\begin{table}%t2 %\centering \par \caption{\label{tab:sources}List of sources extracted from the LABOCA map.} \begin{tabular}{l c c c c c c c } \hline \hline \noalign{\smallskip} Source & $\alpha$(J2000) & $\delta$(J2000) & Flux density\tablefootmark{a} & Deboosted\tablefootmark{b} & Demagnified\tablefootmark{c} & $F/\Delta F$\tablefootmark{d} \\ & & & & flux density &flux density \\ & (h:m:s) & ($^\circ:':''$) & (mJy) & (mJy) & (mJy) & \\ \hline 1 & 06:58:37.62 & --55:57:04.8 & $48.6\pm 1.3$\tablefootmark{e} & $ 48.0\pm 1.3$ & 0.64 & 82.8\\ 2 & 06:58:24.47 & --55:55:12.5 & $15.1\pm 1.0$ & $ 14.7\pm 1.0$ & 8.8 & 29.9\\ 3 & 06:58:25.45 & --55:56:40.1 & $6.9\pm 0.9$ & $ 6.4\pm 1.0$ & 2.2 & 17.8\\ 4 & 06:58:19.36 & --55:58:30.3 & $8.2\pm 0.9$ & $ 7.7\pm 0.9$ & 4.7 & 16.2\\ 5 & 06:58:27.27 & --56:01:16.3 & $9.0\pm 1.3$ & $ 8.0\pm 1.3$ & 6.3 & 15.9\\ 6 & 06:58:28.94 & --55:53:48.4 & $9.3\pm 1.2$ & $ 8.6\pm 1.2$ & 6.3 & 15.4\\ 7 & 06:59:01.39 & --55:52:18.1 & $11.9\pm 2.1$ & $ 9.7\pm 2.1$ & 8.4 & 14.2\\ 8 & 06:58:24.05 & --55:57:23.0 & $5.3\pm 0.9$ & $ 4.7\pm 1.0$ & 1.8 & 13.1\\ 9 & 06:58:55.98 & --55:56:51.7 & $5.4\pm 1.2$ & $ 4.4\pm 1.3$ & 3.3 & 12.8\\ 10 & 06:58:45.60 & --55:58:48.0 & $6.2\pm 1.1$ & $ 5.5\pm 1.1$ & 3.6 & 12.0\\ 11 & 06:58:53.22 & --56:00:45.0 & $7.8\pm 1.5$ & $ 6.4\pm 1.6$ & 5.2 & 11.9\\ 12 & 06:58:52.22 & --55:55:45.7 & $5.5\pm 1.2$ & $ 4.5\pm 1.2$ & 3.4 & 11.2\\ 13 & 06:58:22.88 & --56:00:40.7 & $4.8\pm 1.2$ & $ 3.8\pm 1.3$ & 2.9 & 11.0\\ 14 & 06:58:46.68 & --56:02:11.8 & $7.2\pm 1.9$ & $ 4.6\pm 2.5$ & 3.8 & 10.8\\ 15 & 06:58:33.69 & --55:54:40.8 & $4.6\pm 1.1$ & $ 3.6\pm 1.2$ & 2.5 & 10.1\\ 16 & 06:58:12.44 & --55:57:29.7 & $4.9\pm 1.0$ & $ 4.2\pm 1.0$ & 1.9 & 9.2\\ 17 & 06:59:15.72 & --56:01:07.5 & $23.6\pm 5.9$ & --\tablefootmark{f} & -- & 9.0\\ \hline \end{tabular} \tablefoot{Statistical uncertainties on the listed positions are 1--2\arcsec, which is smaller than the pointing uncertainty. \tablefoottext{a}{Flux density as extracted from the map.} \tablefoottext{b}{Flux density corrected for boosting due to confusion noise.} \tablefoottext{c}{Flux density corrected for lensing.} \tablefoottext{d}{Significance of the detection in the Gaussian-matched-filtered map.} \tablefoottext{e}{Source~\#1 is extended relative to the $22''$ beam: it has an apparent size of $29.2''\times 23.3''$.} \tablefoottext{f}{Source~\#17 lies in the outer part of the map where the noise level is high and the method used to deboost the flux densities fails.}} \end{table}