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Fig. B.3.
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Amplitude spectra for the long-period Ap stars, continued. For TIC 158275114, S14 and S26 are plotted separately, showing that the low frequency peak near 1 d−1 is not present in both sectors, hence is not a rotation signal. This star is a well-studied roAp star, KIC 8677585 (Balona et al. 2013) (section 2.1).
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