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Fig. 3


Spectral power distributions for the light curve period (which corresponds to half the rotation period for a shape-induced double-peaked light curve) of 358P using a statistical approach. For any period in the range, the distributions provide the spectral power as derived with a Lomb–Scargle algorithm; the coloured lines denote different Fourier orders. We are unable to identify a clear periodicity in the period range that was probed.

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