Polar coordinate transformations for machine learning based dark matter subhalo detection in strong gravitational lenses

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ID: 332458
2026
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Abstract
Abstract Strong gravitational lensing provides a powerful probe of dark matter, particularly on small scales where the gravitational effects of dark matter subhalos within galaxies can manifest as perturbations within the extended arcs of gravitationally lensed sources. We investigate whether transforming lensed images into polar coordinates improves the ability of convolutional neural networks to infer subhalo mass. We introduce a machine learning architecture that outputs a prediction uncertainty alongside a mass prediction to enable assessment of network reliability. Using simulated Hubble Space Telescope observations, we compare our models trained on Cartesian and polar representations under different initialisation schemes, noise levels, and subhalo concentrations (c = 60, c = 30). We find that polar-transformed inputs consistently yield higher subhalo detection fractions than standard Cartesian images across all tested masses. For subhalos with mass 109M⊙ ≤ M ≤ 109.5M⊙, the fraction of subhalos the network is able to detect increases by ~15 per cent. Pretrained networks outperform randomly initialized networks, and the polar transform consistently improves network performance in both low signal-to-noise data and for lower-concentration subhalos. These results demonstrate that presenting strong lensing images in a polar representation provides a computationally inexpensive way of improving CNN-based subhalo detection.
Reference Key
openalex_W7167604255 Use this key to autocite in the manuscript while using SciMatic Manuscript Manager or Thesis Manager
Authors J Campbell, Simon Dye, Emma Chapman, Adam Moss
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Journal monthly notices of the royal astronomical society
Year 2026
DOI
10.1093/mnras/stag1955
URL
https://doi.org/10.1093/mnras/stag1955
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