Code for Anisotropies in the Microwave Background
-
Updated
Jun 10, 2025 - Fortran
Code for Anisotropies in the Microwave Background
Public version of PolyChord: See polychord.co.uk for PolyChordPro
The 3D version of C2-Ray for multiple sources, hydrogen only
Augmented halo model for accurate non-linear matter power spectrum calculations
C2-Ray radiative transfer / photo-ionziation code, version with helium, combining 1D and 3D
ASPIC: Accurate Slow-roll Prediction for Inflationary Cosmology
N-body code for cosmological structure formation in cubic vector Galileon gravity
BINGO: BI-spectra and Non-Gaussianity Operator is a FORTRAN 90 code that numerically evaluates the scalar bi-spectrum and the non-Gaussianity parameter fNL in single field inflationary models involving the canonical scalar field.
Mock cone facility for astrophysical applications
FieldInf: an exact solver for linear cosmological perturbations during inflation
We analyze the LambdaCDM model using the scipy.integrate.cumtrapz, scipy.integrate.quad, and F2py implementations.
Wagoner / Kawano BBN code modifications to measure abundance
A ray tracing code to compute integrated cosmological observables on the fly in AMR CFD simulations
A large scale structure void identifier for galaxy surveys based on the Beta-Skeleton graph
Code solving cosmological perturbation equations as well as background evolution
Code to analyze Cepheids' lightcurves to derive Hubble and Cosmological Constants
Calculate the correlation function of Maxima in 3D Gaussian random fields, sampling the components of the Hessian.
Add a description, image, and links to the cosmology topic page so that developers can more easily learn about it.
To associate your repository with the cosmology topic, visit your repo's landing page and select "manage topics."