Fig. 14
Histograms of the interpolated data. The left panel shows the initial ZAMS masses, and the right panel shows the ages since the ZAMS was used later to derive a star-formation history (see Fig. 15). The solid lines represent the data obtained with IFMR defined by Eq. (14), while the thin dotted (red) lines repeat the histograms from Fig. 8 for comparison.
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