**Table 5:** Magnitudes, parallaxes, corresponding masse and metallicity estimates of M-dwarf neighbors.
$\begin{displaymath}{\begin{tabular}{llr@{~$\pm$~}lcl@{~$\pm$~}rl@{~$\pm$~}rlll} ... ... &167.50 &1.50 &0.479 &0.421 &$-$0.52\\ \hline \end{tabular}} \end{displaymath}$ $^\dagger$ M: Mermilliod et al. (1997), G: Gliese & Jareiss (1991), W: Weis (1991). $^\ddagger$ K-band photometry given by Leggett (1992) and transformed to 2MASS system using the relation given by Carpenter (2001). The mass estimates use the listed photometry and the M/L relations of Delfosse et al. (2000). The K-band photometry originates from 2MASS and the parallaxes are adopted from the compilation of Delfosse et al. (2005, in prep.).

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