Similar to Figure 12, but for properties of breakout emission associated with jets launched from BHs. The upper, middle, and lower panels show the breakout luminosity, duration, and delay time, respectively. Since emission from nonjetted AGNs is generally faint in the MeV band compared to these BH-driven flares (e.g., P. Padovani et al. 2017), the luminosity of BH-driven flares is not compared with AGN luminosity, unlike in Figure 12.