天文学中的超立方体数据分析:光学干涉测量和毫秒脉冲星搜索

P. Gorham, T. Prince, S. Anderson
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引用次数: 3

摘要

天文数据集在其规模和所需分析的复杂性方面开始名符其实。在这里,我们讨论了两个天文数据分析问题,我们已经开始在超立方体并发处理器环境中实现:光学干涉测量项目所需的密集图像处理,以及搜索毫秒周期射电脉冲星所需的大规模功率谱分析。在这两种情况下,分析主要在傅里叶域中进行,我们发现问题很容易适应并发环境。在下面的报告中,我们简要概述了每个问题的天文学背景,然后讨论了一般的计算要求,最后介绍了可能的超立方体算法和迄今为止取得的结果。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Hypercube data analysis in astronomy: optical interferometry and millisecond pulsar searches
Astronomical data sets are beginning to live up to their name, in both their sizes and the complexity of the analysis required. Here we discuss two astronomical data analysis problems which we have begun to implement on a hypercube concurrent processor environment: The intensive image processing required in an optical interferometry project, and the large scale power spectral analysis required by a search for millisecond-period radio pulsars. In both cases the analysis proceeds largely in the Fourier domain, and we find that the problems are readily adapted to a concurrent environment. In the following report, we outline briefly the astronomical background for each problem, then discuss the general computational requirements, and finally present possible hypercube algorithms and results achieved to date.
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