1.3k citations · 6.2k across the 81 of their papers we have counts for
8 papers · 1 filter
QSO obscuration at high redshift (): Predictions from the BlueTides simulation
Yueying Ni, Tiziana Di Matteo, Roberto Gilli +3
High- AGNs hosted in gas rich galaxies are expected to grow through significantly obscured accretion phases. This may limit or bias their observability. In this work, we use \te…
Imaging Systematics and Clustering of DESI Main Targets
Ellie Kitanidis, Martin White, Yu Feng +10
We evaluate the impact of imaging systematics on the clustering of luminous red galaxies (LRG), emission-line galaxies (ELG) and quasars (QSO) targeted for the upcoming Dark Energy…
The Quijote simulations
Francisco Villaescusa-Navarro, ChangHoon Hahn, Elena Massara +26
The Quijote simulations are a set of 44,100 full N-body simulations spanning more than 7,000 cosmological models in the hyperplane.…
High mass and halo resolution from fast low resolution simulations
Biwei Dai, Yu Feng, Uros Seljak +1
Generating mocks for future sky surveys requires large volumes and high resolutions, which is computationally expensive even for fast simulations. In this work we try to develop nu…
Cosmic variance of galaxies: Prediction from BlueTides
Aklant K. Bhowmick, Rachel S. Somerville, Tiziana DiMatteo +3
In the coming decade, a new generation of telescopes, including JWST and WFIRST, will probe the period of the formation of first galaxies and quasars, and open up the last frontier…
The early growth of supermassive black holes in cosmological hydrodynamic simulations with constrained Gaussian realizations
Kuan-Wei Huang, Yueying Ni, Yu Feng +1
The paper examines the early growth of supermassive black holes (SMBHs) in cosmological hydrodynamic simulations with different BH seeding scenarios. Employing the constrained Gaus…
Predictions for the Abundance of High-redshift Galaxies in a Fuzzy Dark Matter Universe
Yueying Ni, Mei-Yu Wang, Yu Feng +1
During the last decades, rapid progress has been made in measurements of the rest-frame ultraviolet (UV) luminosity function (LF) for high-redshift galaxies (). The faint…
Nebular Line Emission During the Epoch of Reionization
Stephen M. Wilkins, Christopher C. Lovell, Ciaran Fairhurst +6
Nebular emission lines associated with galactic HII regions carry information about both physical properties of the ionised gas and the source of ionising photons as well as provid…