\begin{table}%t2
\caption{\label{table:radio:atca}ATCA results. Given are the peak coordinates, peak and
  integrated  flux densities, and sizes.} 
%\centerline
{
\begin{tabular}[h]{cccccccccccc}
\hline \hline \\[-5pt]
\multicolumn{1}{c}{}&
\multicolumn{5}{c}{4.8 GHz} &
\multicolumn{1}{c}{}&
\multicolumn{5}{c}{8.6 GHz} \\
\cline {2-6} \cline {8-12}\\[-5pt]
\multicolumn{1}{c}{Source} &
\multicolumn{1}{c}{Component} &
\multicolumn{1}{c}{Peak coordinates$^a$} &
\multicolumn{1}{c}{Peak$^{b}$} &
\multicolumn{1}{c}{Integ.$^{c,\lhd}$} &
\multicolumn{1}{c}{Source$^d$} &
\multicolumn{1}{c}{} &
\multicolumn{1}{c}{Comp.} &
\multicolumn{1}{c}{Peak coordinates$^a$} &
\multicolumn{1}{c}{Peak$^{b}$} &
\multicolumn{1}{c}{Integ.$^{c,\lhd}$} &
\multicolumn{1}{c}{Source$^d$} \\
\multicolumn{2}{c}{} &
\multicolumn{1}{c}{(RA, Dec)} &
\multicolumn{1}{c}{$S_{\nu}$} &
\multicolumn{1}{c}{$S_{\nu}$} &
\multicolumn{1}{c}{size} &
\multicolumn{2}{c}{} &
\multicolumn{1}{c}{(RA, Dec)} &
\multicolumn{1}{c}{$S_{\nu}$} &
\multicolumn{1}{c}{$S_{\nu}$} &
\multicolumn{1}{c}{size} \\[5pt]
\hline \\[-5pt]
IRAS 10589  
& & 11:01:00.16 $-$60:50:22.4 & 79 & 1218 & $14\times12$ &
& & 11:01:00.20 $-$60:50:22.2 & 24 & 1343 & $14\times12$\\%[2pt]
IRAS 11143
& & 11:16:32.91 $-$61:30:12.7 & 6 & 2733 & $81\times54^{\natural}$ & 
& & $\star$\\%[2pt]
IRAS 12063
& & & & 1961 & $28\times25$ & 
& & & & 1400 & $16\times7$\\
... & A              & 12:09:01.12 $-$63:15:52.9 & 158 & & & 
    & A              & 12:09:01.04 $-$63:15:52.9 &  63 & \\
... & B              & 12:09:01.01 $-$63:16:00.8 & 106 & & & 
    & B1$^\triangle$ & 12:09:00.99 $-$63:15:59.3 &  41 & \\
& & & & & & 
    & B2$^\triangle$ & 12:09:01.17 $-$63:16:02.2 & 37  & \\%[2pt]
IRAS 12073 
& & & & 15~377$^\Diamond$ & & 
& & & & 12~853$^\Diamond$\\
... & A & 12:10:01.11 $-$62:49:53.9 & 383 & 4955 & $9\times7$ & 
    & A & 12:10:01.06 $-$62:49:53.6 & 184 & 4098 & 5.8\\
... & B & 12:09:57.88 $-$62:49:33.5 & 141 & 1145 & $10\times5$ & 
    & B & 12:09:58.10 $-$62:49:32.8 &  57 &  656 & $4.5\times1.8$\\%[2pt]
IRAS 12331
& & 12:36:01.23 $-$61:51:18.8 & 15 & 3528 & $73\times62$ &  
& & 12:36:01.28 $-$61:51:17.7 &  4 & 2699 & $68\times52$\\%[2pt]
IRAS 15384
& & 15:42:16.86 $-$53:58:33.4 & 59 & 4753        & $44\times37$ & 
& & 15:42:16.87 $-$53:58:33.8 & 16 & 3505        & $31.5\times26$\\%[2pt]
IRAS 15502 
& & & & 2172 & &  
& & & & 3202\\
... & A & 15:54:06.40 $-$53:11:40.2 & 555 & 1853 & 4.7 & 
    & A & 15:54:06.43 $-$53:11:40.6 & 543 & 3013 & 3.6\\
... & B & 15:54:05.26 $-$53:11:39.4 & 90  &  234 & 2.5 & 
    & B & $\rhd$\\
IRAS 16128
& & & &  9266$^\Diamond$ & $22.5\times14 ^\dagger$ &
& & & &  5795              & $22.5\times14 ^\dagger$ \\
... & A             & 16:16:41.06 $-$51:17:02.0 & 182 & & & 
    & A             & 16:16:41.06 $-$51:17:02.1 & 65\\
... & B             & 16:16:40.55 $-$51:17:08.5 & 161 & & &
    & B             & 16:16:40.78 $-$51:17:09.2 & 45\\
... & C             & 16:16:40.32 $-$51:17:13.1 & 155 & & &
    & C             & 16:16:40.44 $-$51:17:08.2 & 55\\
... & D             & 16:16:40.25 $-$51:17:13.1 & 164 & & &
    & D             & 16:16:40.23 $-$51:17:13.0 & 74\\%[2pt]
IRAS 17160
& & & & 5475$^\Diamond$ \\
... & A & 17:19:27.51 $-$37:11:02.7 & 123 & 1230$^\ddagger$ & 13$^\dagger$ &
    & A & 17:19:27.48 $-37$:11:04.6 &  41 & 2365            & $27\times19$\\
... & B & 17:19:26.92 $-$37:10:24.6 &  49 &  110            & 4.4 & 
    & B & 17:19:27.01 $-37$:10:25.2 &  14 &   67            & 3.2 \\
... & C & 17:19:32.74 $-$37:10:46.8 &  53 &  200            & $10\times5$ & 
    & C & 17:19:32.76 $-37$:10:47.4 &  18 &   54            & 2.7 \\
... & D & 17:19:35.69 $-$37:10:56.5 & 142 &  213            & 3.1 & 
    & D & 17:19:35.68 $-37$:10:56.4 &  81 &  223            & 2.2\\
... & E & 17:19:25.55 $-37$:10:04.6 &  4 &     5            & $<2.3$ &  
    & E & 17:19:25.60 $-37$:10:04.9 &  38 &   39            & $<$1.1\\%[2pt]
IRAS 17221
& & 17:25:31.05 $-$36:21:51.9 & 19 & 2905 & 67 &  
& & 17:25:31.01 $-$36:21:52.1 &  5 & 1479 & 44\\ 
IRAS 17279
& & & & 1532$^\Diamond$ & &\\
... & A & 17:31:17.62 $-$33:52:45.4 & 24 &     & $16\times11^\dagger$ & 
    & A & 17:31:17.63 $-$33:52:45.1 & 10 & 517 & 20$^\dagger$\\
... & B & 17:31:20.54 $-$33:53:25.7 & 95 & 103 & 2.7 & 
    & B & 17:31:20.54 $-$33:53:25.7 & 46 & 62  & 1.9\\
... & C & 17:31:15.04 $-$33:51:16.0 & 85 & 124 & 3.4 & 
    & C & 17:31:15.03 $-$33:51:15.8 & 47 & 113 & 2.0\\
     \\[-8pt] \hline \\[-10pt]
   \end{tabular}} 
   \smallskip  
$^a$ Coordinates in right ascension and declination (J2000.0); the
units of right ascension are hours, minutes and seconds; the units of
declination are degrees, arcmin and arcsec.
\\
$^b$ Peak flux density in mJy beam$^{-1}$.
$^c$ Total integrated flux density in mJy.
$^d$ Source size in arcsec.
$^\natural$ The structure on the north extends up to 40\arcsec.
$^\star$ Not properly reconstructed.
\\
$^\triangle$ The component B observed at 4.8 GHz 
is decomposed in two
components (B1 and B2) by the 8.6 GHz observation.
$^\rhd$ Weak component.
$^\dagger$ Core size.
$^\ddagger$ Core flux density.
\\
$^\Diamond$ Emission integrated over the whole field.
($\lhd$) Uncertainty is not larger than 10\%.
\end{table}