Clustering of high-redshift galaxies: relating LBGs to dark matter halos

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dc.creatorWechsler, Risa H.
dc.creatorBullock, James S.
dc.creatorSomerville, Rachel S.
dc.creatorKolatt, Tsafrir
dc.creatorPrimack, Joel R.
dc.creatorBlumenthal, George R.
dc.creatorDekel, Avishai
dc.date1999-10-20
dc.date.accessioned2026-07-07T02:33:57Z
dc.date.available2026-07-07T02:33:57Z
dc.descriptionWe investigate the clustering properties of high-redshift galaxies within three competing scenarios for assigning luminous galaxies to dark matter halos from N-body simulations: a one galaxy per massive halo model, a quiescent star formation model, and a collisional starburst model. We compare these models to observations of Lyman-Break galaxies at z~3$ With current data and the simple statistic used here, one cannot rule out any of these models, but we see potential for finding distinguishing features using statistics that are sensitive to the tails of the distribution, and statistics based on the number of multiple galaxies per halo, which we explore in an ongoing study.
dc.description5 pages, 2 figures, newpasp.sty, contribution to the Proceedings of Rencontres Internationales de l'IGRAP, Clustering at High Redshift, Marseille 1999
dc.identifierhttps://arxiv.org/abs/astro-ph/9910359
dc.identifierhttp://arxiv.org/abs/astro-ph/9910359
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15050
dc.subjectAstrophysics
dc.titleClustering of high-redshift galaxies: relating LBGs to dark matter halos
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