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Examples
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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
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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
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