**Table 1:** Radio properties of selected AGNs.
Source name	z	$L_{1.4~{\rm GHz}}$ ^a	Log $\left(\frac{L(5~\mu{\rm m})}{\nu L_{1.4~{\rm GHz}}}\right)$
		(W Hz^-1)
IsOQ/LH_A4	2.54	25.04 $\pm$ 0.02	5.27
IsOQ/LH_A5	1.94	24.54 $\pm$ 0.02	4.97
IsOQ/LH_A6	2.20	24.42 $\pm$ 0.03	5.09
IsOQ/LH_A8	2.42	26.71 $\pm$ 0.02	3.22
IsOQ/N2_09	1.98	25.69 $\pm$ 0.03	4.15
MIPS22204	2.08	25.68 $\pm$ 0.02	4.30
Median(IsOQ)^b	2.14 $\pm$ 0.19	25.68 $\pm$ 0.68	4.97 $\pm$ 0.61
Range(IsOQ)^b	1.94-2.54	24.42-26.71	3.22-5.27
Median(HzRG)	1.90 $\pm$ 0.53	27.89 $\pm$ 0.48	1.11 $\pm$ 0.37
Range(HzRG)	1.08-3.09	26.55-28.53	0.60-2.30
Median(SMG/AGN)	2.20 $\pm$ 0.43	24.31 $\pm$ 0.28	4.25 $\pm$ 0.39
Range(SMG/AGN)	0.98-2.58	23.25-24.63	3.71-5.18

^a The radio luminosities are from the deep VLA survey of the Lockman Hole (Polletta et al. 2006, Owen et al., in prep.) for LH_A4, LH_A5, LH_A6, and LH_A8, from the FIRST survey for N2_09, and from the VLA-FLS survey (Sajina et al. 2007b) for MIPS22204. The radio luminosities for the HzRGs and SMG/AGNs are from Seymour et al. (2007) and Pope et al. (2006), respectively.
^b Includes only the 6 IsOQs with available radio data. The median redshift for the whole IsOQ sample is $2.23\pm0.31$ , and the redshift range is 1.29-2.96.

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