Observing Simulated Images of the High Redshift Universe: The Faint End Luminosity Function
abstract: Numerical simulations are very helpful in understanding the physics of the formation of structure and galaxies. However, it is sometimes difficult to interpret model data with respect to observations, partly due to the difficulties and background noise inherent to observation. The goal, he...
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| Format: | Doctoral Thesis |
| Language: | English |
| Published: |
2012
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| Online Access: | http://hdl.handle.net/2286/R.I.14913 |