A corner plot showing the collective 1D and 2D posterior distributions for the parameters constrained for each of the 125 million Augustus-Gold stars. These parameters are (from left to right): the initial mass (M _init), initial metallicity ([Fe/H]_init), EEP, age (﹩\mathrm{log}{t}_{\mathrm{age}}﹩), effective temperature (﹩\mathrm{log}{T}_{\mathrm{eff}}﹩), bolometric luminosity (﹩\mathrm{log}{L}_{\mathrm{bol}}﹩), surface gravity (﹩\mathrm{log}g﹩), distance ﹩\mathrm{log}d﹩, extinction (A _V ), and “differential” extinction (R _V ). The titles of each column show the median and the interval encompassing 95% of the sample. As expected, the majority the sample comprises sources with low extinction (A _V ≲ 1 mag) and initial masses ranging from 0.55 M _⊙ < M _init < 1.2 M _⊙, with the lower limit imposed by the lower M _init bound on our underlying grid of stellar models. Gridding effects can be seen in a few panels.