Fig. 5.
Effect of using different apertures on the retrieved cumulative mass fraction of DG-5 (top) and DG-22 (bottom): the above plots show the comparison of the cumulative SFRs from considering three different apertures, where blue (solid), green (dotted), and orange (dashed) lines represent the solved SFR from considering 1.5 kpc, 1.0 kpc, and 0.5 kpc radial apertures from the center of the galaxy, respectively.
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