Modeling high-redshift galaxies: what can we learn from high and ultra-high resolution hydrodynamical simulations?
We present results from a high resolution cosmological galaxy formation simulation called Mare Nostrum and a ultra-high resimulation of the first 500 million years of a single, Milky Way (MW) sized galaxy. Using the cosmological run, we measure UV luminosity functions and assess their sensitivity to...
| Main Authors: | , , , , |
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| Format: | Conference item |
| Published: |
2010
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