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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
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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
Including Population III Stars
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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