Galaxies living in rich environments are suffering different perturbations able to drastically
affect their evolution. Among these, ram pressure stripping, ie the pressure exerted by the …

Early observations with JWST indicate an overabundance of bright galaxies at redshifts z≳
10 relative to Hubble-calibrated model predictions. More puzzling still is the apparent lack of …

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 …

We present a new version of the galform semi-analytical model of galaxy formation. This
brings together several previous developments of galform into a single unified model …

We present an analytic formalism that describes the evolution of the stellar, gas and metal
content of galaxies. It is based on the idea, inspired by hydrodynamic simulations, that …

Using data from the COSMOS survey, we perform the first joint analysis of galaxy–galaxy
weak lensing, galaxy spatial clustering, and galaxy number densities. Carefully accounting …

We construct merger trees of dark matter haloes and quantify their merger rates and mass
growth rates using the joint data set from the Millennium and Millennium-II simulations. The …

We report and provide fitting functions for the abundance of dark matter haloes and
subhaloes as a function of mass, circular velocity, and redshift from the new Bolshoi–Planck …

Using the cosmological baryonic accretion rate and normal star formation (SF) efficiencies,
we present a very simple model for star-forming galaxies that accounts for the mass and …

We present the hestia simulation suite: High-resolutions Environmental Simulations of The
Immediate Area, a set of cosmological simulations of the Local Group. Initial conditions …