\begin{table}%t4
\caption{{\it Coronet} sources, radio data.\label{sourceralist}}
%\centerline
{\begin{tabular}{lrrrrrrrrrrr}
\hline\hline
No. &  R1    & R2    & R3    & R4   & R5   & R6   & R7    & R8   & R9    & Combined$^{a}$ & FCW98$^{b}$ \\
    & (mJy) & (mJy) & (mJy) & (mJy)& (mJy)& (mJy)& (mJy) & (mJy)& (mJy) & (mJy)              & (mJy) \\ 
\hline
1  &  0.30  &$<$$0.27^{c}$&$<$$0.30^{c}$& 0.29 & 0.35 & 0.32 &$<$$0.30^{c}$& 0.36 & 0.30  & --		     & 0.67 \\
2  &  0.40  & 0.68  & 1.15  & 1.04 & 0.76 & 0.93 & 0.52  & 1.21 & 0.58  & --		     & 1.08 \\
3  &  n.d.  & n.d.  & n.d.  & n.d. & n.d. & n.d. & n.d.  & n.d. & n.d.  & --		     & n.d. \\ 
4  &  1.96  & 1.10  & 0.75  & 1.32 & 1.11 & 2.97 & 2.31  & 3.28 & 1.67  & --		     & 1.36 \\ 
4$V$   & $<$$0.09^{c}$& 0.22  & 0.15  & 0.25 & 0.26 & 0.29 & 0.34  & 0.65 & 0.36  & --         & 0.23 \\
5  &  n.d.  & n.d.  & n.d.  & n.d. & n.d. & n.d. & n.d.  & n.d. & n.d.  & 0.10  	     & n.d. \\
6  &  n.d.  & n.d.  & n.d.  & n.d. & n.d. & n.d. & n.d.  & n.d. & n.d.  & 0.15  	     & n.d. \\
7  &  0.42  & 0.36  & 0.59  & 0.44 & 0.47 & 0.45 & 0.55  & 0.49 & 0.46  & --		     & 0.45 \\
8  &  n.d.  & n.d.  & n.d.  & n.d. & n.d. & n.d. & n.d.  & n.d. & n.d.  & $<$$0.035^{c}$   & n.d. \\
9  &  0.16  & 0.21  & 0.17  & 0.22 & 0.17 & 0.23 & 0.24  & 0.20 & 0.26  & --		     & 0.23 \\
10 &  n.d.  & n.d.  & n.d.  & n.d. & n.d. & n.d. & n.d.  & n.d. & n.d.  & 0.12  	     & n.d. \\
11 &  0.93  & 0.78  & 0.89  & 0.85 & 0.78 & 0.72 & 1.04  & 0.94 & 0.84  & --		     & 1.58 \\
12 &  4.26  & 4.15  & 5.01  & 4.27 & 4.31 & 4.11 & 5.29  & 4.52 & 4.31  & --		     & 3.74 \\
13 &  n.d.  & n.d.  & n.d.  & n.d. & n.d. & n.d. & n.d.  & n.d. & n.d.  & 0.11  	     & n.d. \\
14 &  1.38  & 1.53  & 2.10  & 1.66 & 1.83 & 1.54 & 2.04  & 1.75 & 1.62  & --		     & 2.03 \\
15 &  n.d.  & n.d.  & n.d.  & n.d. & n.d. & n.d. & n.d.  & n.d. & n.d.  & 0.13  	     & n.d. \\
\hline
\end{tabular}}
\par
\smallskip
$^{a}$ Sources detected in combined AM596 data (10~h). \\
$^{b}$ 3.5~cm flux on 19/20 Jan 1997, as published by \citet{fcw98}.\\
$^{c}$ Local 3$\sigma$ limit, in the case of IRS~2: accounting for primary beam attenuation. \\
\end{table}