Using transfer learning to detect galaxy mergers
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Abstract (arXiv)
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 GM20. 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 ± 1 down to 0.032 ± 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.
Key facts. Cited by 11 papers in the map (data through 7 Oct 2026). First posted on arXiv 25 May 2018.
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Citing papers per year: 2021: 4; 2022: 3; 2023: 2; 2024: 0; 2025: 2.
11 papers.
- 2021A Data Quality-Driven View of MLOpscited by 31
- 2022ButterflyFlow: Building Invertible Layers with Butterfly Matricescited by 12
- 2021DeepMerge II: Building Robust Deep Learning Algorithms for Merging Galaxy Identification Across Domainscited by 10
- 2021CInC Flow: Characterizable Invertible 3x3 Convolutioncited by 4
- 2021Morphological classification of compact and extended radio galaxies using convolutional neural networks and data augmentation techniquescited by 3
- 2022How Well Do Vision Transformers (VTs) Transfer To The Non-Natural Image Domain? An Empirical Study Involving Art Classificationcited by 3
- 2022Using Machine Learning to Determine Morphologies of z<1 AGN Host Galaxies in the Hyper Suprime-Cam Wide Surveycited by 1
- 2023Galaxy Classification Using Transfer Learning and Ensemble of CNNs With Multiple Colour Spacescited by 1
- 2025Automatic Machine Learning Framework to Study Morphological Parameters of AGN Host Galaxies within z < 1.4 in the Hyper Supreme-Cam Wide Surveycited by 1
- 2025CDFlow: Building Invertible Layers with Circulant and Diagonal Matricescited by 1
- 2023A Deep Neural Network -- Mechanistic Hybrid Model to Predict Pharmacokinetics in Ratcited by 0
- 2025CDFlow: Building Invertible Layers with Circulant and Diagonal Matrices29 Oct 2025
- 2025Automatic Machine Learning Framework to Study Morphological Parameters of AGN Host Galaxies within z < 1.4 in the Hyper Supreme-Cam Wide Survey27 Jan 2025
- 2023A Deep Neural Network -- Mechanistic Hybrid Model to Predict Pharmacokinetics in Rat13 Oct 2023
- 2023Galaxy Classification Using Transfer Learning and Ensemble of CNNs With Multiple Colour Spaces26 Mar 2023
- 2022Using Machine Learning to Determine Morphologies of z<1 AGN Host Galaxies in the Hyper Suprime-Cam Wide Survey20 Dec 2022
- 2022ButterflyFlow: Building Invertible Layers with Butterfly Matrices28 Sep 2022
- 2022How Well Do Vision Transformers (VTs) Transfer To The Non-Natural Image Domain? An Empirical Study Involving Art Classification9 Aug 2022
- 2021CInC Flow: Characterizable Invertible 3x3 Convolution3 Jul 2021
- 2021Morphological classification of compact and extended radio galaxies using convolutional neural networks and data augmentation techniques1 Jul 2021
- 2021DeepMerge II: Building Robust Deep Learning Algorithms for Merging Galaxy Identification Across Domains2 Mar 2021
- 2021A Data Quality-Driven View of MLOps15 Feb 2021