activity
20182024
most citedThe impact of galaxy selection on the splashback boundaries of galaxy clusters

15 citations · 25 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA20242 cited

How DREAMS are made: Emulating Satellite Galaxy and Subhalo Populations with Diffusion Models and Point Clouds

Tri Nguyen, Francisco Villaescusa-Navarro, Siddharth Mishra-Sharma +16

The connection between galaxies and their host dark matter (DM) halos is critical to our understanding of cosmology, galaxy formation, and DM physics. To maximize the return of upc…

astro-ph.GA20242 cited

Introducing the DREAMS Project: DaRk mattEr and Astrophysics with Machine learning and Simulations

Jonah C. Rose, Paul Torrey, Francisco Villaescusa-Navarro +27

We introduce the DREAMS project, an innovative approach to understanding the astrophysical implications of alternative dark matter models and their effects on galaxy formation and…

astro-ph.GA202215 cited

The impact of galaxy selection on the splashback boundaries of galaxy clusters

Stephanie O'Neil, Josh Borrow, Mark Vogelsberger +1

We explore how the splashback radius () of galaxy clusters, measured using the number density of the subhalo population, changes based on various selection criteria usi…

astro-ph.GA2020

The splashback boundary of haloes in hydrodynamic simulations

Stephanie O'Neil, David J. Barnes, Mark Vogelsberger +1

The splashback radius, , is a physically motivated halo boundary that separates infalling and collapsed matter of haloes. We study in the hydrodynamic and…

astro-ph.GA20196 cited

Simulating dust grain-radiation coupling on a moving mesh

Ryan McKinnon, Rahul Kannan, Mark Vogelsberger +3

We present a model for the interaction between dust and radiation fields in the radiation hydrodynamic code AREPO-RT, which solves the moment-based radiative transfer equations on…

astro-ph.GA2018

Dust in and around galaxies: dust in cluster environments and its impact on gas cooling

Mark Vogelsberger, Ryan McKinnon, Stephanie O'Neil +3

Simulating the dust content of galaxies and their surrounding gas is challenging due to the wide range of physical processes affecting the dust evolution. Here we present cosmologi…