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 present the new semi-analytic model of galaxy evolution, Dark Sage, a heavily modified
version of the publicly available sage code. The model is designed for detailed evolution of …

… Because h is a dimensionless constant and not a unit (see Croton 2013), we dissociate
explicit factors of h from relevant units, in favour of it either being attached to the number in …

We introduce the the three hundred project, an endeavour to model 324 large galaxy clusters
with full-physics hydrodynamical re-simulations. Here we present the data set and study …

We present the public release of the MultiDark-Galaxies: three distinct galaxy catalogues
derived from one of the Planck cosmology MultiDark simulations (ie MDPL2, with a volume of (…

We use the hydrodynamic, cosmological EAGLE simulations to investigate how the hot gas
in haloes condenses to form and grow galaxies. We select haloes from the simulations that …

We present a comparison of nine galaxy formation models, eight semi-analytical, and one
halo occupation distribution model, run on the same underlying cold dark matter simulation (…

We present a comparison of the observed evolving galaxy stellar mass functions with the
predictions of eight semi-analytic models and one halo occupation distribution model. While …

Many techniques have been used in the literature for determining which particles or cells in
a hydrodynamic simulation are attached to a galaxy. Often these invoke a spherical aperture …

We use eagle to quantify the effect galaxy mergers have on the stellar specific angular
momentum of galaxies, j stars . We split mergers into dry (gas-poor)/wet (gas-rich), major/minor …