20We examine subhaloes and galaxies residing in a simulated Λ cold dark matter galaxy cluster (M^crit_{200}=1.1× 10^{15} h^{-1} M_{☉}) produced by hydrodynamical codes ranging from classic smooth particle hydrodynamics (SPH), newer SPH codes, adaptive and moving mesh codes. These codes use subgrid models to capture galaxy formation physics. We compare how well these codes reproduce the same subhaloes/galaxies in gravity-only, non-radiative hydrodynamics and full feedback physics runs by looking at the overall subhalo/galaxy distribution and on an individual object basis. We find that the subhalo population is reproduced to within ≲10 per cent for both dark matter only and non-radiative runs, with individual objects showing code-to-code scat...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
We combine 10 high resolution resimulations of cluster--sized dark haloes with semi--analytic galaxy...
We examine subhaloes and galaxies residing in a simulated Λ cold dark matter galaxy cluster (M^crit_...
We examine subhaloes and galaxies residing in a simulated $\Lambda$ cold dark matter galaxy cluster ...
We have simulated the formation of a massive galaxy cluster (M_{200}^crit = 1.1 × 1015 h-1 M⊙) in a ...
We have simulated the formation of a massive galaxy cluster (M_{200}^crit = 1.1 7 1015 h-1 M 99) in...
22We examine the properties of the galaxies and dark matter haloes residing in the cluster infall re...
24Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and c...
Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and con...
(Abridged) We present a semi-analytic model for Cold Dark Matter halo substructure that can be used ...
The abundance and structure of dark matter subhaloes have been analysed extensively in recent studie...
We have simulated the formation of a galaxy cluster in a \u39b cold dark matter universe using 13 di...
International audienceBy comparing a collisionless cosmological N-body simulation (DM) to a smoothed...
We have simulated the formation of a galaxy cluster in a Ʌ cold dark matter universe using 13 differ...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
We combine 10 high resolution resimulations of cluster--sized dark haloes with semi--analytic galaxy...
We examine subhaloes and galaxies residing in a simulated Λ cold dark matter galaxy cluster (M^crit_...
We examine subhaloes and galaxies residing in a simulated $\Lambda$ cold dark matter galaxy cluster ...
We have simulated the formation of a massive galaxy cluster (M_{200}^crit = 1.1 × 1015 h-1 M⊙) in a ...
We have simulated the formation of a massive galaxy cluster (M_{200}^crit = 1.1 7 1015 h-1 M 99) in...
22We examine the properties of the galaxies and dark matter haloes residing in the cluster infall re...
24Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and c...
Building on the initial results of the nIFTy simulated galaxy cluster comparison, we compare and con...
(Abridged) We present a semi-analytic model for Cold Dark Matter halo substructure that can be used ...
The abundance and structure of dark matter subhaloes have been analysed extensively in recent studie...
We have simulated the formation of a galaxy cluster in a \u39b cold dark matter universe using 13 di...
International audienceBy comparing a collisionless cosmological N-body simulation (DM) to a smoothed...
We have simulated the formation of a galaxy cluster in a Ʌ cold dark matter universe using 13 differ...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
We examine the properties of the galaxies and dark matter haloes residing in the cluster infall regi...
We combine 10 high resolution resimulations of cluster--sized dark haloes with semi--analytic galaxy...