The inferred progenitor masses as a function of their associated explosion energies from our investigation of the properties of the individual stars that can accurately model the abundances of each EMP DLA in our sample. The properties of the progenitor associated with each DLA have been found independently from one another. We represent the resulting parameter distributions by their median value and their interquartile range. These distributions are mostly non-Gaussian. In some cases, the median is close to an edge of the region bounded by the interquartile range. This is caused by a strong peak in the distribution around a particular parameter value. Compared to the full parameter space that has been explored, these DLAs show remarkably consistent progenitor properties.