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This article has an erratum: [https://doi.org/10.1051/0004-6361/201525920e]


Fig. 2

image

Example of the period adjustment based on the harmonic ambiguity of the estimated rotation periods from the frequency spectra of the light curves (Hartman et al. 2009). The darker gray line shows the fiducial ridge line shifted to the cluster “I” sequence. The lighter gray line was obtained by halving the periods corresponding to this cluster ridge line. The uncorrected (i.e., originally published) periods are displayed as black dots.

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