activity
20102026
most citedThe Romulus Cosmological Simulations: A Physical Approach to the Formation, Dynamics and Accretion Models of SMBHs

335 citations · 3.5k across the 72 of their papers we have counts for

collaborators
Showing 2022Show all

6 papers · 1 filter

astro-ph.GA2022★ 33 cited

Can Cosmological Simulations Reproduce the Spectroscopically Confirmed Galaxies Seen at ?

B. W. Keller, F. Munshi, M. Trebitsch +1

Recent photometric detections of extreme redshift galaxies from the JWST have been shown to be in strong tension with existing simulation models for galaxy formation, and…

astro-ph.GA2022★ 5 cited

AGN quenching in simulated dwarf galaxies

Ray S. Sharma, Alyson M. Brooks, Michael Tremmel +2

We examine the quenching characteristics of isolated dwarf galaxies within the \Rom{} cosmological hydrodynamic simula…

astro-ph.GA2022★ 1 cited

A vast population of wandering and merging IMBHs at cosmic noon

Tiziana Di Matteo, Yueying Ni, Nianyi Chen +5

Massive black holes in the centers of galaxies today must have grown by several orders of magnitude from seed black holes formed at early times. Detecting a population of intermedi…

astro-ph.GA2022★ 39 cited

Properties and Evolution of Dual and Offset AGN in the ASTRID Simulation at

Nianyi Chen, Tiziana Di Matteo, Yueying Ni +7

We examine the dual (both BHs active) and offset (one BH active) AGN population (comprising 2000 pairs at ) at in the AS…

astro-ph.GA2022★ 23 cited

A hidden population of massive black holes in simulated dwarf galaxies

Ray S. Sharma, Alyson M. Brooks, Michael Tremmel +3

We explore the characteristics of actively accreting MBHs within dwarf galaxies in the \textsc{Romulus25} cosmological hydrodynamic simulation. We examine the MBH occupation fracti…

astro-ph.GA2022★ 32 cited

Massive central galaxies of galaxy groups in the Romulus simulations: an overview of galaxy properties at z=0

Seoyoung Lyla Jung, Douglas Rennehan, Vida Saeedzadeh +6

Contrary to many stereotypes about massive galaxies, observed brightest group galaxies (BGGs) are diverse in their star formation rates, kinematic properties, and morphologies. Stu…