Deep learning for clustering of continuous gravitational wave candidates

B. Beheshtipour and M. A. Papa
Phys. Rev. D 101, 064009 – Published 5 March 2020

Abstract

In searching for continuous gravitational waves over very many (1017) templates, clustering is a powerful tool which increases the search sensitivity by identifying and bundling together candidates that are due to the same root cause. We implement a deep learning network that identifies clusters of signal candidates in the output of continuous gravitational wave searches and assess its performance. For loud signals, our network achieves a detection efficiency higher than 97% with a very low false alarm rate and maintains a reasonable detection efficiency for signals with lower amplitudes, i.e., at current upper limit values.

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  • Received 14 January 2020
  • Accepted 10 February 2020

DOI:https://doi.org/10.1103/PhysRevD.101.064009

© 2020 American Physical Society

Physics Subject Headings (PhySH)

Gravitation, Cosmology & AstrophysicsInterdisciplinary PhysicsStatistical Physics & Thermodynamics

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 Ave, Milwaukee, Wisconsin 53211, USA

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

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Issue

Vol. 101, Iss. 6 — 15 March 2020

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