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Table · dataset · 2025

Catalogue of inspected PRGs - CIPRG

Listed in IVOA Registry (Virtual Observatory)

Polar ring galaxies (PRGs) play an important role in understanding the evolution of galaxies, especially as unique cases of gas accretion and merging process between early and late morphological galaxy types.

Description

Regardless of their spectacular shape, these objects are very few in number and hard to find. Most of them were visually discovered, and then several of them were photometrically validated and kinematically confirmed galaxies (PRGs) are vary rare objects that are important for understanding galaxy evolution.

The aim of our research is to create a catalogue of candidates for PRGs using existing catalogues of PRGs. After revision of existing catalogues to develop an image-based approach with machine learning methods for the search and discovery of PRGs in a big sky survey. We visually inspected galaxies from existing catalogues of PRGs and created a training sample based on high-quality SDSS images.

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Our training sample is extremely small - only 87 objects where are strong and good PRGs candidates. For the first time, we applied deep learning to search for PRGs. Augmentation, image segmentation, ensemble, and transfer learning techniques were applied to mitigate the problem of an insufficient dataset (87 strong and good PRGs).

To search for PRGs, we applied our models to the SDSS catalogue of galaxies at z<0.1 (Vavilova et al., 2022, 2022KNIT...28....3V). Transfer learning with synthetic GALFIT images demonstrated that, despite overtraining, we were able to find galaxies with a ring pattern. Our deep learning approach has resulted in the discovery of three PRGs (SDSS J140644.42+471602.0; SDSS J133650.48+492745.3; SDSS J095717.30+364953.5).

Four PRGs were discovered through the visual inspection of ~2200 galaxies from the Catalogue of the SDSS Ring galaxies at z<0.1 (SDSS J095851.32+320422.9; SDSS J104211.05+234448.2; SDSS J162212.63+272032.2; SDSS J104600.10+090627.2). One galaxy discovered with transfer learning, SDSS J140644.42+471602.0, was studied using CIGALE software to determine its spectral energy distribution from IR to UV bands. Finally, we present a catalogue of 179 galaxies, among them 87 objects are strong and good PRG candidates, 79 objects are weak candidates, seven objects are from our current research and six objects from new research of Skrybina et al., 2024 (arXiv:2406.13496), Akhil et al., 2024MNRAS.530.2907A, Freitas-Lemes et al. 2024Ap&SS.369...93F, and Stanonik et al., 2009ApJ...696L...6S.

This catalogue will be useful for the CNN approach and theoretical studies. Our strategies represent valuable opportunities for future development of deep learning models to increase PRG identification in sky surveys.

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