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Modelling the evolution of galaxy clustering
C. M. Baugh, A. J. Benson, S. Cole +2
Measurements of galaxy clustering are now becoming possible over a range of redshifts out to z=3. We use a semi-analytic model of galaxy formation to compute the expected evolution…
Semi-analytical galaxy formation models and the high redshift universe
Cedric Lacey, Carlton Baugh, Shaun Cole +2
Semi-analytical models of galaxy formation based on hierarchical clustering now make a wide range of predictions for observable properties of galaxies at low and high redshift. Thi…
Hybrid galaxy formation
A. J. Benson, S. Cole, C. S. Frenk +2
We model the two-point correlation function of galaxies in a cold dark matter Universe by combining two powerful theoretical tools - dissipationless N-body simulations of dark matt…
Galaxy Clusters in the Hubble Volume Simulations
Joerg M. Colberg, Simon D. M. White, Thomas J. MacFarland +8
We report on analyses of cluster samples obtained from the Hubble Volume Simulations. These simulations, an model named CDM and a flat low model with a cosmological co…
Early type galaxies in the hierarchical universe
C. M. Baugh, S. Cole, C. S. Frenk +2
Any realistic theory of galaxy formation must be set in the context of a model for the formation of structure in the universe. We describe a powerful approach -- semi-analytic mode…
Semianalytic modelling of the formation and evolution of galaxies
C. M. Baugh, C. G. Lacey, S. Cole +1
The high redshift observations of galaxies now becoming available from the Hubble Space Telescope and from large ground based telescopes are opening fresh windows on galaxy formati…
Peculiar Velocities of Galaxy Clusters
J. M. Colberg, S. D. M. White, T. J. MacFarland +5
We investigate the peculiar velocities predicted for galaxy clusters by theories in the cold dark matter family. A widely used hypothesis identifies rich clusters with high peaks o…
The seeds of rich galaxy clusters in the Universe
F. Governato, C. M. Baugh, C. S. Frenk +4
The discovery of a population of young galaxies at an epoch when the universe was about one tenth of its current age has shed new light on the question of when and how galaxies for…
Measuring Omega_0 using cluster evolution
V. R. Eke, S. Cole, C. S. Frenk +1
The evolution of the galaxy cluster abundance depends sensitively on the value of the cosmological density parameter, Omega_0. Recent ASCA data are used to quantify this evolution…
Mock 2dF and SDSS galaxy redshift surveys
Shaun Cole, Steve Hatton, David H. Weinberg +1
We present a comprehensive set of mock 2dF and SDSS galaxy redshift surveys constructed from a set of large, high-resolution cosmological N-body simulations. The radial selection f…