Table 1: Identification with sources in Linden-Vørnle et al.
\begin{displaymath}{ \begin{tabular}{lrllr@{$\;\pm\;$}l} \hline \hline \mult... ...$\pm$ 27 & & 1NW023/092 & 434 & 57 \\ \hline \end{tabular}}\end{displaymath}
a The flux values by Linden-Vørnle et al. are multiplied by a factor of 1.63 so that the C_90 flux of Lockman E4_1 (UGC06009) is equal to the IRAS value.
b These sources are detected by DAOPHOT, but with $SNR{\rm s} < 3$.

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