Image Details
Caption: Figure 8.
Same as Figure 6 but for T-1 d. However, T-1 d had no stable H2O–CO2 outgassed, O2-dominated atmospheres, so that row is absent from the figure. Moreover, as T-1 d has no published emission data, both transmission and emission spectra are colored by that model’s fit to the available transmission data (C. Piaulet-Ghorayeb et al. 2025). All modeled atmospheres in this study fit the T-1 d transmission data to <1σ.
© 2026. The Author(s). Published by the American Astronomical Society.