Simulating the impact of dust cooling on the statistical properties of the intracluster medium

Simulating the universe on an intercontinental grid of supercomputers

Simulating the Universe with MICE: The abundance of massive clusters

Simulating the WFXT sky

Simulating X-ray Supercavities and Their Impact on Galaxy Clusters

Simulation of the Cosmic Evolution of Atomic and Molecular Hydrogen in Galaxies

Simulation of the Polarized Sky at 1.4 GHz

Simulation studies of dark energy clustering induced by the formation of dark matter halos

Simulations and Observations of the Microwave Universe

Simulations of AGN feedback in galaxy clusters and groups

Simulations of BAO reconstruction with a quasar Lyman-alpha survey

Simulations of Baryon Acoustic Oscillations II: Covariance matrix of the matter power spectrum

Simulations of binary galaxy mergers and the link with Fast Rotators, Slow Rotators, and Kinematically Distinct Cores

Simulations of Early Baryonic Structure Formation with Stream Velocity: I. Halo Abundance

Simulations of galaxy formation with radiative transfer: Hydrogen reionization and radiative feedback

Simulations of MHD Instabilities in Intracluster Medium Including Anisotropic Thermal Conduction

Simulations of momentum feedback by black hole winds

Simulations of Nuclear Cluster formation

Simulations of Quintessential Cold Dark Matter: beyond the cosmological constant

Simulations of structure formation in interacting dark energy cosmologies