Fig. 12
Top: differential light curve of V893 Sco of the night of 2000 June 9/10. Bottom: low frequency part of the power spectrum of the light curve, after masking the eclipses. The orbital frequency and its first harmonic are marked by dashed vertical lines. The solid line in the upper frame is a 4 term sine fit (eclipses masked) with periods fixed to the values corresponding to the dominant peaks in the power spectrum.
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