**Table 4:** Apparent magnitudes, parallaxes, masses derived from the M/L relations of DFS00, and metallicities from this study and from WW05.
$\begin{displaymath}{\begin{tabular}{llr@{~$\pm$~}rcr@{~$\pm$~}rr@{~$\pm$~}lcccr@... ... &G &0.398 &0.465 &$-$0.07 &0.05 &a \\ \hline \end{tabular}} \end{displaymath}$ $^\dagger$ M: Mermilliod et al. (1997), G: Gliese & Jareiss (1991), N: Gould & Chanamé (2004), T: Tycho Input Catalogue (Egret et al. 1992), S: Simbad database. Unfortunately their is no uncertainties on V-band photometry in the Gliese & Jareiss catalogue. $^{\dagger\dagger}$ H: ESA (1997), Y: van Altena et al. (1995), G: Gould & Chanamé (2004). $^\ddagger$ a: this paper, b: Woolf & Wallerstein (2005). The K-band photometry is from 2MASS. The mass estimates use the listed photometry and the M/L relations of Delfosse et al. (2000).

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