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

Section Navigation

  • Introduction
    • Data structures
    • High level interface
    • Low level API
  • Data exploration
    • H.E.S.S. with Gammapy
    • CTAO with Gammapy
    • MAGIC with Gammapy
    • Fermi-LAT with Gammapy
    • HAWC with Gammapy
    • VERITAS with Gammapy
  • Model Gallery
  • Detailed explanation
    • Using Gammapy IRFs
    • Observational clustering
    • Make a theta-square plot
    • Makers - Data reduction
    • Datasets - Reduced data, IRFs, models
    • Maps
    • Mask maps
    • Source catalogs
    • Models
    • Priors
    • Modelling
    • Fitting
    • Bayesian analysis with nested sampling
    • Estimators
    • Constraining parameter limits
  • Data analysis
    • Point source sensitivity
    • Spectral analysis
    • Spectral analysis with the HLI
    • Spectral analysis of extended sources
    • 1D spectrum simulation
    • Flux point fitting
  • 2D Image
    • Source detection and significance maps
    • Ring background map
    • 2D map fitting
  • 3D Cube
    • 3D detailed analysis
    • Basic image exploration and fitting
    • Multi instrument joint 3D and 1D analysis
    • 3D map simulation
    • Event sampling
    • Sample a source with energy-dependent temporal evolution
    • Flux Profile Estimation
    • Computing flux upper limits
  • Time series
    • Light curves
    • Light curves for flares
    • Estimation of time variability in a lightcurve
    • Time resolved spectroscopy estimator
    • Simulating and fitting a time varying source
  • Astrophysics use cases
    • Dark matter spatial and spectral models
    • Account for spectral absorption due to the EBL
    • Morphological energy dependence estimation
    • Pulsar analysis
    • Dark Matter Indirect Detection with Gammapy: Basics
  • Scripts
    • Survey Map Script
  • Tutorials
  • Astrophysics use cases

Astrophysics use cases#

This section outlines some source specific use cases.

Dark matter spatial and spectral models

Dark matter spatial and spectral models

Account for spectral absorption due to the EBL

Account for spectral absorption due to the EBL

Morphological energy dependence estimation

Morphological energy dependence estimation

Pulsar analysis

Pulsar analysis

Dark Matter Indirect Detection with Gammapy: Basics

Dark Matter Indirect Detection with Gammapy: Basics
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