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Table 11:

Derived star cluster properties for all the galaxies (Sample).
ID RA Dec. x y B $\sigma$ V $\sigma$ I $\sigma$ U
  J2000 J2000 Pix Pix F435W F435W F555W F555W F814W F814W F335W
$\sigma$ FWHMB FWHMB FWHMV FWHMI E(B-V) E(B-V) E(B-V) E(B-V) E(B-V) E(B-V) $\log({Age}/{yr})$
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
$\log(\rm {Age}/{yr})$ $\log(\rm {Age}/{yr})$ $\log(\rm {Age}/{yr})$ $\log({Age}/{yr})$ $\log(\rm {Age}/{yr})$ $\log(M/M_{\odot})$ $\log(M/M_{\odot})$ $\log(M/M_{\odot})$ $\log(M/M_{\odot})$ $\log(M/M_{\odot})$ $\log(M/M_{\odot})$  
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  
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.

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