The THREE HUNDRED
collaboration
The Three Hundred Project aims to exploit a large sample of
simulated galaxy clusters and their environment modelled
using a range of simulation packages and physics modules. In
addition
to the standard post-processing analysis, mock observational
maps are available mimicking X-ray, optical, gravitational
lensing, radio, and SZ observations. This dataset will be
used to:
In this website we provide access to the halo catalogues for the 324 zoomed regions simulated with different physics hydro codes:
- Study the formation and evolution of galaxy clusters in relation to the underlying cosmological framework.
- Quantify the influence of baryonic physics via various sub-grid physics models, including both full physics cosmological simulations and semi-analytical galaxy formation models.
- Constrain the properties of the intra-cluster medium.
- Prepare derived data products mocking observations in various wave-bands (e.g. X-rays, optical, and also gravitational lensing signals, SZ maps, etc.).
- Study galaxy formation and evolution in a range of environments by supplementing our cluster dataset with field region simulations.
In this website we provide access to the halo catalogues for the 324 zoomed regions simulated with different physics hydro codes:
- GADGET-MUSIC (Classical SPH method + S&H 03
Sar formation + SN feedback model)
- GADGETX-AGN ( New SPH method + SN + Super Massive
Black hole feedback)
- GIZMO-SIMBA (GIZMO hydro SPH +
SN + AGN feedback modelling )
- DMONLY-LOWRES ( same mass resolution as for the hydro runs)
- DMONLY-HIGHRES ( 8 times better mass resolution )
- In MOVIES you can find animations of the dark matter distribution for all the zoomed regions (324 original + 68 new extensions) showing the redshift evolution and 3d rotation at z=0.
- IN MOVIES_FHD you can find movies for the extended sample of 68 new regions in Full HD (1920x1080)