Image Details
Caption: Figure 7.
1D marginalized posterior distributions for a subset of retrieval parameters on the full NIRISS/SOSS, NIRSpec/G395H, and MIRI/LRS spectrum for different choices of MIRI pixel shifts. Despite MIRI/LRS pixel shifts resulting in different preferred gases when analyzed individually, these differences are insignificant when combined with NIR data.
© 2025. The Author(s). Published by the American Astronomical Society.