\begin{table}%t3
 %\centering
\par
 \caption{\label{sersic}Parameters from Sersic profiles.} 
\begin{tabular}{lccc}
\hline
\hline
\noalign{\smallskip}
Galaxy&$r_{\rm h}$\tablefootmark{a}&$r_{\rm h,red}$\tablefootmark{b}&$n$\\
\hline
\object{KKs57}&$17.5\pm0.8$&$14.2\pm0.6$&$0.97\pm0.14$\\
\object{KKs55}&$45.3\pm0.6$&$43.9\pm0.6$&$0.79\pm0.04$\\
\object{CenN}&$23.3\pm0.6$&$22.5\pm0.5$&$0.73\pm0.05$\\
\object{KK189}&$16.8\pm0.5$&$14.9\pm0.4$&$0.88\pm0.06$\\
\object{KK197}&$68.1\pm1.5$&$47.2\pm1.0$&$0.60\pm0.05$\\
\object{ESO269-66, KK190}&$49.6\pm0.6$&$43.6\pm0.5$&$0.76\pm0.04$\\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Computed from surface brightness as a function of elliptical radius.}
\tablefoottext{b}{Computed from surface brightness as a function of ``reduced'' radius $r_{\rm red}=\sqrt {ab}$ (see text for details).}}
\end{table}