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

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Table 10:

List of parameters used to construct the theoretical SED.
$\log P_{\rm r}$	$\log P_{\rm B}$	$\log P_{\rm e}$	$\log P_{\rm p}$
(1)	(2)	(3)	(4)
46.5	45.3	46.6	48.0
46.2	45.0	46.4	48.0

Explanation of columns: (1), (2), (3) and (4): jet power in the form of radiation, magnetic field, bulk motion of electrons and protons (assuming one proton per emitting electron). These powers are derived quantities, not input parameters. For all cases the X-ray corona luminosity $L_{\rm X}=0.3 L_{\rm d}$ . Its spectral shape is assumed to be $\propto$ $\nu^{-1} \exp(-h\nu/150~{\rm keV})$ .

Source LaTeX | All tables | In the text

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