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
pip install frank
Documentation
Check out the docs.
Attribution
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}
}
These papers cite frank.
Authors
Contact
Submit a bug report or feature request on the issues page. For anything else, feel free to email Jeff.
License
frank is free software licensed under the LGPLv3 License. For more details see the LICENSE.
© Copyright 2019-2022 Richard Booth, Jeff Jennings, Marco Tazzari.
Image: Universal Studios, NBCUniversal [Public domain]
Metadata
Release files for frank 1.2.3
For a detailed explanation of source distributions (sdists) and built distributions (wheels), please see the package formats documentation.
Source distribution (sdist)
| File | Size | Uploaded | Provenance | |
|---|---|---|---|---|
| frank-1.2.3.tar.gz | 81.7 kB | Without provenance | Details |
Release files / frank-1.2.3.tar.gz
| Download URL | frank-1.2.3.tar.gz |
|---|---|
| Size | 81.7 kB |
| Tags | Source |
|
SHA-256 checksum How to use checksums |
d20666bd582088a8d8b62b2c52b21bdd18bc6640fea5105d4aee7ba4d63fb378
|
|
BLAKE2b-256 checksum How to use checksums |
d5911e3f1ebd401bff820f79ccc26fb59119d77d377997ffc782ded72d598740
|
| Upload date | |
|
Uploaded using Trusted Publishing? What is trusted publishing? |
No |
| Uploaded via |
twine/3.8.0 colorama/0.4.4 importlib-metadata/4.6.4 keyring/23.5.0 pkginfo/1.8.2 readme-renderer/34.0 requests-toolbelt/0.9.1 requests/2.25.1 rfc3986/1.5.0 tqdm/4.57.0 urllib3/1.26.5 CPython/3.10.12
|
Security for frank 1.2.3
Provenance
Provenance describes where a file came from. On PyPI, provenance is shared via attestations, which provide a verifiable record of the build or publishing details. View details, limitations and caveats.
No provenance found
None of the files in this release were uploaded with provenance metadata.
A note on package security
PyPI is a repository for distributing packages, not a service for auditing them. While third-party security researchers and our staff do their best to detect and remove malicious packages, PyPI cannot guarantee the quality, security or suitability of any given package.
To learn more about protecting yourself from malicious actors, visit our package security documentation.