COUGS-DESI: A Catalog of Unusual Galaxies with polar Structures in the DESI Legacy Imaging Surveys

• 出版年: Astronomy & Astrophysics
• 主要な著者: Bahr Seneca K. H., Mosenkov Aleksandr V., Guerrette Jacob A., Jensen Isaac H., George Jonah X., Spigarelli Thea E., Smith Ryan P., Burton Brandon T., Beckstead Kevan W., Seguine Jonah D., Casper Harrison K., Pineda Nefi, Holland Michael
• フォーマット: 論文
• 言語: 英語
• 出版事項: EDP Sciences 2026-06-01
• 主題: methods: data analysis; techniques: image processing; atlases; catalogs; surveys; galaxies: peculiar
• オンライン･アクセス: https://www.aanda.org/articles/aa/full_html/2026/06/aa58534-25/aa58534-25.html
• ISSN: 0004-6361; 1432-0746

Context. Polar-structure galaxies (PSGs) host photometrically and kinematically decoupled components oriented at large angles to one another. These systems, which include polar rings, polar disks, polar halos, polar bulges, polar dust lanes, and polar tidal structures, provide valuable insights into galaxy formation and evolution, although statistical studies are limited by their rarity. Aims. We aim to construct the largest and most homogeneous catalog of PSGs to date to enable robust statistical studies of their properties and occurrence rates in the Local Universe. Methods. Using DESI Legacy Imaging Surveys (DR10) data, we identified PSG candidates in the Siena Galaxy Atlas (SGA) through visual inspection, convolutional neural network (CNN) classification, and cross-matching with previously reported systems. Each galaxy was assigned a PSG subtype and host morphology. We analyzed the general properties of PSGs and compared them with those for all galaxies in the SGA. Simple image simulations were used to evaluate projection effects. Results. The resulting Catalog of Unusual Galaxies with polar Structures in the DESI Legacy Imaging Surveys (COUGS-DESI) contains 2989 PSG candidates, including 342 previously known objects. Projection effects from random galaxy overlaps are negligible. The sample spans a wide range of polar morphologies, with 1113 polar rings, 75 polar bulges, 216 polar halos, 185 polar dust lanes, and 1315 polar tidal structures. Overall, PSGs constitute 2.2% of local non-dwarf galaxies, with polar rings representing 0.7%. Approximately 1% of S0 galaxies in the SGA host polar rings, whereas spirals constitute the most common morphological type among the PSG hosts in our catalog. Conclusions. COUGS–DESI increases the number of known PSG candidates by an order of magnitude and provides a foundation for detailed studies of the formation and evolution of polar structures.