Published May 20, 2024 | Version v1
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Products and Data for "A High Internal Heat Flux and Large Core for the Inflated Warm Neptune WASP-107b"

Creators

  • 1. ROR icon Arizona State University
  • 2. BAER Institute
  • 3. NASA Ames Research Center
  • 4. ROR icon University of Wisconsin–Madison
  • 5. ROR icon National Astronomical Observatory of Japan
  • 6. ROR icon University of California, Santa Cruz
  • 7. Steward Observatory
  • 8. NASA's Ames Research Center (ARC)
  • 9. University of Michigan
  • 10. ROR icon Lawrence Livermore National Laboratory
  • 11. ROR icon Université Côte d'Azur
  • 12. ROR icon Observatoire de la Côte d'Azur
  • 13. ROR icon Centre National de la Recherche Scientifique
  • 14. Laboratoire Lagrange
  • 15. ROR icon Bay Area Environmental Research Institute
  • 16. ROR icon Université Paris-Saclay

Description

Products and data for the JWST NIRCam/F322W2, NIRCam/F444W, and MIRI/LRS transit observations of WASP-107b as presented in Welbanks et al. 2024 (Nature).

For the NIRCam observations, the Eureka! Control Files (.ecf files) and Eureka! Parameter Files (.epf files) were used with version 0.9 of the Eureka! pipeline, CRDS version 11.17.0 and context 1093 (for F322W2) or 1097 (for F444W), and jwst package version 1.10.2. The F322W2 data used in the retrievals of Welbanks+2024 were offset by -81 ppm. For the MIRI/LRS observations, these ECF and EPF files were used with a custom version 0.9 of the Eureka! pipeline (modified to include the 390 Hz noise removal step merged through PR #556), CRDS version 11.17.0 and context 1097, and jwst package version 1.10.2. Welbanks+2024 retrieved an offset of +282 ppm for the MIRI/LRS data.

Files

FinalResults.zip

Files (8.6 MB)

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md5:c91d3d78a1574a06d48ae7e9bfe29d8f
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Additional details

Software

Repository URL
https://github.com/kevin218/Eureka
Programming language
Python
Development Status
Active