1 code implementation • 17 Dec 2018 • T. Morishita, L. E. Abramson, T. Treu, G. B. Brammer, T. Jones, P. Kelly, M. Stiavelli, M. Trenti, B. Vulcani, X. Wang
In this paper, we study star formation histories (SFHs) of 24 massive galaxies at 1. 6<z<2. 5.
Astrophysics of Galaxies
1 code implementation • 6 Nov 2015 • Jae-hong Park, Han-Seek Kim, J. Stuart B. Wyithe, C. G. Lacey, C. M. Baugh, R. L. Barone-Nugent, M. Trenti, R. J. Bouwens
We find that for the detection limits of the XDF field central LBGs at $z\sim 4$ predominantly reside in haloes of mass $\sim 10^{11}-10^{12}h^{-1}M_{\rm \odot}$ and that satellites reside in larger haloes of mass $\sim 10^{12}-10^{13}h^{-1}M_{\rm \odot}$.
Astrophysics of Galaxies Cosmology and Nongalactic Astrophysics
