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    Neural network-based search for unmodeled transients in LIGO-Virgo-KAGRA’s third observing run

    Eric A. Moreno1,2, Katya Govorkova1,2, Ryan Raikman1,*, Siddharth Soni2, Ethan Marx1,2, William Benoit3, Alec Gunny1,2, Deep Chatterjee2, Christina Reissel1 et al.

    Malina M. Desai2, Rafia Omer3, Muhammed Saleem3, Philip Harris1, Erik Katsavounidis1,2, Michael W. Coughlin3, and Dylan Rankin4

    • 1Department of Physics, MIT, Cambridge, Massachusetts 02139, USA
    • 2LIGO Laboratory, 185 Albany Street, MIT, Cambridge, Massachusetts 02139, USA
    • 3School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
    • 4Department of Physics and Astronomy, University of Pennsylvania, Philadelphia, Pennsylvania, 19104, USA

    • *Contact author: rraikman@mit.edu

    Phys. Rev. D 112, 022003 – Published 15 July, 2025

    DOI: https://doi.org/10.1103/zykf-8klg

    Abstract

    This paper presents the results of a neural network (NN)-based search for short-duration gravitational-wave transients in data from the third observing run of LIGO, Virgo, and KAGRA. The search targets unmodeled transients with durations of milliseconds to a few seconds in the 30–1500 Hz frequency band, without assumptions about the incoming signal direction, polarization, or morphology. Using the gravitational wave anomalous knowledge (GWAK) method, three compact binary coalescences (CBCs) identified by existing pipelines are successfully detected, and a range of detector glitches are identified. The algorithm constructs a low-dimensional embedded space to capture the physical features of signals, enabling the detection of CBCs, detector glitches, and unmodeled transients. This study explores the potential of GWAK to generalize gravitational-wave searches and complement existing pipelines and demonstrates sensitivity to several classes of simulated short-duration GW transients, including core-collapse supernovae and other modeled sources, which have not yet been observed.

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