\begin{table}%t2 \caption{\label{tab2}Millimeter sources found in our MAMBO-2 maps.} %\centerline {\begin{tabular}{l|l|ccccc} \hline\hline\ Source name & Star Field & $\alpha$(J2000) $^a$ & $\delta$(J2000) $^a$ & Integrated flux density $^b$ & $S/N$ & Source \\ & & & & at 1.2~mm (mJy) & & {\it FWHM} \\ \hline MM145428+160439 & GJ569 & 14 ~54 ~28.2 & 16 ~04 ~39 & $ 5.3 \pm 1.1$ & 4.9 & $11''$ \\ & & & & & & \\ MM184222+593828 & GJ725 & 18 ~42 ~22.7 & 59 ~38 ~28 & $30{-}63$ $^c$ & $6.7{-}7.3$ & $13''{-}15''$ \\ MM184253+593756 & GJ725 & 18 ~42 ~53.3 & 59 ~37 ~56 & $ 9.7 \pm 1.9 $ & 5.1 & $11''$ \\ & & & & & & \\ MM134539+145139 & GJ526 & 13 ~45 ~39.0 & 14 ~51 ~39 & $3.2 \pm 0.7 $ & 4.4 & $11''$ \\ MM134540+145446 & GJ526 & 13 ~45 ~40.7 & 14 ~54 ~46 & $4.3 \pm 0.8 $ & 5.2 & $11''$ \\ MM134541+145417 & GJ526 & 13 ~45 ~41.3 & 14 ~54 ~17 & $6.3 \pm 1.0 $ & 6.1 & $11''$ \\ MM134543+145317 & GJ526 & 13 ~45 ~43.1 & 14 ~53 ~17 & $3.0 \pm 0.7 $ & 4.9 & $11''$ \\ MM134546+145240 & GJ526 & 13 ~45 ~46.7 & 14 ~52 ~40 & $5.6 \pm 0.7 $ & 8.6 & $11''$ \\ & & & & & & \\ MM163007-123942 & GJ628 $^d$ & 16 ~30 ~07.6 & $-$12 ~39 ~42 & $7.3 \pm 1.2 $ & 6.2 & $14\pm 4''$ \\ MM163022-123925 & GJ628 $^e$ & 16 ~30 ~22.3 & $-$12 ~39 ~25 & $3.8 \pm 0.9 $ & 4.4 & $17\pm 5''$ \\ MM163019-123830 & GJ628 $^f$ & 16 ~30 ~19.7 & $-$12 ~38 ~30 & $4.1 \pm 0.8 $ & 4.9 & $11''$ \\ MM163015-123911 & GJ628 $^g$ & 16 ~30 ~15.6 & $-$12 ~39 ~11 & $4.8 \pm 0.8 $ & 6.2 & $11''$ \\ MM163013-124057 & GJ628 $^h$ & 16 ~30 ~13.7 & $-$12 ~40 ~57 & $4.3 \pm 1.0 $ & 4.8 & $11''$ \\ \hline \end{tabular}} \medskip \par $^a$ The MAMBO coordinate uncertainties are $\sim$$3.5''$. $^b$ Flux density (mJy) is integrated under the fitted 2D-Gaussian. $^c$ Flux density is provided as lower and upper limits because the source is located close to one of the borders of the map where some systematics remain in the data (see text). $^d$, $^e$, $^f$, $^g$, $^h$ These sources were found in survey I; $^d$ is GJ628-W, $^e$ is GJ628-E, $^f$ is GJ628-NE, $^g$ is GJ628-NW, and $^h$ is GJ628-SW in Fig.~\ref{fig2} and Table~\ref{tab3} of Lestrade et~al. (\cite{Lestrade2006}). Note that there are typographic errors in the $minute$ column of declinations in Table~\ref{tab3} of Lestrade et~al. (\cite{Lestrade2006}). The positions of the GJ628 sources given now are correct and supersede this first publication. Also, the flux densities in this first publication were peak flux densities while they are integrated flux densities now. \end{table}