Code for Anisotropies in the Microwave Background
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Updated
Apr 28, 2025 - Fortran
Code for Anisotropies in the Microwave Background
⚡️⚡️⚡️Blazing fast correlation functions on the CPU.
Analysis kit for large-scale structure datasets, the massively parallel way
Large suite of N-body simulations
NumCosmo main code
This is the public repository for the AbacusSummit suite, intended for specifications of the simulations and instructions for reading the files.
A pure Python halo-model implementation for power spectra of any large-scale structure tracer combination.
Python code to interface with halo catalogs and other Abacus N-body data products
Augmented halo model for accurate non-linear matter power spectrum calculations
JAX-based linear Einstein-Boltzmann solver for cosmology
A pure python implementation of HMcode
Full-Shape Power Spectrum and Bispectrum Likelihoods
a lightweight Python binding of the CLASS CMB Boltzmann code
Simulator Expansion for Likelihood-Free Inference (SELFI): a python implementation
Accurate predictions for the clustering of galaxies in redshift-space in Python
Code for leveraging Information Maximising Neural Networks for optimal cosmological field compression and Bayesian inference for cosmological parameters
Cosmology Group repo for its public webpage, reviews & publications on tensions in ΛCDM, redshift and the CMB
Estimators and data for window-free analysis of power spectra and bispectra
Public release of data products following the BORG SDSS analysis
This is a short astro-physical program showing how to compute the adhesion model, describing the large-scale structure of the Universe, using regular triangulations in CGAL (www.cgal.org), as well as using the Convex Hull algorithm present in Python's Scipy.
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