The case of WASP-43b: emission spectrum from a Hot Jupiter

Taken from MIRI TSO Recommended Strategies part of the JWST User Documentation

Image taken from starry: Analytic Occultation Light Curves , by Luger et al., AJ, 157, 64 (2019)

Taken from Fig 1 of Bell et al., Nature Astronomy, Apr 2024

Taken from Supplementary Fig 2 of Bell et al., Nature Astronomy, Apr 2024

Taken from Figure 2 of Yang et al., arXiv 2406.03490 (2024)

Taken from Figure 2 of Yang et al., arXiv 2406.03490 (2024)

Taken from Figure B1 of Yang et al., arXiv 2406.03490 (2024)

For more information

• Entry for WASP-43b in NASA Exoplanet Archive
• Nightside clouds and disequilibrium chemistry on the hot Jupiter WASP-43b by Bell, T. J., et al., Nature Astronomy, Apr 2024
• Simultaneous retrieval of orbital phase resolved JWST/MIRI emission spectra of the hot Jupiter WASP-43b: evidence of water, ammonia and carbon monoxide by Yang, J., et al., MNRAS (accepted) 2024

Copyright © Michael Richmond. This work is licensed under a Creative Commons License.