Table 1: Basic properties of LMC clusters in our sample.

NGC		 RA(J2000) Dec SWBa sb log tc [Fe/H]d E(B-V)e Dia.f Vg B-Vg U-Bg
1651 04 37 32.1 -70 35 07 V 39 9.30 -0.37 0.11 62V 12.67 0.69 0.30
1711 04 50 37.2 -69 59 03 I 20 7.70 -0.57 0.16 60V 10.11 0.12 -0.37
1783 04 59 10.0 -65 59 14 V 37 9.00 -0.45 0.10 72V 10.93 0.62 0.23
1786 04 59 07.9 -67 44 38 VII 48 10.18 -1.87 0.12 60V 10.88 0.74 0.10
1806 05 02 13.2 -67 59 07 V 40 9.30 -0.23 0.12 88V 11.10 0.73 0.26
1818 05 04 14.8 -66 26 04 I 18 7.40 -0.4$\sim$0.0 0.10 72V 9.70 0.18 -0.47
1831 05 06 15.6 -64 55 03 IVA 31 8.50 0.01 0.10 60V 11.18 0.34 0.13
1847 05 07 05.4 -68 58 41 I 21 7.42 -0.37 0.10 72V 11.06 0.20 -0.33
1850 05 08 45.8 -68 45 42 II 21 7.50 -0.12 0.15 50T 9.57 0.15 -0.27
1856 05 09 30.3 -69 08 05 IVA 30 8.12 -0.52 0.24 62V 10.06 0.34 0.07
1866 05 13 39.1 -65 27 56 III 27 8.12 -0.50 0.10 72V 9.73 0.25 -0.04
1868 05 14 35.4 -63 57 16 IVA 33 8.74 -0.50 0.07 62V 11.56 0.45 0.15
1967 05 26 44.3 -69 06 06 I 12 7.00   0.14 50T 10.83 0.05 -0.75
1978 05 28 44.3 -66 14 08 VI 45 9.70 -0.42 0.10 62V 10.70 0.78 0.23
1983 05 27 44.3 -68 59 03 I 13 6.90   0.09 45V 9.94 0.10 -0.76
1987 05 27 18.2 -70 44 05 IVB 35 8.80   0.12 62V 12.08 0.52 0.20
2004 05 30 40.3 -67 17 10 I 15 7.30 -0.56 0.06 72V 9.60 0.17 -0.68
2031 05 33 40.9 -70 59 06 III 27 8.20 -0.52 0.07$^\dagger$ 72V 10.83 0.27 -0.05
2074 05 39 01.7 -69 29 51 0 10 6.60   0.07 150T 9.32 -0.16 -0.91
2100 05 42 07.8 -69 12 42 I 17 7.20 -0.32 0.24 60V 9.60 0.16 -0.56
2107 05 43 12.1 -70 38 24 IVA 32 8.60   0.19 60V 11.51 0.38 0.13
2134 05 51 56.7 -71 05 45 III 28 8.00 -1.0 0.10 60V 11.05 0.25 -0.02
2136 05 52 57.7 -69 29 24 III 26 8.00 -0.55 0.10 60V 10.54 0.28 -0.13
2154 05 57 38.3 -67 15 37 V 39 9.20 -0.56 0.10 62V 12.13 0.68 0.30
2155 05 58 34.6 -65 28 36 VI 45 9.51 -0.45 0.10 62V 12.60 0.80 0.23
2157 05 57 34.9 -69 11 45 III 25 7.60 -0.45 0.10 60V 10.16 0.19 -0.16
2164 05 58 56.8 -68 30 56 II 23 7.70 -0.45 0.10 60V 10.34 0.10 -0.24
2214 06 12 58.4 -68 15 33 II 22 7.60 -0.45 0.10 60V 10.93 0.11 -0.27
$^{a,\ b}$ SWB classification and s parameter from Bica et al. (1996, hereafter BCDSP96).

$^{c,\ d}$ Logarithmic age and metallicity from Mackey & Gilmore (2003), except for NGC 1651, which is from Sarajedini et al. (2002).

e Reddening from Persson83. Except for NGC 1847 from Nelson & Hodge (1983), and NGC 1967, NGC 1983, NGC 2074 from Meurer et al. (1990).

f Aperture diameter in arcsec for BV photometry. Suffix V and T indicates photometry sources, respectively van den Bergh (1981, hereafter VDB81) and BCDSP96.

g Optical photometry data from VDB81 and BCDSP96.

$^\dagger$ Adopted mean value across the LMC of E(B-V)=0.07 taken from Burnstein & Heiles (1984).


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