\begin{table}%t3
\caption{Radio sources detected at 3.6 and/or 6~cm.
\label{tab:radiosources}      }
%\centerline
 {\begin{tabular}{lcccccccc}
\hline\hline        
\noalign{\smallskip}
Source &\multicolumn{2}{c}{Position$^a$ 
} &
 $S_{\rm 3.6\ cm}$$^b$  
& $S^{\rm peak}_{\rm 3.6\ cm}$$^c$&
 $S_{\rm 6\ cm}$ & $S^{\rm peak}_{\rm 6\ cm}$
& $\alpha$$^d$
& Offset$^e$ 
 \\
 & RA (2000) & Dec (2000) &($\mu{\rm Jy}$)  & ($\mu{\rm Jy/beam}$) & 
($\mu{\rm Jy}$)& ($\mu{\rm Jy}$/beam)& & (\arcsec)\\
\noalign{\smallskip}
\hline                        
\noalign{\smallskip}
%----------------------------------------------------------------------------------------------------------------------
L1582A & & & & & &\\
1  \ldots\dots& 
$05^{\rm h}\ 32^{\rm m}\ 00.5^{\rm s}$ & $+12\degr\ 30^\prime\ 40^{\prime\prime}$ & $142\pm23$ &$139\pm13$& $280\pm530$ & $280\pm30$ &$-1.3\pm0.5$ & 18 \\
2  \ldots\dots& 
$05^{\rm h}\ 32^{\rm m}\ 06.3^{\rm s}$ & $+12\degr\ 32^\prime\ 41^{\prime\prime}$&$200\pm60$&$137\pm26$ &--&--&-- & 165 \\
3  \ldots\dots&
$05^{\rm h}\ 32^{\rm m}\ 08.9^{\rm s}$ &  $+12\degr\ 29^\prime\ 34^{\prime\prime}$ &--&  -- & $300\pm100$ &$180\pm40$ &--& 138\\
%----- L1689A ------------------------------------------------------------------------------------------------------------
L1689A & & & & & & & &\\
1  \ldots\dots&
 $16^{\rm h}\ 32^{\rm m}\ 23.3^{\rm s}$ & $-25\degr\ 00^\prime\ 34^{\prime\prime} $ & $8610\pm130$& $8180\pm70$ & $5800\pm600$  & $ 4600\pm 500$ & $\ \ 0.8\pm0.2$& 235\\
2  \ldots\dots&
 $16^{\rm h}\ 32^{\rm m}\ 25.4^{\rm s}$ & $-25\degr\ 02^\prime\ 16^{\prime\prime} $  &$830\pm70$& $490\pm30$    & $1100\pm400$  &$ 640\pm 170$ & $-0.6\ \ \pm0.7$& 188\\
3  \ldots\dots& 
$16^{\rm h}\ 32^{\rm m}\ 13.9^{\rm s}$ & $-25\degr\ 02^\prime\ 25^{\prime\prime} $  &$544\pm26$& $496\pm14$     & $750\pm70$ & $ 740\pm 70$ &$-0.63\pm0.21$ & 80\\
4  \ldots\dots&
 $16^{\rm h}\ 32^{\rm m}\ 14.2^{\rm s}$ & $-25\degr\ 02^\prime\ 04^{\prime\prime} $  &$520\pm30$&  $347\pm15$   & $550\pm70$ & $ 550\pm 70$ & $-0.11\  \ \pm0.28$&  101 \\
5  \ldots\dots&
 $16^{\rm h}\ 32^{\rm m}\ 13.8^{\rm s}$ & $-25\degr\ 02^\prime\ 38^{\prime\prime} $  &$440\pm40$& $174\pm13$    & $660\pm60$& $ 640\pm 60$ &$-0.79 \pm0.25$&  67\\
6  \ldots\dots& 
$16^{\rm h}\ 32^{\rm m}\ 13.3^{\rm s}$ & $-25\degr\ 03^\prime\ 45^{\prime\prime} $  &$58\pm12$& $58\pm12$       &-- &--&-- & 1\\
%------ B133 %-----------------------------------------------------------------------------------------------------
B133 & & & &  & & \\
1 \ldots\dots & 
$19^{\rm h}\ 06^{\rm m}\ 05.7^{\rm s}$ & $-06\degr\ 50^\prime\ 06^{\prime\prime} $& $31850\pm50$ & $28730\pm30$ &$67800\pm300$ &$66550\pm150$& $-1.48\pm0.01$& 171\\
2 \ldots\dots & 
$19^{\rm h}\ 06^{\rm m}\ 14.0^{\rm s}$ & $-06\degr\ 49^\prime\ 35^{\prime\prime} $& $730\pm130$&$420\pm50$&-- &--&$>$$1.7\pm0.3$& 214\\
3 \ldots\dots & 
$19^{\rm h}\ 06^{\rm m}\ 08.4^{\rm s}$ & $-06\degr\ 53^\prime\ 32^{\prime\prime} $& $120\pm30$&$71\pm12$&-- &-- &--&40\\
4 \ldots\dots & 
$19^{\rm h}\ 06^{\rm m}\ 07.0^{\rm s}$ & $-06\degr\ 53^\prime\ 58^{\prime\prime} $& $100\pm25$&$81\pm13$&-- &--&--&69\\
%--------- B68 --------------------------------------------------------------------------------------------------------
B68$^f$ & & & & & & &\\
1   \ldots\dots  & 
$17^{\rm h}\ 22^{\rm m}\ 35.0^{\rm s}$ & $-23\degr\ 47^\prime\ 58^{\prime\prime} $& $9310\pm40$ &$8550\pm21$ &  -- &--  & -- &136\\
2   \ldots\dots  & 
$17^{\rm h}\ 22^{\rm m}\ 31.8^{\rm s}$ & $-23\degr\ 48^\prime\ 18^{\prime\prime} $& $223\pm24$&$223\pm24$ &  -- & --&-- & 145\\
3   \ldots\dots  & 
$17^{\rm h}\ 22^{\rm m}\ 28.0^{\rm s}$ & $-23\degr\ 50^\prime\ 32^{\prime\prime} $& $410\pm26$&$410\pm26$ &   -- &--&-- & 157\\
4   \ldots\dots  & 
$17^{\rm h}\ 22^{\rm m}\ 35.4^{\rm s}$ & $-23\degr\ 52^\prime\ 34^{\prime\prime} $& $150\pm50$& $143\pm27$ &   -- &--& -- & 166\\
\noalign{\smallskip}
\hline                        
\end{tabular}}
\par
\smallskip
$^a$ Positional errors are expected to be $\sim$$1\arcsec$;
$^b$ {Flux density ($\mu{\rm Jy}$) and 1-$\sigma$ errors,
corrected for the primary beam response;}
$^c$ {peak flux density ($\mu{\rm Jy/beam}$)
and 1-$\sigma$ errors,
corrected for the primary beam response;}
$^d$ {spectral index between~3.6 and 6~cm;}
$^e$ {angular displacement of the source from the peak of the submm emission;}
$^f$ {B68 was not observed at 6~cm.}
\par
\end{table}