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Published June 22, 2022 | Version 1.0.2
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Frankenstein fits

Authors/Creators

  • 1. University of Cambridge

Contributors

  • 1. Imperial College London
  • 2. University of Cambridge
  • 3. University of Leicester

Description

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 .fits pseudo-2D image of each frank brightness profile is reprojected according to the source geometry (inclination, PA) given in the header of the corresponding *_brightness_profile.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.

Files

frank_fits.zip

Files (63.1 MB)

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