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E(2) Equivariant Self-Attention for Radio Astronomy

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arxiv 2111.04742 v2 pith:NRA6V7A2 submitted 2021-11-08 astro-ph.IM cs.CV

classification astro-ph.IMcs.CV
keywords equivarianceself-attentionastronomyequivariantexplainablemodelsradioaddress
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In this work we introduce group-equivariant self-attention models to address the problem of explainable radio galaxy classification in astronomy. We evaluate various orders of both cyclic and dihedral equivariance, and show that including equivariance as a prior both reduces the number of epochs required to fit the data and results in improved performance. We highlight the benefits of equivariance when using self-attention as an explainable model and illustrate how equivariant models statistically attend the same features in their classifications as human astronomers.

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Cited by 1 Pith paper

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  1. Radio Halo Detection in MWA Data using Deep Neural Networks and Generative Data Augmentation

    astro-ph.GA 2024-11 conditional novelty 6.0 of 10

    A diffusion-based generative augmentation pipeline enables a small-data neural classifier to detect diffuse radio halos in MWA/GLEAM images, rediscovering known halos and proposing new candidates.

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