reionization
There are 20 repositories under reionization topic.
garrelt/C2-Ray3Dm
The 3D version of C2-Ray for multiple sources, hydrogen only
mirochaj/ares
Accelerated Reionization Era Simulations
JulianBMunoz/Zeus21
Zeus21: Lightning-fast simulations of cosmic dawn
annehutter/grid-model
Code to compute ionization field from density fields and source catalogue (CIFOG)
garrelt/C2-Ray3Dm1D_Helium
C2-Ray radiative transfer / photo-ionziation code, version with helium, combining 1D and 3D
rajeshmondal18/N-body
A code to compute the non-linear evolution of the cosmological matter density contrast.
rajeshmondal18/ReionYuga
A semi-numerical code to generate the Epoch of Reionization (EoR) neutral Hydrogen (HI) field.
phirling/pyc2ray
Python interface to C2Ray, with GPU-acceleration
smutch/meraxes
The Meraxes semi-analytic galaxy formation model.
annehutter/astraeus
Home of the semi-analytical / semi-numerical galaxy evolution and reionization code ASTRAEUS
rajeshmondal18/FoF-Halo-finder
A code to identify the location and size of the gravitationally collapsed dark matter halos.
annehutter/21cm-grid-model
Code to compute the HI 21cm and 3HeII 3.5cm field from density fields and source catalogues
ronniyjoseph/SCAR
Simulating the Calibration of Arrays with Redundancy: a project to understand the impact of position errors on redundant calibration.
yunfanz/21cmpy
PyCUDA based implementation of 21cmFAST
mrileyowens/owens202Y
Software release for 'Connecting Lyman-α and ionizing photon escape in the Sunburst Arc'
ronniyjoseph/Beam-Perturbations
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.
ronniyjoseph/Hybrid-Calibration
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
why-keith/ReHILAE
PHYS369: Astrophysics Group Project
smsharma/twentyone-global
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.