Fig. B.1
Photometric analysis of SAO206462. Top row from left to right: V-band differential magnitudes versus Heliocentric Julian Day, Lomb-Scargle periodogram, and the periodogram after filtering. For the Lomb-Scargle periodogram, we show the spectral window function (red dotted line), the power level corresponding to FAP = 1% (horizontal dashed line), and the peak corresponding to the rotation period (red arrow). Bottom panel: Light curve phased with the rotation period. The solid line represents the sinusoidal fit.
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