Documentation
Welcome to the Frankenstein (frank) documentation, you monster. frank fits the 1D radial brightness profile of an
interferometric source given a set of visibilities. This site details how to
install and run the code, provides examples for applying the model and
interpreting its results, and hosts the code’s API.
Using the code
Under the hood
License & attribution
Frankenstein is free software licensed under the GPLv3 License. For more details see the LICENSE.
If you use frank for your research, please cite Jennings, Booth, Tazzari et al. 2020 MNRAS 495(3) 3209 [MNRAS] [ADS] [arXiv] [Zenodo]:
@ARTICLE{2020MNRAS.495.3209J,
author = {{Jennings}, Jeff and {Booth}, Richard A. and {Tazzari}, Marco and {Rosotti}, Giovanni P. and {Clarke}, Cathie J.},
title = "{frankenstein: protoplanetary disc brightness profile reconstruction at sub-beam resolution with a rapid Gaussian process}",
journal = {\mnras},
keywords = {methods: data analysis, protoplanetary discs, techniques: interferometric, planets and satellites: detection, submillimetre: general, submillimetre: planetary systems, Astrophysics - Earth and Planetary Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2020,
month = jul,
volume = {495},
number = {3},
pages = {3209-3232},
doi = {10.1093/mnras/staa1365},
archivePrefix = {arXiv},
eprint = {2005.07709},
primaryClass = {astro-ph.EP},
adsurl = {https://ui.adsabs.harvard.edu/abs/2020MNRAS.495.3209J},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
Contact
Submit a bug report or feature request on the issues page. For anything else, feel free to email Jeff.