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arXiv 2012.04381gr-qcastro-ph.HEcs.LG

Deep learning for clustering of continuous gravitational wave candidates II: identification of low-SNR candidates

Max Planck Institute for Gravitational Physics (Albert Einstein Institute)(马克斯·普朗克引力物理研究所(阿尔伯特·爱因斯坦研究所));Leibniz Universität Hannover(莱布尼茨汉诺威大学);University of Wisconsin Milwaukee(威斯康星大学密尔沃基分校)

Banafsheh Beheshtipour, Maria Alessandra Papa

英文摘要:

Broad searches for continuous gravitational wave signals rely on hierarchies of follow-up stages for candidates above a given significance threshold. An important step to simplify these follow-ups and reduce the computational cost is to bundle together in a single follow-up nearby candidates. This step is called clustering and we investigate carrying it out with a deep learning network. In our first paper [1], we implemented a deep learning clustering network capable of correctly identifying clusters due to large signals. In this paper, a network is implemented that can detect clusters due to much fainter signals. These two networks are complementary and we show that a cascade of the two networks achieves an excellent detection efficiency across a wide range of signal strengths, with a false alarm rate comparable/lower than that of methods currently in use.

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