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agnpy

integration_instructionsResearch softwarekeyboard_double_arrow_right Software 17 Nov 2022 English Publisher:ZenodoFunded by:EC | ESCAPE
Authors: Nigro, Cosimo; Sitarek, Julian; Gliwny, Pawel; Sanchez, David; Craig, Matthew; Vuillaume, Thomas; Viale, Ilaria; +1 Authors

doi: 10.5281/zenodo.7633553 , 10.5281/zenodo.18500060 , 10.5281/zenodo.18505251 , 10.5281/zenodo.7331150 , 10.5281/zenodo.4055175

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 responsible 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

CTA, astroparticle physics, active galactic nuclei, blazars, jupyter-notebook, radio active galactic nuclei, radio jets, radiative processes

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Jupyter Notebook

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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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