Similar to Figure 5, but for the bolometric (top) and optical (bottom) luminosities. The P_15.9–P_84.1 range is about an order of magnitude, and an overall spread is about 2 orders of magnitude at the P_2.3–P_97.7 range. The median offset between the optical and bolometric peaks is about a factor of 1.9, which can be used as a rough proxy for the overall optical-bolometric correction of the class.