Fig. 14
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Left panels: distributions of extinction-corrected absolute V-band magnitudes for our sample of clusters. The overall distribution is shown as well as the luminosity function split into young (blue) and old (red) age bins. We also show a sample of GCs in more distant dIrr galaxies, taken from Georgiev et al. (2009). Right panels: the same but for the (V − I)0 colour distributions.
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