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

11 citations · 16 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.CO20241 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.CO20241 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.GA20241 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.HE20232 cited

Constraints on thermal conductivity in the merging cluster Abell 2146

A. Richard-Laferrière, H. R. Russell, A. C. Fabian +9

The cluster of galaxies Abell 2146 is undergoing a major merger and is an ideal cluster to study ICM physics, as it has a simple geometry with the merger axis in the plane of the s…

astro-ph.CO202311 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…