\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}