Fig. 5.
Distribution of the snapshot difference between the KDC birth and the closest merger undergone by the host galaxy for the actual KDC births (in blue) compared to the distribution where the KDC births were permuted within the sample (in orange), with the bin size of three snapshots. The inset is a zoom around zero for the actual births, with the bin size of one snapshot. One snapshot is approximately 0.16 Gyr.
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