Table 3: Radio sources detected at 3.6 and/or 6 cm.

Source		 Positiona $S_{\rm 3.6\ cm}$b $S^{\rm peak}_{\rm 3.6\ cm}$c $S_{\rm 6\ cm}$ $S^{\rm peak}_{\rm 6\ cm}$ $\alpha$d Offsete
  RA (2000) Dec (2000) ( $\mu{\rm Jy}$) ( $\mu{\rm Jy/beam}$) ( $\mu{\rm Jy}$) ( $\mu{\rm Jy}$/beam)   ( $^{\prime \prime }$)
L1582A                
1 ...... $05^{\rm h}\ 32^{\rm m}\ 00.5^{\rm s}$ $+12\hbox{$^\circ$ }\ 30^\prime\ 40^{\prime\prime}$ $142\pm23$ $139\pm13$ $280\pm530$ $280\pm30$ $-1.3\pm0.5$ 18
2 ...... $05^{\rm h}\ 32^{\rm m}\ 06.3^{\rm s}$ $+12\hbox{$^\circ$ }\ 32^\prime\ 41^{\prime\prime}$ $200\pm60$ $137\pm26$ - - - 165
3 ...... $05^{\rm h}\ 32^{\rm m}\ 08.9^{\rm s}$ $+12\hbox{$^\circ$ }\ 29^\prime\ 34^{\prime\prime}$ - - $300\pm100$ $180\pm40$ - 138
L1689A                
1 ...... $16^{\rm h}\ 32^{\rm m}\ 23.3^{\rm s}$ $-25\hbox{$^\circ$ }\ 00^\prime\ 34^{\prime\prime} $ $8610\pm130$ $8180\pm70$ $5800\pm600$ $ 4600\pm 500$ $\ \ 0.8\pm0.2$ 235
2 ...... $16^{\rm h}\ 32^{\rm m}\ 25.4^{\rm s}$ $-25\hbox{$^\circ$ }\ 02^\prime\ 16^{\prime\prime} $ $830\pm70$ $490\pm30$ $1100\pm400$ $ 640\pm 170$ $-0.6\ \ \pm0.7$ 188
3 ...... $16^{\rm h}\ 32^{\rm m}\ 13.9^{\rm s}$ $-25\hbox{$^\circ$ }\ 02^\prime\ 25^{\prime\prime} $ $544\pm26$ $496\pm14$ $750\pm70$ $ 740\pm 70$ $-0.63\pm0.21$ 80
4 ...... $16^{\rm h}\ 32^{\rm m}\ 14.2^{\rm s}$ $-25\hbox{$^\circ$ }\ 02^\prime\ 04^{\prime\prime} $ $520\pm30$ $347\pm15$ $550\pm70$ $550\pm70$ $-0.11\ \ \pm0.28$ 101
5 ...... $16^{\rm h}\ 32^{\rm m}\ 13.8^{\rm s}$ $-25\hbox{$^\circ$ }\ 02^\prime\ 38^{\prime\prime} $ $440\pm40$ $174\pm13$ $660\pm60$ $ 640\pm 60$ $-0.79 \pm0.25$ 67
6 ...... $16^{\rm h}\ 32^{\rm m}\ 13.3^{\rm s}$ $-25\hbox{$^\circ$ }\ 03^\prime\ 45^{\prime\prime}$ $58\pm12$ $58\pm12$ - - - 1
B133                
1 ...... $19^{\rm h}\ 06^{\rm m}\ 05.7^{\rm s}$ $-06\hbox{$^\circ$ }\ 50^\prime\ 06^{\prime\prime} $ $31850\pm50$ $28730\pm30$ $67800\pm300$ $66550\pm150$ $-1.48\pm0.01$ 171
2 ...... $19^{\rm h}\ 06^{\rm m}\ 14.0^{\rm s}$ $-06\hbox{$^\circ$ }\ 49^\prime\ 35^{\prime\prime} $ $730\pm130$ $420\pm50$ - - >$1.7\pm0.3$ 214
3 ...... $19^{\rm h}\ 06^{\rm m}\ 08.4^{\rm s}$ $-06\hbox{$^\circ$ }\ 53^\prime\ 32^{\prime\prime} $ $120\pm30$ $71\pm12$ - - - 40
4 ...... $19^{\rm h}\ 06^{\rm m}\ 07.0^{\rm s}$ $-06\hbox{$^\circ$ }\ 53^\prime\ 58^{\prime\prime} $ $100\pm25$ $81\pm13$ - - - 69
B68f                
1 ...... $17^{\rm h}\ 22^{\rm m}\ 35.0^{\rm s}$ $-23\hbox{$^\circ$ }\ 47^\prime\ 58^{\prime\prime} $ $9310\pm40$ $8550\pm21$ - - - 136
2 ...... $17^{\rm h}\ 22^{\rm m}\ 31.8^{\rm s}$ $-23\hbox{$^\circ$ }\ 48^\prime\ 18^{\prime\prime} $ $223\pm24$ $223\pm24$ - - - 145
3 ...... $17^{\rm h}\ 22^{\rm m}\ 28.0^{\rm s}$ $-23\hbox{$^\circ$ }\ 50^\prime\ 32^{\prime\prime} $ $410\pm26$ $410\pm26$ - - - 157
4 ...... $17^{\rm h}\ 22^{\rm m}\ 35.4^{\rm s}$ $-23\hbox{$^\circ$ }\ 52^\prime\ 34^{\prime\prime} $ $150\pm50$ $143\pm27$ - - - 166
a Positional errors are expected to be $\sim$ $1\hbox{$^{\prime\prime}$ }$; b Flux density ( $\mu{\rm Jy}$) and 1-$\sigma $ errors, corrected for the primary beam response; c peak flux density ( $\mu{\rm Jy/beam}$) and 1-$\sigma $ errors, corrected for the primary beam response; d spectral index between 3.6 and 6 cm; e angular displacement of the source from the peak of the submm emission; f B68 was not observed at 6 cm.


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