The Evolution of Galaxy Clustering in Hierarchical Models

Astronomy and Astrophysics – Astrophysics

Scientific paper

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To appear in the proceedings of the Marseille IGRAP99 conference "Clustering at High Redshift"

Scientific paper

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.

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