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[ascl:2109.010] Frankenstein: Flux reconstructor

Frankenstein (frank) 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. Frankenstein can perform a fit in 2 ways, by running the code directly from the terminal or using the code as a Python module.

Code site:
https://github.com/discsim/frank https://pypi.org/project/frank/
Described in:
https://ui.adsabs.harvard.edu/abs/2020MNRAS.495.3209J
Bibcode:
2021ascl.soft09010J

Views: 132

ascl:2109.010
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