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Number density profiles of galaxy groups and clusters in the SDSS

dc.contributor.advisorBerlind, Andreas
dc.contributor.authorNorris, Jackson M.
dc.date.accessioned2009-05-12T21:05:15Z
dc.date.available2009-05-12T21:05:15Z
dc.date.issued2008-04-20
dc.identifier.urihttp://hdl.handle.net/1803/2982
dc.descriptionHighest Honors in Astronomy
dc.description.abstractWe use projected number density profiles of galaxy groups to investigate the relationship between galaxy group structure and dark matter structure within halos. We primarily study a specific model of how galaxies populate dark matter halos by comparing the number density profiles of galaxy groups from the Sloan Digital Sky Survey with number density profiles of galaxy groups taken from dark matter halo simulations. We also investigate the dependence of galaxy locations within galaxy groups on luminosity and color.en
dc.language.isoen_USen
dc.publisherVanderbilt University. Dept. of Physics and Astronomyen
dc.subjectGalaxy groupsen
dc.subjectHalo occupation distributionen
dc.subjectHODen
dc.subjectColor segregationen
dc.subjectLuminosity segregationen
dc.subjectDensity profilesen
dc.subjectDark matter halosen
dc.subjectCosmological N-body simulationsen
dc.subject.lcshGalaxies -- Clustersen
dc.subject.lcshDark matter (Astronomy)en
dc.subject.lcshGalactic halosen
dc.subject.lcshCosmologyen
dc.subject.lcshAstronomyen
dc.subject.lcshSloan Digital Sky Surveyen
dc.subject.lcshMany-body problemen
dc.titleNumber density profiles of galaxy groups and clusters in the SDSSen
dc.typeThesisen
dc.description.collegeCollege of Arts and Scienceen
dc.description.departmentDept. of Physics and Astronomyen


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