\begin{table}%t11
\par
\caption {\label{TABLAFIN}Derived star cluster properties for all the galaxies (Sample).}
%%\centerline

 {\scriptsize   
\begin{tabular}{cccccccccccc} 
\hline
\hline
  {ID}  & {RA}    &  {Dec.}  & {$x$}   & {$y$}   &  $B$    &    ${\sigma}$    & {$V$}  &  ${\sigma}$  &    {$I$}     &${\sigma}$  &  {$U$}      \\ 
             & {J2000} & {J2000} & {Pix} & {Pix} &{\it F435W} &  {\it F435W}   & {\it F555W}  &  {\it F555W}  &  {\it F814W} &  {\it F814W}  &  {\it F335W}  \\ 
\hline 
   ${\sigma}$    & {{\it FWHMB}} & {{\it FWHMB}} & {{\it FWHMV}} & {{\it FWHMI}} & ${E(B-V)}$  & ${E(B-V)}$  &  {$E(B-V)$} & {$E(B-V)$} & {$E(B-V)$}  & {$E(B-V)$}  & {$\log({Age}/{yr})$} \\ 
     {\it F336W}    &    {pix}  &   {pix}   &   {pix}   &   {pix}   & {$Z=0.004$} & {$Z=0.008$} &  {$Z=0.02$} & {$Z=0.05$} & {$Z=0.004$} & {$Z=0.019$} & {$Z=0.004$}             \\ 
\hline 
 {$\log(\rm {Age}/{yr})$}   & {$\log(\rm {Age}/{yr})$}  & {$\log(\rm {Age}/{yr})$}  &  {$\log({Age}/{yr})$}  &  {$\log(\rm {Age}/{yr})$}  &  {$\log(M/M_{\odot})$}  & {$\log(M/M_{\odot})$}  & {$\log(M/M_{\odot})$}  &  {$\log(M/M_{\odot})$}  &  {$\log(M/M_{\odot})$}  &  {$\log(M/M_{\odot})$}  & \\ 
     {$Z=0.008$}         &           {$Z=0.02$}         &       {$Z=0.05$}          &       {$Z=0.004$}         &       {$Z=0.019$}         &       {$Z=0.004$}          &       {$Z=0.008$}          &        {$Z=0.02$}          &       {$Z=0.05$}           &       {$Z=0.004$}                  & {$Z=0.019$}         \\ 
 NGC~1313\_1\_1  & 3:18:35.8632  & --66:28:03.459  & 2429.980  & 757.311  & 21.418 & 0.010 & 21.405 & 0.011 & 21.364 & 0.012 & 20.258\\ 
 0.032 & 19.080 & 1.300 & 1.210 & 1.430 & 0.000 & 0.000 & 0.000 & 0.180 & 0.300 & 0.120 & 6.950\\ 
 6.850 & 6.770 & 6.700 & 6.700 & 6.750 & 3.410 & 2.860 & 2.770 & 3.100 & 3.400 & 3.010 \\ 
 NGC~1313\_1\_2  & 3:18:33.6487  &--66:27:43.434  & 1951.000  & 794.048  & 21.362 & 0.009 & 21.093 & 0.008 & 20.307 & 0.006 & 21.168\\  
 0.053 & 5.080 & 2.030 & 1.780 & 1.320 & 0.000 & 0.150 & 0.170 & 0.190 & 0.120 & 0.210 & 6.900\\ 
 8.280 & 8.160 & 8.020 & 8.400 & 8.150 & 4.290 & 4.370 & 4.350 & 4.340 & 4.450 & 4.500 \\ 
 NGC~1313\_1\_3  & 3:18:32.4677  & --66:27:32.069  & 1683.567  & 807.000  & 22.647 & 0.023 & 22.439 & 0.020 & 21.890 & 0.017 & 22.209\\  
 0.107 & 5.690 & 1.590 & 1.230 & 1.100 & 0.000 & 0.200 & 0.140 & 0.090 & 0.220 & 0.090 & 6.860\\ 
 7.660 & 7.830 & 7.990 & 7.800 & 8.100 & 3.390 & 3.440 & 3.510 & 3.600 & 3.650 & 3.710 \\ 
 NGC~1313\_1\_4  & 3:18:33.4053  & --66:27:32.911  & 1752.953  & 717.063  & 21.153 & 0.013 & 20.853 & 0.010 & 20.279 & 0.011 & 21.333\\ 
   0.060 & 13.750 & 6.660 & 6.410 & 7.220 & 0.000 & 0.130 & 0.210 & 0.220 & 0.070 & 0.280 & 7.940\\ 
 8.610 & 8.340 & 8.230 & 8.850 & 8.350 & 5.110 & 5.080 & 5.040 & 5.030 & 5.230 & 5.260 \\ 
 NGC~1313\_1\_5  & 3:18:33.7834  & --66:27:47.653  & 2032.560  & 821.021  & 21.407 & 0.013 & 21.159 & 0.011 & 20.542 & 0.010 & 21.244\\   
 0.053 & 11.010 & 4.170 & 3.850 & 4.550 & 0.000 & 0.160 & 0.210 & 0.230 & 0.130 & 0.240 & 7.570\\ 
 8.180 & 8.090 & 7.990 & 8.300 & 8.100 & 4.360 & 4.460 & 4.530 & 4.550 & 4.550 & 4.670 \\ 
 NGC~1313\_1\_6  & 3:18:30.8600  & --66:27:33.740  & 1619.000  & 991.545  & 22.467 & 0.021 & 22.168 & 0.018 & 21.229 & 0.011 & 22.039\\  
 0.099 & 14.570 & 4.570 & 4.500 & 6.480 & 0.440 & 0.650 & 0.490 & 0.630 & 0.600 & 0.530 & 7.050\\ 
 7.080 & 7.200 & 6.970 & 7.000 & 7.250 & 4.240 & 4.100 & 4.000 & 4.090 & 3.980 & 4.210 \\ 
 NGC~1313\_1\_7  & 3:18:31.0300  & --66:27:55.795  & 2014.263  & 1188.420  & 22.574 & 0.021 & 22.346 & 0.017 & 21.878 & 0.015 & 22.530\\ 
   0.133 & 5.780 & 2.060 & 1.930 & 1.130 & 0.000 & 0.170 & 0.000 & 0.000 & 0.210 & 0.000 & 7.780\\ 
 7.990 & 8.440 & 8.320 & 8.000 & 8.550 & 3.650 & 3.670 & 3.780 & 3.760 & 3.800 & 3.990 \\ 
 NGC~1313\_1\_8  & 3:18:31.8406  & --66:28:10.642  & 2320.923  & 1248.120  & 22.161 & 0.016 & 22.078 & 0.015 & 21.969 & 0.017 & 21.212\\ 
   0.059 & 3.270 & 0.540 & 0.730 & 0.730 & 0.000 & 0.170 & 0.240 & 0.350 & 0.320 & 0.350 & 6.770\\ 
 6.770 & 6.680 & 6.620 & 6.750 & 6.650 & 2.730 & 2.710 & 2.710 & 2.910 & 3.020 & 2.970 \\ 
 NGC~1313\_1\_9  & 3:18:30.9189  & --66:28:00.003  & 2081.302  & 1241.000  & 22.454 & 0.019 & 22.195 & 0.016 & 21.556 & 0.012 & 22.051\\ 
   0.090 & 7.640 & 3.170 & 3.130 & 1.850 & 0.000 & 0.190 & 0.580 & 0.590 & 0.180 & 0.140 & 6.790\\ 
 7.910 & 6.600 & 6.600 & 8.000 & 8.050 & 3.190 & 3.840 & 3.300 & 3.380 & 3.950 & 3.980 \\ 
 NGC~1313\_1\_10  & 3:18:34.0503  & --66:28:42.311  & 3003.000  & 1325.275  & 22.000 & 0.017 & 22.100 & 0.016 & 22.076 & 0.019 & 20.562\\  
 0.035 & 3.500 & 0.760 & 0.460 & 5.220 & 0.060 & 0.160 & 0.020 & 0.160 & 0.220 & 0.020 & 7.080\\ 
 7.080 & 7.200 & 6.900 & 7.150 & 6.950 & 3.330 & 3.190 & 3.110 & 3.120 & 3.450 & 2.950 \\ 
\hline
\end{tabular}
}
\par
\smallskip
 {First row: 1) Galaxy ID: Name\_Field\_N;  2)  RA (J2000); 3)  Dec (J2000);
  4)  X (pix); 5)  Y (pix). 6.-  $B_{\it F435W}$; 7)  Error of $B_{ \it F435W}$ photometry;
   8)~Same as 6 but for $V_{\it F555W}$; 9)  Same as 7 but for $V_{\it F555W}$;
    10) Same as 6 but for $I_{\it F814W}$; 11)  Same as 7 but for $I_{\it F814W}$;
     12) Same as 6 but for $U_{\it F336W}$.
Second row: 1)  Error of $U_{\it F336W}$ photometry; 2)  ${\it FWHM}_B$ according to SExtractor;
 3)  ${\it FWHM}_B$ according to Ishape; 4)  ${\it FWHM}_V$ according to Ishape;
  5)~${\it FWHM}_I$ according to Ishape;  6)  Extinction derived using GALEV considering $Z=0.004$;   7)  Same as 6 but for $Z=0.008$;
   8)  Same as 6 but for $Z=0.02$;
    9)  Same as 6 but for $Z=0.05$;
     10) Extinction derived using Girardi considering $Z=0.004$;
      11) Same as 10 but for $Z=0.019$;
       12)~Log of the star cluster age derived from GALEV for $Z=0.004$. 
Third row: 1.- Log of the star cluster age derived from GALEV for $Z=0.008$;
 2)~Same as~1 but for $Z=0.02$;
  3) Same as 1 but for $Z=0.05$;
   4) Log of the star cluster age derived from Girardi for $Z=0.004$;
    5) Same as~4 but for $Z=0.019$;
     6) Log of the mass derived from GALEV for $Z=0.004$;
      7) Same as 6 but for $Z=0.008$;
       8) Same as 6 but for $Z=0.002$;
        9) Same as 6 but for $Z=0.005$;
          10) Log of the mass derived from Giradi for $Z=0.004$;
           11) Same as 10 but for $Z=0.019$.}
\end{table}