\begin{table}%t1
\caption{Adopted photometric quantities.\label{MeasuredPhotQTable}}
\begin{tabular}{llllll}
\hline\hline
ID & $m$ & $E(B - V)$ & ${M - m}_0$ & $\log {r_{\rm e}}$ & $^a$\\
\hline
ARP 2 & $12.74 \pm 0.03$ & $0.11 \pm 0.011$ & $17.37 \pm 0.18$ & $2.1 \pm 0.02$ & $2.85$ \\
FORNAX 1 & $15.44 \pm 0.08$ & $0.071 \pm 0.007$ & $20.68 \pm 0.22$ & $1.24 \pm 0.06$ & $5.15$ \\
FORNAX 2 & $13.64 \pm 0.06$ & $0.054 \pm 0.005$ & $20.68 \pm 0.22$ & $1.07 \pm 0.05$ & $3.31$ \\
FORNAX 3 & $12.73 \pm 0.09$ & $0.035 \pm 0.004$ & $20.68 \pm 0.21$ & $0.85 \pm 0.11$ & $7.49$ \\
FORNAX 4 & $13.56 \pm 0.13$ & $0.14 \pm 0.014$ & $20.68 \pm 0.24$ & $0.78 \pm 0.15$ & $3.01$ \\
FORNAX 5 & $13.52 \pm 0.08$ & $0.031 \pm 0.003$ & $20.68 \pm 0.21$ & $0.83 \pm 0.09$ & $3.78$ \\
IC 4499 & $9.91 \pm 0.02$ & $0.175 \pm 0.013$ & $16.53 \pm 0.1$ & $2.04 \pm 0.02$ & $4.17$ \\
LMC-HODGE 11 & $11.24 \pm 0.06$ & $0.046 \pm 0.005$ & $18.5 \pm 0.21$ & $1.49 \pm 0.05$ & $3.81$ \\
LMC-HODGE 14 & $12.88 \pm 0.14$ & $0.105 \pm 0.01$ & $18.5 \pm 0.23$ & $1.38 \pm 0.16$ & $3.34$ \\
LMC-NGC 1466 & $11.18 \pm 0.04$ & $0.09 \pm 0.009$ & $18.43 \pm 0.1$ & $1.3 \pm 0.03$ & $3.28$ \\
LMC-NGC 1711 & $9.57 \pm 0.06$ & $0.002 \pm 0.001$ & $18.5 \pm 0.2$ & $1.36 \pm 0.07$ & $3.25$ \\
LMC-NGC 1754 & $11.47 \pm 0.07$ & $0.096 \pm 0.01$ & $18.5 \pm 0.23$ & $1.19 \pm 0.09$ & $2.71$ \\
LMC-NGC 1777 & $11.44 \pm 0.06$ & $0 \pm 0.001$ & $18.5 \pm 0.2$ & $1.53 \pm 0.05$ & $3.26$ \\
LMC-NGC 1786 & $10.48 \pm 0.06$ & $0.125 \pm 0.012$ & $18.5 \pm 0.24$ & $1.26 \pm 0.07$ & $2.15$ \\
LMC-NGC 1805 & $10.29 \pm 0.07$ & $0.144 \pm 0.014$ & $18.5 \pm 0.24$ & $1.2 \pm 0.08$ & $2.6$ \\
LMC-NGC 1818 & $9.25 \pm 0.07$ & $0.15 \pm 0.015$ & $18.5 \pm 0.25$ & $1.38 \pm 0.08$ & $2.77$ \\
LMC-NGC 1831 & $10.4 \pm 0.05$ & $0.104 \pm 0.01$ & $18.5 \pm 0.23$ & $1.52 \pm 0.04$ & $2.84$ \\
LMC-NGC 1835 & $9.94 \pm 0.04$ & $0.105 \pm 0.01$ & $18.5 \pm 0.23$ & $1.02 \pm 0.04$ & $2.47$ \\
LMC-NGC 1847 & $10.01 \pm 0.13$ & $0.165 \pm 0.016$ & $18.5 \pm 0.25$ & $1.73 \pm 0.13$ & $3.07$ \\
LMC-NGC 1850 & $8.42 \pm 0.1$ & $0.102 \pm 0.01$ & $18.5 \pm 0.23$ & $1.59 \pm 0.11$ & $4.23$ \\
LMC-NGC 1856 & $9.28 \pm 0.1$ & $0.228 \pm 0.023$ & $18.5 \pm 0.27$ & $1.5 \pm 0.11$ & $3.16$ \\
LMC-NGC 1868 & $11.23 \pm 0.05$ & $0.132 \pm 0.013$ & $18.5 \pm 0.24$ & $1.18 \pm 0.05$ & $2.48$ \\
LMC-NGC 1898 & $10.91 \pm 0.07$ & $0.083 \pm 0.008$ & $18.5 \pm 0.23$ & $1.44 \pm 0.09$ & $4.36$ \\
LMC-NGC 1916 & $10.17 \pm 0.04$ & $0.188 \pm 0.019$ & $18.5 \pm 0.26$ & $0.97 \pm 0.04$ & $4.26$ \\
LMC-NGC 2004 & $9.15 \pm 0.09$ & $0.117 \pm 0.012$ & $18.5 \pm 0.24$ & $1.33 \pm 0.12$ & $3.84$ \\
LMC-NGC 2005 & $10.92 \pm 0.08$ & $0.12 \pm 0.012$ & $18.5 \pm 0.24$ & $1.07 \pm 0.09$ & $2.34$ \\
LMC-NGC 2011 & $9.76 \pm 0.14$ & $0.045 \pm 0.004$ & $18.5 \pm 0.21$ & $1.42 \pm 0.14$ & $4.08$ \\
LMC-NGC 2019 & $10.59 \pm 0.07$ & $0.138 \pm 0.014$ & $18.5 \pm 0.24$ & $1.09 \pm 0.1$ & $3.36$ \\
LMC-NGC 2031 & $10.05 \pm 0.08$ & $0.119 \pm 0.012$ & $18.5 \pm 0.24$ & $1.6 \pm 0.09$ & $3.38$ \\
LMC-NGC 2100 & $9.2 \pm 0.08$ & $0.208 \pm 0.021$ & $18.5 \pm 0.26$ & $1.31 \pm 0.11$ & $3.26$ \\
LMC-NGC 2121 & $11.02 \pm 0.12$ & $0.122 \pm 0.012$ & $18.5 \pm 0.24$ & $1.67 \pm 0.08$ & $4.32$ \\
LMC-NGC 2136 & $10.34 \pm 0.08$ & $0.189 \pm 0.019$ & $18.5 \pm 0.26$ & $1.17 \pm 0.07$ & $2.5$ \\
LMC-NGC 2153 & $13.11 \pm 0.3$ & $0.028 \pm 0.003$ & $18.5 \pm 0.21$ & $1.01 \pm 0.32$ & $11.96$ \\
LMC-NGC 2155 & $11.68 \pm 0.1$ & $0.079 \pm 0.008$ & $18.5 \pm 0.22$ & $1.63 \pm 0.09$ & $2.45$ \\
LMC-NGC 2157 & $9.56 \pm 0.06$ & $0.098 \pm 0.01$ & $18.5 \pm 0.23$ & $1.42 \pm 0.08$ & $2.67$ \\
LMC-NGC 2159 & $10.74 \pm 0.13$ & $0.188 \pm 0.019$ & $18.5 \pm 0.26$ & $1.5 \pm 0.19$ & $2.16$ \\
LMC-NGC 2162 & $12.32 \pm 0.11$ & $0.012 \pm 0.001$ & $18.5 \pm 0.2$ & $1.31 \pm 0.1$ & $5.38$ \\
LMC-NGC 2172 & $11.08 \pm 0.12$ & $0.092 \pm 0.009$ & $18.5 \pm 0.23$ & $1.52 \pm 0.15$ & $2.26$ \\
LMC-NGC 2173 & $11.53 \pm 0.09$ & $0.108 \pm 0.011$ & $18.5 \pm 0.23$ & $1.62 \pm 0.09$ & $2.65$ \\
LMC-NGC 2193 & $12.53 \pm 0.23$ & $0.044 \pm 0.004$ & $18.5 \pm 0.21$ & $1.39 \pm 0.24$ & $2.48$ \\
LMC-NGC 2210 & $10.75 \pm 0.05$ & $0.096 \pm 0.01$ & $18.5 \pm 0.23$ & $1.17 \pm 0.04$ & $3.61$ \\
LMC-NGC 2213 & $11.92 \pm 0.12$ & $0.021 \pm 0.002$ & $18.5 \pm 0.21$ & $1.34 \pm 0.13$ & $2.48$ \\
LMC-NGC 2214 & $10.05 \pm 0.09$ & $0.018 \pm 0.002$ & $18.5 \pm 0.21$ & $1.6 \pm 0.13$ & $2.63$ \\
LMC-NGC 2231 & $12.12 \pm 0.15$ & $0.106 \pm 0.011$ & $18.5 \pm 0.23$ & $1.48 \pm 0.12$ & $5.13$ \\
LMC-NGC 2249 & $11.9 \pm 0.15$ & $0.052 \pm 0.005$ & $18.5 \pm 0.22$ & $1.21 \pm 0.13$ & $3.55$ \\
LMC-NGC 2257 & $11.33 \pm 0.07$ & $0 \pm 0.001$ & $18.5 \pm 0.2$ & $1.7 \pm 0.04$ & $2.9$ \\
LMC-SL 842 & $13.42 \pm 0.22$ & $0.104 \pm 0.01$ & $18.5 \pm 0.23$ & $1.25 \pm 0.17$ & $6.15$ \\
NGC 104 & $4 \pm 0.01$ & $0.04 \pm 0.003$ & $13.29 \pm 0.06$ & $2.23 \pm 0.02$ & $4.48$ \\
NGC 1261 & $8.62 \pm 0.02$ & $0.012 \pm 0.001$ & $16.01 \pm 0.05$ & $1.62 \pm 0.02$ & $3.46$ \\
NGC 1851 & $7.24 \pm 0.04$ & $0.02 \pm 0.001$ & $15.42 \pm 0.05$ & $1.51 \pm 0.05$ & $2.42$ \\
NGC 1904 & $8.08 \pm 0.02$ & $0.01 \pm 0.001$ & $15.64 \pm 0.05$ & $1.62 \pm 0.02$ & $2.88$ \\
NGC 2808 & $6.38 \pm 0.01$ & $0.164 \pm 0.012$ & $15.09 \pm 0.1$ & $1.65 \pm 0.01$ & $3.22$ \\
NGC 288 & $8.21 \pm 0.02$ & $0.03 \pm 0.003$ & $14.67 \pm 0.11$ & $2.13 \pm 0.01$ & $6.07$ \\
NGC 3201 & $7.07 \pm 0.02$ & $0.227 \pm 0.016$ & $13.5 \pm 0.1$ & $2.18 \pm 0.01$ & $3.8$ \\
NGC 362 & $6.59 \pm 0.02$ & $0.004 \pm 0.001$ & $14.72 \pm 0.07$ & $1.62 \pm 0.03$ & $2.99$ \\
NGC 4147 & $10.29 \pm 0.02$ & $0.012 \pm 0.001$ & $16.4 \pm 0.07$ & $1.45 \pm 0.02$ & $3.36$ \\
NGC 4590 & $8.29 \pm 0.01$ & $0.044 \pm 0.003$ & $15.12 \pm 0.05$ & $1.93 \pm 0.01$ & $3$ \\
NGC 5024 & $7.69 \pm 0.01$ & $0.01 \pm 0.001$ & $16.35 \pm 0.08$ & $1.84 \pm 0.01$ & $3.91$ \\
NGC 5053 & $9.66 \pm 0.04$ & $0.03 \pm 0.003$ & $16.17 \pm 0.08$ & $2.21 \pm 0.02$ & $4.53$ \\
NGC 5272 & $6.53 \pm 0.02$ & $0.01 \pm 0.001$ & $14.99 \pm 0.05$ & $1.85 \pm 0.02$ & $3.92$ \\
NGC 5286 & $7.2 \pm 0.01$ & $0.24 \pm 0.024$ & $15.25 \pm 0.17$ & $1.72 \pm 0.02$ & $2.75$ \\
NGC 5466 & $9.48 \pm 0.02$ & $0 \pm 0.001$ & $16.12 \pm 0.1$ & $2.12 \pm 0.01$ & $3.73$ \\
NGC 5634 & $9.93 \pm 0.02$ & $0.01 \pm 0.001$ & $17.17 \pm 0.09$ & $1.61 \pm 0.02$ & $2.8$ \\
NGC 5694 & $10.12 \pm 0.01$ & $0.101 \pm 0.007$ & $17.77 \pm 0.09$ & $1.38 \pm 0.02$ & $2.58$ \\
NGC 5824 & $8.84 \pm 0.01$ & $0.128 \pm 0.009$ & $17.6 \pm 0.08$ & $1.44 \pm 0.01$ & $2.68$ \\
NGC 5897 & $8.67 \pm 0.02$ & $0.08 \pm 0.008$ & $15.61 \pm 0.09$ & $2.11 \pm 0.01$ & $3.9$ \\
NGC 5904 & $5.86 \pm 0.01$ & $0.03 \pm 0.002$ & $14.37 \pm 0.05$ & $2.04 \pm 0.01$ & $4.29$ \\
NGC 5986 & $7.81 \pm 0.01$ & $0.27 \pm 0.027$ & $15.39 \pm 0.16$ & $1.73 \pm 0.01$ & $3.63$ \\
NGC 6093 & $7.45 \pm 0.01$ & $0.196 \pm 0.014$ & $15.05 \pm 0.09$ & $1.59 \pm 0.01$ & $3.35$ \\
NGC 6121 & $5.67 \pm 0.01$ & $0.36 \pm 0.036$ & $11.62 \pm 0.21$ & $2.48 \pm 0.01$ & $2.89$ \\
NGC 6139 & $8.86 \pm 0.02$ & $0.72 \pm 0.072$ & $15.45 \pm 0.3$ & $1.87 \pm 0.02$ & $2.23$ \\
NGC 6171 & $8.28 \pm 0.01$ & $0.38 \pm 0.027$ & $13.81 \pm 0.15$ & $2.1 \pm 0.01$ & $2.43$ \\
NGC 6205 & $5.89 \pm 0.01$ & $0.012 \pm 0.001$ & $14.46 \pm 0.07$ & $1.99 \pm 0.01$ & $5.52$ \\
NGC 6218 & $7.17 \pm 0.01$ & $0.189 \pm 0.013$ & $13.58 \pm 0.16$ & $2.04 \pm 0.01$ & $4.23$ \\
NGC 6229 & $9.56 \pm 0.01$ & $0.012 \pm 0.001$ & $17.42 \pm 0.05$ & $1.35 \pm 0.01$ & $3.71$ \\
NGC 6254 & $6.66 \pm 0.01$ & $0.28 \pm 0.028$ & $13.35 \pm 0.19$ & $2.04 \pm 0.01$ & $4.05$ \\
NGC 6256 & $11.24 \pm 0.02$ & $1.18 \pm 0.118$ & $14 \pm 0.43$ & $1.68 \pm 0.01$ & $3.41$ \\
NGC 6266 & $6.46 \pm 0.02$ & $0.5 \pm 0.035$ & $14.15 \pm 0.2$ & $1.81 \pm 0.03$ & $2.79$ \\
NGC 6273 & $6.74 \pm 0.01$ & $0.34 \pm 0.034$ & $15.05 \pm 0.18$ & $1.96 \pm 0.01$ & $2.55$ \\
NGC 6284 & $8.7 \pm 0.02$ & $0.29 \pm 0.029$ & $16.06 \pm 0.16$ & $1.7 \pm 0.01$ & $2.48$ \\
NGC 6287 & $9.46 \pm 0.01$ & $0.66 \pm 0.066$ & $14.79 \pm 0.27$ & $1.71 \pm 0.01$ & $2.64$ \\
NGC 6293 & $7.97 \pm 0.02$ & $0.62 \pm 0.062$ & $14.22 \pm 0.26$ & $1.92 \pm 0.02$ & $2.16$ \\
NGC 6316 & $9.02 \pm 0.02$ & $0.51 \pm 0.051$ & $15.59 \pm 0.25$ & $1.74 \pm 0.02$ & $2.5$ \\
NGC 6325 & $10.49 \pm 0.01$ & $1.03 \pm 0.103$ & $14.42 \pm 0.39$ & $1.74 \pm 0.01$ & $2.3$ \\
NGC 6333 & $7.75 \pm 0.01$ & $0.36 \pm 0.036$ & $14.62 \pm 0.26$ & $1.77 \pm 0.01$ & $3.01$ \\
NGC 6341 & $6.56 \pm 0.01$ & $0.02 \pm 0.002$ & $14.74 \pm 0.11$ & $1.75 \pm 0.01$ & $4.45$ \\
NGC 6342 & $9.78 \pm 0.02$ & $0.46 \pm 0.046$ & $14.95 \pm 0.22$ & $1.65 \pm 0.02$ & $3.15$ \\
NGC 6356 & $8.13 \pm 0.01$ & $0.28 \pm 0.028$ & $16 \pm 0.17$ & $1.79 \pm 0.01$ & $2.37$ \\
NGC 6362 & $7.54 \pm 0.01$ & $0.08 \pm 0.008$ & $14.48 \pm 0.11$ & $2.16 \pm 0.01$ & $2.37$ \\
NGC 6366 & $8.68 \pm 0.01$ & $0.69 \pm 0.069$ & $12.88 \pm 0.31$ & $2.28 \pm 0.01$ & $3.53$ \\
NGC 6388 & $6.87 \pm 0.01$ & $0.37 \pm 0.037$ & $15.42 \pm 0.2$ & $1.51 \pm 0.01$ & $3.49$ \\
NGC 6397 & $5.95 \pm 0.01$ & $0.18 \pm 0.018$ & $11.89 \pm 0.16$ & $2.24 \pm 0.02$ & $3.14$ \\
NGC 6401 & $9.57 \pm 0.02$ & $0.91 \pm 0.091$ & $14.55 \pm 0.41$ & $1.84 \pm 0.02$ & $2.67$ \\
NGC 6402 & $7.73 \pm 0.01$ & $0.66 \pm 0.066$ & $14.91 \pm 0.28$ & $1.91 \pm 0.01$ & $3.65$ \\
NGC 6440 & $9.43 \pm 0.01$ & $1.09 \pm 0.077$ & $14.69 \pm 0.32$ & $1.51 \pm 0.01$ & $2.59$ \\
NGC 6441 & $7.19 \pm 0.03$ & $0.47 \pm 0.047$ & $15.77 \pm 0.23$ & $1.61 \pm 0.04$ & $2.4$ \\
NGC 6517 & $10.54 \pm 0.01$ & $1.23 \pm 0.123$ & $15.04 \pm 0.45$ & $1.58 \pm 0.01$ & $2.56$ \\
NGC 6522 & $8.46 \pm 0.03$ & $0.54 \pm 0.054$ & $14.66 \pm 0.25$ & $1.63 \pm 0.03$ & $8.3$ \\
NGC 6528 & $9.59 \pm 0.06$ & $0.62 \pm 0.062$ & $14.35 \pm 0.39$ & $1.43 \pm 0.05$ & $2.54$ \\
NGC 6539 & $9.64 \pm 0.03$ & $0.97 \pm 0.097$ & $14.9 \pm 0.37$ & $2.06 \pm 0.04$ & $2.39$ \\
NGC 6553 & $8.03 \pm 0.01$ & $0.84 \pm 0.084$ & $13.44 \pm 0.46$ & $1.88 \pm 0.01$ & $2.72$ \\
NGC 6569 & $8.8 \pm 0.02$ & $0.57 \pm 0.057$ & $15.26 \pm 0.25$ & $1.76 \pm 0.02$ & $2.63$ \\
NGC 6584 & $8.93 \pm 0.01$ & $0.023 \pm 0.002$ & $15.76 \pm 0.06$ & $1.71 \pm 0.01$ & $3.16$ \\
NGC 6624 & $7.82 \pm 0.01$ & $0.28 \pm 0.028$ & $14.43 \pm 0.18$ & $1.79 \pm 0.01$ & $2.25$ \\
NGC 6637 & $7.46 \pm 0.01$ & $0.17 \pm 0.012$ & $14.7 \pm 0.1$ & $1.8 \pm 0.01$ & $2.52$ \\
NGC 6638 & $8.89 \pm 0.01$ & $0.39 \pm 0.039$ & $15.14 \pm 0.21$ & $1.53 \pm 0.01$ & $2.82$ \\
NGC 6642 & $9.35 \pm 0.03$ & $0.44 \pm 0.044$ & $14.83 \pm 0.22$ & $1.63 \pm 0.02$ & $2.59$ \\
NGC 6652 & $8.98 \pm 0.02$ & $0.103 \pm 0.007$ & $15.01 \pm 0.09$ & $1.53 \pm 0.01$ & $2.74$ \\
NGC 6681 & $7.93 \pm 0.02$ & $0.064 \pm 0.005$ & $15 \pm 0.08$ & $1.78 \pm 0.02$ & $2.44$ \\
NGC 6712 & $8.11 \pm 0.03$ & $0.419 \pm 0.03$ & $14.27 \pm 0.15$ & $1.93 \pm 0.03$ & $3.97$ \\
NGC 6723 & $7.24 \pm 0.02$ & $0.05 \pm 0.005$ & $14.74 \pm 0.11$ & $1.95 \pm 0.02$ & $3.6$ \\
NGC 6752 & $5.67 \pm 0.01$ & $0.04 \pm 0.004$ & $13.13 \pm 0.16$ & $2.08 \pm 0.02$ & $3.84$ \\
NGC 6809 & $6.84 \pm 0.01$ & $0.07 \pm 0.007$ & $13.78 \pm 0.12$ & $2.22 \pm 0.02$ & $5.19$ \\
NGC 6864 & $8.52 \pm 0.02$ & $0.21 \pm 0.021$ & $16.49 \pm 0.15$ & $1.44 \pm 0.02$ & $3.87$ \\
NGC 6934 & $8.77 \pm 0.01$ & $0.09 \pm 0.006$ & $16.05 \pm 0.08$ & $1.56 \pm 0.01$ & $3.4$ \\
NGC 6981 & $9.3 \pm 0.02$ & $0.05 \pm 0.004$ & $16.1 \pm 0.06$ & $1.71 \pm 0.02$ & $3.39$ \\
NGC 7006 & $10.63 \pm 0.01$ & $0.05 \pm 0.005$ & $18.03 \pm 0.17$ & $1.41 \pm 0.01$ & $2.61$ \\
NGC 7078 & $6.38 \pm 0.01$ & $0.09 \pm 0.006$ & $15.15 \pm 0.08$ & $1.8 \pm 0.01$ & $3.18$ \\
NGC 7089 & $6.41 \pm 0.01$ & $0.01 \pm 0.001$ & $15.47 \pm 0.09$ & $1.78 \pm 0.01$ & $3.42$ \\
NGC 7099 & $7.57 \pm 0.01$ & $0.03 \pm 0.002$ & $14.7 \pm 0.07$ & $1.8 \pm 0.01$ & $2.92$ \\
NGC 7492 & $11.39 \pm 0.03$ & $0 \pm 0.001$ & $17.1 \pm 0.1$ & $1.84 \pm 0.02$ & $4.24$ \\
SMC-KRON 3 & $11.1 \pm 0.07$ & $0.016 \pm 0.002$ & $18.89 \pm 0.2$ & $1.59 \pm 0.06$ & $4.99$ \\
SMC-NGC 121 & $10.71 \pm 0.05$ & $0.146 \pm 0.015$ & $18.89 \pm 0.25$ & $1.37 \pm 0.06$ & $2.31$ \\
SMC-NGC 152 & $11.65 \pm 0.08$ & $0.12 \pm 0.012$ & $18.89 \pm 0.24$ & $1.7 \pm 0.06$ & $3.35$ \\
SMC-NGC 176 & $12.21 \pm 0.19$ & $0 \pm 0.001$ & $18.89 \pm 0.2$ & $1.34 \pm 0.18$ & $2.97$ \\
SMC-NGC 361 & $11.13 \pm 0.09$ & $0.069 \pm 0.007$ & $18.89 \pm 0.22$ & $1.55 \pm 0.06$ & $5.02$ \\
SMC-NGC 411 & $11.61 \pm 0.11$ & $0.054 \pm 0.005$ & $18.89 \pm 0.22$ & $1.42 \pm 0.1$ & $2.69$ \\
SMC-NGC 416 & $11.18 \pm 0.06$ & $0.127 \pm 0.013$ & $18.89 \pm 0.24$ & $1.24 \pm 0.05$ & $4.7$ \\
SMC-NGC 458 & $11.09 \pm 0.09$ & $0.022 \pm 0.002$ & $18.89 \pm 0.21$ & $1.44 \pm 0.07$ & $2.41$ \\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Cluster name.}  
\tablefoottext{b}{$V$-band integrated apparent magnitude, this paper, based on model-independent smoothing and integration of \cite{CatTrager} surface brightness profiles, mag.}  
\tablefoottext{c}{Line-of-sight reddening, \cite{FerraroDistances} and \cite{RecioBlancoDistances} (galactic GCs), \cite{RecioBlancoDistances} (extragalactic clusters), mag.}
\tablefoottext{d}{True distance modulus \cite{FerraroDistances} and \cite{RecioBlancoDistances} (galactic GCs), \cite{RecioBlancoDistances} (extragalactic clusters), mag.}  
\tablefoottext{e}{Log projected angular half-light radius, this paper, based on model-independent smoothing and integration of \cite{CatTrager} surface brightness profiles, arcsec.} 
\tablefoottext{f}{Slope of the outermost surface brightness profile, this paper, dimensionless.}}
\end{table}