collaborators

7 papers

astro-ph.CO2026

Testing warm dark matter with kinematics of the smallest galaxies

M. Sten Delos, Niusha Ahvazi, Andrew Benson

Every dark matter halo forms with a density cusp at its center. For warm dark matter (WDM), these prompt cusps can be massive enough to influence the kinematic…

astro-ph.GA2026

Correlation between baryonic process and galaxy assembly bias

Zilan Xiao, Junyu Hua, Zhongxu Zhai +2

Galaxy assembly bias (GAB) is the dependence of galaxy clustering on secondary properties beyond halo mass. In this work, we study the connections between GAB and baryonic processe…

astro-ph.CO2026

The pre-infall bias of subhalos

M. Sten Delos, Andrew Benson

Dark matter halos destined to fall into a more massive host differ from typical field halos of the same mass even before infall. In cosmological simulations, we find that the proge…

astro-ph.GA2026

The Curious Case of Centaurus A II: On the Subject of the Quenched satellites

Sachi Weerasooriya, Mia Sauda Bovill, Matthew A. Taylor +6

The satellite system of Centaurus A presents a curious cosmological puzzle: while the global population is consistent with theoretical expectations, its inner regions (d<150 kpc) e…

astro-ph.GA2026

Stellar Mass Growth in the First Galaxies: Theory and Observation

Alan Dressler, Andrew Benson

We compare the growth in stellar mass of galaxies in the epoch with predictions of a semi-analytic galaxy formation model - Galacticus. In contrast to diverse and controve…

astro-ph.GA2025

The abundance and properties of the lowest luminosity dwarf galaxies around the Milky Way: Insights from Semi-Analytic Models

Niusha Ahvazi, Andrew B. Pace, Christopher T. Garling +11

We investigate the formation and observable properties of faint satellite galaxies (M$_\rm V > -3$) in Milky Way-like halos using the semi-analytic galaxy formation model Galacticu…