Fig. 5
Lomb–Scargle periodogram of KOI-976’s short-cadence photometry before (black) and after (red) subtracting stellar variability. LASR reduced the spectral power of all oscillations from ~ 104 at the max to ~1.0. We reduce the representative significance of all subtracted oscillations by at least 98% and find that all significant oscillations are well-modelled as sinusoids.
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