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Table 4

Same as Table 3, but for clusters retrieved from the ESO archive.

Cluster RA Dec log age (yr) Distance (pc) z (pc) RGC (kpc) N stars [Fe/H]
Berkeley 20 83.152 0.185 9.68 8728 −2606 16.3 6 −0.38 ± 0.04
Collinder 110 99.677 2.069 9.26 2183 −71 10.3 6 −0.1 ± 0.04
Ruprecht 4 102.248 −10.524 8.93 4087 −378 11.7 5 −0.13 ± 0.01
Berkeley 29 103.268 16.93 9.49 12 604 1750 20.6 6 −0.36 ± 0.07
Ruprecht 7 104.456 −13.227 8.37 5851 −469 13.1 5 −0.24 ± 0.03
Tombaugh 2 105.773 −20.82 9.21 9316 −1115 15.8 12 −0.24 ± 0.07
NGC 2324 106.033 1.046 8.73 4214 242 12.1 8 −0.18 ± 0.01
NGC 2660 130.667 −47.201 8.97 2788 −146 8.9 5 −0.05 ± 0.04
M67 132.846 11.814 9.63 889 470 8.9 131 0.0 ± 0.02
NGC 3960 177.644 −55.679 8.9 2345 252 7.7 10 0.0 ± 0.01
NGC 4337 186.022 −58.125 9.16 2450 194 7.4 7 0.24 ± 0.03
Collinder 261 189.519 −68.377 9.8 2850 −275 7.3 7 −0.05 ± 0.07
NGC 5822 226.051 −54.366 8.96 1404 42 7.7 4 0.02 ± 0.02
NGC 6192 250.077 −43.355 8.38 1737 64 6.7 6 −0.08 ± 0.07
NGC 6404 264.916 −33.224 8.0 2500 −51 5.8 5 0.01 ± 0.06
NGC 6583 273.962 −22.143 9.08 2053 −91 6.3 4 0.22 ± 0.01
Ruprecht 147 289.087 −16.333 9.48 323 −71 8.05 6 0.12 ± 0.02
NGC 6791 290.221 37.778. 9.8 4231 800 7.9 8 +0.23 ± 0.20

Notes. Only UVES spectra are considered.

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