All Figures

$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F1.PS} \end{figure}$ Figure 1: Upper panel: Varuna's magnitude versus time (days) from our observatios. Middle panel: our data and Jewitt & Sheppard's (2002) data phased to the period we propose. Our data are shown as plus signs and Jewitt & Sheppard's (2002) are shown as triangles. Lower panel: our data and Jewitt & Sheppard's (2002) data phased to the period proposed by Jewitt & Sheppard (2002). Our data are shown as plus signs and Jewitt & Sheppard's (2002) are shown as triangles. As can be seen, the data are not in phase, which implies that 6.3442 h is incorrect.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F2.PS} \end{figure}$ Figure 2: Upper panel: 1999 TD₁₀ magnitude versus time (days). Lower panels: rotational phase curves for two possible periods, 7.71 h and 5.8 h, respectively. As can be seen, a period of 5.8 h does not yield an acceptable phase curve. Different symbols correspond to different dates.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F3.PS} \end{figure}$ Figure 3: Upper panel: 2001 PT₁₃'s magnitude versus time (days). Lower panel: rotational phase curves for a possible spin period of 8.3091 h. Different symbols correspond to different dates.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F4.PS} \end{figure}$ Figure 4: Upper panel: 2000 QC₂₄₃'s magnitude versus time (days). Lower panel: rotational phase curve for a period of 9.14 h. Different symbols correspond to different dates.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F5.PS} \end{figure}$ Figure 5: Upper panel: 2000 EB₁₇₃'s magnitude versus time (days). Lower panel: rotational phase curve for one possible period. The different symbols correspond to different dates.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F6.PS} \end{figure}$ Figure 6: Upper panel: 2000 PN₃₄'s magnitude versus time (days). Lower panels: rotational phase curves for two possible periods, 8.45 h and 10.22 h. Different symbols correspond to different dates.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F7.PS} \end{figure}$ Figure 7: Upper panel: 2002 GO₉'s magnitude versus time (days). Lower panels: rotational phase curves for two possible periods, 9.67 h and 6.97 h. Different symbols correspond to different dates. The line is a sinusoidal fit to the data.
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In the text

$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F2.PS} \end{figure}$	Figure 2: Upper panel: 1999 TD₁₀ magnitude versus time (days). Lower panels: rotational phase curves for two possible periods, 7.71 h and 5.8 h, respectively. As can be seen, a period of 5.8 h does not yield an acceptable phase curve. Different symbols correspond to different dates.
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$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F3.PS} \end{figure}$	Figure 3: Upper panel: 2001 PT₁₃'s magnitude versus time (days). Lower panel: rotational phase curves for a possible spin period of 8.3091 h. Different symbols correspond to different dates.
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$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F4.PS} \end{figure}$	Figure 4: Upper panel: 2000 QC₂₄₃'s magnitude versus time (days). Lower panel: rotational phase curve for a period of 9.14 h. Different symbols correspond to different dates.
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$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F5.PS} \end{figure}$	Figure 5: Upper panel: 2000 EB₁₇₃'s magnitude versus time (days). Lower panel: rotational phase curve for one possible period. The different symbols correspond to different dates.
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$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F6.PS} \end{figure}$	Figure 6: Upper panel: 2000 PN₃₄'s magnitude versus time (days). Lower panels: rotational phase curves for two possible periods, 8.45 h and 10.22 h. Different symbols correspond to different dates.
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$\begin{figure} \par\includegraphics[angle=90,width=8.5cm,clip]{H4443F7.PS} \end{figure}$	Figure 7: Upper panel: 2002 GO₉'s magnitude versus time (days). Lower panels: rotational phase curves for two possible periods, 9.67 h and 6.97 h. Different symbols correspond to different dates. The line is a sinusoidal fit to the data.
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