Table 2: Structural parameters derived from 2MASS data.
      RDP   SBP
GC $1\hbox{$^\prime$ }$   $R_{\rm c}$ $R_{\rm hSC}$ $R_{\rm t}$ c   $R_{\rm c}$ $R_{\rm hL}$ $R_{\rm t}$ c
  (pc)   ($^\prime$) ($^\prime$) ($^\prime$)     ($^\prime$) ($^\prime$) ($^\prime$)  
(1) (2)   (3) (4) (5) (6)   (7) (8) (9) (10)
IC 1257 7.3   $0.2\pm0.1$ $1.4\pm0.3$ $7.1\pm2.0$ $1.5\pm0.2$   $0.3\pm0.1$ $1.4\pm0.2$ $10.7\pm2.8$ $1.6\pm0.2$
Lyngä 7 2.1   $0.9\pm0.2$ $1.2\pm0.1$ $8.4\pm1.2$ $1.0\pm0.1$   $0.9\pm0.3$ $1.2\pm0.3$ $7.7\pm1.4$ $0.9\pm0.2$
Tz 4 2.6   $0.8\pm0.4$ $1.9\pm0.2$ $6.2\pm1.4$ $0.9\pm0.2$   $1.0\pm0.4$ $1.8\pm0.2$ $7.6\pm1.3$ $0.9\pm0.2$
Tz 10 1.7   $1.0\pm0.3$ $1.6\pm0.2$ $5.9\pm2.0$ $0.8\pm0.2$   $0.8\pm0.4$ $1.5\pm0.2$ $3.4\pm0.8$ $0.7\pm0.3$
BH 176 4.5   $0.9\pm0.2$ $1.0\pm0.1$ $7.6\pm1.1$ $0.9\pm0.1$   $0.9\pm0.2$ $0.8\pm0.1$ $5.9\pm0.5$ $0.8\pm0.1$
ESO 452-SC11 2.3   $0.5\pm0.2$ $0.5\pm0.2$ $5.4\pm1.8$ $1.0\pm0.2$   $0.5\pm0.2$ $0.5\pm0.2$ $4.8\pm1.2$ $1.0\pm0.2$
ESO 280-SC06 6.3   $0.7\pm0.2$ $1.1\pm0.2$ $5.3\pm0.9$ $0.9\pm0.1$   $0.5\pm0.2$ $1.0\pm0.2$ $5.0\pm1.1$ $0.9\pm0.2$
2MASS-GC01 0.9   $1.0\pm0.2$ $1.7\pm0.2$ $7.5\pm1.3$ $0.9\pm0.1$   $0.7\pm0.2$ $1.6\pm0.2$ $4.4\pm0.4$ $0.8\pm0.2$
2MASS-GC02 1.1   $0.6\pm0.1$ $0.6\pm0.2$ $4.8\pm0.6$ $0.9\pm0.1$   $0.4\pm0.1$ $0.5\pm0.2$ $3.7\pm0.4$ $1.0\pm0.1$
GLIMPSE-C01 1.1   $0.4\pm0.1$ $0.8\pm0.1$ $8.0\pm1.0$ $1.3\pm0.1$   $0.4\pm0.1$ $0.5\pm0.1$ $4.5\pm0.5$ $1.1\pm0.1$
AL 3 1.7   $0.4\pm0.3$ $0.5\pm0.2$ $4.1\pm0.5$ $1.0\pm0.3$   $(\dag )$ $0.6\pm0.2$ $(\dag )$ $(\dag )$
Notes. Column 2: arcmin to parsec scale. Columns 4 and 8: half-star count and half-light radii, respectively. Columns 6 and 10: concentration parameter, $c=\log(\mbox{$R_{\rm t}$ }/\mbox{$R_{\rm c}$ })$. $(\dag )$: the SBP of AL 3 could not be fitted because of exceeding noise, especially beyond $R=1\hbox{$^\prime$ }$.

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