Frankenstein fits

Frankenstein brightness profiles, visibility fits and pseudo-2D images for interferometric datasets. Current datasets are: - Taurus survey (see Long et al. 2018, 2019): 23 disks (Jennings et al. accepted - arXiv) - DSHARP survey (see Andrews et al. 2018): 20 disks (Jennings et al. 2022 - ADS) The .fits pseudo-2D image of each frank brightness profile is reprojected according to the source geometry (inclination, PA), which is given in the header of the corresponding *_visibility_fit.txt file. The .fits image centers the profile at (dRA, dDec) = (0, 0). Please cite the linked paper if using fits from that work, thanks! Frankenstein is on GitHub and Read the Docs.