We review the progress in modeling the galaxy population in hydrodynamical simulations of
the ΛCDM cosmogony. State-of-the-art simulations now broadly reproduce the observed …

Numerical methods have become a powerful tool for research in astrophysics, but their utility
depends critically on the availability of suitable simulation codes. This calls for continuous …

We measure weak lensing cosmic shear power spectra from the 3-year galaxy shear catalog
of the Hyper Suprime-Cam (HSC) Subaru Strategic Program imaging survey. The shear …

We perform an extensive review of the numerous studies and methods used to determine
the total mass of the Milky Way. We group the various studies into seven broad classes …

We present the full public release of all data from the TNG100 and TNG300 simulations of
the IllustrisTNG project. IllustrisTNG is a suite of large volume, cosmological, gravo …

We present the ultraviolet luminosity function and an estimate of the cosmic star formation
rate density at 8< z< 13 derived from deep NIRCam observations taken in parallel with the …

Hydrodynamical simulations of galaxy formation have now reached sufficient volume to
make precision predictions for clustering on cosmologically relevant scales. Here, we use …

The IllustrisTNG project is a new suite of cosmological magnetohydrodynamical simulations
of galaxy formation performed with the arepo code and updated models for feedback …

We introduce the first two simulations of the IllustrisTNG project, a next generation of
cosmological magnetohydrodynamical simulations, focusing on the optical colours of …

We introduce the IllustrisTNG project, a new suite of cosmological magnetohydrodynamical
simulations performed with the moving-mesh code arepo employing an updated Illustris …