Image Details
Caption: Figure 10.
Retrieved temperature, mixing ratios, and haze parameters for the Atmos exo-Titan model. Left: retrieved volume mixing ratios for all three retrieval cases shown at the approximate depth of the haze layer. Right: haze opacity as a function of pressure and altitude. The temperature compared to the Atmos truth are also shown with their errors shown as shaded regions. Note that the POSEIDON haze location is inferred from the pressure contribution functions.
© 2026. The Author(s). Published by the American Astronomical Society.