{ "id": "2210.12264", "version": "v1", "published": "2022-10-21T21:40:32.000Z", "updated": "2022-10-21T21:40:32.000Z", "title": "A machine learning approach to assessing the presence of substructure in quasar host galaxies using the Hyper Suprime-Cam Subaru Strategic Program", "authors": [ "Chris Nagele", "John D. Silverman", "Tilman Hartwig", "Junyao Li", "Connor Bottrell", "Xuheng Ding", "Yoshiki Toba" ], "comment": "Comments are welcome", "categories": [ "astro-ph.GA" ], "abstract": "The conditions under which galactic nuclear regions become active are largely unknown, although it has been hypothesized that secular processes related to galaxy morphology could play a significant role. We investigate this question using optical i-band images of 3096 SDSS quasars and galaxies at 0.3