Image Details
Caption: Figure 8.
Spectra for both visits for each of the Eureka! (left) and Tiberius (right) reductions. We show the differences between the two visits within a reduction pipeline on the bottom panels in units of σ (black) and ppm (blue). While there are some differences between the visits, the points generally agree, with median differences of <1σ. Only two points in the Eureka! spectra and one point in the Tiberius spectra deviate by more than 3σ between visits.
© 2026. The Author(s). Published by the American Astronomical Society.