Image Details
Caption: Figure E1.
The finalized, binned transmission spectra, shown by code, using Eureka1, ExoticJEDI, and Eureka2 reductions. We find a generally good agreement for the visits between both visits, on average within 2σ of each other. The binned spectra have 120 spectral channels with 40 nm bins.
© 2026. The Author(s). Published by the American Astronomical Society.