Confronting predictions of the galaxy stellar mass function with observations at high redshift
We investigate the evolution of the galaxy stellar mass function at high redshift (z ≥ 5) using a pair of large cosmological hydrodynamical simulations: MassiveBlack and Massive Black-II. By combining these simulations, we can study the properties of galaxies with stellar masses greater than 108M⊙ h...
| Huvudupphovsmän: | , , , , , , |
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| Materialtyp: | Journal article |
| Språk: | English |
| Publicerad: |
2013
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