\begin{table}%t2
\caption{\label{ksresults}Fitting results for the light curves of SN~2006aj attained 
by either excluding early data (top) or including an additional 
power-law component decaying with index~$\alpha$ (see
text for details).}
\small%\centering
\par
\begin{tabular}{llccr}
\hline\hline\noalign{\smallskip}
	&	$\chi^2_\nu$	&	$k$	&	$s$	&	$\alpha$	\\ \hline
$B$	&	1.83	&	$0.734\pm0.014$	&	$0.620\pm0.006$	&	$\cdots$	\\
$V$	&	1.02	&	$0.724\pm0.007$	&	$0.682\pm0.005$	&	$\cdots$	\\
$R$	&	1.93	&	$0.735\pm0.007$	&	$0.689\pm0.006$	&	$\cdots$	\\
$I$	&	0.71	&	$0.761\pm0.008$	&	$0.686\pm0.008$	&	$\cdots$	\\ \hline
$B$	&	1.79	&	$0.721\pm0.022$	&	$0.613\pm0.005$	&	$1.53\pm0.43$	\\
$V$	&	0.35	&	$0.640\pm0.014$	&	$0.659\pm0.008$	&	$0.40\pm0.09$	\\
$R$	&	0.94	&	$0.621\pm0.022$	&	$0.656\pm0.012$	&	$0.12\pm0.10$	\\
$I$	&	0.48	&	$0.667\pm0.039$	&	$0.663\pm0.022$	&	$-0.10\pm0.34$	\\ 
\hline
\end{tabular}
\end{table}