\begin{table}%t2
\caption{\label{correl}Most important correlations found using the light curve parameters
and orbital/physical variables as described in the text. The parameters
presented are the light curve amplitude (Ampl.), the perihelion~($q$) and
aphelion ($Q$) distances, inclination ($i$), eccentricity ($e$) and absolute
magnitude ($H$).} 
\small %\centering
\par
\begin{tabular}{llccc}
\hline\hline \noalign{\smallskip}
Population     & Correlated Magnitudes  & $\rho$ & SL(\%) & $n$ \\
\hline  
All KBOs & Ampl. vs. $Q$ & $-$0.22  & 96.96 & 100 \\
          & Ampl. vs. $H$ &  0.35  & 99.94 & 100 \\
\hline
Classical  & Period vs. $B-V$   & 0.66  & 98.49 & 17 \\
           & Ampl. vs. $Q$      & $-$0.36 & 97.95 & 42 \\
           & Ampl. vs. $H$      & 0.49  & 99.80 & 42 \\
           & Ampl. vs. $i$      & $-$0.37 & 98.16 & 42 \\
           & Ampl. vs. $e$      & $-$0.34 & 96.74 & 42 \\
\hline
Hot        & Period vs. $B-V$   & 0.66  & 98.11 & 15 \\
\hline
Cold       & Period vs. $Q$     & $-$0.80  & 94.97 & 7 \\
\hline
Centaurs & Period vs. $B-V$& 0.49 & 91.40 & 14 \\
         & Period vs. $e$  & 0.47 & 94.04 & 18 \\
\hline
Plutinos & Period vs. $H$  & $-$0.48 & 94.14 & 17 \\
\hline
SDO's     & Period vs. $V-R$  & $-$0.65 & 91.55 & 8 \\
          & Ampl. vs. $H$     & 0.57  & 92.86 & 14 \\ 
\hline
\end{tabular}
\end{table}