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dc.contributor.authorAlegre, Lara
dc.contributor.authorBest, Philip
dc.contributor.authorSabater, Jose
dc.contributor.authorRottgering, Huub
dc.contributor.authorHardcastle, Martin
dc.contributor.authorWilliams, Wendy
dc.date.accessioned2024-10-21T16:45:00Z
dc.date.available2024-10-21T16:45:00Z
dc.date.issued2024-06-11
dc.identifier.citationAlegre , L , Best , P , Sabater , J , Rottgering , H , Hardcastle , M & Williams , W 2024 , ' Identification of multi-component LOFAR sources with multi-modal deep learning ' , Monthly Notices of the Royal Astronomical Society , vol. 532 , no. 3 . https://doi.org/10.1093/mnras/stae1454
dc.identifier.issn0035-8711
dc.identifier.otherArXiv: http://arxiv.org/abs/2405.18584v2
dc.identifier.otherORCID: /0000-0003-4223-1117/work/170343181
dc.identifier.urihttp://hdl.handle.net/2299/28370
dc.description© 2024 The Author(s). Published by Oxford University Press on behalf of Royal Astronomical Society. This is an Open Access article distributed under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0/).
dc.description.abstractModern high-sensitivity radio telescopes are discovering an increased number of resolved sources with intricate radio structures and fainter radio emissions. These sources often present a challenge because source detectors might identify them as separate radio sources rather than components belonging to the same physically connected radio source. Currently, there are no reliable automatic methods to determine which radio components are single radio sources or part of multi-component sources. We propose a deep learning classifier to identify those sources that are part of a multi-component system and require component association on data from the LOFAR Two-Metre Sky Survey (LoTSS). We combine different types of input data using multi-modal deep learning to extract spatial and local information about the radio source components: a convolutional neural network component that processes radio images is combined with a neural network component that uses parameters measured from the radio sources and their nearest neighbours. Our model retrieves 94 per cent of the sources with multiple components on a balanced test set with 2,683 sources and achieves almost 97 per cent accuracy in the real imbalanced data (323,103 sources). The approach holds potential for integration into pipelines for automatic radio component association and cross-identification. Our work demonstrates how deep learning can be used to integrate different types of data and create an effective solution for managing modern radio surveys.en
dc.format.extent19
dc.format.extent2452319
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.subjectastro-ph.IM
dc.subjectastro-ph.GA
dc.titleIdentification of multi-component LOFAR sources with multi-modal deep learningen
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1093/mnras/stae1454
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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