Fig. 4.
Comparison of mock CMDs with solution CMDs of DG-5 (top) and DG-22 (bottom): as indicated, the first column represents the mock or observed CMDs, the second column represents the solution CMDs, the third column represents the residuals, and the fourth column represents the significance for the simulated dwarf galaxies DG-5 (upper panel) and DG-22 (lower panel).
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