Raul E. Angulo

TL;DR: In this paper, the Munich galaxy formation model was updated to the Planck first-year cosmology, while modifying the treatment of baryonic processes to reproduce recent data on the abundance and passive fractions of galaxies from z = 3 down to z = 0.

TL;DR: The Millennium-XXL or MXXL simulation as mentioned in this paper uses 303 billion particles to represent the formation of dark matter structures throughout a 4.1 Gpc box in a Λ cold dark matter cosmology.

TL;DR: In this article, the authors scale the Millennium and Millennium-II simulations of structure growth in aCDM universe from the cosmo- logical parameters with which they were carried out (based on first-year results from the Wilkinson Microwave Anisotropy Probe, WMAP1) to parameters consistent with the seven-year WMAP data (WMAP7).

TL;DR: In this article, a suite of cosmological simulations were used to study the mass-concentration-redshift relation of dark matter haloes, and the mass profiles of CDM and WDM haloes were self-similar and well approximated by the Einasto profile.

TL;DR: In this paper, the authors use the Millennium Simulation series to investigate the mass and redshift dependence of the concentration of equilibrium cold dark matter (CDM) halos, and show how the latter may be used to predict concentrations for halos of all masses and at any redshift.