Fig. 4

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Results from the validation run outlined in Sect. 3. (a) Corner plot for the posterior distributions of the planetary surface temperature T0, surface pressure P0, radius Rpl, mass Mpl, and retrieved abundances of different molecules. The red lines indicate the values used to generate the input spectrum. Additionally, we plot the retrieved median and the 16th and 84th percentile as dashed lines in every posterior plot. (b) Retrieved P−T profile. The shaded green regions show the uncertainties on the retrieved profile. In the bottom left corner of the P−T profile plot, we display P0 and T0. The red cross marks the input values. (c) The retrieved emission spectrum Fretrieved relative to the input emission spectrum for the retrieval Finput.
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