24Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and contrast the impact of baryonic physics with a single massive galaxy cluster, run with 11 state-of-the-art codes, spanning adaptive mesh, moving mesh, classic and modern smoothed particle hydrodynamics (SPH) approaches. For each code represented we have a dark-matter-only (DM) and non-radiative (NR) version of the cluster, as well as a full physics (FP) version for a subset of the codes. We compare both radial mass and kinematic profiles, as well as global measures of the cluster (e.g. concentration, spin, shape), in the NR and FP runs with that in the DM runs. Our analysis reveals good consistency ⪅20 per cent) between global properties of th...
We examine subhaloes and galaxies residing in a simulated Λ cold dark matter galaxy cluster (M^crit_...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
The back-reaction of baryons on the dark matter halo density profile is of great interest, not least...
Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and con...
Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and co...
77Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and c...
We carry out an analysis of a set of cosmological smoothed particle hydrodynamics (SPH) hydrodynamic...
22We examine the properties of the galaxies and dark matter haloes residing in the cluster infall re...
20We examine subhaloes and galaxies residing in a simulated Λ cold dark matter galaxy cluster (M^cri...
We have simulated the formation of a massive galaxy cluster (M_{200}^crit = 1.1 7 1015 h-1 M 99) in...
We discuss an extended set of Tree+SPH (smoothed particle hydrodynamics) simulations of the formatio...
The role of baryon models in hydrodynamic simulations is still unclear. Future surveys that use clus...
7siLuminous matter produces very energetic events, such as active galactic nuclei and supernova expl...
We have simulated the formation of a massive galaxy cluster (M_{200}^crit = 1.1 × 1015 h-1 M⊙) in a ...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
We examine subhaloes and galaxies residing in a simulated Λ cold dark matter galaxy cluster (M^crit_...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
The back-reaction of baryons on the dark matter halo density profile is of great interest, not least...
Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and con...
Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and co...
77Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and c...
We carry out an analysis of a set of cosmological smoothed particle hydrodynamics (SPH) hydrodynamic...
22We examine the properties of the galaxies and dark matter haloes residing in the cluster infall re...
20We examine subhaloes and galaxies residing in a simulated Λ cold dark matter galaxy cluster (M^cri...
We have simulated the formation of a massive galaxy cluster (M_{200}^crit = 1.1 7 1015 h-1 M 99) in...
We discuss an extended set of Tree+SPH (smoothed particle hydrodynamics) simulations of the formatio...
The role of baryon models in hydrodynamic simulations is still unclear. Future surveys that use clus...
7siLuminous matter produces very energetic events, such as active galactic nuclei and supernova expl...
We have simulated the formation of a massive galaxy cluster (M_{200}^crit = 1.1 × 1015 h-1 M⊙) in a ...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
We examine subhaloes and galaxies residing in a simulated Λ cold dark matter galaxy cluster (M^crit_...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
The back-reaction of baryons on the dark matter halo density profile is of great interest, not least...