Published June 22, 2022 | Version 1.0.3
Dataset Open

Frankenstein fits

Creators

  • 1. University of Cambridge

Contributors

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

Description

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.

Files

frank_fits.zip

Files (63.1 MB)

Name Size Download all
md5:5c8f4e69c22c7b3ece764f7ff7bee49a
63.1 MB Preview Download