Examples

Running Individual Simulations for Reionization and Re-Heating

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

Advanced Source Populations

• More Realistic Galaxy Populations
• Including Models for Population III Stars
• Self-Consistent Dust Reddening

Parameter Studies and Inference

• Simple Parameter Study: 2-D Model Grid
• Analyzing Model Grids / Monte Carlo Simulations
• Monte-Carlo Sampling Higher Dimensional Spaces
• Halo Abundance Matching
• Fitting the Global 21-cm Signal
• Fitting Galaxy Luminosity Functions
• Analyzing MCMC Calculations
• Inline Analysis

The Meta-Galactic Radiation Background

• 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)
• Including Helium in 1-D Radiative Transfer Calculations

Extensions

• Working with Data and Models From the Literature
  • The high-z galaxy luminosity function
  • Stellar population models
  • Parametric SEDs for galaxies and quasars
  • Reproducing Models from ARES Papers
• Embedding ARES in your own code
• The ParameterizedQuantity Framework
  • Multi-Variable ParameterizedQuantity
  • Multiple ParameterizedQuantity objects at once
  • Allowed Parameters
• Creating New Source Populations
  • Step One: A Simple Source Population
  • Step Two: Integrating with ARES
  • Step Three: Testing the new population