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Published September 20, 2017 | Version v1
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Far-infrared to millimeter data of protoplanetary disks: dust growth in the Taurus, Ophiuchus, and Chamaeleon I star-forming regions

  • 1. Boston University
  • 2. Laboratoire d'astrophysique de Bordeaux
  • 3. Harvard-Smithsonian Center for Astrophysics
  • 4. University of Michigan
  • 5. University of Lethbridge
  • 6. Instituto de Ciencia de Materiales de Madrid (CSIC)
  • 7. University of Lethbridge & The Netherlands Institute for Radio Astronomy

Description

This repository contains the data set presented in the manuscript "Far-infrared to millimeter data of protoplanetary disks: dust growth in the Taurus, Ophiuchus, and Chamaeleon I star-forming regions" (Ribas et al. 2017), and includes a table with several sample properties (e.g. stellar properties, Herschel photometry, different spectral indices), spectral energy distributions, Spitzer/IRS and Herschel/SPIRE spectra, the median SEDs of Taurus, Ophiuchus and Chamaeleon I, and the Herschel maps used.

 

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