activity
20062026
most citedOn Halo Formation Times and Assembly Bias

170 citations · 741 across the 25 of their papers we have counts for

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Showing 2025Show all

6 papers · 1 filter

astro-ph.GA2025

Interpreting the strong clustering of ultra-diffuse galaxies by halo spin bias

Qinglin Ma, Cheng Li, Yangyao Chen +1

We use the IllustrisTNG300-ODM simulation to investigate the spin bias of low-mass halos and its connection to the strong clustering of ultra-diffuse galaxies (UDGs) reported by Zh…

astro-ph.GA2025

Radio AGN feedback sustains quiescence only in a minority of massive galaxies

Huiling Liu, Yan Lu, Hui Hong +11

Radio active galactic nuclei (AGNs) eject a huge amount of energy into the surrounding medium and are thought to potentially prevent gas cooling and maintain the quiescence of mass…

astro-ph.GA2025★ 1 cited

Two-phase formation of galaxies: the coevolution between galaxies and dark matter halos

Qinglin Ma, Yangyao Chen, Houjun Mo

We use FIRE-2 cosmological zoom-in hydrodynamic simulations to investigate the co-evolution between Milky Way-size galaxies and their host dark matter halos. We find that the forma…

astro-ph.GA2025★ 1 cited

A two-phase model of galaxy formation: IV. Seeding and growing supermassive black holes in dark matter halos

Yangyao Chen, Houjun Mo, Huiyuan Wang

We present a theoretical framework for seeding and growing supermassive black holes (SMBHs) in dark matter halos along their assembly histories. Seeds are bred out of Pop-III stars…

astro-ph.GA2025

The Bigfoot: A footprint of a Coma cluster progenitor at z=3.98

Hanwen Sun, Tao Wang, Emanuele Daddi +13

Protoclusters, galaxy clusters' high redshift progenitors, hold the keys to understanding the formation and evolution of clusters and their member galaxies. However, their cosmolog…

astro-ph.CO2025★ 5 cited

Unexpected clustering pattern in dwarf galaxies challenges formation models

Ziwen Zhang, Yangyao Chen, Yu Rong +4

The galaxy correlation function serves as a fundamental tool for studying cosmology, galaxy formation, and the nature of dark matter. It is well established that more massive, redd…