PyCUDA based implementation of 21cmFAST
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Updated
May 2, 2017 - Python
PyCUDA based implementation of 21cmFAST
Code to compute the HI 21cm and 3HeII 3.5cm field from density fields and source catalogues
C2-Ray radiative transfer / photo-ionziation code, version with helium, combining 1D and 3D
Simulating the Calibration of Arrays with Redundancy: a project to understand the impact of position errors on redundant calibration.
A project to investigate the impact of broken dipole antennas in the Murchison Widefield Array and its ability to detect the 21-cm Power Spectrum.
PHYS369: Astrophysics Group Project
A project in which we study the feasibility of correlation calibration (Sievers 2016) in the Murchison Widefield Array in attempt to bridge the gap between Redudant Calibration and Sky Model Based Calibration
Simplified framework for modeling the global 21-cm absorption signal, with a focus on studying the implications of non-standard 21-cm CMB temperature evolution.
A code to compute the non-linear evolution of the cosmological matter density contrast.
A code to identify the location and size of the gravitationally collapsed dark matter halos.
A semi-numerical code to generate the Epoch of Reionization (EoR) neutral Hydrogen (HI) field.
Code to compute ionization field from density fields and source catalogue (CIFOG)
The 3D version of C2-Ray for multiple sources, hydrogen only
Accelerated Reionization Era Simulations
Python interface to C2Ray, with GPU-acceleration
The Meraxes semi-analytic galaxy formation model.
Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS
Zeus21: Lightning-fast simulations of cosmic dawn
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