\begin{table}%T1
\caption{\label{tab1}Radio emission data of the sources in the three
epochs of the observations (a = 22 Aug. 1998; b = 10 Sep. 1998; c = 21
Sep. 1998).   
Column~[1], IAU name; Col.~[2] optical id.; Col.~[3] redshift
(values in parentheses are photometric redshifts, using the GPS~galaxy
Hubble diagram); Cols.~[4]$-$[7]
flux density of the arc second core and any additional radio emission
at 1.36 and 1.66~GHz
(values in parentheses indicate that in our judgment, the radio
emission likely comes from an unrelated object). Flux density errors
for compact strong components are dominated by the calibration
uncertainties estimated around 3$\%$, while for extended weak
components the flux density errors are dominated by the limits of the
self-cal/imaging process in the presence of a strong source nearby,
and the flux densities given can be considered only rough estimates.
* ~It accounts for the region South of the arcsecond core only.}
%\centering
\par
\begin{tabular}{llc|rr|rr}
\hline \hline
\multicolumn{3}{c}{}& \multicolumn{2}{c}{1.36~GHz} &     \multicolumn{2}{c}{1.66~GHz} \\
\hline 
Name&id & $z$ & Peak & Extended & Peak & Extended  \\
& & &mJy & mJy & mJy & mJy  \\
\hline
B0019--000a &G& 0.305 & 2932 & -- &  2652 & --   \\
 B0108+388ac&G& 0.669 & 414  & 9.3&  595 & 6.0   \\
B0237--233a &Q& 2.223 & 6282 & (62.0)  & 5950 & (51.5)  \\
 B0248+430a &Q& 1.310 & 1197 & (26.2) &  1281 & (25.1)\\
 B0316+162a &G& (1.57)& 7820 & (25.0) &  7167 & (21.9)  \\
 B0428+205a &G& 0.219 & 3720 & --  &  3665 & -- \\
 B0457+024a &Q& 2.384 & 2242 & -- &   2417 & --\\
 B0457+024c &Q& 2.384 & 2248 & --  &    2232 & -- \\
 B0500+019a &G& 0.583 & 2144 & (42.1) &   2341 & (30.5) \\
 B0710+439a &G& 0.518 & 1953 & -- &     &        \\
 B0738+313a &Q& 0.631 & 2036 & 86 &    2461 & 57 \\
 B0742+103a &Q& 2.624 & 3308 & -- &   3795 & --  \\
B0743--006a &Q& 0.994 & 690  & (25.2) &   841 & (17.9)  \\
B0941--080ab&G& 0.228 & 2725 & 31.1 &  2401 & 24.4 \\
 B1031+567a &G& 0.460 & 1791 & -- &  1741 & -- \\
 B1117+146a &G& 0.362 & 2445 & -- &  2153 & --  \\
B1127--145b &Q& 1.187 & 5448 & 96.2 &5371&75.4  \\
B1143--245b &Q& 1.940 & 1557 & --    &1676&-- \\
B1245--197b &Q& 1.273 & 5322 &(54.6)& 4708 &(45.4)     \\
 B1323+321a &G& 0.369 & 4855 & -- &   4339 & --  \\
 B1345+125ac&G& 0.122 & 5262 & 35.4 &   4734 & 32.1 \\
 B1358+624c &G& 0.431 & 4357 & -- &   3860 & -- \\
 B1404+286a &G& 0.077 & 792  & (7.3) &   1070 & (5.8)  \\
 B1442+101a &Q& 3.522 & 2432 & -- &    2220 & --  \\
 B1518+047a &Q& 1.296 & 3963 & (243) &    3457 & (211)  \\
 B1600+335a &G& (1.10) & 2914 & -- &  2834 & --  \\
 B1607+268a &G& 0.473 & 4875 & -- & 4387 & -- \\
B2008--068a &G& (0.70) & 2576 & (55.4) &   2523 & (58.3)  \\
B2126--158a &Q& 3.270 &  562 & -- &  684 & --  \\
 B2128+048a &G& 0.990 & 3970 & (19.2) &  3747 & (18.5)  \\
 B2134+004a &Q& 1.932 & 3412 & 11.0* &  4608 &  7.1* \\
 B2210+016a &G& (0.68)  & 2823 & -- &  2522 & --\\
 B2342+821a &Q& 0.735 & 3797 & --  & 3286 & -- \\
 B2352+495a &G& 0.237 & 2532 & --  & 2390 & --  \\
 \hline
\end{tabular}
\end{table}