sample of 96 sources with deep 1.4 GHz data available is the subject of this paper.

The spectral indices and flux density distributions of the full sample of 296 sources studied in Paper I and the sub-sample of 96 sources studied in this paper are plotted in Fig. \[fig:sample\_properties\]. The spectral index distributions of the two samples are relatively similar, although all nine of the very steeply rising sources, with $\alpha^{15.7}_{1.4} < -0.8$, in the full sample are not included in the sample studied in this paper. Seven of these nine sources are below the 10C completeness limits (0.5 mJy in the deep regions and 1 mJy in the shallow regions) and are not detected at 1.4 GHz so the spectral indices are upper limits calculated from the $3\sigma$ noise in the WSRT map. The flux density distributions of the full sample and sub-sample used in this paper are also very similar, although none of the faintest sources in the full sample appear in the sample studied here, as this sample only contains sources above the 10C completeness limits (0.5 and 1 mJy in the deep and shallow regions respectively).

The Lockman Hole SERVS Data Fusion {#section:FUSED-data}
----------------------------------

The *Spitzer* 