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  • Getting started
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Section Navigation

  • Gammapy analysis workflow and package structure
    • Data access and selection (DL3)
    • Instrument Response Functions (DL3)
    • Data reduction (DL3 to DL4)
    • Sky maps (DL4)
    • Datasets (DL4)
    • Modeling and Fitting (DL4 to DL5)
    • Estimators (DL4 to DL5, and DL6)
    • High Level Analysis Interface
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    • Astrophysics
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  • How To
  • Model gallery
    • Piecewise norm spatial model
    • Shell2 spatial model
    • Template spatial model
    • Constant spatial model
    • Shell spatial model
    • Gaussian spatial model
    • Disk spatial model
    • Point spatial model
    • Generalized gaussian spatial model
    • Constant spectral model
    • Exponential cutoff power law spectral model
    • Exponential cutoff power law norm spectral model
    • Compound spectral model
    • Super Exponential Cutoff Power Law Model used for 4FGL-DR3
    • Broken power law spectral model
    • Super exponential cutoff power law model used for 3FGL
    • Template spectral model
    • Power law 2 spectral model
    • Log parabola spectral norm model
    • EBL absorption spectral model
    • Piecewise norm spectral model
    • Log parabola spectral model
    • Naima spectral model
    • Power law norm spectral model
    • Super Exponential Cutoff Power Law Model used for 4FGL-DR1 (and DR2)
    • Power law spectral model
    • Exponential cutoff power law spectral model used for 3FGL
    • Gaussian spectral model
    • Smooth broken power law spectral model
    • Sine temporal model
    • Phase curve temporal model
    • PowerLaw temporal model
    • Gaussian temporal model
    • Generalized Gaussian temporal model
    • Constant temporal model
    • ExpDecay temporal model
    • Light curve temporal model
    • Linear temporal model
  • Gammapy recipes
  • Glossary and references
  • User guide
  • Astrophysics
  • Astrophysica...

Astrophysical source models#

Introduction#

The gammapy.astro.source module contains classes of source models, which can be used for population synthesis of galactic gamma-ray sources.

Getting started#

TODO: add basic example.

Using gammapy.astro.source#

The following source models are available:

  • Supernova Remnant Models
  • Pulsar Wind Nebula Source Models
  • Pulsar Source Models
On this page
  • Introduction
  • Getting started
  • Using gammapy.astro.source
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Last updated on 11 Oct 2024.

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