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1-D trend of quantities through a 100Mpc volume
1-dimensional trend of simulated fields for long beams through the simulated volume. Each dataset is a column formatted file containing: a) x-position [kpc] b) gas density... -
Tabulated volume filling factor of simulated extragalactic fields (23 models)
23 tabulated files for all magnetic field models (at z=0) investigated in Vazza et al. 2017 http://iopscience.iop.org/article/10.1088/1361-6382/aa8e60 See Table 1 and 2 for a... -
ENZO-AMR data for cluster E1
Hdf5 monolitic 256^3 files for a simulated galaxy cluster at z=0, using with ENZO-AMR. The uniform resolution is 34kpc everywhere. The data belongs to the simulations by Vazza... -
Mock radio skies from z=0 to z=0.5
Integrated radio emission from a 14x14 degree field, containing all projected cosmological volume up to z=0.5 (obtained by stacking several boxes along the line of sight). Each... -
1D profile of a cosmic volume from z=0 to z=1
1-dimensional profile of simulated fields for long beams through a simulated volume from z=0 to z=1. Each dataset is a column formatted file containing: a) x-position [kpc] b)... -
E5a, AMR8 at z=0.2, reconstructed down to the 6th AMR level (16kpc/cell)
Each HDF5 dataset contains triplets of fields: -6_8mdm001R_dt_012 contains "Density", "Dark_Matter_Density" and "Temperature" (a 640^3 grid for each); -6_8mdm001R_v_012... -
Tabulated volume filling factor of simulated extragalactic fields (23 models)
23 tabulated files for all magnetic field models (at z=0) investigated in Vazza et al. 2017 http://iopscience.iop.org/article/10.1088/1361-6382/aa8e60 See Table 1 and 2 for a... -
E18 cluster data at the 6th AMR level
3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015), employing 6 levels of... -
E5a, AMR8 at z=0.02, reconstructed down to the 6th AMR level (16kpc/cell)
Each HDF5 dataset contains triplets of fields: -6_8mdm001R_dt_015 contains "Density", "Dark_Matter_Density" and "Temperature" (a 640^3 grid for each); -6_8mdm001R_v_015... -
E14 high resolution dataset (innermost volume)
3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015). The data are mapped onto... -
E18 cluster data at the 4th and 5th AMR levels
3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015), employing 4 or 5 levels... -
E18B high resolution dataset (innermost volume)
3D dimensional dataset (256^3 cells) in HDF5 format, of a high-resolution MHD cosmological simulations obtained with the ENZO code (Bryan et al. 2015). The data are mapped onto... -
Statistics of star formation and magnetic seeding
Tabular data for the cosmic star formation history in cosmological simulations, and of the relative magnetisation output of stellar activity. For meaning of the models please... -
E5a, AMR8 at z=0.05, reconstructed down to the 6th AMR level (16kpc/cell)
Each HDF5 dataset contains triplets of fields: -6_8mdm001R_dt_014 contains "Density", "Dark_Matter_Density" and "Temperature" (a 640^3 grid for each); -6_8mdm001R_v_014... -
Simulated cosmic volume - Primordial magnetic seeding models.
These are 2 subsets (300^3 cells each) derived from larger 1024^3 cosmological MHD simulations produced using ENZO on Piz-Daint (CSCS) by F.Vazza& collaborators. In these... -
Simulated cosmic volume - dynamo amplification
This is one subset (300^3 cells) derived from a larger 1024^3 cosmological MHD simulation produced using ENZO on Piz-Daint (CSCS) by F.Vazza& collaborators. In these...
