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agnpy: Modelling Active Galactic Nuclei radiative processes with python.

integration_instructionsResearch softwarekeyboard_double_arrow_right Software 29 Jun 2021Publisher:Zenodo
Authors: Cosimo Nigro; Julian Sitarek; Paweł Gliwny; David Sanchez; Matthew Craig;
Code repository: https://github.com/cosimoNigro/agnpy/tree/v0.1.0

doi: 10.5281/zenodo.5040242 , 10.5281/zenodo.5748085 , 10.5281/zenodo.5153369 , 10.5281/zenodo.5705600

agnpy: Modelling Active Galactic Nuclei radiative processes with python.

Abstract

agnpy is a python package focusing on the computation of the radiative processes of relativistic particles accelerated in the jets of Active Galactic Nuclei (AGN). It includes classes describing the galaxy components responsibles for line and thermal emission and calculates the absorption due to gamma-gamma pair production on soft (IR-UV) photon fields.

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Keywords

jets, python, numpy, blazars, radiative processes, AGN, astropy, MWL, radio galaxies

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selected citations
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This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
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