Fig. 6.
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Normalised PM histograms and CMDs for field (in red) and cluster (in blue) stars. We fit the Gaussian distributions (dashed lines) using means and standard deviations listed in Table 2. (a) FSR 0009, (b) FSR 1775, (c) FSR 1767, (d) VVV-CL110, (e) VVV-CL119, (f) VVV-CL128, (g) VVV-CL131, (h) VVV-CL143, (i) VVV-CL150 (j) VVV-CL153, (k) VVV-CL154, (l) VVV-CL160, (m) ESO 393-12, (n) ESO 456-09, (o) DB 044, (p) Kronberger 49.
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