Fig. 6.
Effects of the adopted extinction prescription on the observed CMDs of DG-5 (top) and DG-22 (bottom). Left column: dust-free CMDs; middle panel: CMDs computed using the extinction prescription (5); and right column: CMDs computed for three times the nominal amount of extinction. As explained in Sect. 3.2, sharp features are visible in the CMDs due to each star particle constituting a single stellar population, but this does not affect the analysis.
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