A cosmologically significant population of very luminous high-redshift galaxies has recently
been discovered at submillimeter (submm) wavelengths. Advances in submm detector …

▪ Abstract Observations of damped Lyα systems offer a unique window on the neutral-gas
reservoirs that gave rise to galaxies at high redshifts. This review focuses on critical …

This paper describes a new publicly available codebase for modeling galaxy formation in a
cosmological context, the" Semi-Analytic Galaxy Evolution" model, or sage for short. 5 sage …

We have updated and extended our semi-analytic galaxy formation modelling capabilities
and applied them simultaneously to the stored halo/subhalo merger trees of the Millennium …

The extragalactic background light (EBL) is of fundamental importance both for
understanding the entire process of galaxy evolution and for γ-ray astronomy, but the overall …

We characterize mass, momentum, energy, and metal outflow rates of multiphase galactic
winds in a suite of FIRE-2 cosmological 'zoom-in'simulations from the Feedback in Realistic …

We simulate the growth of galaxies and their central supermassive black holes by
implementing a suite of semi-analytic models on the output of the Millennium Run, a very …

We simulate the assembly of a massive rich cluster and the formation of its constituent
galaxies in a flat, low-density universe. Our most accurate model follows the collapse, the …

We analyze star formation (SF) as a function of stellar mass (M*) and redshift z in the All-
Wavelength Extended Groth Strip International Survey. For 2905 field galaxies, complete to …

Recent observations of the distant Universe suggest that much of the stellar mass of bright
galaxies was already in place at z> 1. This presents a challenge for models of galaxy …