The Evolution of Galaxy Clustering in Hierarchical Models

Simple item page
dc.creatorCole, Shaun
dc.creatorBenson, Andrew
dc.creatorBaugh, Carlton
dc.creatorLacey, Cedric
dc.creatorFrenk, Carlos
dc.date1999-10-13
dc.date.accessioned2026-07-07T02:33:49Z
dc.date.available2026-07-07T02:33:49Z
dc.descriptionThe 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.
dc.descriptionTo appear in the proceedings of the Marseille IGRAP99 conference "Clustering at High Redshift"
dc.identifierhttps://arxiv.org/abs/astro-ph/9910233
dc.identifierhttp://arxiv.org/abs/astro-ph/9910233
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/14999
dc.subjectAstrophysics
dc.titleThe Evolution of Galaxy Clustering in Hierarchical Models
dc.typetext

Files

Collections

arXiv