Welcome to PyStaff’s documentation!

PyStaff fits model templates to optical and near-infrared spectra of nearby galaxies. These pages will give you a quick introduction on how it works. It’s MIT-licensed, been used most recently in the paper Vaughan et al 2018b and is being actively updated and developed on Github.

Contents:

• Quick Introduction
  • PyStaff: Stellar Absorption Feature Fitting in python
• A simple example
  • Setting Up
  • A simple fitting process with emcee
  • Results
• Using MPI

Indices and tables

• Index
• Module Index
• Search Page