Figure 5.
Combined probability distribution between age and mass for the galaxy with the largest CSFH age uncertainty. As described in Section 3.1, while the median values of these properties are associated with the largest peak of the probability distribution, the uncertainties (which are defined by the 16th and 84th percentiles of the distribution) can span a much larger range. The horizontal and vertical lines indicate the adopted stellar mass and CSFH age, respectively.