salient features, which are then used in a Boosting classifier to perform the detection. The validity of our method is demonstrated using 19 images that compose a 2.5° x 2.5° radio mosaic, obtained with the Giant Metrewave Radio Telescope, centered on the MGRO J2019+37 peak of gamma emission at the Cygnus region. A comparison with two previously published radio catalogues of this region (task SAD of AIPS and SExtractor) is also provided.
机译:到目前为止已经提出了几种阈值化技术,以便在宽场干涉式无线图像中执行微小的紧凑源检测。由于它们的强度/噪声比低,这些自动检测方法可以很容易地错过一些物体。在本文中,我们提出了一种克服这个问题的新方法。我们的提案是基于使用从滤波器组中提取的本地功能。这些特征提供了不同类型的微弱源结构的描述。我们的方法执行初始训练步骤,以便自动学习和选择最突出的功能,然后在升压分类器中使用以执行检测。我们的方法的有效性使用19张图像与巨型Metrewave无线电望远镜一起获得2.5°x 2.5°的无线电马赛克,以Cygnus地区的MGRO J2019 + 37峰值为中心。还提供了与两个先前发表的此区域的无线电目录(AIPS和SUSTRACTOR的任务)的比较。

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