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Fig. 14


Comparison of the present-day cumulative mass profiles of observations and models with primordial binaries. The thick solid (red) lines are derived from the ensemble en2250PL without binaries, the dashed (green) line is derived from the ensemble enb2250PL with 33% primordial binaries, and the dotted (magenta) line is derived from the best-fitting ensemble with 33% primordial binaries enb2125PL. The dashed (blue) line represents the observations. The standard errors are shown as filled areas.

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