\begin{table}%T7
\caption{Spectral data for 0222+36. \label{tab0222+36sp}}
%\centerline
 {
\begin{tabular}{lcccc}
\hline\hline
Frequency & Total & Halo & Lobes & Core \\
(GHz) & (mJy) & (mJy) & (mJy) & (mJy) \\
\hline
0.074 (VLSS)  & 580 & -- & -- & -- \\
0.325 (WENSS) & 380 & 188$^{{a}}$ & 191$^{{b}}$ & 0.9$^{{b}}$ \\
0.365 (TEXAS) & 352 & 174$^{{a}}$ & 177$^{{b}}$ & 1.2$^{{b}}$ \\
0.408 (B2)    & 337 & 170$^{{a}}$ & 165$^{{b}}$ & 1.8$^{{b}}$ \\
1.4 (VLA)  & 190 & 36   & 52   & 102$^{{\rm c}}$ \\
5.0 (VLA)  & 224 & 8    & 36   & 180 \\
8.4 (VLA)  & 192 & nd   & 26   & 166 \\
22.5 (VLA) & 96  & nd   & 6    & 90 \\
\hline 
\end{tabular}
}\smallskip
Notes -- $^a$ The flux density of the halo is computed from subtraction of the
nuclear and lobe components from the total flux density listed in Col.~2; $^b$
lobes and core flux densities at low frequency (0.325, 0.365, and 0.408~GHz)
are extrapolated from data between 1.4 and 22~GHz (see text); $^c$ from VLBA
data at 1.6~GHz.
\end{table}