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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.COShow all

8 papers · 1 filter

astro-ph.CO2024★ 1 cited

Closing Pandora's Box -- The deepest X-ray observations of Abell 2744 and a multi-wavelength merger picture

Urmila Chadayammuri, Ákos Bogdán, Gerrit Schellenberger +1

Abell 2744, also known as Pandora's Cluster, is a complex merging galaxy cluster. While a major merger is clear along the north-south axis, the dynamical state of the northwest sub…

astro-ph.CO2024★ 1 cited

Improved Constraints on Mergers with SZ, Hydrodynamical simulations, Optical, and X-ray (ICM-SHOX). Paper II: Galaxy cluster sample overview

Emily M. Silich, Elena Bellomi, Jack Sayers +12

Galaxy cluster mergers are representative of a wide range of physics, making them an excellent probe of the properties of dark matter and the ionized plasma of the intracluster med…

astro-ph.CO2023★ 1 cited

ICM-SHOX. Paper I: Methodology overview and discovery of a gas--dark matter velocity decoupling in the MACS J0018.5+1626 merger

Emily M. Silich, Elena Bellomi, Jack Sayers +12

Galaxy cluster mergers are rich sources of information to test cluster astrophysics and cosmology. However, cluster mergers produce complex projected signals that are difficult to…

astro-ph.CO2023★ 11 cited

Painting baryons onto N-body simulations of galaxy clusters with image-to-image deep learning

Urmila Chadayammuri, Michelle Ntampaka, John ZuHone +2

Galaxy cluster mass functions are a function of cosmology, but mass is not a direct observable, and systematic errors abound in all its observable proxies. Mass-free inference can…

astro-ph.CO2022★ 24 cited

Weak-lensing mass bias in merging galaxy clusters

Wonki Lee, Sangjun Cha, M. James Jee +6

Although weak lensing (WL) is a powerful method to estimate a galaxy cluster mass without any dynamical assumptions, a model bias can arise when the cluster density profile departs…

astro-ph.CO2022★ 6 cited

The X-ray Angular Power Spectrum of Extended Sources in the eROSITA Final Equatorial Depth Survey

Erwin T. Lau, Akos Bogdan, Urmila Chadayammuri +3

The eROSITA Final Equatorial Depth Survey (eFEDS), with a sky area of 140 square degrees with depth equivalent to the equatorial patch of the final eROSITA all-sky survey, represen…

astro-ph.CO2019★ 3 cited

Probing Macro-Scale Gas Motions and Turbulence in Diffuse Cosmic Plasmas

Esra Bulbul, Massimo Gaspari, Gabriella Alvarez +31

Clusters of galaxies, the largest collapsed structures in the Universe, are located at the intersection of extended filaments of baryons and dark matter. Cosmological accretion ont…

astro-ph.CO2011★ 9 cited

The Scale Factor in the Universe with Dark Energy

M. V. Sazhin, O. S. Sazhina, U. Chadayammuri

Friedmans cosmological equations for the scale factor are analyzed for the Universe containing dark energy. The parameter of the equation of state of the dark energy is treated as…