In our modern understanding of galaxy formation, every galaxy forms within a dark matter
halo. The formation and growth of galaxies over time is connected to the growth of the halos …

Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …

We present a method to flexibly and self-consistently determine individual galaxies' star
formation rates (SFRs) from their host haloes' potential well depths, assembly histories, and …

We introduce a suite of cosmological volume simulations to study the evolution of galaxies
as part of the Feedback in Realistic Environments project. FIREbox, the principal simulation …

The two-point correlation function (2PCF) is the most widely used tool for quantifying the
spatial distribution of galaxies. Since the distribution of galaxies is determined by galaxy …

Using cosmological simulations, we address the properties of high-redshift star-forming
galaxies (SFGs) across their main sequence (MS) in the plane of star formation rate (SFR) …

We review the field of collisionless numerical simulations for the large-scale structure of the
Universe. We start by providing the main set of equations solved by these simulations and …

Using cosmological simulations, we address the interplay between structure and star
formation in high-redshift galaxies via the evolution of surface density profiles. Our sample …

The map** between the distributions of the observed galaxy stellar mass and the
underlying dark matter haloes provides the crucial link from theories of large-scale structure …

The similarity between the distributions of spins for galaxies (λgal) and for dark-matter
haloes (λhalo), indicated both by simulations and observations, is naively interpreted as a …