Attention-gating for improved radio galaxy classification
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Abstract (arXiv)
In this work we introduce attention as a state of the art mechanism for classification of radio galaxies using convolutional neural networks. We present an attention-based model that performs on par with previous classifiers while using more than 50% fewer parameters than the next smallest classic CNN application in this field. We demonstrate quantitatively how the selection of normalisation and aggregation methods used in attention-gating can affect the output of individual models, and show that the resulting attention maps can be used to interpret the classification choices made by the model. We observe that the salient regions identified by the our model align well with the regions an expert human classifier would attend to make equivalent classifications. We show that while the selection of normalisation and aggregation may only minimally affect the performance of individual models, it can significantly affect the interpretability of the respective attention maps and by selecting a model which aligns well with how astronomers classify radio sources by eye, a user can employ the model in a more effective manner.
Key facts. Cited by 9 papers in the map (data through 13 Oct 2026). First posted on arXiv 2 Dec 2020.
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Citing papers per year: 2021: 3; 2022: 0; 2023: 3; 2024: 2; 2025: 0; 2026: 1.
9 papers.
- 2023MiraBest: A Dataset of Morphologically Classified Radio Galaxies for Machine Learningcited by 4
- 2021E(2) Equivariant Self-Attention for Radio Astronomycited by 2
- 2024Evaluating Bayesian deep learning for radio galaxy classificationcited by 2
- 2024Insights on Galaxy Evolution from Interpretable Sparse Feature Networkscited by 2
- 2021Can semi-supervised learning reduce the amount of manual labelling required for effective radio galaxy morphology classification?cited by 0
- 2021Weight Pruning and Uncertainty in Radio Galaxy Classificationcited by 0
- 2023Advances on the classification of radio image cubescited by 0
- 2023Deep Learning for Morphological Identification of Extended Radio Galaxies using Weak Labelscited by 0
- 2026STRADAViT: Self-Supervised Domain Adaptation of Vision Transformer Backbones for Radio Astronomycited by 0
- 2026STRADAViT: Self-Supervised Domain Adaptation of Vision Transformer Backbones for Radio Astronomy31 Mar 2026
- 2024Insights on Galaxy Evolution from Interpretable Sparse Feature Networks30 Dec 2024
- 2024Evaluating Bayesian deep learning for radio galaxy classification28 May 2024
- 2023Deep Learning for Morphological Identification of Extended Radio Galaxies using Weak Labels9 Aug 2023
- 2023MiraBest: A Dataset of Morphologically Classified Radio Galaxies for Machine Learning18 May 2023
- 2023Advances on the classification of radio image cubes5 May 2023
- 2021Weight Pruning and Uncertainty in Radio Galaxy Classification23 Nov 2021
- 2021E(2) Equivariant Self-Attention for Radio Astronomy8 Nov 2021
- 2021Can semi-supervised learning reduce the amount of manual labelling required for effective radio galaxy morphology classification?8 Nov 2021