Metadata-Version: 2.1
Name: jetset
Version: 1.3.0
Summary: A framework for self-consistent modeling and fitting of  astrophysical relativistic jets SEDs
Home-page: https://github.com/andreatramacere/jetset
Author: Andrea Tramacere
Author-email: andrea.tramacere@gmail.com
Requires-Python: >=3.8
Description-Content-Type: text/markdown
License-File: LICENSE.txt
Requires-Dist: setuptools
Requires-Dist: scipy<=1.13.1,>=1.5.0
Requires-Dist: numpy<2.0,>=1.22
Requires-Dist: astropy<=6,>=5.0.1
Requires-Dist: matplotlib>=3.1.0
Requires-Dist: future
Requires-Dist: iminuit<=2.17.0,>=2.0.0
Requires-Dist: corner
Requires-Dist: six
Requires-Dist: emcee<=3.1.6,>=3.0.0
Requires-Dist: pyyaml
Requires-Dist: pytest
Requires-Dist: numba<=0.59.1,>0.55
Requires-Dist: tqdm<5
Requires-Dist: jupyter
Requires-Dist: ipython
Requires-Dist: dill


JetSeT is an open source C/Python framework to reproduce radiative and accelerative processes acting in relativistic jets, and galactic objects (beamed and unbeamed), 
allowing to fit the numerical models to observed data. The main features of this framework are:

 * handling observed data: re-binning, definition of data sets, bindings to astropy tables and quantities
   definition of complex numerical radiative scenarios: Synchrotron Self-Compton (SSC), external Compton (EC) and EC 
   against the CMB 
 
 * Constraining of the model in the pre-fitting stage, based on accurate  and already published phenomenological trends. 
   In particular, starting from phenomenological parameters, such as spectral indices, peak fluxes and frequencies, and 
   spectral  curvatures, that the code evaluates automatically, the pre-fitting algorithm is able to provide a good 
   starting model,following the phenomenological trends that I have implemented. fitting of multiwavelength SEDs using  
   both frequentist approach (iminuit) and bayesian MCMC sampling (emcee)
 
 * Self-consistent temporal evolution of the plasma under the effect of radiative and accelerative processes, both first  
   order and second order (stochastic acceleration) processes.



## Acknowledgements

If you use this code in any kind of scientific publication please cite the following papers:

* `Tramacere A. 2020`  https://ui.adsabs.harvard.edu/abs/2020ascl.soft09001T/abstract
* `Tramacere A. et al. 2011` http://adsabs.harvard.edu/abs/2011ApJ...739...66T
* `Tramacere A. et al. 2009` http://adsabs.harvard.edu/abs/2009A%26A...501..879T
* `Massaro E. et. al 2006`   http://adsabs.harvard.edu/abs/2006A%26A...448..861M

## Licence

JetSeT is released under a 3-clause BSD  license,  for deatils see
[License](https://github.com/andreatramacere/jetset/blob/master/LICENSE.txt) file 


# Documentation
visit: https://jetset.readthedocs.io/en/latest/

visit: https://github.com/andreatramacere/jetset
