Image Details
Caption: Figure 9.
Comparison between the rms of the residuals for fits that used the Eureka! pipeline and fits that used either ExoTiC-JEDI or katahdin. Each point represents a like-for-like comparison where every modeling choice is the same (cadence, trend type, GP kernel, etc.) except for the reduction used.
© 2026. The Author(s). Published by the American Astronomical Society.