Fig. 3
Composite lightcurve of (215619) 2003 SQ168 from 2015. The solid line is the fit second-order Fourier series showing that there is a low-amplitude signal for the period obtained from the 2013 data. The exact ligthcurve shape is not well revealed due to noisy 2015 observations that were taken close to the aphelion of the asteroid’s orbit (see Table 1).
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