\begin{table} %t4
\caption{\label{res}1.2~mm and radio data.}
%\centerline
 {\begin{tabular}{lcccccccc}
\hline\hline
Source ID  & $F_{\rm{1.2~mm}}$$^a$ & $F_{\rm{20~cm}}$$^b$ & $F_{\rm{50~cm}}$$^b$ & $F_{\rm{90~cm}}$$^b$ & Major axis & Minor axis &  $\alpha$$^c$ & $q$ \\
  & (mJy) & ($\mu$Jy) & ($\mu$Jy) & ($\mu$Jy) & ($\arcsec$) & ($\arcsec$) &  &  \\
\hline
\multicolumn{9}{c}{1.2~mm detections {\it S/N}~$>$~4}\\
L-1  	&	  2.95~$\pm$~0.66 	&		   76.3~$\pm$~9.0 	&	 142~$\pm$~19 	&	      327~$\pm$~74 	&	  \textless2.9 	&	   X 	&	 $-$0.84~$\pm$~0.18		&	 2.49$^{+0.20}_{-0.20}$ \\																	
\vspace{0.4 ex}	
L-9  	&	  4.00~$\pm$~0.55 	&		  116.5~$\pm$~9.2 	&	 195~$\pm$~22 	&	      266~$\pm$~69 	&	           1.9	&	 0.7	&	 $-$0.54~$\pm$~0.03		&	 2.35$^{+0.20}_{-0.20}$ \\
\vspace{0.4 ex}																		
L-11 	&	  3.08~$\pm$~0.58 	&		  314.8~$\pm$~4.1 	&	 425~$\pm$~43 	&	      651~$\pm$~72 	&	             X 	&	   X 	&	 $-$0.45~$\pm$~0.06		&	 2.06$^{+0.25}_{-0.25}$ \\
\vspace{0.4 ex}																		
L-22 	&	  3.41~$\pm$~0.73 	&		  100.9~$\pm$~7.1 	&	 238~$\pm$~26 	&	      447~$\pm$~70 	&	  \textless1.7 	&	   X 	&	 $-$1.02~$\pm$~0.01		&	 2.00$^{+0.23}_{-0.23}$ \\
\hline
\multicolumn{9}{c}{1.2~ mm tentative detections ${\it S/N}>3$}\\
L-5  	&	  2.75~$\pm$~0.76 	&		  71.0~$\pm$~20.0 	&	 177~$\pm$~23 	&	      322~$\pm$~74 	&	  \textless4.5 	&	   X 	&	 $-$1.03~$\pm$~0.06		&	 2.28$^{+0.21}_{-0.21}$ \\
\vspace{0.4 ex}																		
L-14 	&	  2.13~$\pm$~0.71 	&		  159.5~$\pm$~6.0 	&	 322~$\pm$~33 	&	      426~$\pm$~70 	&	           0.7	&	   X 	&	 $-$0.73~$\pm$~0.09		&	 1.81$^{+0.26}_{-0.26}$ \\
\vspace{0.4 ex}																		
L-15 	&	  2.36~$\pm$~0.62 	&	           68.6~$\pm$~3.7 	&	 181~$\pm$~21 	&	      258~$\pm$~69 	&	  \textless1.0 	&	   X 	&	 $-$1.03~$\pm$~0.14		&	 2.31$^{+0.20}_{-0.20}$ \\
\vspace{0.4 ex}																		
L-17 	&	  2.24~$\pm$~0.64 	&		 341.0~$\pm$~33.0 	&	 756~$\pm$~78 	&	     1052~$\pm$~75 	&	             X 	&	   X 	&	 $-$0.76~$\pm$~0.10		&	 1.68$^{+0.20}_{-0.20}$ \\
\vspace{0.4 ex}																		
L-20 	&	  2.66~$\pm$~0.78 	&		   51.1~$\pm$~4.7 	&	 166~$\pm$~19 	&	      264~$\pm$~72 	&	  \textless1.5 	&	   X 	&	 $-$1.25~$\pm$~0.18		&	 1.95$^{+0.17}_{-0.17}$ \\
\vspace{0.4 ex}																		
L-21 	&	  3.09~$\pm$~0.81 	&		 138.3~$\pm$~35.8 	&	 176~$\pm$~38 	&	      350~$\pm$~76 	&	           4.1	&	 1.8	&	 $-$0.64~$\pm$~0.28		&	 2.51$^{+0.37}_{-0.37}$ \\
\vspace{0.4 ex}																		
L-23 	&	  3.13~$\pm$~0.86 	&		   86.4~$\pm$~7.2 	&	 172~$\pm$~21 	&	      242~$\pm$~71 	&	  \textless1.3 	&	   X 	&	 $-$0.77~$\pm$~0.07		&	 2.23$^{+0.23}_{-0.23}$ \\
\vspace{0.4 ex}																		
L-25 	&	  2.56~$\pm$~0.74 	&		   69.0~$\pm$~9.0 	&	 166~$\pm$~20 	&	      348~$\pm$~72 	&	  \textless1.4 	&	   X 	&	 $-$1.09~$\pm$~0.04		&	 2.63$^{+0.25}_{-0.25}$ \\
\vspace{0.4 ex}																		
L-27 	&	  2.48~$\pm$~0.73 	&		  77.2~$\pm$~13.7 	&	 106~$\pm$~18 	&	    \textless219 	&	  \textless2.1 	&	   X 	&	 $-$0.38~$\pm$~0.39		&	 2.47$^{+0.27}_{-0.27}$ \\
\hline
\multicolumn{9}{c}{Other non detections at 1.2~mm}\\
L-2  	&	  \textless3.04 (1.46~$\pm$~0.79) 	&		  \textless42.0 	&	  90~$\pm$~17 	&	    \textless215 	&	        X 	&	   X 	&      [$-$0.64]		&	      \\
\vspace{0.4 ex}																		
L-3  	&	  \textless3.33 (1.04~$\pm$~1.11) 	&		 105.0~$\pm$~35.0 	&	  50~$\pm$~17 	&	    \textless227 	&  \textless7.6 	&	   X 	& +0.89~$\pm$~0.85		&	      \\
\vspace{0.4 ex}																		
L-4  	&	  \textless3.42 (0.76~$\pm$~1.14) 	&		  \textless93.0 	&	  76~$\pm$~17 	&	    \textless220 	&	          X 	&	   X 	&	[$-$0.64]		&	      \\
\vspace{0.4 ex}																		
L-6  	&	  \textless2.22 (0.59~$\pm$~0.74) 	&		   37.1~$\pm$~6.4 	&	  69~$\pm$~12 	&	    \textless202 	&	  \textless1.4 	&	   X 	& $-$0.75~$\pm$~0.42		&	  \\
\vspace{0.4 ex}																		
L-7  	&	  \textless2.97 (1.39~$\pm$~0.79) 	&		 101.7~$\pm$~13.3 	&	 200~$\pm$~23 	&	    \textless216 	&	           2.0	&	 0.8	& $-$0.81~$\pm$~0.29		&	  \\
\vspace{0.4 ex}																		
L-8  	&	  \textless2.70 (--0.36~$\pm$~0.90) 	&		 124.0~$\pm$~14.0 	&	 219~$\pm$~25 	&	      250~$\pm$~72 	&	           1.4	&	   X 	& $-$0.58~$\pm$~0.13		&	           \\
\vspace{0.4 ex}																		
L-10 	&	  \textless3.01 (1.39~$\pm$~0.81) 	&		  67.2~$\pm$~11.7 	&	  94~$\pm$~17 	&	 $\mathellipsis$ 	&	  \textless3.7 	&	   X 	& $-$0.40~$\pm$~0.37		&	 \\
\vspace{0.4 ex}																		
L-12 	&	  \textless3.64 (2.06~$\pm$~0.79) 	&		   94.4~$\pm$~4.7 	&	 182~$\pm$~28 	&	      315~$\pm$~69 	&	  \textless1.3 	&	   X 	& $-$0.81~$\pm$~0.02		&	  \\
\vspace{0.4 ex}																		
L-13 	&	  \textless3.15 (--0.49~$\pm$~1.05) 	&		  \textless39.0 	&	  58~$\pm$~16 	&	    \textless219 	&	             X 	&	   X 	&        [$-$0.64]		&	          \\
\vspace{0.4 ex}																		
L-16 	&	  \textless2.58 (0.51~$\pm$~0.86) 	&	        $\mathellipsis$ 	&	 145~$\pm$~32 	&	      319~$\pm$~77 	&	             X 	&	   X 	& $-$1.25~$\pm$~0.76		&	       \\
\vspace{0.4 ex}																		
L-18 	&	  \textless2.43 (--0.72~$\pm$~0.81) 	&		   93.2~$\pm$~9.4 	&	 162~$\pm$~19 	&	    \textless209 	&	           2.4	&	   X 	& $-$0.67~$\pm$~0.36		&	           \\
\vspace{0.4 ex}																		
L-19 	&	  \textless2.91 (0.89~$\pm$~0.97) 	&		 102.2~$\pm$~12.0 	&	 138~$\pm$~18 	&	      231~$\pm$~69 	&	           3.9	&	 1.8	& $-$0.44~$\pm$~0.13		&	  \\
\vspace{0.4 ex}																		
L-24 	&	  \textless2.64 (0.14~$\pm$~0.88) 	&		  \textless24.0 	&	  45~$\pm$~14 	&	    \textless211 	&	             X 	&	   X 	&        [$-$0.64]		&	        \\
\vspace{0.4 ex}																		
L-26 	&	  \textless2.58 (0.37~$\pm$~0.86) 	&		  54.9~$\pm$~13.4 	&	  84~$\pm$~14 	&	      255~$\pm$~72 	&	           3.5	&	   X 	& $-$0.86~$\pm$~0.53		&	  \\
\vspace{0.4 ex}																		
L-28 	&	  \textless2.96 (1.64~$\pm$~0.66) 	&		  \textless23.0 	&	  47~$\pm$~12 	&	    \textless213 	&	             X 	&	   X 	&        [$-$0.64]		&	      \\
\vspace{0.4 ex}																		
L-29 	&	  \textless2.94 (0.45~$\pm$~0.98) 	&		  55.0~$\pm$~12.0 	&	  76~$\pm$~16 	&	    \textless216 	&	             X 	&	   X 	& $-$0.39~$\pm$~0.52		&	 \\
\vspace{0.4 ex}																		
L-30 	&	  \textless1.89 (0.42~$\pm$~0.63) 	&		  \textless70.0 	&	  84~$\pm$~18 	&	    \textless236 	&	             X 	&	   X 	&        [$-$0.64]		&	  \\
\vspace{0.4 ex}																	
L-31 	&	  \textless2.82 (1.62~$\pm$~0.60) 	&		 121.0~$\pm$~39.0 	&	 157~$\pm$~20 	&	    \textless221 	&	           6.6	&	   X 	& $-$0.31~$\pm$~0.50		&	  \\
\vspace{0.4 ex}																		
L-32 	&	  \textless2.89 (1.61~$\pm$~0.64) 	&		  \textless48.0 	&	  60~$\pm$~16 	&	 $\mathellipsis$ 	&	             X 	&	   X 	&        [$-$0.64]		&	        \\
\vspace{0.4 ex}																		
L-33 	&	  \textless3.27 (-0.28~$\pm$~1.09) 	&		 109.0~$\pm$~33.0 	&	  87~$\pm$~19 	&	    \textless235 	&	 \textless10.0 	&	   X 	&   +0.27~$\pm$~0.61		&	         \\
\hline
\end{tabular}}
\par
 \smallskip
$^a$ The limits on $F_{\rm{1.2~mm}}$  are ``3$\sigma$'' limits, except for the sources with 1.5~$<$~$ {\it S/N}$~$<$~3 where they are the observed value plus~2$\sigma$. 
  The values in brackets are the observed values used in stacks.\\
$^b$ The radio flux density limits are ``3$\sigma$'' limits.\\
$^c$ The values of~$\alpha$ in brackets show the cases where~$\alpha$ cannot be determined and is assumed equal to~--0.64  (see text).
\par
\vspace{-3mm}
\par
\end{table}