Table 2: ATCA results. Given are the peak coordinates, peak and integrated flux densities, and sizes.
  4.8 GHz   8.6 GHz
Source Component Peak coordinatesa Peakb Integ.$^{c,\lhd}$ Sourced   Comp. Peak coordinatesa Peakb Integ.$^{c,\lhd}$ Sourced
  (RA, Dec) $S_{\nu}$ $S_{\nu}$ size   (RA, Dec) $S_{\nu}$ $S_{\nu}$ size
IRAS 10589   11:01:00.16 -60:50:22.4 79 1218 $14\times12$     11:01:00.20 -60:50:22.2 24 1343 $14\times12$
IRAS 11143   11:16:32.91 -61:30:12.7 6 2733 $81\times54^{\natural}$     $\star$      
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    
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 $4.5\times1.8$
IRAS 12331   12:36:01.23 -61:51:18.8 15 3528 $73\times62$     12:36:01.28 -61:51:17.7 4 2699 $68\times52$
IRAS 15384   15:42:16.86 -53:58:33.4 59 4753 $44\times37$     15:42:16.87 -53:58:33.8 16 3505 $31.5\times26$
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    
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
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
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 $^{\prime \prime }$. $^\star$ 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%.

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