A one-parameter two-zone leptonic model for the blazar sequence

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Table A.2.

Resulting peak frequencies and luminosities of the synchrotron and inverse Compton components in the theoretical blazar sequence.

Class	$ν_{syn}^{pk}$ $\nu_{\mathrm{syn}}^{\mathrm{pk}}$	$L_{syn}^{pk}$ $L_{\mathrm{syn}}^{\mathrm{pk}}$	$ν_{IC}^{pk}$ $\nu_{\mathrm{IC}}^{\mathrm{pk}}$	$L_{IC}^{pk}$ $L_{\mathrm{IC}}^{\mathrm{pk}}$	Γ_γ	log(CD)
	(log Hz)	(log erg s⁻¹)	(log Hz)	(log erg s⁻¹)
FSRQ	13.2	46.4	22.8	47.3	3.00	0.92
LBL	15.5	45.0	23.3	45.1	2.14	0.12
HBL	17.1	43.8	26.3	44.0	1.46	0.21

Notes. The acceleration zone is at a distance of z = 0.01 pc from the central black hole, assumed to have a mass ℳ = 10⁸ M_⊙. The external photon field is produced from isotropic scattering of disk photons on wind particles between radii R₁ = 9 × 10¹⁴ cm and R₂ = 3 × 10¹⁸ cm. The efficiencies of the magnetic field and the external photon field are η_b = 0.01 and ϵ = 0.05, respectively. The number of electrons injected in the acceleration process, assumed to be of Type I Fermi, depends linearly on the mass accretion rate. The bulk Lorentz factor is Γ = 30 and the Doppler factor is δ = 15. The characteristic temperature of the accretion disk is T_disk = 3 × 10³ K.

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