Extended Data Fig. 3: Transit light curves of KIC-5351250.06/Kepler-150f 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
Each row shows a different model fit to the same data. Whilst the planet–moon model is clearly a better fit than the planet-only model, a 2-spot model is able to out-perform either and is well motivated from the activity levels observed in the out-of-transit light curve.
