**Table 1:** Source properties.
Source	Class	z	$N_{\rm H,Gal}$	$\log M_{\rm BH}^a$	$S_{\rm core,5GHz}^b$	$S_{\rm tot,5GHz}^b$	$\Re^b$
			$[{\rm 10^{20}~cm^{-2}}]$	$[M_{\odot}]$	[Jy]	[Jy]	$[S_{\rm core}/S_{\rm ext}]$
NGC 1692	FRI	0.035	3.54	9.01	0.04	1.81	0.023
PKS 0625-35	FRI	0.055	7.08	9.19	0.60	2.12	0.395
3C 88	FRI/FRII	0.030	8.81	8.70	0.16	2.14	0.087
3C 444	FRII	0.153	2.61	9.28	<0.002	1.99	<0.0009

^a From Bettoni et al. (2003); the uncertainty is $\sim$ 0.4 dex.
^b From Morganti et al. (1993).

Source LaTeX | All tables | In the text