Deep learning for clustering of continuous gravitational wave candidates. II. Identification of low-SNR candidates

B. Beheshtipour and M. A. Papa
Phys. Rev. D 103, 064027 – Published 15 March 2021

Abstract

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 [B. Beheshtipour and M. A. Papa, Phys. Rev. D 101, 064009 (2020)], 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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  • Received 9 December 2020
  • Accepted 22 February 2021

DOI:https://doi.org/10.1103/PhysRevD.103.064027

© 2021 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsStatistical Physics & ThermodynamicsNetworks

Authors & Affiliations

B. Beheshtipour1,2,* and M. A. Papa1,2,3,†

  • 1Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Callinstrasse 38, 30167 Hannover, Germany
  • 2Leibniz Universität Hannover, D-30167 Hannover, Germany
  • 3University of Wisconsin Milwaukee, 3135 N Maryland Avenue, Milwaukee, Wisconsin 53211, USA

  • *b.beheshtipour@aei.mpg.de
  • maria.alessandra.papa@aei.mpg.de

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Issue

Vol. 103, Iss. 6 — 15 March 2021

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