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20112024
most citedIntroducing RomulusC: A Cosmological Simulation of a Galaxy Cluster with Unprecedented Resolution

130 citations · 412 across the 24 of their papers we have counts for

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Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2024★ 2 cited

ERGO-ML: A continuous organization of the X-ray galaxy cluster population in TNG-Cluster with contrastive learning

Urmila Chadayammuri, Lukas Eisert, Annalisa Pillepich +3

The physical properties of the intracluster medium (ICM) reflect signatures of the underlying gravitational potential, mergers and strong interactions with other halos and satellit…

astro-ph.GA2024★ 1 cited

A candidate supermassive black hole in a gravitationally-lensed galaxy at

Orsolya E. Kovacs, Akos Bogdan, Priyamvada Natarajan +8

While supermassive black holes (BHs) are widely observed in the nearby and distant universe, their origin remains debated with two viable formation scenarios with light and heavy s…

astro-ph.GA2024

Decoding the Early Universe: Exploring a Merger Scenario for the High-Redshift Cluster JKCS041 using Numerical Models

Sharon Felix, Antareep Gogoi, Kaitlyn Shavelle +6

JKCS041 () is one of the most distant galaxy cluster systems known, seen when the Universe was less than 4 billion years old. Recent Sunyaev-Zeldovich (SZ) observations show…

astro-ph.GA2023★ 20 cited

Evidence for heavy seed origin of early supermassive black holes from a z~10 X-ray quasar

Akos Bogdan, Andy Goulding, Priyamvada Natarajan +9

Observations of quasars reveal that many supermassive black holes (BHs) were in place less than 700 million years after the Big Bang. However, the origin of the first BHs remains a…

astro-ph.GA2022★ 16 cited

Constraints from dwarf galaxies on black hole seeding and growth models with current and future surveys

Urmila Chadayammuri, Akos Bogdan, Angelo Ricarte +1

Dwarf galaxies are promising test beds for constraining models of supermassive and intermediate-mass black holes (MBH) via their black hole occupation fraction (BHOF). Disentanglin…

astro-ph.GA2022★ 3 cited

Testing galaxy feedback models with the first resolved profiles of the circumgalactic medium

Urmila Chadayammuri, Akos Bogdan, Benjamin Oppenheimer +3

The hot ( K) phase of the circumgalactic medium (CGM) contains a large fraction of baryons in galaxies. It also retains signatures of the processes that shaped the galaxies,…

astro-ph.GA2020★ 37 cited

Fountains and storms: The role of AGN and mergers in disrupting the cool-core in the RomulusC simulation

Urmila Chadayammuri, Michael Tremmel, Daisuke Nagai +2

The intracluster medium (ICM) is a multi-phase environment, dynamically regulated by Active Galactic Nuclei (AGN), the motions of galaxies through it, and mergers with other cluste…

astro-ph.GA2018★ 130 cited

Introducing RomulusC: A Cosmological Simulation of a Galaxy Cluster with Unprecedented Resolution

Michael Tremmel, Thomas R. Quinn, Angelo Ricarte +6

We present the first results from RomulusC, the highest resolution cosmological hydrodynamic simulation of a galaxy cluster run to date. RomulusC, a zoom-in simulation of a halo wi…

astro-ph.GA2017★ 101 cited

Mapping substructure in the HST Frontier Fields cluster lenses and in cosmological simulations

Priyamvada Natarajan, Urmila Chadayammuri, Mathilde Jauzac +14

We map the lensing-inferred substructure in the first three clusters observed by the Hubble Space Telescope Frontier Fields Initiative (HSTFF): Abell 2744 (z = 0.308), MACSJ0416, (…