Fig. 3.
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(a) PSD of the Kepler star KIC 8179973 on which a sliding box (shaded pink area) was used to compute the PS2 (inset) with Γ = 2 and filtered as explained in Section 3.1.1. (b) The red line is the averaged filtered PS2 normalized to its maximum value as a function of the center of the sliding windows. The dashed black line is the Gaussian fit.
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