The radiation features of the breakout outflow-driven shocked shell. The top panels represent the estimated luminosity ﹩{L}_{\mathrm{bre}}﹩ of the breakout photon for different cases of s = 0.2, 0.5, and 0.8, with the bolometric luminosity of the AGN shown by the orange lines; the bottom panels represent the blackbody temperature T _rad of the breakout photon. Each column represents a case with different SMBH masses of M = 10⁶ M _⊙, 10⁷ M _⊙, and 10⁸ M _⊙, respectively. The discontinuity and the steep drop derive from the disk truncation by outflow.