Modelling Active Galactic Nuclei radiative processes with python.
agnpy focuses on the numerical computation of the photon spectra produced by leptonic radiative processes in jetted Active Galactic Nuclei (AGN).
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As a general acknowledgement of agnpy usage, we recommend citing the agnpy release paper.
Additionaly, to specify which version of agnpy is being used, that version's zenodo record can be cited.
We recommend citing both.
At the following links you can find:
You are invited to check the documentation at https://agnpy.readthedocs.io/en/latest/.
To get familiar with the code you can run the notebooks in the tutorials section
of the documentation.
The only dependencies are:
numpy managing the numerical computation;
astropy managing physical units and astronomical distances.
matplotlib for visualisation and reproduction of the tutorials.
scipy for interpolation
The code is available in the python package index and can be installed via pip
pip install agnpy
The code can also be installed using conda
conda install -c conda-forge agnpy
A test suite is available in agnpy/tests, to run it just type
pytest in the main directory.
FAQs
Modelling jetted Active Galactic Nuclei radiative processes with python
We found that agnpy demonstrated a healthy version release cadence and project activity because the last version was released less than a year ago. It has 1 open source maintainer collaborating on the project.
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