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Early Insights for Atmospheric Retrievals of Exoplanets Using JWST Transit Spectroscopy

  • Authors: Savvas Constantinou, Nikku Madhusudhan, Siddharth Gandhi

Savvas Constantinou et al 2023 The Astrophysical Journal Letters 943 .

  • Provider: AAS Journals

Caption: Figure 4.

Full posterior distribution from the retrieval using the JWST/NIRSpec PRISM 3–5 μm spectrum, reduced with the Tiberius pipeline, combined with HST/WFC3 data (0.8–1.7 μm). The model parameters correspond to the canonical atmospheric model described in Section 3. Horizontal error bars denote the median and 1σ interval for each retrieved parameter. Also shown is the retrieved P-T profile, with the black line denoting the median retrieved profile, while darker and lighter orange contours indicate the 1σ and 2σ intervals.

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