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

Beheshtipour, B., & Papa, M. A. (in preparation). Deep learning for clustering of continuous gravitational wave candidates II: identification of low-SNR candidates.

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2012.04381.pdf (Preprint), 4MB
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2012.04381.pdf
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 Urheber:
Beheshtipour, Banafsheh1, Autor           
Papa, Maria Alessandra1, Autor           
Affiliations:
1Searching for Continuous Gravitational Waves, AEI-Hannover, MPI for Gravitational Physics, Max Planck Society, ou_2630691              

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Schlagwörter: General Relativity and Quantum Cosmology, gr-qc, Astrophysics, High Energy Astrophysical Phenomena, astro-ph.HE,Computer Science, Learning, cs.LG
 Zusammenfassung: 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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 Datum: 2020-12-08
 Publikationsstatus: Keine Angabe
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 Identifikatoren: arXiv: 2012.04381
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