Large-scale structure in the distant Universe and the build-up of the passive population
In this thesis I use the UKIDSS Ultra-Deep Survey to investigate the evolution in clustering of the galaxy population across the redshift range $0<z<3$. Selected in the K-band, the sample does not suffer as greatly from biases against passive and dusty objects that plague optically-selected sa...
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| Format: | Thesis (University of Nottingham only) |
| Language: | English |
| Published: |
2010
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| Online Access: | https://eprints.nottingham.ac.uk/11558/ |