Image Details
Caption: Figure 8.
Retrieved spectra with the WASP-39 b Tiberius data. The solid curves show the best-fit retrieved spectra obtained from the pRT baseline retrieval (including H2O) and the ones with added SO2 and CH4, as described in Section 4.1.2. We see that SO2 and CH4 both improve the fit in a similar wavelength range (≈7.5−8 μm), hence their partial degeneracy described in Appendix D.2. We note that the last data point at 11.375 μm is below the figure, with a transit depth of ﹩1.7{5}_{-0.117}^{+0.117} \% ﹩.
© 2026. The Author(s). Published by the American Astronomical Society.