Fig. 10
Light curves (plotted using grey dots, showing a zoom-in to slightly less than 1/10th of the full data set) and the power spectra (plotted using red solid lines) of the five SPB stars studied in this paper along with the ones of KIC 10526294 and KIC 7760680 from Pápics et al. (2014, 2015) ordered according to the frequency of maximum power. For further information see Sect. 3.5.
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