Image Details
Caption: Figure 10.
The time series of residuals for three fits from the MLE grid that differ only by which reduction was used. All fits here used an exponential trend, quadratic limb darkening, 5 minutes cadence, and an Matérn 3/2 kernel, though we find that this pattern of ExoTiC-JEDI and katahdin achieving comparable residual rms values while Eureka! arrives at a solutions with higher scatter holds for all modeling combinations.
© 2026. The Author(s). Published by the American Astronomical Society.