Hydrodynamical simulations of galaxy formation and evolution attempt to fully model the
physics that shapes galaxies. The agreement between the morphology of simulated and real …

Image simulations are essential tools for preparing and validating the analysis of current and
future wide-field optical surveys. However, the galaxy models used as the basis for these …

We investigate the dependence of galaxy structure on a variety of galactic and
environmental parameters for∼ 500 000 galaxies at z< 0.2, taken from the Sloan Digital Sky …

We analyse the optical morphologies of galaxies in the IllustrisTNG simulation at z∼ 0 with a
convolutional neural network trained on visual morphologies in the Sloan Digital Sky …

We examine morphology-separated color–mass diagrams to study the quenching of star
formation in∼ 100,000 (z∼ 0) Sloan Digital Sky Survey (SDSS) and∼ 20,000 (z∼ 1) …

We present a detailed comparison between numerical cosmological hydrodynamic zoom
simulations and the semi-analytic model (SAM) of Somerville et al., run within merger trees …

Recent cosmological hydrodynamical simulations are able to reproduce numerous statistical
properties of galaxies that are consistent with observational data. Yet, the adopted subgrid …

Measuring the morphological parameters of galaxies is a key requirement for studying their
formation and evolution. Surveys such as the Sloan Digital Sky Survey have resulted in the …

Understanding the physical processes that drive star formation is a key challenge for galaxy
formation models. In this paper, we study the tight correlation between the star formation rate …

Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …