Fig. 2.
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Top: light curve of the pulsating DBV star GD 358 observed in sector 25. The black dots show the residual flux, while the red lines show all prewhitened variations from the light curve. Bottom: fourier transform of the pulsating DBV star GD 358 observed with 120-sec cadence. The dotted horizontal blue line indicates the 0.1% false-alarm-probability (FAP) significance threshold. The black line is the FT of the prewhitened light curve.
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