Analysis of Ring Galaxies Detected Using Deep Learning with Real and Simulated Data
Harish Krishnakumar, J. Bryce Kalmbach

TL;DR
This study develops a CNN-based method trained on simulated data to identify ring galaxies, creating a large catalog and highlighting challenges like false positives due to data imbalance, with implications for future large-scale surveys.
Contribution
Introduces a CNN approach trained on simulated galaxies and transfer learned to real data for efficient ring galaxy detection, incorporating GAN-based data augmentation.
Findings
Generated a catalog of 1967 ring galaxies.
Achieved a false-positive rate of 41.1%.
Demonstrated potential of ML pipelines for rare galaxy morphologies.
Abstract
Understanding the formation and evolution of ring galaxies, which possess an atypical ring-like structure, is crucial for advancing knowledge of black holes and galaxy dynamics. However, current catalogs of ring galaxies are limited, as manual analysis takes months to accumulate an appreciable sample of rings. This paper presents a convolutional neural network (CNN) to identify ring galaxies from unclassified samples. A CNN was trained on 100,000 simulated galaxies, transfer learned to a sample of real galaxies, and applied to a previously unclassified dataset to generate a catalog of rings which was then manually verified. Data augmentation with a generative adversarial network (GAN) to simulate images of galaxies was also employed. The resulting catalog contains 1967 ring galaxies. The properties of these galaxies were then estimated from their photometry and compared to the Galaxy…
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Taxonomy
TopicsData Visualization and Analytics · Computational Physics and Python Applications · Galaxies: Formation, Evolution, Phenomena
