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Subhaloes gone Notts: the clustering properties of subhaloes
2014
Monthly notices of the Royal Astronomical Society
We present a study of the substructure finder dependence of subhalo clustering in the Aquarius Simulation. We run 11 different subhalo finders on the haloes of the Aquarius Simulation and we study their differences in the density profile, mass fraction and 2-point correlation function of subhaloes in haloes. We also study the mass and vmax dependence of subhalo clustering. As the Aquarius Simulation has been run at different resolutions, we study the convergence with higher resolutions. We find
doi:10.1093/mnras/stt2446
fatcat:fyxisywoz5bybgl2hqpv6b5esa