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    Hybrid algorithm combining matched filtering and convolutional neural networks for searching gravitational waves from binary black hole mergers

    Takahiro S. Yamamoto1,*, Kipp Cannon1,†, Hayato Motohashi2,‡, and Hiroaki W. H. Tahara2,§

    • 1Research Center for the Early Universe (RESCEU), Graduate School of Science, The University of Tokyo, Tokyo 113-0033, Japan
    • 2Department of Physics, Tokyo Metropolitan University, 1-1 Minami-Osawa, Hachioji, Tokyo 192-0397, Japan

    • *Contact author: yamamoto.s.takahiro@resceu.s.u-tokyo.ac.jp
    • †Contact author: kipp@resceu.s.u-tokyo.ac.jp
    • ‡Contact author: motohashi@tmu.ac.jp
    • §Contact author: tahara@tmu.ac.jp

    Phys. Rev. D 113, 062004 – Published 26 March, 2026

    DOI: https://doi.org/10.1103/5x62-9ldh

    Abstract

    Efficient searches for gravitational waves from compact binary coalescence are crucial for gravitational-wave observations. We present a proof-of-concept for a method that utilizes a neural network taking a signal-to-noise ratio map, a stack of signal-to-noise ratio time series calculated by the matched filter, as input and predicting the presence or absence of gravitational waves in observational data. We train the neural network with a data set of gravitational-wave signals from stellar-mass black hole mergers injected into stationary Gaussian noise. We use data set 1 of the mock data challenge MLGWSC-1 to assess the ability of the proposed algorithm. The estimated sensitivity distance is 2428.10 Mpc at the false alarm rate of 1 per month. These results indicate that our algorithm achieves reasonable sensitivity with practical computational resources.

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