Data products from the study by Altamura et al. (2022)
The data are supplied in hdf5
format. They can be inspectes with h5dump
, HDFView
and can be read programmatically using the supplied file load_data.py
.
load_data.py
organises the data in categories through the following classes:
RefModelExtendedSample
PropertiesReducedSample
ProfilesReducedSample
For each class, the data structure is the same as in the hdf5
files and can be navigated using class attributes. The datasets already include the units from the unyt
module.
This is an example code to plot the profile for the group (VR2915
) at high resolution (+1res
in the hdf5
file or plus_1res
in the class instance attributes), run with the reference EAGLE-like model (Ref
).
from load_data import ProfilesReducedSample
profiles = ProfilesReducedSample()
entropy_profile = profiles.data.VR2915_plus_1res.Ref.entropy_profile
# The entropy profile is in dimensionless units, normalised to the self-similar scaling $K_{500}$
print(entropy_profile)
# The radial distance of the shells used to bin the particles is scaled by $r_{500}$
radial_bin_centres = profiles.data.VR2915_plus_1res.Ref.radial_bin_centres
from matplotlib import pyplot as plt
# To display the dimensionless profile, use matplotlib
plt.plot(radial_bin_centres, entropy_profile)
plt.xlabel(r"$r/r_{500}$")
plt.ylabel(r"$K/K_{500}$")
plt.show()
RefModelExtendedSample()
|
|-- resolution_minus_8res
| |-- entropy_profile
| |-- gas_fraction
| |-- m500
| |-- radial_bin_centres
| |-- star_fraction
| |-- VR_numbers
|
|-- resolution_plus_1res
|-- ...
PropertiesReducedSample()
|
|-- redshift_0
| |-- VR18_minus_1res
| | |-- AGNdT8
| | | |-- entropy_core
| | | |-- fbary {Baryon fraction == fgas + fstar}
| | | |-- fgas
| | | |-- fstar
| | | |-- m500
| | | |-- mbh {Mass of the SMBH}
| | | |-- mgas {Mass of the hot gas inside r500}
| | | |-- mstar_100kpc {Stellar mass of the BCG}
| | | |-- ssfr_100kpc {1Gyr-averaged specific star-formation rate in the BCG}
| | |
| | |-- AGNdT9 [same fields]
| | |-- Bipolar [...]
| | |-- Isotropic [...]
| | |-- Random [...]
| | |-- Ref [...]
| | |-- alpha0 [...]
| | |-- noAGN [...]
| | |-- noMetalCooling [...]
| | |-- noSN [...]
| |
| |-- VR18_plus_8res
| | |-- ...
| |
| |-- VR2915_plus_1res
| | |-- ...
| |
| |-- VR2915_minus_8res
| |-- ...
|
|
|-- redshift_1
|-- ...
ProfilesReducedSample()
|
|-- VR18_minus_1res
| |-- AGNdT8
| | |-- density_profile
| | |-- entropy_profile
| | |-- temperature_profile
| | |-- radial_bin_centers
| |
| |-- AGNdT9 [same fields]
| |-- Bipolar [...]
| |-- Isotropic [...]
| |-- Random [...]
| |-- Ref [...]
| |-- alpha0 [...]
| |-- noAGN [...]
| |-- noMetalCooling [...]
| |-- noSN [...]
|
|-- VR18_plus_8res
| |-- ...
|
|-- VR2915_plus_1res
| |-- ...
|
|-- VR2915_minus_8res
|-- ...
The raw data for the simulated cluster at
If you use these raw data files for your work, please consider citing the MNRAS paper, as well as the Zenodo dataset with this BibTeX handle:
@dataset{edoardo_altamura_2023_8410619,
author = {Edoardo Altamura},
title = {{Simulated galaxy cluster data at $z=0$ demonstrating
the entropy core problem with the SWIFT-EAGLE
galaxy formation model}},
month = oct,
year = 2023,
note = {{Main snapshot data: snap\_2640.hdf5 Main catalogue
data: snap\_2640.properties}},
publisher = {Zenodo},
version = {1.0},
doi = {10.5281/zenodo.8410619},
url = {https://doi.org/10.5281/zenodo.8410619}
}