Published October 20, 2021 | Version 1
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Research Compendium for Harrington et al. (2021): "An Open-Source Bayesian Atmospheric Radiative Transfer (BART) Code: I. Design, Tests, and Application to Exoplanet HD 189733 b"

  • 1. Planetary Sciences Group, Department of Physics and Florida Space Institute, University of Central Florida
  • 2. Planetary Sciences Group, Department of Physics, University of Central Florida
  • 3. Space Research Institute, Austrian Academy of Sciences; Planetary Sciences Group, Department of Physics, University of Central Florida
  • 4. Department of Physics, New York University Abu Dhabi; Center for Astro, Particle and Planetary Physics, New York University Abu Dhabi; Planetary Sciences Group, Department of Physics, University of Central Florida
  • 5. Departamento de Astronomia, Universidad de Chile
  • 6. Planetary Sciences Group, Department of Physics, University of Central Florida; Department of Astronomy, University of Michigan
  • 7. Planetary Sciences Group, Department of Physics, University of Central Florida; Department of Astrophysical Sciences, Princeton University
  • 8. Planetary Sciences Group, Department of Physics, University of Central Florida; Department of Physics, University of Oxford
  • 9. Department of Physics, New York University Abu Dhabi; Center for Astro, Particle and Planetary Physics, New York University Abu Dhabi; Center for Space Science, NYUAD Institute, New York University Abu Dhabi
  • 10. Planetary Sciences Group, Department of Physics, University of Central Florida; Center for Astrophysics and Planetary Science, Cornell University
  • 11. Center for Astrophysics and Planetary Science, Cornell University

Description

This archive is the Reproducible Research Compendium for

An Open-Source Bayesian Atmospheric Radiative Transfer (BART) Code: I. Design, Tests, and Application to Exoplanet HD 189733 b

by Harrington et al. (2021), published in The Planetary Science Journal.

BART is an atmospheric parameter retrieval code.  It infers the properties of planetary atmospheres from spectroscopic observations.  The compendium includes all the software, documentation, configuration files, plots, and data published in the paper.  The compendium is under the Reproducible Research Software License; see LICENSE file.  The README provides additional information and describes the contents of each compressed .tar.gz file.

Notes

Part of this work is based on observations made with the Spitzer Space Telescope, which is operated by the Jet Propulsion Laboratory, California Institute of Technology under a contract with NASA. This work was supported by NASA Planetary Atmospheres grant NNX12AI69G, NASA Astrophysics Data Analysis Program grant NNX13AF38G, and NASA Exoplanets Research Program grant NNX17AB62G, held by JH. MDH held NASA Fellowship Activity fellowship 80NSSC20K0682. JB held NASA Earth and Space Science Fellowship NNX12AL83H. IDD and JB held NASA Exoplanets Research Program grant NNX17AC03G. PEC was supported by the Fulbright Program for Foreign Students. PMR acknowledges support from CONICYT project Basal AFB-170002.

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Additional details

References

  • Harrington et al. (2021), An Open-Source Bayesian Atmospheric Radiative Transfer (BART) Code: I. Design, Tests, and Application to Exoplanet HD 189733 b, Planetary Science Journal