frank 0.1.0

WARNING Though you've found this repo, the code isn't quite released yet! v1.0 will be concurrent with the arXiv posting of the code's methods paper (we aim for April). Please email Jeff if you'd like to use the code before then. Thanks!

.. image:: https://circleci.com/xx/frank.svg?branch=master :target: https://circleci.com/xx/frank

.. image:: https://img.shields.io/pypi/v/frank.svg :target: https://pypi.python.org/pypi/frank

.. image:: https://img.shields.io/github/release/discsim/frank/all.svg :target: https://github.com/discsim/frank/releases

Frankenstein (frank) is a library that fits the 1D radial brightness profile of an interferometric source given a set of visibilities. It uses a Gaussian process that performs the fit in <1 minute for a typical protoplanetary disc continuum dataset.

Get the code

frank's on PyPI, so you can just use pip,

pip install frank

Documentation

The docs have it all.

Attribution

If you use frank for your research please cite Jennings, Booth, Tazzari et al. (2020) MNRAS xx xx [MNRAS] [arXiv] [ADS]:

xx

Authors

• Richard 'Dr. Frankenstein' Booth (University of Cambridge)

• Jeff 'The Monster' Jennings (University of Cambridge)

• Marco 'It's Alive!!!' Tazzari (University of Cambridge)

Contact

Interested in collaborating to improve, extend or apply frank? Or just have questions about the code that don't require submitting an issue? Email Jeff!

License

frank is free software licensed under the LGPLv3 License. For more details see the LICENSE.

© Copyright 2019-2020 Richard Booth, Jeff Jennings, Marco Tazzari.

Image: Universal Studios, NBCUniversal [Public domain]