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Fig. 2

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Lightcurve of (190491) 2000 FJ10 obtained in the Sloan r filter. There are no apparent periodic variations during 20 min with a peak-to-peak amplitude greater than 0.05 mag. The slope in the linear fit is too small to be significant. For comparison, brightness variations of one of the SDSS stars are also presented. The observed scatter of points is caused by the residual effects of the flat fielding procedure.

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