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.

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. - In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. - ISSN 0035-8711. - 514:1(2022), pp. 977-996. [10.1093/mnras/stac1402]

The Three Hundred project: The gizmo-simba run

Ferragamo Antonio;
2022

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.
2022
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. - In: MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY. - ISSN 0035-8711. - 514:1(2022), pp. 977-996. [10.1093/mnras/stac1402]
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11588/989240
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