Fig. A.1.
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Fourier spectra of the five photometrically variable CP2 stars. The data source (ZTF or ATLAS) is indicated in the upper right corner of each panel. In the case of Gaia DR3 3907547639444408064, the highest peak corresponds to half the true rotational period. For all other objects, the rotational periods correspond to the highest peaks (indicated by the red arrow in each panel).
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