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...

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書目詳細資料
Main Authors: Wilkins, S, Di Matteo, T, Croft, R, Khandai, N, Feng, Y, Bunker, A, Coulton, W
格式: Journal article
語言:English
出版: 2013