\begin{table}%t2
%%\centering
\par
\caption {\label{tab2}Structural parameters derived from the RDPs.}
\renewcommand{\tabcolsep}{4.85mm}
\par
\begin{tabular}{ccccccccc}
\hline\hline
\noalign{\smallskip}
Cluster&$\sigma_0$&\rc&\rl&$1\arcmin$&$\sigma_0$&\rc&\rl\\
       &$\rm(*~\arcmin^{-2})$&(\arcmin)&(\arcmin) &(pc)&$\rm(*~pc^{-2})$&(pc)&(pc)\\
(1)&(2)&(3)&(4)&(5)&(6)&(7)&(8)\\
\hline
\multicolumn{8}{c}{Quality 1}\\
\hline
Teu~7  &$46.5\pm14.9$&$0.45\pm0.10$&$4.0\pm0.5$&2.051&$11.1\pm3.5$&$0.92\pm0.20$&$8.2\pm1.0$\\
Teu~11 &$50.5\pm23.5$&$0.20\pm0.06$&$2.0\pm0.4$&1.449&$24.1\pm11.2$&$0.29\pm0.09$&$2.9\pm0.6$\\
Teu~12 &$73.7\pm39.0$&$0.16\pm0.05$&$3.3\pm0.5$&2.582&$11.0\pm5.8$&$0.41\pm0.13$&$8.5\pm0.8$\\
Teu~13 &$45.3\pm30.4$&$0.15\pm0.06$&$3.0\pm0.5$&0.806&$69.7\pm46.8$&$0.12\pm0.04$&$2.4\pm0.4$\\
Teu~14a&$29.1\pm16.4$&$0.29\pm0.10$&$3.5\pm0.5$&0.498&$117\pm66$&$0.14\pm0.05$&$1.7\pm0.3$\\
Teu~23 &$16.8\pm7.3$&$0.53\pm0.17$&$4.0\pm0.5$&0.848&$27.9\pm18.1$&$0.41\pm0.13$&$3.1\pm0.4$\\
Teu~27 &$63.4\pm47.9$&$0.20\pm0.15$&$1.8\pm0.5$&0.719&$123\pm93$&$0.14\pm0.09$&$1.3\pm0.4$\\
Teu~40 &$69.1\pm29.7$&$0.19\pm0.05$&$2.5\pm0.5$&0.865&$92.4\pm39.7$&$0.16\pm0.04$&$2.2\pm0.4$\\
Teu~48 &$47.4\pm31.1$&$0.27\pm0.12$&$2.5\pm0.5$&2.292&$9.0\pm5.9$&$0.62\pm0.27$&$5.7\pm1.2$\\
Teu~49 &$22.4\pm5.8$&$0.67\pm0.12$&$4.2\pm0.5$&1.113&$18.1\pm4.7$&$0.74\pm0.14$&$4.7\pm0.6$\\
Teu~52 &$134\pm45$&$0.13\pm0.02$&$2.4\pm0.3$&0.939&$152\pm51$&$0.12\pm0.02$&$2.2\pm0.3$\\
Teu~54 &$11.3\pm7.5$&$0.61\pm0.31$&$4.0\pm0.5$&0.838&$16.1\pm10.6$&$0.51\pm0.26$&$3.4\pm0.4$\\
Teu~55 &$26.6\pm20.4$&$0.37\pm0.21$&$4.0\pm0.5$&1.744&$8.7\pm6.7$&$0.64\pm0.37$&$7.0\pm0.9$\\
Teu~64 &$67.0\pm30.0$&$0.21\pm0.06$&$2.3\pm0.3$&0.865&$90.1\pm40.2$&$0.18\pm0.05$&$2.0\pm0.3$\\
Teu~66 &$53.2\pm16.2$&$0.21\pm0.04$&$1.8\pm0.4$&1.598&$20.8\pm6.3$&$0.33\pm0.06$&$2.9\pm0.6$\\
Teu~76 &$41.2\pm23.1$&$0.18\pm0.07$&$1.5\pm0.2$&1.205&$28.4\pm15.9$&$0.22\pm0.08$&$1.8\pm0.2$\\
Teu~79 &$89.2\pm33.6$&$0.21\pm0.05$&$2.2\pm0.3$&0.364&$674\pm253$&$0.08\pm0.02$&$0.8\pm0.1$\\
Teu~126&$23.5\pm12.9$&$0.45\pm0.15$&$4.5\pm0.5$&0.506&$91.8\pm50.7$&$0.23\pm0.07$&$2.3\pm0.3$\\
Teu~132&$10.6\pm4.5$&$0.67\pm0.21$&$2.5\pm0.5$&1.558&$4.4\pm1.8$&$1.05\pm0.31$&$3.9\pm0.8$\\
Teu~144&$16.0\pm7.4$&$0.54\pm0.18$&$4.2\pm0.3$&0.662&$36.5\pm16.9$&$0.36\pm0.12$&$2.8\pm0.2$\\
\hline
\multicolumn{8}{c}{Quality 2}\\
Teu~2  &$34.3\pm15.9$&$0.32\pm0.10$&$2.8\pm0.4$&1.046&$31.3\pm14.5$&$0.33\pm0.10$&$2.9\pm0.4$\\
Teu~28 &$20.4\pm11.8$&$0.38\pm0.16$&$2.2\pm0.3$&0.899&$25.2\pm14.6$&$0.34\pm0.14$&$2.0\pm0.3$\\
Teu~31 &$278\pm37$&$0.09\pm0.01$&$0.9\pm0.2$&0.943&$312\pm42$&$0.08\pm0.01$&$0.8\pm0.2$\\
Teu~43 &$79.8\pm18.4$&$0.14\pm0.02$&$1.3\pm0.3$&0.610&$215\pm50$&$0.09\pm0.02$&$0.8\pm0.2$\\
Teu~44 &--&--&$2.0\pm0.5$&2.148&--&--&$4.3\pm1.1$\\
Teu~45 &--&--&$2.0\pm0.5$&1.962&--&--&$3.9\pm1.0$\\
Teu~50 &$59.7\pm27.7$&$0.18\pm0.05$&$2.2\pm0.3$&0.940&$67.5\pm31.3$&$0.17\pm0.05$&$2.1\pm0.3$\\
Teu~77 &--&--&$3.5\pm0.8$&0.422&--&--&$1.5\pm0.4$\\
Teu~85 &--&--&$2.0\pm0.5$&0.366&--&--&$0.7\pm0.2$\\
Teu~106&$36.4\pm27.8$&$0.32\pm0.18$&$1.6\pm0.3$&1.931&$9.7\pm7.4$&$0.59\pm0.31$&$3.1\pm0.6$\\
Teu~124&$62.6\pm25.6$&$0.19\pm0.05$&$2.0\pm0.2$&0.244&$1050\pm430$&$0.05\pm0.01$&$0.5\pm0.1$\\
\hline
\multicolumn{8}{c}{Quality 3}\\
Teu~39 &--&--&$17.0\pm5.0$&0.234&--&--&$4.0\pm1.2$\\
Teu~53 &--&--&$2.5\pm0.5$&--&--&--&--\\
Teu~162&--&--&$4.5\pm0.5$&0.594&--&--&$2.6\pm0.3$\\
\hline
\end{tabular}
\tablefoot {
Column~5: arcmin to parsec scale. For comparison with other clusters, the King-like 
central stellar density ($\sigma_0$), core radius (\rc), and cluster radius (\rl) are 
given both in angular and absolute units. 
}
\end{table}