\begin{table}%t2
\caption{\label{tab:cr_point_sources}Unresolved sources which are denoted in Figs.~\ref{fig:n253v90_tp_dss_b70}$-$\ref{fig:n253cm3e_tp_clean_dss_b84}. The error of the flux densities was calculated assuming a~5\% calibration error.}
%\centering
\small
\begin{tabular}{l|lllllll}
\hline\hline
No. \T\B & RA & Dec & $S_{\lambda90}~{\rm [mJy]}$ &
$S_{\lambda20}~{\rm [mJy]}$ & $S_{\lambda6.2}~{\rm [mJy]}$ &
$S_{\lambda3.6}~{\rm [mJy]}$ & $\alpha$\\
\hline
1 \T & $00^{\rm h} 47^{\rm m} 00\fs02$ & $-25^\circ 23' 50\farcs1$ & &
$4.1\pm 0.2$ & $2.2\pm 0.1$ & & $0.5\pm0.2$\\ 
2 & $00^{\rm h} 47^{\rm m} 12\fs01$ & $-25^\circ 17' 43\farcs9$ & &
$17.3\pm 1.0$ & $6.6\pm 0.3$ & & $0.8\pm0.2$\\ 
3 & $00^{\rm h} 47^{\rm m} 33\fs12$ & $-25^\circ 17' 17\farcs3$ &
$3960\pm 80$ & $2040\pm 100$ & $1270\pm 60$ & $980\pm 50$ &
$0.44\pm0.02$\\ 
4 & $00^{\rm h} 47^{\rm m} 44\fs91$ & $-25^\circ
13' 38\farcs4$ & & $26\pm 2$ & $7.9\pm 0.4$ & & $1.0\pm0.2$\\ 
5 & $00^{\rm h} 47^{\rm m} 52\fs41$ & $-25^\circ
15' 44\farcs8$ & & & $1.5\pm 0.2$ & &\\ 
6 & $00^{\rm h} 47^{\rm m} 58\fs90$ & $-25^\circ 18' 31\farcs9$ &
$190\pm 10$ & $53\pm 3$ & $19\pm 1$ & $9.5\pm 0.5$ & $0.84\pm0.02$\\ 
7 & $00^{\rm h} 48^{\rm m} 00\fs84$ & $-25^\circ 16' 26\farcs3$ & &
$2.1\pm 0.3$ & $1.10\pm 0.06$ & & $0.5\pm0.2$\\ 
8 \B & $00^{\rm h} 48^{\rm m} 05\fs0$ & $-25^\circ 11' 11\farcs8$ & &
$5.3\pm 0.3$ & $3.05\pm 0.15$ & & $0.4\pm0.2$\\
\hline
\end{tabular}
\end{table}