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  • Getting started
  • User guide
  • Tutorials
  • API reference
  • Developer guide
  • Release notes
  • Github
  • Slack

Section Navigation

  • Fundamental Concepts: Gammapy analysis workflow and package structure
    • Data access and selection (DL3)
    • Instrument Response Functions (DL3)
      • Effective area
      • Background
      • Energy Dispersion
      • Point Spread Function
    • Data reduction (DL3 to DL4)
      • FoV background
      • Reflected regions background
      • Ring background
    • Sky maps (DL4)
      • HEALPix-based maps
      • RegionGeom and RegionNDMap
    • Datasets (DL4)
    • Modeling and Fitting (DL4 to DL5)
    • Estimators (DL4 to DL5, and DL6)
    • High Level Analysis Interface
    • Command line tools
    • Source catalogs
    • Astrophysics
      • Astrophysical source models
        • Supernova Remnant Models
        • Pulsar Wind Nebula Source Models
        • Pulsar Source Models
      • Astrophysical source population models
      • Dark matter
    • Statistics in Gammapy
      • Fit statistics
      • Derivation of the WStat formula
    • Visualization
    • Utility functions
  • How To
  • Model gallery
    • Spatial models
      • Gaussian spatial model
      • Generalized gaussian spatial model
      • Shell spatial model
      • Constant spatial model
      • Template spatial model
      • Shell2 spatial model
      • Disk spatial model
      • Point spatial model
      • Piecewise norm spatial model
    • Spectral models
      • Constant spectral model
      • Super exponential cutoff power law model used for 3FGL
      • Naima spectral model
      • Super Exponential Cutoff Power Law Model used for 4FGL-DR3
      • EBL absorption spectral model
      • Compound spectral model
      • Super Exponential Cutoff Power Law Model used for 4FGL-DR1 (and DR2)
      • Power law 2 spectral model
      • Exponential cutoff power law spectral model
      • Log parabola spectral model
      • Exponential cutoff power law spectral model used for 3FGL
      • Piecewise norm spectral model
      • Exponential cutoff power law norm spectral model
      • Log parabola spectral norm model
      • Smooth broken power law spectral model
      • Power law norm spectral model
      • Power law spectral model
      • Broken power law spectral model
      • Template spectral model
      • Gaussian spectral model
    • Temporal models
      • Gaussian temporal model
      • PowerLaw temporal model
      • Generalized Gaussian temporal model
      • Light curve temporal model
      • Phase curve temporal model
      • Linear temporal model
      • Constant temporal model
      • Sine temporal model
      • ExpDecay temporal model
  • Gammapy recipes
  • Glossary and references
  • User guide
  • Fundamental Concepts: Gammapy analysis workflow and package structure
  • Astrophysics
  • Astrophysical source models

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.

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
  • Using gammapy.astro.source

This Page

  • Show Source

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