Frankenstein fits
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Frankenstein brightness profiles and visibility fits for interferometric datasets. Current datasets (continually updated) are: - DSHARP: All 20 disks (Jennings et al. 2022 - ADS) The <em>.fits</em> images of each frank profile are 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：
2021-10-25
