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  • TSMapEstimator vs. ExcessMapEstimator
    • Flux
    • Flux Error
    • Flux UL
    • Flux Error Pos.
    • Flux Error Neg.
    • Sqrt(TS)
    • NPred Excess
    • NPred Ref.
    • NPred Err
    • NPred Error Pos.
    • NPred Error Neg.
    • NPred UL
  • Phase computation for pulsar using PINT
    • 0. Dependencies and imports
    • 1. Reading DataStore
    • 2. Phase-folding with PINT for one observation
    • 2.1 An ephemeris file from Fermi-LAT data.
    • 2.2 Computing pulsar phases
    • 3. Adding phases and metadata to an EventList and put it in a new Observation.
    • 4. Save new Event List and writing a modify HDU index table
    • 5. Opening the new DataStore
    • 6. Pulsar analysis tools with gammapy
  • MCMC sampling using the emcee package
    • Introduction
      • How does it work ?
      • Why should I use it ?
    • Simulate an observation
    • Estimate parameter correlations with MCMC
      • Define priors
    • Plot the results
    • Plot the model dispersion
    • Fun Zone
    • PeVatrons in CTA ?
  • Recipe to show the interactively edit the Sky model on the notebook
    • Load the changed parameters and verify that the model has been updated
  • Generating synthetic lightcurves and fitting the power spectral density of a lightcurve
    • Imports
    • Reference Lightcurve
    • Simulation
    • Gammapy setup and simulation
      • Fitting
  • Dark matter spatial and spectral models
    • Introduction
    • Setup
    • Profiles
    • J Factors
    • Gamma-ray spectra at production
    • Flux maps
  • Create a template background model
    • Context
    • Proposed approach
    • Setup
    • Select off data
    • Background model
    • Zenith dependence
    • Index tables
    • Exercises
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