Code for Anisotropies in the Microwave Background
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Updated
Aug 27, 2024 - 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
Mock cone facility for astrophysical applications
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.
N-body code for cosmological structure formation in cubic vector Galileon gravity
ASPIC: Accurate Slow-roll Prediction for Inflationary Cosmology
We analyze the LambdaCDM model using the scipy.integrate.cumtrapz, scipy.integrate.quad, and F2py implementations.
FieldInf: an exact solver for linear cosmological perturbations during inflation
Wagoner / Kawano BBN code modifications to measure abundance
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
Calculate the correlation function of Maxima in 3D Gaussian random fields, sampling the components of the Hessian.
A ray tracing code to compute integrated cosmological observables on the fly in AMR CFD simulations
Code to analyze Cepheids' lightcurves to derive Hubble and Cosmological Constants
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