Argus ===== .. image:: https://github.githubassets.com/images/modules/logos_page/GitHub-Mark.png :width: 24px :target: https://github.com/tomkimpson/Argus :alt: GitHub Repo Welcome to the **Argus** project documentation. **Argus** is a research project for the `detection of nHz gravitational waves `_ using Pulsar Timing Arrays (PTAs), leveraging a `state-space representation `_. It is an ongoing effort to open-source methods developed at the `University of Melbourne `_ and `OzGrav `_. For the accompanying papers please see: - `Kimpson et al. 2024a `_ - `Kimpson et al. 2024b `_ - `Kimpson et al. 2025 `_ About this Documentation ------------------------ This documentation provides an overview of the project, installation and usage instructions, API details, and developer notes for contributors. .. note:: If you're new to Argus, start with the "Getting Started" page in the table of contents below. Example Usage ------------- You can find an example of a standard PTA analysis using NANOGrav data here: link to jupyter tutorial (TBD)... Etymology --------- The project is named **Argus**, after the hundred-eyed giant of Greek mythology. > In a pulsar timing array, multiple pulsars across the sky act as a network of cosmic "eyes", continuously watching for gravitational waves. ---- .. toctree:: :caption: Table of Contents :maxdepth: 3 Getting Started State-Space Methods API Documentation <_apidoc/tkimpson_2025a> Contributing Index ===== * :ref:`genindex` * :ref:`modindex`