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The Durham/UKST Galaxy Redshift Survey - VI. Power spectrum analysis of clustering
F. Hoyle, C. M. Baugh, T. Shanks +1
We present the power spectrum analysis of clustering in the Durham/UKST Galaxy Redshift Survey, which covers 1450 square degrees and consists of 2501 galaxy redshifts sampled at a…
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…
The implications of the large scale galaxy power spectrum for Cold Dark Matter
C. M. Baugh, E. Gaztanaga
The APM Galaxy Survey maps the angular positions of more than one million galaxies to , covering a volume comparable to the forthcoming Sloan Digital Sky Survey. A nume…
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…
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…