Modeling galaxy formation in a cosmological context presents one of the greatest
challenges in astrophysics today due to the vast range of scales and numerous physical …

We present a comprehensive review of keV-scale sterile neutrino Dark Matter, collecting
views and insights from all disciplines involved—cosmology, astrophysics, nuclear, and …

We present the new TNG50 cosmological, magnetohydrodynamical simulation–the third and
final volume of the IllustrisTNG project. This simulation occupies a unique combination of …

We present emerge, an E mpirical M od E l for the fo R mation of G alaxi E s, describing the
evolution of individual galaxies in large volumes from z∼ 10 to the present day. We assign a …

We present an overview of galaxy evolution across cosmic time in the Illustris simulation.
Illustris is an N-body/hydrodynamical simulation that evolves 2× 18203 resolution elements …

We have updated the Munich galaxy formation model to the Planck first-year cosmology,
while modifying the treatment of baryonic processes to reproduce recent data on the …

We combine molecular gas masses inferred from CO emission in 500 star-forming galaxies
(SFGs) between z= 0 and 3, from the IRAM-COLDGASS, PHIBSS1/2, and other surveys, with …

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 …

The rapidly expanding field of galaxy formation lies at the interface between astronomy,
particle physics, and cosmology. Covering diverse topics from these disciplines, all of which …

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 …