Image Details
Caption: Figure 2.
The posterior distributions associated with the 15 close transit retrievals for each of the 10 noise instances shown in Figure 1. We confidently detect CO2 in all noise instances, and sometimes are able to detect CH4 as well, while we do not detect (and therefore do not rely on detecting) H2O.
© 2026. The Author(s). Published by the American Astronomical Society.