Extended Data Fig. 2: Transit light curves of KIC-8681125.01 for the first (left) and second (right) epochs.
From: An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i
Top: Each panel shows the method marginalised detrended photometry centred on the times of transit, with the maximum likelihood planet–moon fit overlaid in solid black. Model comparison statistics are provided within the inset box. Bottom: Same as above but for a model with a single planet and variable blend factor between the two epochs. This model substantially outperforms the planet–moon model.
