ares
v0.7
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Installation
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
Embedding
ARES
in your own code
The
ParameterizedQuantity
Framework
Creating New Source Populations
Performance
Under the Hood
Troubleshooting
ARES
Development: Staying Up To Date
ARES
Development: Contributing!
Development History
Acknowledgements
ares
Docs
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Examples
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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
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