Welcome to CosmoWAP Documentation
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COSMOlogy with Wide-separation, relAtivistic and Primordial non-gaussian contributions
CosmoWAP is a Python framework for forecasts of large-scale galaxy clustering using 3D power spectrum and/or bispectrum multipoles. The modelling covers relativistic effects, wide-separation corrections, and Primordial non-Gaussianity (PNG) in standard perturbation theory.
The core analytical expressions are derived in Mathematica using MathWAP and exported as .py files. These expressions take a cosmology (via CLASS) and a set of bias models as input. Built around this core is the forecasting machinery: bias modelling with HOD/luminosity functions, theoretical covariances, Fisher matrices, and MCMC modules.
Getting Started:
Biases:
Power Spectra and Bispectra:
Forecasting:
MathWAP:
Reference: