activity
20032026
most citedSimulating the joint evolution of quasars, galaxies and their large-scale distribution

5.1k citations · 13.5k across the 77 of their papers we have counts for

collaborators

77 papers

astro-ph.CO2026

ELUCID-DESI II. Revealing dark matter mass, tidal, and velocity (MTV) fields using galaxy group phase information

Qingyang Li, Xiaohu Yang, Wensheng Hong +24

We introduce a novel method for reconstructing the cosmic mass, tidal, and velocity (MTV) fields over the redshift range using the phase information of galaxy groups.…

astro-ph.GA2023★ 8 cited

The mass accretion history of dark matter haloes down to Earth mass

Yizhou Liu, Liang Gao, Sownak Bose +6

We take advantage of the unprecedented dynamical range provided by the "Cosmic-Zoom" project to study the mass accretion history (MAH) of present-day dark matter haloes over the en…

astro-ph.GA2021★ 4 cited

The Formation and Evolution of Massive Galaxies

Yingjie Jing, Yu Rong, Jie Wang +2

The discovery of massive galaxies at high redshifts, especially the passive ones, poses a big challenge for the current standard galaxy formation models. Here we use the semi-analy…

astro-ph.GA2021★ 27 cited

The galaxy size to halo spin relation of disk galaxies in cosmological hydrodynamical simulations

Hang Yang, Liang Gao, Carlos S. Frenk +4

In the standard disk galaxy formation model, the sizes of galactic disks are tightly related to the spin parameters of their dark matter haloes. The model has been wildly adopt…

astro-ph.GA2021★ 9 cited

The role of mergers and gas accretion in black hole growth and galaxy evolution

TianChi Zhang, Qi Guo, Yan Qu +1

We use a semi-analytic galaxy formation model to study the co-evolution of supermassive black holes (SMBHs) with their host galaxies. Although the coalescence of SMBHs is not impor…

astro-ph.GA2021★ 7 cited

The impact of filaments on dwarf galaxy properties in the Auriga simulations

Haonan Zheng, Shihong Liao, Jia Hu +4

With a hydrodynamical simulation using a simple galaxy formation model without taking into account feedback, our previous work has shown that dense and massive filaments at high re…