If you came here trying to figure out how to create simulated X-ray photons and observations, you should go here instead.
This functionality provides the ability to create metallicity-dependent X-ray luminosity, emissivity, and photon emissivity fields for a given photon energy range. This works by interpolating from emission tables created from the photoionization code Cloudy or the collisional ionization database AtomDB. If you installed yt with the install script, these data files should be located in the data directory inside the installation directory, or can be downloaded from http://yt-project.org/data. Emission fields can be made for any interval between 0.1 keV and 100 keV.
Fields will be created for luminosity , emissivity , and photon emissivity . The only required arguments are the dataset object, and the minimum and maximum energies of the energy band.
import yt from yt.analysis_modules.spectral_integrator.api import \ add_xray_emissivity_field xray_fields = add_xray_emissivity_field(ds, 0.5, 7.0)
Additional keyword arguments are:
- filename (string): Path to data file containing emissivity values. If None, a file called “cloudy_emissivity.h5” is used, for photoionized plasmas. A second option, for collisionally ionized plasmas, is in the file “apec_emissivity.h5”, available at http://yt-project.org/data. These files contain emissivity tables for primordial elements and for metals at solar metallicity for the energy range 0.1 to 100 keV. Default: None.
- with_metals (bool): If True, use the metallicity field to add the contribution from metals. If False, only the emission from H/He is considered. Default: True.
- constant_metallicity (float): If specified, assume a constant metallicity for the emission from metals. The with_metals keyword must be set to False to use this. It should be given in unit of solar metallicity. Default: None.
The resulting fields can be used like all normal fields. The function will return the names of the created fields in a Python list.
import yt from yt.analysis_modules.spectral_integrator.api import \ add_xray_emissivity_field xray_fields = add_xray_emissivity_field(ds, 0.5, 7.0, filename="apec_emissivity.h5") ds = yt.load("enzo_tiny_cosmology/DD0046/DD0046") plot = yt.SlicePlot(ds, 'x', 'xray_luminosity_0.5_7.0_keV') plot.save() plot = yt.ProjectionPlot(ds, 'x', 'xray_emissivity_0.5_7.0_keV') plot.save() plot = yt.ProjectionPlot(ds, 'x', 'xray_photon_emissivity_0.5_7.0_keV') plot.save()
The X-ray fields depend on the number density of hydrogen atoms, in the yt field
H_number_density. If this field is not defined (either in the dataset or by the user),
the primordial hydrogen mass fraction (X = 0.76) will be used to construct it.