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"
Creators
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Joseph Harrington1
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Michael D. Himes2
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Patricio E. Cubillos3
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Jasmina Blecic4
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Patricio M. Rojo5
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Ryan C. Challener6
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Nate B. Lust7
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M. Oliver Bowman2
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Sarah D. Blumenthal8
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Ian Dobbs-Dixon9
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Andrew S. D. Foster10
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Austin J. Foster2
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M. R. Green2
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Thomas J. Loredo11
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Kathleen J. McIntyre2
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Madison M. Stemm2
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David C. Wright2
- 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
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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