Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations
Because of the electromagnetic (EM) radiation produced during the merger, compact binary coalescences with neutron stars may result in multi-messenger observations. In order to follow up on the gravitational-wave (GW) signal with EM telescopes, it is critical to promptly identify the properties of these sources. This identification must rely on the properties of the progenitor source, such as the component masses and spins, as determined by low-latency detection pipelines in real time. The output of these pipelines, however, might be biased, which could decrease the accuracy of parameter recovery. Machine learning algorithms are used to correct this bias. In this work, we revisit this problem and discuss two new implementations of supervised machine learning algorithms, K-nearest neighbors and random forest, which are able to predict the presence of a neutron star and post-merger matter remnant in low-latency compact binary coalescence searches across different search pipelines and data sets. Additionally, we present a novel approach for calculating the Bayesian probabilities for these two metrics. Instead of metric scores derived from binary machine learning classifiers, our scheme is designed to provide the astronomy community well-defined probabilities. This would deliver a more direct and easily interpretable product to assist EM telescopes in deciding whether to follow up on GW events in real time.
Berbel, Marina
4aacf5a9-a35e-4522-9279-2fe848d42b72
Miravet-Tenés, Miquel
398b0819-ed3a-44a3-aa0c-4e912ebcbef1
Chaudhary, Sushant Sharma
1c42965b-d5da-45b6-bc8b-25a1ea09592c
Albanesi, Simone
c835aa2a-cc69-4df6-a1fe-e80e34df390a
Cavaglià, Marco
6408d168-df08-4724-bc4b-5e703a197774
Zertuche, Lorena Magaña
9e50276f-8054-47c7-8c09-28643cc6b346
Tseneklidou, Dimitra
e8ba2daf-4d68-4284-ab29-6cf9030922b8
Zheng, Yanyan
2ee71365-e5ee-4ab0-bb3f-239d710e86b2
Coughlin, Michael W
81e44f63-66cd-4f48-b89d-9167524a8426
Toivonen, Andrew
657c11f1-a93d-4a5c-b806-6116581a7e5b
2 April 2024
Berbel, Marina
4aacf5a9-a35e-4522-9279-2fe848d42b72
Miravet-Tenés, Miquel
398b0819-ed3a-44a3-aa0c-4e912ebcbef1
Chaudhary, Sushant Sharma
1c42965b-d5da-45b6-bc8b-25a1ea09592c
Albanesi, Simone
c835aa2a-cc69-4df6-a1fe-e80e34df390a
Cavaglià, Marco
6408d168-df08-4724-bc4b-5e703a197774
Zertuche, Lorena Magaña
9e50276f-8054-47c7-8c09-28643cc6b346
Tseneklidou, Dimitra
e8ba2daf-4d68-4284-ab29-6cf9030922b8
Zheng, Yanyan
2ee71365-e5ee-4ab0-bb3f-239d710e86b2
Coughlin, Michael W
81e44f63-66cd-4f48-b89d-9167524a8426
Toivonen, Andrew
657c11f1-a93d-4a5c-b806-6116581a7e5b
Berbel, Marina, Miravet-Tenés, Miquel, Chaudhary, Sushant Sharma, Albanesi, Simone, Cavaglià, Marco, Zertuche, Lorena Magaña, Tseneklidou, Dimitra, Zheng, Yanyan, Coughlin, Michael W and Toivonen, Andrew
(2024)
Bayesian real-time classification of multi-messenger electromagnetic and gravitational-wave observations.
Classical and Quantum Gravity, 41 (8), [085012].
(doi:10.1088/1361-6382/ad3279).
Abstract
Because of the electromagnetic (EM) radiation produced during the merger, compact binary coalescences with neutron stars may result in multi-messenger observations. In order to follow up on the gravitational-wave (GW) signal with EM telescopes, it is critical to promptly identify the properties of these sources. This identification must rely on the properties of the progenitor source, such as the component masses and spins, as determined by low-latency detection pipelines in real time. The output of these pipelines, however, might be biased, which could decrease the accuracy of parameter recovery. Machine learning algorithms are used to correct this bias. In this work, we revisit this problem and discuss two new implementations of supervised machine learning algorithms, K-nearest neighbors and random forest, which are able to predict the presence of a neutron star and post-merger matter remnant in low-latency compact binary coalescence searches across different search pipelines and data sets. Additionally, we present a novel approach for calculating the Bayesian probabilities for these two metrics. Instead of metric scores derived from binary machine learning classifiers, our scheme is designed to provide the astronomy community well-defined probabilities. This would deliver a more direct and easily interpretable product to assist EM telescopes in deciding whether to follow up on GW events in real time.
This record has no associated files available for download.
More information
Published date: 2 April 2024
Identifiers
Local EPrints ID: 503232
URI: http://eprints.soton.ac.uk/id/eprint/503232
ISSN: 0264-9381
PURE UUID: 4050a5c5-e04a-4560-915b-06088a3ab607
Catalogue record
Date deposited: 24 Jul 2025 17:02
Last modified: 25 Jul 2025 02:15
Export record
Altmetrics
Contributors
Author:
Marina Berbel
Author:
Miquel Miravet-Tenés
Author:
Sushant Sharma Chaudhary
Author:
Simone Albanesi
Author:
Marco Cavaglià
Author:
Lorena Magaña Zertuche
Author:
Dimitra Tseneklidou
Author:
Yanyan Zheng
Author:
Michael W Coughlin
Author:
Andrew Toivonen
Download statistics
Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.
View more statistics