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 …

The dark energy plus cold dark matter (ΛCDM) cosmological model has been a
demonstrably successful framework for predicting and explaining the large-scale structure of …

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 …

This paper introduces C olossus, a public, open-source python package for calculations
related to cosmology, the large-scale structure (LSS) of matter in the universe, and the …

We utilize high-resolution cosmological simulations to reveal that high-redshift galaxies tend
to undergo a robust 'wet compaction'event when near a 'golden'stellar mass of. This is a …

Predicting structural properties of dark matter haloes is one of the fundamental goals of
modern cosmology. We use the suite of MultiDark cosmological simulations to study the …

We use cosmological simulations from the FIRE (Feedback In Realistic Environments)
project to study the baryon cycle and galaxy mass assembly for central galaxies in the halo …

We present a robust method to constrain average galaxy star formation rates (SFRs), star
formation histories (SFHs), and the intracluster light (ICL) as a function of halo mass. Our …

The relation between halo mass, M, and concentration, c, is a critical component in our
understanding of the structure of dark matter halos. While numerous models for this relation …

We use cosmological simulations to study a characteristic evolution pattern of high-redshift
galaxies. Early, stream-fed, highly perturbed, gas-rich discs undergo phases of dissipative …