Over recent decades, cosmological simulations of galaxy formation have been instrumental
in advancing our understanding of structure and galaxy formation in the Universe. These …

The relation between halo mass, M, and concentration, c, is a critical component in our
understanding of the structure of dark matter halos. While numerous models for this relation …

We report on the successful completion of a 2 trillion particle cosmological simulation to z= 0
z=0 run on the Piz Daint supercomputer (CSCS, Switzerland), using 4000+ GPU nodes for a …

Precision cosmology has recently triggered new attention on the topic of approximate
methods for the clustering of matter on large scales, whose foundations date back to 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 …

Abstract We describe the Outer Rim cosmological simulation, one of the largest high-
resolution N-body simulations performed to date, aimed at promoting science to be carried …

Profiles of dark matter-dominated halos at the group and cluster scales play an important
role in modern cosmology. Using results from two very large cosmological N-body …

We study the modelling of the halo occupation distribution (HOD) for the eBOSS DR16
emission line galaxies (ELGs). Motivated by previous theoretical and observational studies …

Large-scale simulations of cosmic structure formation play an important role in interpreting
cosmological observations at high precision. The simulations must cover a parameter range …

Abstract We present the MAssive ClusterS and Intercluster Structures (MACSIS) project, a
suite of 390 clusters simulated with baryonic physics that yields realistic massive galaxy …