PKS 0537-286, carrying the information of the environment of SMBHs in the early Universe

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Table 9:

List of parameters used to construct the theoretical SED.
$R_{\rm diss}$	M	$R_{\rm BLR}$	$P^\prime_{\rm i}$	$L_{\rm d}$	B	$\Gamma$	$\theta_{\rm v}$	$\gamma_{\rm b}$	$\gamma_{\rm max}$	s₁	s₂
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)	(11)	(12)
4.2 (2)	7	$1.3\times10$ ³	0.3	168 (0.16)	0.1	18	3	40	10⁴	-1	2.6
3.2 (1.5)	7	916	0.2	84 (0.08)	0.09	18	3	25	10⁴	-1	2.6

Explanation of columns: (1) = dissipation distance in units of 10¹⁸ cm and (in parenthesis) in units of 10³ $R_{\rm S}$ ; the (spherical) emitting size is ten times smaller; (2) = black hole mass in 10⁹ solar masses; (3) = size of the BLR in units of 10¹⁵ cm; (4) = power injected in the blob calculated in the comoving frame, in units of 10⁴⁵ erg s^-1; (5) = accretion-disk luminosity in units of 10⁴⁵ erg s^-1 and (in parenthesis) in units of $L_{\rm Edd}$ ; (6) = magnetic field in Gauss; (7) = bulk Lorentz factor at $R_{\rm diss}$ ; (8) = viewing angle in degrees; (9) and (10) = break and maximum random Lorentz factors of the injected electrons; (11) and (12) = slopes of the injected electron distribution ( $Q(\gamma)$ ) below and above $\gamma_{\rm b}$ .

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