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arXiv 0812.4933astro-phstat.AP
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用于无线电干涉测量的压缩感知成像技术

Compressed sensing imaging techniques for radio interferometry

Y. Wiaux, L. Jacques, G. Puy, A. M. M. Scaife, P. Vandergheynst

摘要:

无线电干涉测量通过不完整和嘈杂的傅立叶测量来探测天体物理信号。压缩传感理论表明,此类测量实际上足以准确重建稀疏或可压缩信号。我们提出了新的通用成像技术的基础上凸优化的全局最小化问题定义在这方面。该框架的多功能性,特别是允许引入特定的先验信息的信号,这提供了显着改善的重建相对于标准的本地匹配追求算法CLEAN在射电天文学的可能性。我们通过研究两种不同类型的信号与非常通用的干涉配置观察到的模拟重建性能,说明了这种方法的潜力。第一类是致密天体的强度场。第二类是宇宙弦在宇宙微波背景辐射温度场中的印记,这对宇宙学特别有意义。

英文摘要:

Radio interferometry probes astrophysical signals through incomplete and noisy Fourier measurements. The theory of compressed sensing demonstrates that such measurements may actually suffice for accurate reconstruction of sparse or compressible signals. We propose new generic imaging techniques based on convex optimization for global minimization problems defined in this context. The versatility of the framework notably allows introduction of specific prior information on the signals, which offers the possibility of significant improvements of reconstruction relative to the standard local matching pursuit algorithm CLEAN used in radio astronomy. We illustrate the potential of the approach by studying reconstruction performances on simulations of two different kinds of signals observed with very generic interferometric configurations. The first kind is an intensity field of compact astrophysical objects. The second kind is the imprint of cosmic strings in the temperature field of the cosmic microwave background radiation, of particular interest for cosmology.

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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