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Table 4:

Observed stars in template globular clusters.
Cluster ID V B-V $\Sigma W$(Å)
M 5 II-45 14.75 0.82 4.62
  II-50 13.92 0.96 5.12
  II-51 14.05 0.96 4.90
  II-80 14.31 0.91 4.89
  II-74 13.82 1.01 5.05
  I-2 13.87 1.02 5.24
  I-50 13.91 0.97 5.06
  I-61 13.37 1.17 5.40
  I-68 12.37 1.52 6.25
  I-71 13.01 1.29 5.57
NGC 4372 20 12.88 1.57 3.78
  14 14.29 1.29 2.88
  13 12.72 1.73 4.13
  10 13.82 1.29 3.00
  95 14.48 1.30 2.72
  91 14.45 1.33 2.81
  89 14.49 1.29 2.83
  141 12.93 1.65 4.01
  74 14.17 1.40 3.09
  76 14.18 1.30 3.16
  77 14.19 1.28 3.07
NGC 6171 62 13.97 1.62 5.83
  100 14.21 1.40 5.50
  I 13.89 1.46 5.66
  F 13.39 1.70 6.21
NGC 6397 328 12.07 0.93 3.19
  326 12.78 0.89 2.89
  337 12.58 0.90 2.83
  343 11.42 1.13 3.34
  361 11.67 1.08 3.18
NGC 6528 R2-8 15.79 1.89 6.80
  R1-42 16.46 1.62 6.34
  R2-41 16.30 1.64 6.44
NGC 6752 4 13.70 0.85 3.86
  8 11.96 1.05 4.99
  28 13.17 0.89 4.18
  29 11.79 1.17 4.98
  30 12.15 1.12 4.83
NGC 5927 133 14.75 1.97 6.45
  372 14.66 2.11 6.28
  335 14.44 1.94 6.63
  190 14.29 2.02 6.71
  65 14.64 1.92 6.58
NGC 4590 144 12.80 1.29 3.72
  239 14.19 0.87 2.88
  II72 15.03 0.85 2.60
  30 14.15 0.87 2.64
  74 14.59 0.84 2.36
  119 13.62 0.95 2.90
Notes. The IDs, magnitudes, and colours of stars are those given in the original
photometry papers quoted by Rutledge et al. (1997a).

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