Convolutional neural networks for the classification of glitches in gravitational-wave data streams
| Main Author: | |
|---|---|
| Publication Date: | 2023 |
| Other Authors: | , , , , |
| Format: | Article |
| Language: | eng |
| Source: | Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) |
| Download full: | https://hdl.handle.net/1822/87778 |
Summary: | We investigate the use of convolutional neural networks (including the modern ConvNeXt network family) to classify transient noise signals (i.e. glitches) and gravitational waves (GWs) in data from the Advanced LIGO detectors. First, we use models with a supervised learning approach, both trained from scratch using the Gravity Spy dataset and employing transfer learning by fine-tuning pre-trained models in this dataset. Second, we also explore a self-supervised approach, pre-training models with automatically generated pseudo-labels. Our findings are very close to existing results for the same dataset, reaching values for the F1 score of 97.18% (94.15%) for the best supervised (self-supervised) model. We further test the models using actual GW signals from LIGO-Virgo's O3 run. Although trained using data from previous runs (O1 and O2), the models show good performance, in particular when using transfer learning. We find that transfer learning improves the scores without the need for any training on real signals apart from the less than 50 chirp examples from hardware injections present in the Gravity Spy dataset. This motivates the use of transfer learning not only for glitch classification but also for signal classification. |
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Convolutional neural networks for the classification of glitches in gravitational-wave data streamsdeep learningglitchesgravitational wavesmachine learningCiências Naturais::Ciências FísicasWe investigate the use of convolutional neural networks (including the modern ConvNeXt network family) to classify transient noise signals (i.e. glitches) and gravitational waves (GWs) in data from the Advanced LIGO detectors. First, we use models with a supervised learning approach, both trained from scratch using the Gravity Spy dataset and employing transfer learning by fine-tuning pre-trained models in this dataset. Second, we also explore a self-supervised approach, pre-training models with automatically generated pseudo-labels. Our findings are very close to existing results for the same dataset, reaching values for the F1 score of 97.18% (94.15%) for the best supervised (self-supervised) model. We further test the models using actual GW signals from LIGO-Virgo's O3 run. Although trained using data from previous runs (O1 and O2), the models show good performance, in particular when using transfer learning. We find that transfer learning improves the scores without the need for any training on real signals apart from the less than 50 chirp examples from hardware injections present in the Gravity Spy dataset. This motivates the use of transfer learning not only for glitch classification but also for signal classification.We thank Osvaldo Freitas and Solange Nunes for fruitful discussions during the course of this work. We also thank Christopher Berry, Jools Clarke, Tom Dooney, Melissa López, Jade Powell, Max Razzano, and Agata Trovato for useful comments. A O is supported by the FCT project CERN/FIS-PAR/0029/2019. J C B is supported by a fellowship from ‘la Caixa’ Foundation (ID 100010434) and from the European Union’s Horizon 2020 research and innovation programme under the Marie Skłodowska-Curie Grant Agreement No. 847648 (fellowship code LCF/BQ/PI20/11760016). J C B is also supported by the research grant PID2020-118635GB-I00 from the Spain-Ministerio de Ciencia e Innovación. A T F and J A F are supported by the Spanish Agencia Estatal de Investigación (Grant PID2021-125485NB C21) funded by MCIN/AEI/10.13039/501100011033 and ERDF A way of making Europe). Further support is provided by the EU’s Horizon 2020 research and innovation (RISE) pro gramme H2020-MSCA-RISE-2017 (FunFiCO-777740) and by the European Horizon Europe staff exchange (SE) programme HORIZON-MSCA-2021-SE-01 (NewFunFiCO-101086251). This material is based upon work supported by NSF’s LIGO Laboratory which is a major facility fully funded by the National Science Foundation.info:eu-repo/semantics/publishedVersionIOP PublishingUniversidade do MinhoFernandes, TiagoVieira, SamuelOnofre, A.Calderón Bustillo, JuanTorres-Forné, AlejandroFont, José A.20232023-01-01T00:00:00Zinfo:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/articleapplication/pdfapplication/pdfhttps://hdl.handle.net/1822/87778engFernandes, T., Vieira, S., Onofre, A., Calderón Bustillo, J., Torres-Forné, A., & Font, J. A. (2023, September 4). Convolutional neural networks for the classification of glitches in gravitational-wave data streams. Classical and Quantum Gravity. IOP Publishing. http://doi.org/10.1088/1361-6382/acf26c0264-938110.1088/1361-6382/acf26chttps://iopscience.iop.org/article/10.1088/1361-6382/acf26cinfo:eu-repo/semantics/openAccessreponame:Repositórios Científicos de Acesso Aberto de Portugal (RCAAP)instname:FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiainstacron:RCAAP2024-11-02T01:22:01Zoai:repositorium.sdum.uminho.pt:1822/87778Portal AgregadorONGhttps://www.rcaap.pt/oai/openaireinfo@rcaap.ptopendoar:https://opendoar.ac.uk/repository/71602025-05-28T16:16:09.683731Repositórios Científicos de Acesso Aberto de Portugal (RCAAP) - FCCN, serviços digitais da FCT – Fundação para a Ciência e a Tecnologiafalse |
| dc.title.none.fl_str_mv |
Convolutional neural networks for the classification of glitches in gravitational-wave data streams |
| title |
Convolutional neural networks for the classification of glitches in gravitational-wave data streams |
| spellingShingle |
Convolutional neural networks for the classification of glitches in gravitational-wave data streams Fernandes, Tiago deep learning glitches gravitational waves machine learning Ciências Naturais::Ciências Físicas |
| title_short |
Convolutional neural networks for the classification of glitches in gravitational-wave data streams |
| title_full |
Convolutional neural networks for the classification of glitches in gravitational-wave data streams |
| title_fullStr |
Convolutional neural networks for the classification of glitches in gravitational-wave data streams |
| title_full_unstemmed |
Convolutional neural networks for the classification of glitches in gravitational-wave data streams |
| title_sort |
Convolutional neural networks for the classification of glitches in gravitational-wave data streams |
| author |
Fernandes, Tiago |
| author_facet |
Fernandes, Tiago Vieira, Samuel Onofre, A. Calderón Bustillo, Juan Torres-Forné, Alejandro Font, José A. |
| author_role |
author |
| author2 |
Vieira, Samuel Onofre, A. Calderón Bustillo, Juan Torres-Forné, Alejandro Font, José A. |
| author2_role |
author author author author author |
| dc.contributor.none.fl_str_mv |
Universidade do Minho |
| dc.contributor.author.fl_str_mv |
Fernandes, Tiago Vieira, Samuel Onofre, A. Calderón Bustillo, Juan Torres-Forné, Alejandro Font, José A. |
| dc.subject.por.fl_str_mv |
deep learning glitches gravitational waves machine learning Ciências Naturais::Ciências Físicas |
| topic |
deep learning glitches gravitational waves machine learning Ciências Naturais::Ciências Físicas |
| description |
We investigate the use of convolutional neural networks (including the modern ConvNeXt network family) to classify transient noise signals (i.e. glitches) and gravitational waves (GWs) in data from the Advanced LIGO detectors. First, we use models with a supervised learning approach, both trained from scratch using the Gravity Spy dataset and employing transfer learning by fine-tuning pre-trained models in this dataset. Second, we also explore a self-supervised approach, pre-training models with automatically generated pseudo-labels. Our findings are very close to existing results for the same dataset, reaching values for the F1 score of 97.18% (94.15%) for the best supervised (self-supervised) model. We further test the models using actual GW signals from LIGO-Virgo's O3 run. Although trained using data from previous runs (O1 and O2), the models show good performance, in particular when using transfer learning. We find that transfer learning improves the scores without the need for any training on real signals apart from the less than 50 chirp examples from hardware injections present in the Gravity Spy dataset. This motivates the use of transfer learning not only for glitch classification but also for signal classification. |
| publishDate |
2023 |
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2023 2023-01-01T00:00:00Z |
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info:eu-repo/semantics/publishedVersion |
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info:eu-repo/semantics/article |
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https://hdl.handle.net/1822/87778 |
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eng |
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eng |
| dc.relation.none.fl_str_mv |
Fernandes, T., Vieira, S., Onofre, A., Calderón Bustillo, J., Torres-Forné, A., & Font, J. A. (2023, September 4). Convolutional neural networks for the classification of glitches in gravitational-wave data streams. Classical and Quantum Gravity. IOP Publishing. http://doi.org/10.1088/1361-6382/acf26c 0264-9381 10.1088/1361-6382/acf26c https://iopscience.iop.org/article/10.1088/1361-6382/acf26c |
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IOP Publishing |
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