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...
Main Authors: | Wilkins, S, Di Matteo, T, Croft, R, Khandai, N, Feng, Y, Bunker, A, Coulton, W |
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Format: | Journal article |
Language: | English |
Published: |
2013
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