Roan Haggar
Reconsidering the dynamical states of galaxy clusters using PCA and UMAP
Haggar, Roan; De Luca, Federico; De Petris, Marco; Sazonova, Elizaveta; Taylor, James E.; Knebe, Alexander; Gray, Meghan E.; Pearce, Frazer R; Contreras-Santos, Ana; Cui, Weiguang; Kuchner, Ulrike; Paun, Robert A. Mostoghiu; Power, Chris
Authors
Federico De Luca
Marco De Petris
Elizaveta Sazonova
James E. Taylor
Alexander Knebe
Professor MEGHAN GRAY MEGHAN.GRAY@NOTTINGHAM.AC.UK
PROFESSOR OF ASTRONOMY
Professor FRAZER PEARCE FRAZER.PEARCE@NOTTINGHAM.AC.UK
PROFESSOR OF PHYSICS
Ana Contreras-Santos
Weiguang Cui
Dr Ulrike Kuchner ULRIKE.KUCHNER@NOTTINGHAM.AC.UK
SENIOR RESEARCH FELLOW
Robert A. Mostoghiu Paun
Chris Power
Abstract
Numerous metrics exist to quantify the dynamical state of galaxy clusters, both observationally and within simulations. Many of these correlate strongly with one another, but it is not clear whether all of these measures probe the same intrinsic properties. In this work, we use two different statistical approaches – principal component analysis (PCA) and uniform manifold approximation and projection (UMAP) – to investigate which dynamical properties of a cluster are in fact the best descriptors of its dynamical state. We use measurements taken directly from The Three Hundred suite of galaxy cluster simulations, as well as morphological properties calculated using mock X-ray and SZ maps of the same simulated clusters. We find that four descriptions of dynamical state naturally arise, and although correlations exist between these, a given cluster can be “dynamically relaxed” according to all, none, or some of these four descriptions. These results demonstrate that it is highly important for future observational and theoretical studies to consider in which sense clusters are dynamically relaxed. Cluster dynamical states are complex and multi-dimensional, and so it is not meaningful to classify them simply as “relaxed” and “unrelaxed” based on a single linear scale.
Citation
Haggar, R., De Luca, F., De Petris, M., Sazonova, E., Taylor, J. E., Knebe, A., Gray, M. E., Pearce, F. R., Contreras-Santos, A., Cui, W., Kuchner, U., Paun, R. A. M., & Power, C. (2024). Reconsidering the dynamical states of galaxy clusters using PCA and UMAP. Monthly Notices of the Royal Astronomical Society, 532(1), 1031–1048. https://doi.org/10.1093/mnras/stae1566
Journal Article Type | Article |
---|---|
Acceptance Date | Jun 21, 2024 |
Online Publication Date | Jun 22, 2024 |
Publication Date | 2024-07 |
Deposit Date | Jun 30, 2024 |
Publicly Available Date | Jun 30, 2024 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Oxford University Press |
Peer Reviewed | Peer Reviewed |
Volume | 532 |
Issue | 1 |
Pages | 1031–1048 |
DOI | https://doi.org/10.1093/mnras/stae1566 |
Public URL | https://nottingham-repository.worktribe.com/output/36580070 |
Publisher URL | https://academic.oup.com/mnras/advance-article/doi/10.1093/mnras/stae1566/7697552 |
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Reconsidering the dynamical states of galaxy clusters
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Publisher Licence URL
https://creativecommons.org/licenses/by/4.0/
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