Code for Anisotropies in the Microwave Background

Public version of PolyChord: See polychord.co.uk for PolyChordPro

Augmented halo model for accurate non-linear matter power spectrum calculations

The 3D version of C2-Ray for multiple sources, hydrogen only

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.

ASPIC: Accurate Slow-roll Prediction for Inflationary Cosmology

A large scale structure void identifier for galaxy surveys based on the Beta-Skeleton graph

Algorithm for Void Identification in Cosmology is a comprehensive and significant update to a previous void finder published by Ricciardelli et al. (2013). Density and velocity divergence are used to define unstructured voids, which are formed by combining a set of cubes.

N-body code for cosmological structure formation in cubic vector Galileon gravity

Code solving cosmological perturbation equations as well as background evolution

NUC123 code for simulating Big Bang Nucleosynthesis (BBN) process.

FieldInf: an exact solver for linear cosmological perturbations during inflation

C2-Ray radiative transfer / photo-ionziation code, version with helium, combining 1D and 3D

A ray tracing code to compute integrated cosmological observables on the fly in AMR CFD simulations

The beginnings of an LSS simulation

We analyze the LambdaCDM model using the scipy.integrate.cumtrapz, scipy.integrate.quad, and F2py implementations.

Calculate the correlation function of Maxima in 3D Gaussian random fields, sampling the components of the Hessian.

The program is designed to work with COSmological MODels. Corresponding scripts plot all figures in the papers (see README for details).

A Fortran integrator for GILA cosmology