Absorption¶
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class
gammapy.spectrum.models.
Absorption
(energy_lo, energy_hi, param_lo, param_hi, data)[source]¶ Bases:
object
Gamma-ray absorption models.
Parameters: Examples
Create and plot EBL absorption models for a redshift of 0.5:
import matplotlib.pyplot as plt import astropy.units as u from gammapy.spectrum.models import Absorption # Load tables for z=0.5 redshift = 0.5 dominguez = Absorption.read_builtin('dominguez').table_model(redshift) franceschini = Absorption.read_builtin('franceschini').table_model(redshift) finke = Absorption.read_builtin('finke').table_model(redshift) # start customised plot energy_range = [0.08, 3] * u.TeV ax = plt.gca() opts = dict(energy_range=energy_range, energy_unit='TeV', ax=ax, flux_unit='') franceschini.plot(label='Franceschini 2008', **opts) finke.plot(label='Finke 2010', **opts) dominguez.plot(label='Dominguez 2011', **opts) # tune plot ax.set_ylabel(r'Absorption coefficient [$\exp{(-\tau(E))}$]') ax.set_xlim(energy_range.value) # we get ride of units ax.set_ylim([1.e-4, 2.]) ax.set_yscale('log') ax.set_title('EBL models (z=' + str(redshift) + ')') plt.grid(which='both') plt.legend(loc='best') # legend # show plot plt.show()
()
Attributes Summary
data
energy_hi
energy_lo
param_hi
param_lo
Methods Summary
evaluate
(energy, parameter)Evaluate model for energy and parameter value. read
(filename)Build object from an XSPEC model. read_builtin
(name)Read one of the built-in absorption models. table_model
(parameter[, unit])Table model for a given parameter ( TableModel
).Attributes Documentation
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data
¶
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energy_hi
¶
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energy_lo
¶
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param_hi
¶
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param_lo
¶
Methods Documentation
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classmethod
read
(filename)[source]¶ Build object from an XSPEC model.
Todo: Format of XSPEC binary files should be referenced at https://gamma-astro-data-formats.readthedocs.io/en/latest/
Parameters: - filename : str
File containing the model.
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classmethod
read_builtin
(name)[source]¶ Read one of the built-in absorption models.
Parameters: - name : {‘franceschini’, ‘dominguez’, ‘finke’}
name of one of the available model in gammapy-data
References
[1] Franceschini et al., “Extragalactic optical-infrared background radiation, its time evolution and the cosmic photon-photon opacity”, Link [2] Dominguez et al., ” Extragalactic background light inferred from AEGIS galaxy-SED-type fractions” Link [3] Finke et al., “Modeling the Extragalactic Background Light from Stars and Dust” Link
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table_model
(parameter, unit='TeV')[source]¶ Table model for a given parameter (
TableModel
).Parameters: - parameter : float
Parameter value.
- unit : str, (optional)
desired value for energy axis
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