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

  • 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

Main snapshot data: snap_2640.hdf5 Main catalogue data: snap_2640.properties

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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