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Source-Agnostic Gravitational-Wave Detection with Recurrent Autoencoders
We present an application of anomaly detection techniques based on deep recurrent autoencoders (AEs) to the problem of detecting gravitational wave (GW) signals in laser interferometers. Trained on noise data, this class of algorithms could detect signals using an unsupervised strategy, i.e. without...
Autores principales: | , , , , |
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Lenguaje: | eng |
Publicado: |
2021
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1088/2632-2153/ac5435 http://cds.cern.ch/record/2777883 |
_version_ | 1780971713603829760 |
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author | Moreno, Eric A. Borzyszkowski, Bartlomiej Pierini, Maurizio Vlimant, Jean-Roch Spiropulu, Maria |
author_facet | Moreno, Eric A. Borzyszkowski, Bartlomiej Pierini, Maurizio Vlimant, Jean-Roch Spiropulu, Maria |
author_sort | Moreno, Eric A. |
collection | CERN |
description | We present an application of anomaly detection techniques based on deep recurrent autoencoders (AEs) to the problem of detecting gravitational wave (GW) signals in laser interferometers. Trained on noise data, this class of algorithms could detect signals using an unsupervised strategy, i.e. without targeting a specific kind of source. We develop a custom architecture to analyze the data from two interferometers. We compare the obtained performance to that obtained with other AE architectures and with a convolutional classifier. The unsupervised nature of the proposed strategy comes with a cost in terms of accuracy, when compared to more traditional supervised techniques. On the other hand, there is a qualitative gain in generalizing the experimental sensitivity beyond the ensemble of pre-computed signal templates. The recurrent AE outperforms other AEs based on different architectures. The class of recurrent AEs presented in this paper could complement the search strategy employed for GW detection and extend the discovery reach of the ongoing detection campaigns. |
id | cern-2777883 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2021 |
record_format | invenio |
spelling | cern-27778832023-01-31T08:46:56Zdoi:10.1088/2632-2153/ac5435http://cds.cern.ch/record/2777883engMoreno, Eric A.Borzyszkowski, BartlomiejPierini, MaurizioVlimant, Jean-RochSpiropulu, MariaSource-Agnostic Gravitational-Wave Detection with Recurrent Autoencodersphysics.ins-detDetectors and Experimental Techniquesphysics.data-anOther Fields of Physicscs.LGComputing and Computersastro-ph.IMAstrophysics and Astronomygr-qcGeneral Relativity and CosmologyWe present an application of anomaly detection techniques based on deep recurrent autoencoders (AEs) to the problem of detecting gravitational wave (GW) signals in laser interferometers. Trained on noise data, this class of algorithms could detect signals using an unsupervised strategy, i.e. without targeting a specific kind of source. We develop a custom architecture to analyze the data from two interferometers. We compare the obtained performance to that obtained with other AE architectures and with a convolutional classifier. The unsupervised nature of the proposed strategy comes with a cost in terms of accuracy, when compared to more traditional supervised techniques. On the other hand, there is a qualitative gain in generalizing the experimental sensitivity beyond the ensemble of pre-computed signal templates. The recurrent AE outperforms other AEs based on different architectures. The class of recurrent AEs presented in this paper could complement the search strategy employed for GW detection and extend the discovery reach of the ongoing detection campaigns.We present an application of anomaly detection techniques based on deep recurrent autoencoders to the problem of detecting gravitational wave signals in laser interferometers. Trained on noise data, this class of algorithms could detect signals using an unsupervised strategy, i.e., without targeting a specific kind of source. We develop a custom architecture to analyze the data from two interferometers. We compare the obtained performance to that obtained with other autoencoder architectures and with a convolutional classifier. The unsupervised nature of the proposed strategy comes with a cost in terms of accuracy, when compared to more traditional supervised techniques. On the other hand, there is a qualitative gain in generalizing the experimental sensitivity beyond the ensemble of pre-computed signal templates. The recurrent autoencoder outperforms other autoencoders based on different architectures. The class of recurrent autoencoders presented in this paper could complement the search strategy employed for gravitational wave detection and extend the reach of the ongoing detection campaigns.arXiv:2107.12698oai:cds.cern.ch:27778832021-07-27 |
spellingShingle | physics.ins-det Detectors and Experimental Techniques physics.data-an Other Fields of Physics cs.LG Computing and Computers astro-ph.IM Astrophysics and Astronomy gr-qc General Relativity and Cosmology Moreno, Eric A. Borzyszkowski, Bartlomiej Pierini, Maurizio Vlimant, Jean-Roch Spiropulu, Maria Source-Agnostic Gravitational-Wave Detection with Recurrent Autoencoders |
title | Source-Agnostic Gravitational-Wave Detection with Recurrent Autoencoders |
title_full | Source-Agnostic Gravitational-Wave Detection with Recurrent Autoencoders |
title_fullStr | Source-Agnostic Gravitational-Wave Detection with Recurrent Autoencoders |
title_full_unstemmed | Source-Agnostic Gravitational-Wave Detection with Recurrent Autoencoders |
title_short | Source-Agnostic Gravitational-Wave Detection with Recurrent Autoencoders |
title_sort | source-agnostic gravitational-wave detection with recurrent autoencoders |
topic | physics.ins-det Detectors and Experimental Techniques physics.data-an Other Fields of Physics cs.LG Computing and Computers astro-ph.IM Astrophysics and Astronomy gr-qc General Relativity and Cosmology |
url | https://dx.doi.org/10.1088/2632-2153/ac5435 http://cds.cern.ch/record/2777883 |
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