\begin{table}%t2
\caption{Model star cluster structural parameters for different photometric depths.}
\label{tab2}
\small%\centerline
{\begin{tabular}{cccccccccccc}
\hline\hline
&\multicolumn{3}{c}{RDP}&&\multicolumn{3}{c}{MDP}&&\multicolumn{3}{c}{SBP (\jj\ band)}\\
\cline{2-4}\cline{6-8}\cline{10-12}
$\Delta_{TO}$&\rc&\rhSC&\rt&&\rc&\rhM&\rt&&\rc&\rhL&\rt\\
(mag)&(au)&(au)&(au)&&(au)&(au)&(au)&&(au)&(au)&(au)\\
(1)  &(2) &(3) &(4) &&(5) &(6) &(7) &&(8) &(9) &(10) \\
\hline
&\multicolumn{11}{c}{Model: GC-A; Input RDP parameters:  $\rc=1.0$, $\rt=5.0$}\\
\cline{2-12}
$-5.0$&$0.78\pm(\dag)$&$1.02\pm(\dag)$&$4.61\pm0.01$&&$0.78\pm(\dag)$&$1.02\pm(\dag)$&$4.61\pm0.01$&&$0.75\pm0.01$&$1.01\pm(\dag)$&$4.80\pm0.01$\\
$~0.0$&$0.76\pm(\dag)$&$1.02\pm(\dag)$&$4.77\pm0.01$&&$0.76\pm(\dag)$&$1.02\pm(\dag)$&$4.77\pm0.01$&&$0.75\pm0.01$&$1.01\pm(\dag)$&$4.79\pm0.01$\\
$+6.3$&$1.00\pm(\dag)$&$1.19\pm(\dag)$&$5.00\pm0.01$&&$0.92\pm(\dag)$&$1.14\pm(\dag)$&$4.91\pm(\dag)$&&$0.75\pm0.01$&$1.03\pm(\dag)$&$4.80\pm0.01$\\
\hline
&\multicolumn{11}{c}{Model: GC-B; Input RDP parameters:  $\rc=1.0$, $\rt=20.0$}\\
\cline{2-12}
$-5.0$&$0.87\pm0.01$&$2.03\pm(\dag)$&$17.31\pm0.08$&&$0.87\pm0.01$&$2.03\pm(\dag)$&$17.31\pm0.08$&&$0.86\pm0.01$&$2.04\pm0.01$&$17.82\pm0.05$\\
$~0.0$&$0.83\pm0.01$&$2.03\pm(\dag)$&$18.72\pm0.08$&&$0.83\pm0.01$&$2.03\pm(\dag)$&$18.72\pm0.08$&&$0.86\pm0.01$&$2.03\pm(\dag)$&$17.80\pm0.03$\\
$+6.3$&$1.00\pm(\dag)$&$2.39\pm(\dag)$&$20.00\pm(\dag)$&&$0.95\pm(\dag)$&$2.27\pm(\dag)$&$19.28\pm0.03$&&$0.86\pm0.01$&$2.05\pm(\dag)$&$17.80\pm0.02$\\
\hline
&\multicolumn{11}{c}{Model: GC-C; Input RDP parameters:  $\rc=1.0$, $\rt=20.0$}\\
\cline{2-12}
$-5.0$&$1.00\pm(\dag)$&$2.38\pm0.01$&$20.02\pm0.03$&&$1.00\pm(\dag)$&$2.38\pm0.01$&$20.02\pm0.04$&&$1.00\pm(\dag)$&$2.38\pm0.01$&$19.94\pm0.06$\\
$~0.0$&$1.00\pm(\dag)$&$2.39\pm(\dag)$&$20.00\pm0.01$&&$1.00\pm(\dag)$&$2.39\pm(\dag)$&$20.00\pm0.01$&&$1.00\pm(\dag)$&$2.39\pm(\dag)$&$19.95\pm0.03$\\
$+6.3$&$1.00\pm(\dag)$&$2.39\pm(\dag)$&$20.00\pm(\dag)$&&$1.00\pm(\dag)$&$2.39\pm(\dag)$&$20.00\pm(\dag)$&&$1.00\pm(\dag)$&$2.39\pm(\dag)$&$19.97\pm0.03$\\
\hline
&\multicolumn{11}{c}{Model: GC-D; Input RDP parameters:  $\rc=1.0$, $\rt=40.0$}\\
\cline{2-12}
$-5.0$&$0.90\pm0.01$&$2.81\pm0.02$&$33.96\pm0.19$&&$0.90\pm0.01$&$2.81\pm0.02$&$33.96\pm0.19$&&$0.91\pm0.01$&$2.82\pm(\dag)$&$34.18\pm0.05$\\
$~0.0$&$0.86\pm0.01$&$2.82\pm(\dag)$&$37.15\pm0.17$&&$0.86\pm0.01$&$2.82\pm(\dag)$&$37.15\pm0.17$&&$0.91\pm0.01$&$2.82\pm(\dag)$&$34.00\pm0.05$\\
$+6.3$&$1.00\pm(\dag)$&$3.30\pm(\dag)$&$39.99\pm0.01$&&$0.96\pm(\dag)$&$3.14\pm(\dag)$&$38.51\pm0.07$&&$0.91\pm0.01$&$2.82\pm(\dag)$&$34.20\pm0.04$\\
\hline
&\multicolumn{11}{c}{Model: OC-A; Input RDP parameters: $\rc=1.0$, $\rt=15.0$}\\
\cline{2-12}
$-3.0$&$0.82\pm0.01$&$1.70\pm(\dag)$&$12.85\pm0.07$&&$0.82\pm0.01$&$1.70\pm(\dag)$&$12.85\pm0.07$&&$0.81\pm0.01$&$1.72\pm(\dag)$&$13.18\pm0.02$\\
$~0.0$&$0.78\pm0.01$&$1.72\pm(\dag)$&$13.78\pm0.06$&&$0.78\pm0.01$&$1.72\pm(\dag)$&$13.78\pm0.06$&&$0.82\pm0.01$&$1.72\pm(\dag)$&$13.19\pm0.02$\\
$+8.9$&$1.00\pm(\dag)$&$2.08\pm(\dag)$&$15.00\pm0.01$&&$0.91\pm(\dag)$&$1.93\pm(\dag)$&$14.43\pm0.03$&&$0.81\pm0.01$&$1.73\pm(\dag)$&$13.20\pm0.01$\\
\hline
&\multicolumn{11}{c}{Model: OC-B; Input RDP parameters:  $\rc=1.0$, $\rt=15.0$}\\
\cline{2-12}
$-3.0$&$0.72\pm0.01$&$1.61\pm(\dag)$&$13.30\pm0.08$&&$0.72\pm0.01$&$1.61\pm(\dag)$&$13.30\pm0.08$&&$0.76\pm0.01$&$1.61\pm(\dag)$&$12.75\pm0.03$\\
$~0.0$&$0.70\pm0.02$&$1.61\pm(\dag)$&$13.67\pm0.08$&&$0.70\pm0.02$&$1.61\pm(\dag)$&$13.67\pm0.08$&&$0.77\pm0.01$&$1.61\pm(\dag)$&$12.74\pm0.03$\\
$+11.0$&$1.00\pm(\dag)$&$2.08\pm(\dag)$&$15.00\pm(\dag)$&&$0.84\pm0.01$&$1.84\pm(\dag)$&$14.33\pm0.04$&&$0.74\pm0.02$&$1.63\pm(\dag)$&$12.75\pm0.02$\\
\hline
&\multicolumn{11}{c}{Model: OC-C; Input RDP parameters:  $\rc=1.0$, $\rt=15.0$}\\
\cline{2-12}
$-4.0$&$0.62\pm0.02$&$1.49\pm(\dag)$&$13.06\pm0.10$&&$0.62\pm0.02$&$1.49\pm(\dag)$&$13.05\pm0.10$&&$0.71\pm0.01$&$1.49\pm(\dag)$&$11.99\pm0.03$\\
$~0.0$&$0.62\pm0.02$&$1.49\pm(\dag)$&$13.10\pm0.10$&&$0.62\pm0.02$&$1.49\pm(\dag)$&$13.09\pm0.10$&&$0.71\pm0.01$&$1.49\pm(\dag)$&$11.99\pm0.03$\\
$+14.0$&$1.00\pm(\dag)$&$2.08\pm(\dag)$&$15.00\pm(\dag)$&&$0.70\pm0.02$&$1.70\pm(\dag)$&$14.35\pm0.05$&&$0.64\pm0.03$&$1.49\pm(\dag)$&$12.00\pm0.02$\\
\hline
\end{tabular}}\medskip
 {Notes.}
 ($\dag$): uncertainty smaller than 0.01 arbitrary units (au). The half-type radii are half-star 
counts (\rhSC), half-mass (\rhM) and half-light~(\rhL).
 \end{table}