458 citations · 5.6k across the 114 of their papers we have counts for
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ELUCID V. Lighting dark matter halos with galaxies
Xiaohu Yang, Youcai Zhang, Huiyuan Wang +16
In a recent study, using the distribution of galaxies in the north galactic pole of SDSS DR7 region enclosed in a 500$\mpch$ box, we carried out our ELUCID simulation (Wang et al.…
Constraints on the Evolution of the Galaxy Stellar Mass Function II: Quenching Timescale of Galaxies and its Implication for their Star Formation Rate
E. Contini, X. Kang, A. D. Romeo +2
We study the connection between the observed star formation rate-stellar mass (SFR-) relation and the evolution of the stellar mass function (SMF) by means of a subhalo abunda…
The build up of the correlation between halo spin and the large scale structure
Peng Wang, Xi Kang
Both simulations and observations have confirmed that the spin of haloes/galaxies is correlated with the large scale structure (LSS) with a mass dependence such that the spin of lo…
The large-scale environment from cosmological simulations I: The baryonic cosmic web
Weiguang Cui, Alexander Knebe, Gustavo Yepes +5
Using a series of cosmological simulations that includes one dark-matter-only (DM-only) run, one gas cooling-star formation-supernovae feedback (CSF) run and one that additionally…
ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias
Huiyuan Wang, H. J. Mo, Sihan Chen +17
We examine the quenched fraction of central and satellite galaxies as a function of galaxy stellar mass, halo mass, and the matter density of their large scale environment. Matter…
Halo intrinsic alignment: dependence on mass, formation time and environment
Qianli Xia, Xi Kang, Peng Wang +5
In this paper we use high-resolution cosmological simulations to study halo intrinsic alignment and its dependence on mass, formation time and large-scale environment. In agreement…