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Fig. 2


Hess density diagrams of the five late-type dwarf galaxies studied here, ordered by (increasing) absolute magnitude. We additionally overplot to each CMD the Galactic foreground stellar contamination (red crosses), as simulated with the TRILEGAL models. The simulations include incompleteness effects and photometric errors in their color − magnitude distribution. We point out that the drawn distribution is only one random realization of the Galactic foreground model. On the left side of each diagram, representative 1σ photometric errorbars (as derived from artificial star tests) are shown.

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