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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 5.

Posterior distributions for the SC and haze parameters across the three retrieval models. From left to right: photosphere temperature (Tphot), heterogeneity (spot) temperature (Thet), log heterogeneity (spot) covering fraction (﹩\mathrm{log}{f}_{\mathrm{spot}}﹩), log haze scattering amplitude (﹩\mathrm{log}a﹩), and haze scattering slope (γ). Numerical labels above each panel summarize the parameter constraint: for parameters with two-sided bounded posteriors, we quote the median and 1σ bounds; for parameters with only one bound, we quote either the 5th-percentile lower limit or the 95th-percentile upper limit.

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