\begin{table}%t3
\caption{\label{BrightVAR}Objects with possible short-term brightness variability.} 
\small%\centerline
 {
\begin{tabular}{c c c c c c c}  
\hline\hline  
  & Object & Type & $\Delta t$(min) & $\Delta R$(mag) & $\sigma_{\rm phot}$ & $R$-range\\
\hline 
3$\sigma$ var. 		& 1997SZ$_{10}$ & 2:1  & 33	 & 0.36 & 0.06 & 22.82--23.18\\
& 2000CR$_{105}$& ESDO & 50  & 0.21 & 0.05 & 23.28--23.49\\
& 2000YC$_{2}$  & SDO  & 42  & 0.33 & 0.10 & 22.86--23.19\\				& 2000YU$_{1}$	& Hot  & 44	 & 0.12 & 0.03 & 23.77-23.89\\
& 2003AZ$_{84}$ & 3:2  & 18  & 0.20 & 0.01 & 20.04--20.24\\
& 2003QB$_{112}$& Hot  & 151 & 0.48 & 0.05 & 22.40--22.88\\
& 2003QY$_{111}$& Cold & 156 & 0.72 & 0.11 & 23.10--23.82\\
$\leq$$2\sigma$ var.		    & 2000CP$_{104}$& Hot  & 58  & 0.08 & 0.04 & 23.17--23.25\\
& 2001QX$_{322}$& SDO  & 24  & -- & 0.05 & 21.97--22.01\\ 
& 2002UX$_{25}$ & Hot  & 46  & -- & 0.01 & 19.63--19.64\\	
& 2003QW$_{90}$ & Hot  & 18  & -- & 0.01 & 21.16--21.19\\				\hline 
\end{tabular}}
\medskip
Type, is the dynamical classification of the objects as described in Sect.~\ref{DataAnalysis}: hot (classical with $i>4.5^{\circ}$), cold (classical with $i<4.5^{\circ}$), SDO (scattered disk object), ESDO (extended scattered disk object), 2:1 and 3:2 (Neptune{'}s resonant objects). $\Delta t$, is the measurement interval in minutes. $\Delta R$, is the $R$-magnitude variation. $\sigma_{\rm phot}$~is the uncertainty of the relative photometry of the object (see text). $R$-range, is the total range of the $R$~magnitudes measured. We do not include the $\Delta R$s that are less than~$\sigma_{\rm phot}$.
\end{table}