\begin{table} %%%\begin{center} \par %%\begin{tabular}{l|lcccll} \hline\hline\\\ GJ873 & M3.5 & Single & '' & I & ~~~~ '' & Lestrade et~al. (\cite{Lestrade2006}) \\ GJ65 & M5.5+M5.5 & Binary & 600~Myr & I & ~~~~ '' & '' \\ GJ3379 & M4 & Single & '' & I & ~~~~ '' & '' \\ GJ849 & M3.5 & '' & '' & I & ~~~~ '' & '' \\ GJ791.2 & M4.5 & '' & '' & I & ~~~~ '' & '' \\ GJ109 & M3.5 & '' & '' & I \& II & ~~~~ '' & Lestrade et~al. (\cite{Lestrade2006}) and this work \\\hline GJ699 & M4.0 & Single & 1.82 pc & II & MAMBO & this work \\ GJ406 & M6.0 & '' & 2.38 pc & II & ~~~~ '' & '' \\ GJ411 & M2.0 & '' & 2.54 pc & II & ~~~~ '' & '' \\ GJ905 & M5.5 & '' & 3.16 pc & II & ~~~~ '' & '' \\ GJ725 & M3+M3.5 & Binary & 3.57 pc & II & ~~~~ '' & '' \\ GJ54.1 & M4.5 & Single & 3.72 pc & II & ~~~~ '' & '' \\ GJ273 & M3.5 & '' & 3.79 pc & II & ~~~~ '' & '' \\ GJ83.1 & M4.5 & '' & 4.44 pc & II & ~~~~ '' & '' \\ GJ687 & M3.0 & '' & 4.53 pc & II & ~~~~ '' & '' \\ LHS292 & M6.5 & '' & 4.54 pc & II & ~~~~ '' & '' \\ GJ1002 & M5.5 & '' & 4.69 pc & II & ~~~~ '' & '' \\ GJ412 & M2+M6 & Binary & 4.83 pc & II & ~~~~ '' & '' \\ GJ388 & M3.0 & Single & 4.89 pc & II & ~~~~ '' & '' \\ GJ445 & M3.5 & '' & 5.38 pc & II & ~~~~ '' & '' \\ LHS1723 & M4.5 & '' & 5.43 pc & II & ~~~~ '' & '' \\ GJ526 & M1.5 & '' & 5.43 pc & II & ~~~~ '' & '' \\ GJ251 & M3.0 & '' & 5.57 pc & II & ~~~~ '' & '' \\ GJ205 & M1.5 & '' & 5.71 pc & II & ~~~~ '' & '' \\ GJ213 & M4.0 & '' & 5.87 pc & II & ~~~~ '' & '' \\ GJ908 & M1.0 & '' & 5.93 pc & II & ~~~~ '' & '' \\ GJ581 & M3 & '' & 6.27 pc & II & ~~~~ '' & '' \\ GJ102 & M4 & '' & 7.75 pc & II & ~~~~ '' & '' \\ \hline \end{tabular}} \medskip \par Survey I was presented in Lestrade et~al. (\cite{Lestrade2006}) and its data are included in the statistical analysis of the present paper. Survey II is based on new data with MAMBO-2 presented in the present paper. Selection criteria are ages $<$600~Myr for survey~I and the nearest M-dwarfs but of undetermined ages for survey~II. Ages are based on Moving Groups (Local Association ($20{-}150$~Myr), IC~2391 ($35{-}55$~Myr), AB Dor (\mbox{100--125}~Myr), Castor (200~Myr), Ursa Maj (500~Myr) and Hyades (600~Myr)) identified by Montes et~al. (\cite{Montes2001}) and Zuckerman \& Inseok Song (\cite{Zuckerman2004a}a,b). Some stars were observed in both surveys. \end{table}