\begin{table}%t2
%\centering
\par
\caption{\label{VLA-sources}Details of the detected compact VLA~sources in our VLA~observations on 2004 November~2 (A~configuration) and 2008 March 24 (C~configuration). Shown are also the flux densities at 22~GHz from~UA97 from their observations with the A~and B~configuration.}
\small
 \begin{tabular}{lcccccccccc}
\hline\hline
Config&Source&$\alpha_{J2000}$ & $\delta_{J2000}$& Major axis& Minor axis& P.A. & Peak flux& Integrated flux& $S_\nu$ (VLA-A) &$S_\nu$ (VLA-B)\\
& &00$^{\rm h}$47$^{\rm m}$ & --25\degr17\arcmin & [\arcsec] & [\arcsec] & [$^\circ$]& [mJy]    & [mJy] &[mJy]&[mJy]\\
\hline
A & TH1        & 33\fs30 & 15\farcs54 & $0.24\pm0.02 $ & $0.17\pm0.02 $ & $ 16\pm1$0 & $ 3.8\pm0.4$ &  $9.1\pm1.2$ &  2.09 &  6.72\\
A & TH2        & 33\fs18 & 17\farcs15 & $0.22\pm0.004$ & $0.13\pm0.002$ & $  4\pm1$  & $23.6\pm0.4$ & $38.4\pm0.9$ & 21.53 & 35.79\\
A & TH4        & 33\fs17 & 17\farcs48 & $0.26\pm0.007$ & $0.16\pm0.005$ & $  6\pm2$  & $12.5\pm0.4$ & $29.9\pm1.2$ &  3.78 &  9.69\\
A & TH6        & 33\fs11 & 18\farcs16 & $0.40\pm0.04 $ & $0.24\pm0.02 $ & $176\pm7$  & $ 3.9\pm0.4$ & $21.9\pm2.3$ &  0.94 &  7.88\\
A & TH7        & 33\fs01 & 19\farcs42 & $0.26\pm0.03 $ & $0.19\pm0.02 $ & $ 15\pm1$3 & $ 3.7\pm0.4$ & $10.7\pm1.4$ &  0.88 &  5.84\\
A & TH8        & 32\fs98 & 19\farcs73 & $0.28\pm0.03$  & $0.20\pm0.02 $ & $ 21\pm1$1 & $ 3.9\pm0.4$ & $13.0\pm1.5$ &  1.82 &  5.72\\
A &            & 32\fs93 & 20\farcs31 & $0.26\pm0.04$  & $0.25\pm0.04 $ & $ 48\pm9$0 & $ 2.4\pm0.4$ &  $9.2\pm1.7$ & --    & --   \\
A & TH9        & 32\fs88 & 21\farcs38 & $0.21\pm0.01$  & $0.13\pm0.006$ & $177\pm4$  & $ 7.8\pm0.4$ & $13.1\pm0.9$ &  3.57 &  9.79\\
C & 4.81--43.6 & 32\fs22 & 21\farcs7  & $3.5 \pm0.7 $   &$ 1.1\pm0.2  $  & $  1\pm5$  & $ 0.5\pm0.1$ &  $1.4\pm0.4$ & --    & --   \\
C & 6.40--37.1 & 33\fs79 & 15\farcs3  & $1.5 \pm0.2 $   &$ 0.9\pm0.1  $  & $177\pm9$  & $ 0.9\pm0.1$ &  $0.8\pm0.2$ & --    & --   \\
C & 6.81--29.6 & 34\fs20 & 08\farcs1  & $1.9 \pm0.3 $   &$ 0.8\pm0.1  $  & $  8\pm6$  & $ 0.8\pm0.1$ &  $0.9\pm0.2$ & --    & --   \\
\hline 
\end{tabular}
\end{table}