Published December 19, 2023
| Version v3
Dataset
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High Tide or Rip-Tide? GJ 486b JWST Transits with NIRSpec G395H - Supplementary Material
Creators
- Moran, Sarah E.1
- Stevenson, Kevin B.2
- Sing, David3
- MacDonald, Ryan J.4
- Kirk, James5
- Lustig-Yaeger, Jacob2
- Peacock, Sarah6
- Mayorga, L.C.2
- Bennett, Katherine A.3
- López-Morales, Mercedes7
- May, E.M.2
- Rustamkulov, Zafar3
- Valenti, Jeff8
- Adams Redai, Jéa I.7
- Alam, Munazza8
- Batalha, Natasha9
- Fu, Guangwei3
- Gonzalez-Quiles, Junellie3
- Highland, Alicia N.4
- Kruse, Ethan6, 10
- Lothringer, Joshua D.11
- Ortiz Ceballos, Kevin N.7
- Sotzen, Kristin Showalter2
- Wakeford, Hannah12
- 1. The University of Arizona Department of Planetary Sciences and Lunar and Planetary Laboratory
- 2. Johns Hopkins University Applied Physics Laboratory
- 3. Johns Hopkins University
- 4. University of Michigan–Ann Arbor
- 5. Imperial College London
- 6. Goddard Space Flight Center
- 7. Center for Astrophysics Harvard & Smithsonian
- 8. Space Telescope Science Institute
- 9. NASA Ames Research Center
- 10. University of Maryland, College Park
- 11. Utah Valley University
- 12. University of Bristol
Description
Supplementary material for 'High Tide or Riptide on the Cosmic Shoreline? A Water-rich Atmosphere or Stellar Contamination for the Warm Super-Earth GJ 486b from JWST Observations' by Moran & Stevenson et al., ApJL (2023).
This repository contains four categories of data products:
- White light curves — White light curves produced for Visit 1 and 2, for detectors NRS1 and NRS2 via the FIREFLy pipeline and the open-source codes Eureka! and Tiberius
- Transmission spectra — Reduced transmission spectra from three data reduction codes (Eureka!, FIREFLy, and Tiberius) for both G395H visits.
- Stellar spectra and models — Flux calibrated observed stellar spectra of GJ 486 from each G395H visit, along with best-fit PHOENIX stellar models.
- Atmospheric models — Atmospheric forward models used to interpret the data, produced from the open source PICASO and CHIMERA codes.
For any additional data requests or questions, please contact: sarahemoran@arizona.edu or kevin.stevenson@jhuapl.edu
Files
GJ486b_Zenodo_2023.zip
Files
(1.5 MB)
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Additional details
Related works
- Is documented by
- Preprint: 10.48550/arXiv.2305.00868 (DOI)
- Is published in
- Journal article: 10.3847/2041-8213/accb9c (DOI)
References
- Moran & Stevenson et al 2023 ApJL 948 L11