Image Details

Choose export citation format:

Detection of CO, H2O, and OH in WASP-18 b with JWST/NIRISS Using Direct-extracted Spectra and Cross Correlation

  • Authors: Qinglin Ouyang, Fei Yan, Shuo Liu, Boyue Guo, Guo Chen, Enric Pallé, Yuanheng Yang, Wei Wang, Meng Zhai, Qian Chen

Qinglin Ouyang et al 2026 The Astrophysical Journal 1004 .

  • Provider: AAS Journals

Caption: Figure 12.

Posterior distributions of the VMRs for key atmospheric species in WASP-18 b. The blue lines and shaded regions represent the median VMR profiles and their 1σ uncertainties derived from our equilibrium chemistry retrieval. The red histograms show the posterior distributions of the deep abundances retrieved from our free chemistry with thermal dissociation (free + dissociation) retrieval. For comparison, the yellow-filled histograms display the corresponding results from the free + dissociation retrieval of L.-P. Coulombe et al. (2023).

Other Images in This Article

Show More

Copyright and Terms & Conditions

Additional terms of reuse