The Evolution of Galaxy Clustering in Hierarchical Models
Astrophysics
2007-05-23 v1
Abstract
The main ingredients of recent semi-analytic models of galaxy formation are summarised. We present predictions for the galaxy clustering properties of a well specified LCDM model whose parameters are constrained by observed local galaxy properties. We present preliminary predictions for evolution of clustering that can be probed with deep pencil beam surveys.
Cite
@article{arxiv.astro-ph/9910233,
title = {The Evolution of Galaxy Clustering in Hierarchical Models},
author = {Shaun Cole and Andrew Benson and Carlton Baugh and Cedric Lacey and Carlos Frenk},
journal= {arXiv preprint arXiv:astro-ph/9910233},
year = {2007}
}
Comments
To appear in the proceedings of the Marseille IGRAP99 conference "Clustering at High Redshift"