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Nov 27, 2024 - Jupyter Notebook
reionization
Here are 20 public repositories matching this topic...
The 3D version of C2-Ray for multiple sources, hydrogen only
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Nov 7, 2023 - Fortran
Accelerated Reionization Era Simulations
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Nov 5, 2024 - Python
Zeus21: Lightning-fast simulations of cosmic dawn
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Nov 6, 2024 - Python
Code to compute ionization field from density fields and source catalogue (CIFOG)
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Nov 22, 2022 - C
C2-Ray radiative transfer / photo-ionziation code, version with helium, combining 1D and 3D
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Nov 15, 2024 - Fortran
A code to compute the non-linear evolution of the cosmological matter density contrast.
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Jul 14, 2021 - C
A semi-numerical code to generate the Epoch of Reionization (EoR) neutral Hydrogen (HI) field.
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Jul 14, 2021 - C
Python interface to C2Ray, with GPU-acceleration
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Aug 1, 2024 - Python
The Meraxes semi-analytic galaxy formation model.
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Feb 25, 2024 - C
Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS
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Mar 14, 2024 - C
A code to identify the location and size of the gravitationally collapsed dark matter halos.
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Nov 22, 2024 - C
Code to compute the HI 21cm and 3HeII 3.5cm field from density fields and source catalogues
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Jun 28, 2017 - C
PyCUDA based implementation of 21cmFAST
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May 2, 2017 - Python
Simulating the Calibration of Arrays with Redundancy: a project to understand the impact of position errors on redundant calibration.
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Jul 10, 2019 - Python
Software release for 'Connecting Lyman-α and ionizing photon escape in the Sunburst Arc'
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Oct 4, 2024 - Jupyter Notebook
PHYS369: Astrophysics Group Project
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Mar 20, 2020 - Python
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
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Aug 4, 2020 - Python
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.
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Sep 10, 2020 - Jupyter Notebook
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.
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Jan 22, 2020 - Jupyter Notebook
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