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Identification of multi-component LOFAR sources with multi-modal deep learning

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arxiv 2405.18584 v2 pith:XORWYNIX submitted 2024-05-28 astro-ph.IM astro-ph.GA

classification astro-ph.IMastro-ph.GA
keywords radiosourcescomponentcomponentsdatadeeplearningmulti-component
verification ladder T0 review T1 audit T2 compute T3 formal
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Modern 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.

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Cited by 2 Pith papers

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    astro-ph.GA 2026-07 conditional novelty 6.0 of 10

    An uncertainty-aware transformer reconstructs masked AGN broad lines and spectral halves with 4-16% flux errors and beats eleven purpose-built Lyα-reconstruction algorithms on a blind benchmark.

  2. Radio emission from a massive node of the cosmic web. A discovery powered by machine learning

    astro-ph.CO 2025-02 conditional novelty 6.0 of 10

    A machine learning scan of LOFAR data revealed 5 Mpc-scale diffuse radio emission around cluster PSZ2 G083.29-31.03, likely linked to two merging substructures.

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