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arXiv 1201.5564astro-ph.IM
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离轴源的后相关滤波技术及RFI去除

Post-correlation filtering techniques for off-axis source and RFI removal

A. R. Offringa, A. G. de Bruyn, S. Zaroubi

摘要:

技术,以提高干涉无线电观测的数据质量被认为是。讨论了紫外平面内条纹频率的基本原理,并使用滤波器来衰减射频干扰(RFI)和离轴源。介绍和测试了滤波器的几种新应用。在单基线数据的时间和频率方向上的低通滤波器被成功地用于降低在感兴趣的区域中的噪声,并去除来自未建模的离轴源和RFI的旁瓣。数据整合,平均和网格的相关副作用进行了分析,并显示能够导致鬼和噪声的增加,特别是当使用长基线或干涉仪的元素,有一个大的视野。一种新的投影条纹低通滤波器被证明是潜在的有用的一阶源分离。初步测试表明,与常见的源分离技术相比,过滤器可以快几个因素,例如剥离和剥离的变体,目前正在LOFAR观测中进行测试,称为“分层剥离”。需要进一步测试以支持过滤器的性能。

英文摘要:

Techniques to improve the data quality of interferometric radio observations are considered. Fundaments of fringe frequencies in the uv-plane are discussed and filters are used to attenuate radio-frequency interference (RFI) and off-axis sources. Several new applications of filters are introduced and tested. A low-pass filter in time and frequency direction on single baseline data is successfully used to lower the noise in the area of interest and to remove sidelobes coming from unmodelled off-axis sources and RFI. Related side effects of data integration, averaging and gridding are analysed, and shown to be able to cause ghosts and an increase in noise, especially when using long baselines or interferometric elements that have a large field of view. A novel projected fringe low-pass filter is shown to be potentially useful for first order source separation. Initial tests show that the filters can be several factors faster compared to common source separation techniques such as peeling and a variant of peeling that is currently being tested on LOFAR observations called "demixed peeling". Further testing is required to support the performance of the filters.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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