E(2) Equivariant Self-Attention for Radio Astronomy
Micah Bowles, Matthew Bromley, Max Allen, Anna Scaife

TL;DR
This paper introduces group-equivariant self-attention models for radio galaxy classification, demonstrating improved performance, faster training, and better interpretability aligned with astronomers' feature attention.
Contribution
It presents novel group-equivariant self-attention architectures tailored for radio astronomy, enhancing explainability and efficiency over prior models.
Findings
Equivariant models require fewer training epochs.
Equivariant models outperform non-equivariant counterparts.
Models attend to features similar to human astronomers.
Abstract
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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Taxonomy
TopicsAlgorithms and Data Compression · Fractal and DNA sequence analysis · Computational Physics and Python Applications
