HOW WELL DO COSMOLOGICAL SIMULATIONS REPRODUCE INDIVIDUAL HALO PROPERTIES?

The Ly�� forest at redshifts 0.1���1.6: good agreement between a large hydrodynamic simulation andHSTspectra

(2009) Pascal Paschos et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

The effect of large-scale power on simulated spectra of the Lyα forest

(2009) David Tytler et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

The clustering of the first galaxy haloes

(2009) Darren S. Reed et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

The diversity and similarity of simulated cold dark matter haloes

(2009) Julio F. Navarro et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

The Formation of Population III Binaries from Cosmological Initial Conditions

(2009) M. J. Turk et al.   SCIENCE

Mass, metal, and energy feedback in cosmological simulations

(2008) Benjamin D. Oppenheimer et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

The Aquarius Project: the subhaloes of galactic haloes

(2008) V. Springel et al.   MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY

Prospects for detecting supersymmetric dark matter in the Galactic halo

(2008) V. Springel et al.   NATURE