Galaxy Clustering as a Probe for Galaxy Evolution in Simulations

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dc.contributor.advisorMaartens, Roy
dc.contributor.authorThomas, Nicole
dc.date.accessioned2018-08-07T09:57:43Z
dc.date.accessioned2024-10-30T10:23:51Z
dc.date.available2018-08-31T22:10:06Z
dc.date.available2024-10-30T10:23:51Z
dc.date.issued2017
dc.descriptionMagister Scientiae - MSc (Physics)
dc.description.abstractStudying clustering on small scales (<10Mpc) over a large span of red- shifts allows us to connect galaxies to underlying cosmic large-scale structure, and thereby provide constraints on the physical processes that drive galaxy evolution. Relatedly, studying the relative bias of galaxies and their halo occupancy quanti es how the underlying dark matter distribution is traced by baryons in galaxies. Comparing model predictions to current and future multi-wavelength galaxy surveys, en- ables a greater understanding of how galaxy formation processes impact the relationship between galaxies and dark matter
dc.identifier.urihttps://hdl.handle.net/10566/16689
dc.language.isoen
dc.publisherUniversity of the Western Cape
dc.rights.holderUniversity of the Western Cape
dc.titleGalaxy Clustering as a Probe for Galaxy Evolution in Simulations

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