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How the dark matter halos cluster in Lagrangian space
Cristiano Porciani, Paolo Catelan, Cedric Lacey
We investigate the clustering of dark matter halos in Lagrangian space in terms of their two-point correlation function, spanning more than 4 orders of magnitudes of halo masses. 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…
The Space Density of Spiral Galaxies as function of their Luminosity, Surface Brightness and Scalesize
Roelof S. de Jong, Cedric Lacey
The local space density of galaxies as a function of their basic structural parameters --like luminosity, surface brightness and scalesize-- is still poorly known. Our poor knowled…
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…
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…