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Welcome to the PyKinematicalBroadening wiki!

Hello and welcome to the PyKinematicalBroadening wiki on GitHub! We're excited to have you here and hope that you find the information on this page helpful.

PyKinematicalBroadening is an open-source Python package for modelling the kinematical broadening of spectral lines in astrophysical sources. The package provides a set of tools for analyzing the line-broadening effects due to the Doppler effect and other kinematical processes.

On this wiki, you'll find information about how to install and use PyKinematicalBroadening, as well as documentation on the package's classes, functions, and methods. We encourage you to explore the different sections of the wiki and learn more about how you can use PyKinematicalBroadening in your own astrophysical research.

If you have any questions or comments about PyKinematicalBroadening, feel free to post them in the "Issues" section of the GitHub repository. We welcome contributions from the community and encourage you to submit pull requests with new features or bug fixes.

Thank you for your interest in PyKinematicalBroadening, and we hope that you find this wiki to be a useful resource!