The Evolution of Galaxy Clustering in Hierarchical Models
classification
🌌 astro-ph
keywords
galaxyclusteringevolutionmodelspredictionspropertiesbeamconstrained
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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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