pyRSD is a Python package for computing the theoretical predictions of the redshift-space power spectrum of galaxies. The package also includes functionality for fitting data measurements and finding the optimal model parameters, using both MCMC and nonlinear optimization techniques.
The software is compatible with Python versions 2.7, 3.5, and 3.6.
Testing is performed via the continuous integration service for Python version 2.7, 3.5, and 3.6. The build status of those tests is below.
The package is installable via the conda utility as
conda install -c nickhand -c astropy pyrsdThe theoretical models used in this paper are described in more detail in Hand et al. 2017. Please cite this work if you use this package in your research.
For installation instructions, examples, and full API documentation, please see Read the Docs.