What’s new in version 1.2.2¶
bug fixing¶
hadronic pp: the grid for the equilibrium evolution was not starting from gmin=1, but from the lowest energy of the secondary
temporal evolution: in the light curves with crossing time, the (1+z) factor term was missing in the times column
Introduction of a class for galactic objects (beamed and unbeamed)¶
This class is useful for PWN, SNR, or jetted galactic objects It is still preliminary, and will be improved soon See this section of the user guide Galactic object models
quantile confidence range for MCMC plots¶
The MCMC plot method now accepts quantities for model confidence band eg:
mcmc.plot_model(sed_data=sed_data,fit_range=[1E11, 2E27],size=100,quantiles=[0.05,0.95])
What’s new in version 1.2.1¶
Introduction of depending pars¶
Model parameters can be linked via functional dependence. See this section of the user guide Depending parameters
Temporal Evolution¶
The python interface to perform self-consistent temporal evolution of leptonic emitters under acceleration and cooling has been added. See this section of the user guide temporal evolution
Hadronic pp emission¶
The python interface to perform self-consistent temporal evolution of leptonic emitters under acceleration and cooling has been added. See this section of the user guide Hadronic pp jet model
Theoretical background for SSC model¶
A detailed explanation of the theoretical background for SSC/EC model has been added. See this section of the user guide Phenomenological model constraining: SSC theory
Emitters distributions¶
The emitters distribution has be improved. See this section of the user guide Custom emitters distribution
EBL absorption¶
linking of parameters has been updated See this section of the user guide EBL
Plugins¶
JetSeT plugins to Sherpa (Example to use the Sherpa plugin with the sherpa interface, Example to use the Sherpa minimizer plugin with a JeSeT model)
Gammapy plugin (Example to use the Gamma-py plugin with the JeSeT interface)