activity
20052023
most citedEstimating Black Hole Masses in Active Galactic Nuclei Using the MgII 2800 Emission Line

223 citations · 4k across the 98 of their papers we have counts for

collaborators

98 papers

astro-ph.GA2023

Halo mass-observable proxy scaling relations and their dependencies on galaxy and group properties

Ziwen Zhang, Huiyuan Wang, Wentao Luo +5

Based on the DECaLS shear catalog, we study the scaling relations between halo mass() and various proxies for SDSS central galaxies, including stellar mass(), stell…

astro-ph.GA2023

Dynamical hotness, star formation quenching and growth of supermassive black holes

Hui Hong, Huiyuan Wang, H. J. Mo +8

A stellar system is dynamically hot when its kinetic energy is dominated by random motion represented by the velocity dispersion . We use MaNGA data to obtain in…

astro-ph.GA2023★ 3 cited

Ensemble Mapping the Inner Structure of Luminous Quasars

Liang Wu, Jun-Xian Wang, Hao-Chen Wang +4

A simple prediction of the well-known unification model of active galactic nuclei is that a sample of sources should exhibit an anti-correlation between the solid angle of the dust…

astro-ph.GA2023★ 2 cited

A Conditional Abundance Matching Method of Extending Simulated Halo Merger Trees to Resolve Low-Mass Progenitors and Sub-halos

Yangyao Chen, H. J. Mo, Cheng Li +3

We present an algorithm to extend subhalo merger trees in a low-resolution dark-matter-only simulation by conditionally matching them to those in a high-resolution simulation. The…

astro-ph.GA2022★ 1 cited

Shock-induced stripping of satellite ISM/CGM in IllustrisTNG clusters at

Hao Li, Huiyuan Wang, H. J. Mo +3

Using the IllustrisTNG simulation, we study the interaction of large-scale shocks with the circumgalactic medium (CGM) and interstellar medium (ISM) of star-forming (SF) satellite…

astro-ph.GA2022★ 5 cited

Anisotropy and characteristic scales in halo density gradient profiles

X. Wang, H. Wang, H. J. Mo

We use a large N-body simulation to study the characteristic scales in the density gradient profiles in and around halos with masses ranging from to $10^{15} h^{-1}{\rm M…