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JWST Transmission Spectroscopy of TOI-3235 b: Challenges in Constraining Giant Planet Atmospheres around M Dwarfs amid Stellar Contamination

  • Authors: Zoe Ko, Néstor Espinoza, Andrés Jordán, Daniel Bayliss, Edward M. Bryant, Martin Schlecker, Melissa J. Hobson, Rafael Brahm, Remo Burn, Thomas Henning

Zoe Ko et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 4.

Retrieved trace abundances for all three retrievals. Each panel shows the posterior distribution of ﹩\mathrm{log}{X}_{i}﹩ for one molecular species. Numerical labels above each panel summarize the abundance constraint: for molecules with two-sided bounded posteriors, we quote the median and 1σ bounds; for molecules with only one bound, we quote either the 5th-percentile lower limit or the 95th-percentile upper limit; and for posteriors that reach both prior edges, we label the abundance as unconstrained. For molecules with two-sided bounds, we include the Bayes factor (BF).

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