We investigate the influence of galaxy-galaxy interactions on the star formation by studying a sample of almost 1500 of the nearest galaxies, all within a...
Galaxy morphologies at 0.5 < z < 3 in the TNG50 hydrodynamic simulation
In this project we analyse the optical and structural properties of galaxies with redshifts (0.5 < z < 3.0) and more massive than 10 9 solar masses in the...
Galaxy morphology classification using unsupervised machine learning techniques
Upcoming deep surveys (e.g. LSST, JWST, EUCLID) will provide high quality imaging at unprecedentedly high red shifts, allowing the study of galaxy morphology at...
Galaxy morphology in 5 medium redshift clusters (Ascaso+, 2009)
Following the study presented in our previous paper, based on the Nordic Optical Telescope (NOT) sample, which consists of five clusters of galaxies within the...
Galaxy structure: core radii and central mass deficits
We investigate the nuclear and global structure of early-type galaxies, and the apparent disparity between the Nuker and Sersic models for radial light profiles...
Galaxy Structure: Core Radii, and Central Mass Deficits
We investigate the nuclear and global structure of elliptical galaxies, and the apparent disparity between the Nuker and Sérsic light-profile models. We show...