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Fig. 6


Optical and NIR (dereddened) CMDs for CenA-dE1 and SGC1319.1-4216. Representative photometric errorbars are plotted along the CMDs. The red lines are isochrones from the Padova evolutionary models with improved AGB phases (Girardi et al. 2010). For CenA-dE1, they have the mean metallicity of the galaxy ([Fe/H]  ~   − 1.5) and ages of 2 and 9 Gyr; for SGC1319.1-4216, the metallicity is [Fe/H]  ~     − 1.0 and the ages 2 and 5 Gyr.

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