PHYS369: Astrophysics Group Project
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Updated
Mar 20, 2020 - Python
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.
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.
Code to compute the HI 21cm and 3HeII 3.5cm field from density fields and source catalogues
PyCUDA based implementation of 21cmFAST
A code to identify the location and size of the gravitationally collapsed dark matter halos.
Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS
Python interface to C2Ray, with GPU-acceleration
The Meraxes semi-analytic galaxy formation model.
A semi-numerical code to generate the Epoch of Reionization (EoR) neutral Hydrogen (HI) field.
C2-Ray radiative transfer / photo-ionziation code, version with helium, combining 1D and 3D
A code to compute the non-linear evolution of the cosmological matter density contrast.
Code to compute ionization field from density fields and source catalogue (CIFOG)
Zeus21: Lightning-fast simulations of cosmic dawn
Accelerated Reionization Era Simulations
The 3D version of C2-Ray for multiple sources, hydrogen only
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