Published October 5, 2023
| Version 1.0
Dataset
Open
Simulated galaxy cluster data at z=0 demonstrating the entropy core problem with the SWIFT-EAGLE galaxy formation model
Creators
- 1. Jodrell Bank Centre for Astrophysics, Department of Physics and Astronomy, The University of Manchester, Oxford Road, Manchester M13 9PL, UK
Description
Cluster simulated with the SWIFT hydrodynamic code with the Ref SWIFT-EAGLE model. This dataset contains the redshift 0 snapshot and the VELOCIraptor halo catalogue.
Paper reference: https://arxiv.org/abs/2210.09978
Notes
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(10.7 GB)
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Additional details
Funding
- UK Research and Innovation
- DiRAC: Memory Intensive 2.5y ST/S002502/1
- UK Research and Innovation
- STFC Manchester Physics 2019 DTP ST/T506291/1
- UK Research and Innovation
- DiRAC: Memory Intensive 2.5x ST/R002371/1
- UK Research and Innovation
- DiRAC-2.5 DC - Operations 2017-2020 ST/R000832/1
- UK Research and Innovation
- Durham DiRAC-2 petascale facility ST/K00042X/1
- UK Research and Innovation
- DiRAC-2.5 - the pathway to DiRAC Phase 3 ST/P002293/1
References
- Altamura et al. (2023); EAGLE-like simulation models do not solve the entropy core problem in groups and clusters of galaxies, Monthly Notices of the Royal Astronomical Society, Volume 520, Issue 2, April 2023, Pages 3164–3186, https://doi.org/10.1093/mnras/stad342