Table 2: Model star cluster structural parameters for different photometric depths.
  RDP   MDP   SBP (J band)
$\Delta_{TO}$ $R_{\rm c}$ $R_{\rm hSC}$ $R_{\rm t}$   $R_{\rm c}$ $R_{\rm hM}$ $R_{\rm t}$   $R_{\rm c}$ $R_{\rm hL}$ $R_{\rm t}$
(mag) (au) (au) (au)   (au) (au) (au)   (au) (au) (au)
(1) (2) (3) (4)   (5) (6) (7)   (8) (9) (10)
  Model: GC-A; Input RDP parameters: $\mbox{$R_{\rm c}$ }=1.0$, $\mbox{$R_{\rm t}$ }=5.0$
-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 $1.00\pm(\dag )$ $1.19\pm(\dag )$ $5.00\pm0.01$   $0.92\pm(\dag )$ $1.14\pm(\dag )$ $4.91\pm(\dag )$   $0.75\pm0.01$ $1.03\pm(\dag )$ $4.80\pm0.01$
  Model: GC-B; Input RDP parameters: $\mbox{$R_{\rm c}$ }=1.0$, $\mbox{$R_{\rm t}$ }=20.0$
-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 $1.00\pm(\dag )$ $2.39\pm(\dag )$ $20.00\pm(\dag )$   $0.95\pm(\dag )$ $2.27\pm(\dag )$ $19.28\pm0.03$   $0.86\pm0.01$ $2.05\pm(\dag )$ $17.80\pm0.02$
  Model: GC-C; Input RDP parameters: $\mbox{$R_{\rm c}$ }=1.0$, $\mbox{$R_{\rm t}$ }=20.0$
-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 $1.00\pm(\dag )$ $2.39\pm(\dag )$ $20.00\pm(\dag )$   $1.00\pm(\dag )$ $2.39\pm(\dag )$ $20.00\pm(\dag )$   $1.00\pm(\dag )$ $2.39\pm(\dag )$ $19.97\pm0.03$
  Model: GC-D; Input RDP parameters: $\mbox{$R_{\rm c}$ }=1.0$, $\mbox{$R_{\rm t}$ }=40.0$
-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 $1.00\pm(\dag )$ $3.30\pm(\dag )$ $39.99\pm0.01$   $0.96\pm(\dag )$ $3.14\pm(\dag )$ $38.51\pm0.07$   $0.91\pm0.01$ $2.82\pm(\dag )$ $34.20\pm0.04$
  Model: OC-A; Input RDP parameters: $\mbox{$R_{\rm c}$ }=1.0$, $\mbox{$R_{\rm t}$ }=15.0$
-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 $1.00\pm(\dag )$ $2.08\pm(\dag )$ $15.00\pm0.01$   $0.91\pm(\dag )$ $1.93\pm(\dag )$ $14.43\pm0.03$   $0.81\pm0.01$ $1.73\pm(\dag )$ $13.20\pm0.01$
  Model: OC-B; Input RDP parameters: $\mbox{$R_{\rm c}$ }=1.0$, $\mbox{$R_{\rm t}$ }=15.0$
-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 $1.00\pm(\dag )$ $2.08\pm(\dag )$ $15.00\pm(\dag )$   $0.84\pm0.01$ $1.84\pm(\dag )$ $14.33\pm0.04$   $0.74\pm0.02$ $1.63\pm(\dag )$ $12.75\pm0.02$
  Model: OC-C; Input RDP parameters: $\mbox{$R_{\rm c}$ }=1.0$, $\mbox{$R_{\rm t}$ }=15.0$
-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 $1.00\pm(\dag )$ $2.08\pm(\dag )$ $15.00\pm(\dag )$   $0.70\pm0.02$ $1.70\pm(\dag )$ $14.35\pm0.05$   $0.64\pm0.03$ $1.49\pm(\dag )$ $12.00\pm0.02$
Notes. ($\dag $): uncertainty smaller than 0.01 arbitrary units (au). The half-type radii are half-star counts ( $R_{\rm hSC}$),
half-mass ( $R_{\rm hM}$) and half-light ( $R_{\rm hL}$).

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