Testing a physical galaxy size definition across simulations
Invited Seminar, Institute of Computational Cosmology, Durham, UK
At the ICC I presented the results of Arjona-Gálvez et al. (2025) and outlined planned follow-up work extending the study to satellite galaxies. Preliminary results indicate two distinct satellite populations in the size–stellar mass plane: one population that follows the former relation and a second population that lies systematically above it. The latter population shows systematic trends with redshift and with host-centric distance. The seminar described the planned analysis to identify and characterise these two populations using the AURIGA-Superstars simulations. This investigation will apply the new size metric together with a newly developed, more sophisticated method for detecting galaxy edges created by Giulia Golini. The project will be carried out in collaboration with Giulia and Dr. Francesca Fragkoudi and aims to quantify how satellite sizes depend on environment and cosmic time. Presenting this at the ICC enabled in-depth discussion with experts in simulation analysis and galaxy structure.
