Examples

Running Individual Simulations

• Reionization & Global 21-cm Signal

  • Simple Physical Models for the Global 21-cm Signal
  • Models with Multiple Source Populations
  • Phenomenological Models for the Global 21-cm Signal

• Uniform Radiation Backgrounds

  • The Metagalactic UV Background
  • The Metagalactic X-ray Background

• 1-D Radiative Transfer

  • RT06 Test #1 (Strömgren Sphere, isothermal)
  • RT06 Test #2 (Strömgren Sphere, thermal evolution allowed)

Parameter Studies and Inference

• Running Large Suites of Models

  • Simple Parameter Study: 2-D Model Grid
  • Monte-Carlo Sampling Higher Dimensional Spaces

• Fitting and Forecasting

  • Fitting the Global 21-cm Signal
  • Fitting Galaxy Luminosity Functions

• Analyzing Sets of Models

  • Inline Analysis
  • Analyzing Model Grids / Monte Carlo Simulations
  • Analyzing MCMC Calculations

Extensions

• Advanced physics

  • Including Helium in 1-D Radiative Transfer Calculations

• Advanced source populations

  • More Realistic Galaxy Populations
  • More General Star Formation Histories and Spectral Synthesis
  • Including Population III Stars
  • Fitting EDGES-like Signals

• Comparing to observational data

  • Working with Data and Models From the Literature

• Customization

  • Embedding ARES in your own code
  • The ParameterizedQuantity Framework
  • Creating New Source Populations