activity
20182026
most citedA massive core for a cluster of galaxies at a redshift of 4.3

220 citations · 558 across the 29 of their papers we have counts for

collaborators
Showing 2024Show all

12 papers · 1 filter

astro-ph.GA2024

How the Cookie Crumbles: A Model for Star-forming Clumps in High-redshift Disk Galaxies

Matthew E. Orr, Douglas Rennehan

We present a simple model for the number distribution of maximally star-forming clumps in rotating disk galaxies, at high- with high gas surface densities. By combining assumpti…

astro-ph.GA2024★ 7 cited

Diverse dark matter profiles in FIRE dwarfs: black holes, cosmic rays and the cusp-core enigma

Sophie Koudmani, Douglas Rennehan, Rachel S. Somerville +5

Dwarf galaxies have historically posed challenges to the cold dark matter (CDM) model and, while many of the so-called 'dwarf galaxy problems' have been mitigated by incorporating…

astro-ph.GA2024★ 9 cited

COSMOS Brightest Group Galaxies -- III: Evolution of stellar ages

G. Gozaliasl, A. Finoguenov, A. Babul +15

The unique characteristics of the brightest group galaxies (BGGs) link the evolutionary continuum between galaxies like the Milky Way and more massive BCGs in dense clusters. This…

astro-ph.GA2024

Modelling the multi-wavelength detection of protoclusters. I: An excess of submillimetre galaxies in protocluster cores

Pablo Araya-Araya, Rachel K. Cochrane, Christopher C. Hayward +6

Studies of galaxy protoclusters yield insights into galaxy cluster formation complementary to those obtained via `archaeological' studies of present-day galaxy clusters. Submillime…

astro-ph.GA2024★ 2 cited

Pumping Iron: How turbulent metal diffusion impacts multiphase galactic outflows

Ulrich P. Steinwandel, Douglas Rennehan, Matthew E. Orr +2

Most numerical simulations of galaxy formation and evolution are unable to properly resolve the turbulent cascade at or below the resolution scale and turbulence models are require…

astro-ph.GA2024★ 3 cited

A massive, neutral gas reservoir permeating a galaxy proto-cluster after the reionization era

Kasper E. Heintz, Jake S. Bennett, Pascal A. Oesch +21

Galaxy clusters are the most massive, gravitationally-bound structures in the Universe, emerging through hierarchical structure formation of large-scale dark matter and baryon over…

astro-ph.GA2024★ 8 cited

Hyenas: X-ray Bubbles and Cavities in the Intra-Group Medium

Fred J. Jennings, Arif Babul, Romeel Dave +2

We investigate the role of the Simba feedback model on the structure of the Intra-Group Medium (IGrM) in the new Hyenas suite of cutting-edge cosmological zoom-in simulations. Usin…

astro-ph.GA2024

A 100 Mpc structure traced by hyperluminous galaxies around a massive = 2.85 protocluster

George C. P. Wang, Scott C. Chapman, Nikolaus Sulzenauer +9

We present wide-field mapping at 850 m and 450 m of the = 2.85 protocluster in the HS154919 field using the Submillimetre Common User Bolometer Array 2 (SCUBA-2). Spec…

astro-ph.GA2024

\texttt{Simba}-\texttt{C}: the evolution of the thermal and chemical properties in the intragroup medium

Renier T. Hough, Zhiwei Shao, Weiguang Cui +5

The newly updated \texttt{GIZMO} and \texttt{Simba} based simulation, \texttt{Simba-C}, with its new stellar feedback, chemical enrichment, and recalibrated AGN feedback, allows fo…

astro-ph.GA2024★ 15 cited

The Manhattan Suite: Accelerated galaxy evolution in the early Universe

Douglas Rennehan

Observational advances have allowed the detection of galaxies, protoclusters, and galaxy clusters at higher and higher redshifts, opening a new view into extreme galaxy evolution.…

astro-ph.GA2024★ 5 cited

Identifying Galaxy Cluster Mergers with Deep Neural Networks using Idealized Compton-y and X-ray maps

Ashleigh R. Arendt, Yvette C. Perrott, Ana Contreras-Santos +3

We present a novel approach to identify galaxy clusters that are undergoing a merger using a deep learning approach. This paper uses massive galaxy clusters spanning $0 \leq z \leq…

astro-ph.GA2024★ 11 cited

The Nature and Evolution of Early Massive Quenched Galaxies in the Simba-C Simulation

Jakub Szpila, Romeel Davé, Douglas Rennehan +2

We examine the nature, origin, and fate of early () massive () quenched galaxies (EQGs) in a new run of the Simba-C galaxy…