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Using transfer learning to detect galaxy mergers

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arxiv 1805.10289 v2 pith:OJBMPTUS submitted 2018-05-25 astro-ph.IM cs.LG

classification astro-ph.IMcs.LG
keywords learningtransferdeepmergerbetterclassificationcnnsdetection
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

We investigate the use of deep convolutional neural networks (deep CNNs) for automatic visual detection of galaxy mergers. Moreover, we investigate the use of transfer learning in conjunction with CNNs, by retraining networks first trained on pictures of everyday objects. We test the hypothesis that transfer learning is useful for improving classification performance for small training sets. This would make transfer learning useful for finding rare objects in astronomical imaging datasets. We find that these deep learning methods perform significantly better than current state-of-the-art merger detection methods based on nonparametric systems like CAS and GM$_{20}$. Our method is end-to-end and robust to image noise and distortions; it can be applied directly without image preprocessing. We also find that transfer learning can act as a regulariser in some cases, leading to better overall classification accuracy ($p = 0.02$). Transfer learning on our full training set leads to a lowered error rate from 0.038 $\pm$ 1 down to 0.032 $\pm$ 1, a relative improvement of 15%. Finally, we perform a basic sanity-check by creating a merger sample with our method, and comparing with an already existing, manually created merger catalogue in terms of colour-mass distribution and stellar mass function.

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Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 139 citations worldwide. Full citation record

  1. From DES to KiDS: Domain adaptation for cross-survey detection of low-surface-brightness galaxies

    astro-ph.GA 2026-05 unverdicted novelty 6.0 of 10

    Domain adaptation with an ensemble of CNN and transformer models trained on DES detects 20,180 LSBGs and 434 UDGs in KiDS DR5, with structural parameters and environmental trends consistent with known samples.

  2. Performance of morphological classifiers for galaxy mergers compared to current machine learning methods

    astro-ph.GA 2026-07 conditional novelty 5.0 of 10

    Updated G-M20 and G-C morphological cuts achieve ~70% merger precision comparable to ML, with better high-z robustness, but only select pre-mergers.

  3. Search for spatial coincidences between galaxy mergers and Fermi-LAT 4FGL-DR4 sources

    astro-ph.HE 2025-07 conditional novelty 5.0 of 10

    Twenty-one galaxy mergers show statistically significant spatial coincidences with Fermi-LAT gamma-ray sources, including five unidentified gamma-ray objects.

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