Frankenstein fits
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Frankenstein brightness profiles, visibility fits and pseudo-2D images for interferometric datasets. Current datasets are: - Taurus survey: 10 disks (Jennings et al. accepted - arxiv) - DSHARP survey: 20 disks (Jennings et al. 2022 - ADS) The <em>.fits</em> pseudo-2D image of each frank brightness profile is reprojected according to the source geometry (inclination, PA) given in the header of the corresponding <em>*_brightness_profile.txt </em>file. The <em>.fits</em> 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.
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Zenodo创建时间：
2022-06-22
