Broadband SED of MAD models under different PL electron setups. From top to bottom, lines with the same color represent MADs whose accretion rates are ﹩{\dot{m}}_{0}=1\times 1{0}^{-2}﹩, 1 × 10⁻³, 1 × 10⁻⁴, and 1 × 10⁻⁵, respectively. For each accretion rate, three PL electron setups are considered (lines with the same color), i.e., solid for the ξ_pl,mad = 0 (MAD.th case), dotted for the fixed distribution PL case (ξ_pl,mad = 1%, radiative cooling to PL electrons excluded, a νL_ν ∝ ν^∼+0.23 spectrum is observed at ν ≳ × 10¹⁴ Hz), and dashed for the self-consistent PL case (ξ_pl,mad = 1%, and radiative cooling to PL electrons included). For comparative purposes, the green dotted–dashed curve shows the spectrum without inverse Compton, for the case of PL electrons with γ_cooling. A νL_ν ∝ ν^∼−0.246 spectrum is indeed observed at 10¹⁴-10¹⁷ Hz. Above ∼10¹⁸ Hz is the bremsstrahlung bump.