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
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Moran, Sarah E.1
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Stevenson, Kevin B.2
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Sing, David3
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MacDonald, Ryan J.4
- Kirk, James5
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Lustig-Yaeger, Jacob2
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Peacock, Sarah6
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Mayorga, L.C.2
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Bennett, Katherine A.3
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López-Morales, Mercedes7
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May, E.M.2
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Rustamkulov, Zafar3
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Valenti, Jeff8
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Adams Redai, Jéa I.7
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Alam, Munazza8
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Batalha, Natasha9
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Fu, Guangwei3
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Gonzalez-Quiles, Junellie3
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Highland, Alicia N.4
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Kruse, Ethan6, 10
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Lothringer, Joshua D.11
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Ortiz Ceballos, Kevin N.7
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Sotzen, Kristin Showalter2
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Wakeford, Hannah12
- 1. The University of Arizona Department of Planetary Sciences and Lunar and Planetary Laboratory
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2.
Johns Hopkins University Applied Physics Laboratory
- 3. Johns Hopkins University
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4.
University of Michigan–Ann Arbor
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5.
Imperial College London
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6.
Goddard Space Flight Center
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7.
Center for Astrophysics Harvard & Smithsonian
- 8. Space Telescope Science Institute
- 9. NASA Ames Research Center
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10.
University of Maryland, College Park
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11.
Utah Valley University
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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