Weiguang Cui
The Three Hundred project: The gizmo-simba run
Cui, Weiguang; Dave, Romeel; Knebe, Alexander; Rasia, Elena; Gray, Meghan; Pearce, Frazer; Power, Chris; Yepes, Gustavo; Anbajagane, Dhayaa; Ceverino, Daniel; Contreras-Santos, Ana; de Andres, Daniel; De Petris, Marco; Ettori, Stefano; Haggar, Roan; Li, Qingyang; Wang, Yang; Yang, Xiaohu; Borgani, Stefano; Dolag, Klaus; Zu, Ying; Kuchner, Ulrike; Cañas, Rodrigo; Ferragamo, Antonio; Gianfagna, Giulia
Authors
Romeel Dave
Alexander Knebe
Elena Rasia
Professor MEGHAN GRAY MEGHAN.GRAY@NOTTINGHAM.AC.UK
PROFESSOR OF ASTRONOMY
Professor FRAZER PEARCE FRAZER.PEARCE@NOTTINGHAM.AC.UK
PROFESSOR OF PHYSICS
Chris Power
Gustavo Yepes
Dhayaa Anbajagane
Daniel Ceverino
Ana Contreras-Santos
Daniel de Andres
Marco De Petris
Stefano Ettori
Roan Haggar
Qingyang Li
Yang Wang
Xiaohu Yang
Stefano Borgani
Klaus Dolag
Ying Zu
Dr Ulrike Kuchner ULRIKE.KUCHNER@NOTTINGHAM.AC.UK
SENIOR RESEARCH FELLOW
Rodrigo Cañas
Antonio Ferragamo
Giulia Gianfagna
Abstract
We introduce gizmo-simba, a new suite of galaxy cluster simulations within The Three Hundred project. The Three Hundred consists of zoom re-simulations of 324 clusters with M 200≳ 1014.8, M ⊙ drawn from the MultiDark-Planck N-body simulation, run using several hydrodynamic and semi-analytical codes. The gizmo-simba suite adds a state-of-the-art galaxy formation model based on the highly successful Simba simulation, mildly re-calibrated to match z = 0 cluster stellar properties. Comparing to The Three Hundred zooms run with gadget-x, we find intrinsic differences in the evolution of the stellar and gas mass fractions, BCG ages, and galaxy colour-magnitude diagrams, with gizmo-simba generally providing a good match to available data at z ≈ 0. gizmo-simba's unique black hole growth and feedback model yields agreement with the observed BH scaling relations at the intermediate-mass range and predicts a slightly different slope at high masses where few observations currently lie. Gizmo-Simba provides a new and novel platform to elucidate the co-evolution of galaxies, gas, and black holes within the densest cosmic environments.
Citation
Cui, W., Dave, R., Knebe, A., Rasia, E., Gray, M., Pearce, F., Power, C., Yepes, G., Anbajagane, D., Ceverino, D., Contreras-Santos, A., de Andres, D., De Petris, M., Ettori, S., Haggar, R., Li, Q., Wang, Y., Yang, X., Borgani, S., Dolag, K., …Gianfagna, G. (2022). The Three Hundred project: The gizmo-simba run. Monthly Notices of the Royal Astronomical Society, 514(1), 977-996. https://doi.org/10.1093/mnras/stac1402
Journal Article Type | Article |
---|---|
Acceptance Date | May 16, 2022 |
Online Publication Date | May 14, 2022 |
Publication Date | Jul 1, 2022 |
Deposit Date | Dec 22, 2022 |
Publicly Available Date | Dec 22, 2022 |
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 | 514 |
Issue | 1 |
Pages | 977-996 |
DOI | https://doi.org/10.1093/mnras/stac1402 |
Keywords | Space and Planetary Science; Astronomy and Astrophysics |
Public URL | https://nottingham-repository.worktribe.com/output/15168017 |
Publisher URL | https://academic.oup.com/mnras/article/514/1/977/6590057 |
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Publisher Licence URL
https://creativecommons.org/licenses/by/4.0/
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