Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF

JWST MEP—A World Under Spotty Starlight: Detection of CO2 and H2O in the Hot Saturn WASP-52b with JWST NIRSpec G395H

  • Authors: Yanbo Pan, 彦博 潘, Ryan J. MacDonald, Néstor Espinoza, Bibiana Prinoth, Zafar Rustamkulov, Luis Welbanks, Daniel Kitzmann, Nicolas Crouzet, Anna Walde, Diana Powell, Eva-Maria Ahrer, Adam J. Burgasser, Duncan A. Christie, Wolf Cukier, Carlos Gascón, Måns Holmberg, Thomas Kennedy, Mercedes López- Morales, N. J. Mayne, Dominic Samra, Arjun B. Savel, Maria E. Steinrueck, Christopher P. Wirth

Yanbo Pan et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure B1.

Sensitivity of our WASP-52b NIRSpec/G395H spectra to orbital parameters. Top: transitspectroscopy spectra using orbital parameters derived from the JWST NIRSpec/G395H data (black data) and with orbital parameters fixed to the Spitzer analysis from M. K. Alam et al. (2018) (blue data). The Spitzer data are overlaid for comparison (red data). Bottom: difference between the NIRSpec/G395H spectra for the two orbital parameter treatments, showing a uniform ∼124 ppm offset.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse