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Examples
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
Table of Contents
Examples
Running Individual Simulations for Reionization and Re-Heating
Advanced Source Populations
Parameter Studies and Inference
The Meta-Galactic Radiation Background
1-D Radiative Transfer
Extensions
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Simple Physical Models for the Global 21-cm Signal
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Examples