activity
20172021
most citedA forecast for the detection of the power asymmetry from galaxy surveys

7 citations · 9 across the 3 of their papers we have counts for

collaborators

14 papers

astro-ph.GA2021

Simulating properties of emission line galaxies from Nancy Grace Roman Space Telescope

Zhongxu Zhai, Yun Wang, Andrew Benson +4

We simulate the emission line galaxy properties for the Nancy Grace Roman Space Telescope by creating a 4 deg galaxy mock catalog using Galacticus, a semi-analytic model (SAM…

astro-ph.CO2021

Linear bias and halo occupation distribution of emission line galaxies from Nancy Grace Roman Space Telescope

Zhongxu Zhai, Yun Wang, Andrew Benson +2

We present measurements of the linear galaxy bias of H and [OIII] emission line galaxies (ELGs) for the High Latitude Spectroscopic Survey (HLSS) of Nancy Grace Roman Space Tele…

astro-ph.CO2020

Clustering in the Simulated H Galaxy Redshift Survey from Nancy Grace Roman Space Telescope

Zhongxu Zhai, Chia-Hsun Chuang, Yun Wang +2

We present a realistic 2000 deg H galaxy mock catalog with for the Nancy Grace Roman Space Telescope galaxy redshift survey, the High Latitude Spectroscopic Survey…

astro-ph.CO2020

Forecasting Cosmological Constraints from the Weak Lensing Magnification of Type Ia Supernovae Measured by the Nancy Grace Roman Space Telescope

Zhongxu Zhai, Yun Wang, Dan Scolnic

The weak lensing magnification of Type Ia Supernovae (SNe Ia) is sensitive to the clustering of matter, and provides an independent cosmological probe complementary to SN Ia distan…

astro-ph.CO2019

CMB distance priors revisited: effects of dark energy dynamics, spatial curvature, primordial power spectrum, and neutrino parameters

Zhongxu Zhai, Chan-Gyung Park, Yun Wang +1

As a physical and sufficient compression of the full CMB data, the CMB distance priors, or shift parameters, have been widely used and provide a convenient way to include CMB data…

astro-ph.CO2019

The Aemulus Project IV: Emulating Halo Bias

Thomas McClintock, Eduardo Rozo, Arka Banerjee +6

Models of the spatial distribution of dark matter halos must achieve new levels of precision and accuracy in order to satisfy the requirements of upcoming experiments. In this work…