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Table 4.

Color excesses and distances to the target clusters.

Cluster E(Z − Ks) E(Y − Ks) E(J − Ks) E(H − Ks) R R⊙, Baumgardt19 R⊙, Harris96
(mag) (mag) (mag) (mag) (kpc) (kpc) (kpc)
NGC 6441 0.41 ± 0.10 0.20 ± 0.08 0.18 ± 0.06 0.03 ± 0.02 13.0 ± 0.3 + 0.2 + 0.8 11.83 ± 0.05 11.6
Terzan 10 2.44 ± 0.36 1.54 ± 0.26 0.86 ± 0.12 0.30 ± 0.04 10.3 ± 0.3 − 1.1 + 0.1 5.8
2MASS-GC 02 3.0 ± 0.4 1.12 ± 0.23 6.0 ± 0.9 4.9
NGC 6569 0.65 ± 0.05 0.37 ± 0.04 0.25 ± 0.05 0.07 ± 0.03 10.6 ± 0.3 + 0.3 + 0.3 10.24 ± 1.16 10.9
NGC 6626 (M 28) 0.46 ± 0.09 0.28 ± 0.07 0.23 ± 0.03 0.05 ± 0.02 5.41 ± 0.08 + 0.11 − 0.11 5.42 ± 0.33 5.5
NGC 6656 (M 22) 0.35 ± 0.07 0.24 ± 0.06 0.18 ± 0.04 0.05 ± 0.03 3.24 ± 0.05 + 0.06 − 0.04 3.24 ± 0.08 3.2

Notes. The reported first σ in both distances and color excesses corresponds to the dispersion from the individual RR Lyrae estimations, the second σ in the distance estimation corresponds to the effects of changing the extinction law that we use in the different GGCs according to the text, and the third to changing the PLZ relations.

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