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Table 5

Star cluster ages, extinctions, and masses.

ID Age [Myr] E(B − V) log  (Mass/M) χ2/d.f.

1 265 0.44 5.9 0.56
2 36 0.02 4.6 1.13
3 964 0.00 6.4 5.01
4 88 0.38 5.6 0.60
5 78 0.35 5.6 3.90
6 60 1.15 5.5 14.08
7 184 0.80 6.0 2.50
8 440 0.62 6.4 1.25
9 6 0.31 4.0 2.87
10 75 1.14 5.8 3.71
12 220 0.72 6.1 1.11
13 998 0.93 6.4 1.11
15 130 0.90 6.0 0.72
17 196 0.50 5.6 4.20
18 130 0.23 5.2 2.02
19 122 0.40 5.6 1.54
20 864 0.00 6.1 174.29
21 130 0.56 5.6 1.65
22 140 0.41 6.1 0.37
23 148 0.83 5.6 0.11
24 265 0.00 6.8 340.26
25 234 0.65 5.9 1.52
26 420 0.43 5.8 1.24
27 4 1.26 4.6 0.84
28 700 0.49 6.2 2.29
29 135 0.30 5.8 3.29
30 134 1.00 6.0 21.18
31 828 0.78 6.8 125.41
32 998 0.75 6.5 6.87
33 998 0.44 6.2 1.68
34 996 0.90 6.8 8.48
38 145 0.51 5.9 0.54
39 420 1.04 6.4 4.04
40 490 0.60 6.2 0.12
41 100 1.04 5.5 2.45
42 136 0.31 5.2 1.32
43 216 0.42 5.8 1.15
44 190 0.69 5.6 0.37
45 162 0.50 5.6 0.49
46 450 0.36 5.8 0.52
47 64 0.64 5.3 0.53
48 241 0.21 5.7 0.48
49 122 0.43 5.4 5.49
51 100 0.18 5.7 1.97
52 336 0.72 6.0 0.68
53 836 0.62 6.2 5.88
54 248 1.04 6.0 2.38
55 294 0.58 5.8 2.85

Notes. Results of the χ2 fitting of age (Col. 2), color excess (Col. 3), and mass (Col. 4) of the observed star clusters. Only those candidates that were successfully fitted are listed. The star cluster ID in Col. 1 is the same as those in Table 4.

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