\begin{table}%t4 \caption{Apparent magnitudes, parallaxes, masses derived from the M/L relations of DFS00, and metallicities from this study and from WW05.\label{table:db}} %\centerline $$ {\begin{tabular}{llr@{~$\pm$~}rcr@{~$\pm$~}rr@{~$\pm$~}lcccr@{~$\pm$~}rc} %\begin{tabular}{llllr@{~$\pm$~}rcccr@{~$\pm$~}rc} \hline\hline Star & Spectral&\multicolumn{2}{c}{$V$} & source &\multicolumn{2}{c}{$K$} & \multicolumn{2}{c}{$\pi$} & source& Mass$_{V}$ & Mass$_{K}$&\multicolumn{2}{c}{[Fe/H]} & source\\ & type&\multicolumn{2}{c}{[mag]} &$V^\dagger$ &\multicolumn{2}{c}{[mag]} & \multicolumn{2}{c}{[mas]} &$\pi^{\dagger\dagger}$ &[$M_{\odot}$] & [$M_{\odot}$] & \multicolumn{2}{c}{[dex]}&[Fe/H]$^\ddagger$\\ \hline CD-48~176B &M &\multicolumn{2}{c}{13.50} &S &7.64 &0.02 &66.92 &0.73 &H &0.212 &0.270 &$-$0.08 &0.09 &a\\ GJ~3195~B &M3 &\multicolumn{2}{c}{12.50} &G &8.10 &0.03 &43.74 &0.84 &H &0.408 &0.395 &$-$0.31 &0.04 &a \\ GJ~3825 &esdM1.5 &14.55 &0.03 &M &10.86 &0.01 &36.1 &3.2 &Y &0.255 &0.129 &$-$0.93 &0.06 &b \\ GJ~687 &M3 &9.15 &0.03 &M &4.55 &0.02 &220.9 &0.9 &H &0.389 &0.401 &$+$0.15 &0.09 &b\\ GJ~9192 &K4 &10.70 &0.02 &M &7.76 &0.02 &26.1 &2.1 &H &0.793 &0.691 &$-$0.73 &0.06 &b \\ GJ~9371 &sdM0.0 &12.20 &0.03 &M &8.67 &0.02 &44.3 &2.8 &H &0.439 &0.299 &$-$1.05 &0.04 &b \\ G~22-15 &K5V &9.23 &0.02 &M &6.47 &0.02 &41.2 &1.3 &H &0.855 &0.754 &$-$0.72 &0.07 &b \\ Gl~105~B &M4 &11.67 &0.01 &M &6.57 &0.02 &138.72 &1.04 &H &0.252 &0.248 &$-$0.19 &0.07 &a \\ Gl~107~B &M1.5 &\multicolumn{2}{c}{10.06} &G &5.87 &0.02 &89.03 &0.79 &H &0.517 &0.528 &$-$0.03 &0.09 &a \\ Gl~166~C &M4.5 &\multicolumn{2}{c}{11.17} &G &5.9 &0.10 &198.25 &0.84 &H &0.232 &0.236 &$-$0.33 &0.06 &a \\ Gl~191 &sdM1.0 &8.85 &0.03 &M &5.05 &0.02 &255.1 &0.9 &H &0.388 &0.274 &$-$0.99 &0.04 &b \\ Gl~205 &M1.5 &7.96 &0.01 &M &4.04 &0.26 &175.7 &1.2 &H &0.600 &0.601 &$+$0.21 &0.13 &b \\ Gl~212 &M0.5 &9.80 &0.01 &T &5.76 &0.02 &80.13 &1.67 &H &0.572 &0.598 &$+$0.04 &0.11 &a \\ Gl~231.1~B &M3.5 &\multicolumn{2}{c}{13.42} &G &8.28 &0.02 &51.76 &0.78 &H &0.282 &0.309 &$-$0.02 &0.04 &a \\ Gl~250~B &M2 &\multicolumn{2}{c}{10.09} &G &5.72 &0.04 &114.94 &0.86 &H &0.442 &0.446 &$-$0.15 &0.09 &a \\ Gl~297.2~B &M2 &11.80 &0.01 &M &7.42 &0.02 &44.47 &0.77 &H &0.484 &0.519 &$-$0.09 &0.09 &a \\ Gl~324~B &M3.5 &\multicolumn{2}{c}{13.14} &G &7.67 &0.02 &76.8 &0.84 &H &0.239 &0.273 &$+$0.32 &0.07 &a \\ Gl~380 &K5 &6.60 &0.02 &M &2.96 &0.29 &205.2 &0.8 &H &0.742 &0.759 &$-$0.03 &0.18 &b \\ Gl~411 &M2V &7.49 &0.02 &M &3.25 &0.31 &392.5 &0.9 &H &0.436 &0.410 &$-$0.42 &0.07 &b\\ Gl~412~A &M0.5 &8.75 &0.04 &M &4.77 &0.02 &206.9 &1.2 &H &0.451 &0.387 &$-$0.43 &0.05 &b \\ Gl~414~B &M1.5 &9.98 &0.04 &M &5.73 &0.02 &83.8 &1.1 &H &0.544 &0.584 &$+$0.02 &0.11 &b\\ Gl~505~B &M0.5 &\multicolumn{2}{c}{9.60} &G &5.75 &0.02 &89.07 &0.99 &H &0.554 &0.552 &$-$0.25 &0.05 &a \\ Gl~506.1 &sdK &10.84 &0.02 &M &8.17 &0.02 &27.9 &2.5 &H &0.754 &0.573 &$-$1.16 &0.05 &b\\ Gl~526 &M1.5 &8.46 &0.01 &M &4.42 &0.21 &184.1 &1.3 &H &0.520 &0.431 &$-$0.10 &0.07 &b \\ Gl~53.1~B &M3 &\multicolumn{2}{c}{13.60} &G &8.67 &0.02 &48.2 &1.06 &H &0.280 &0.273 &$+$0.07 &0.12 &a\\ Gl~544~B &M6 &\multicolumn{2}{c}{15.10} &G &9.59 &0.02 &48.12 &1.11 &H &0.215 &0.174 &$-$0.20 &0.19 &a \\ Gl~701 &M1 &9.37 &0.03 &M &5.31 &0.02 &128.3 &1.4 &H &0.503 &0.480 &$-$0.20 &0.08 &b\\ Gl~768.1~B &M3.5 &\multicolumn{2}{c}{13.10} &G &8.01 &0.03 &51.57 &0.77 &H &0.310 &0.349 &$+$0.07 &0.12 &a \\ Gl~783.2~B &M4 &\multicolumn{2}{c}{13.94} &G &8.88 &0.02 &48.83 &0.91 &H &0.251 &0.243 &$-$0.16 &0.08 &a \\ Gl~797~B &M2.5 &\multicolumn{2}{c}{11.88} &G &7.42 &0.02 &47.65 &0.76 &H &0.460 &0.489 &$-$0.07 &0.04 &a \\ Gl~809 &M0.5 &8.54 &0.04 &M &4.62 &0.02 &142.0 &0.8 &H &0.584 &0.576 &$-$0.13 &0.10 &b \\ Gl~81.1~B &K7 &\multicolumn{2}{c}{11.21} &G &7.60 &0.03 &29.43 &0.91 &H &0.684 &0.671 &$+$0.09 &0.06 &a\\ Gl~872~B &M1 &\multicolumn{2}{c}{11.70} &G &7.30 &0.02 &61.54 &0.77 &H &0.414 &0.405 &$-$0.36 &0.11 &a \\ Gl~887 &M0.5 &7.35 &0.02 &M &3.46 &0.20 &303.9 &0.9 &H &0.522 &0.476 &$-$0.22 &0.09 &b \\ LHS~104 &esdK7 &13.74 &0.02 &M &10.4 &0.02 &19.3 &3.0 &Y &0.471 &0.308 &$-$1.33 &0.04 &b \\ LHS~12 &M0.5 &12.26 &0.04 &M &8.68 &0.02 &36.1 &4.3 &H &0.486 &0.367 &$-$0.89 &0.04 &b \\ LHS~170 &sdK &10.68 &0.01 &M &7.60 &0.02 &30.2 &2.4 &H &0.753 &0.658 &$-$0.97 &0.06 &b \\ LHS~173 &sdK7 &11.11 &0.01 &M &7.79 &0.02 &39.2 &2.5 &H &0.615 &0.499 &$-$1.19 &0.05 &b \\ LHS~174 &sdM0.5 &12.75 &0.01 &M &9.14 &0.02 &22.6 &7.4 &Y &0.554 &0.468 &$-$1.11 &0.05 &b \\ LHS~1819 &K4 &10.88 &0.02 &M &8.29 &0.03 &17.0 &2.6 &H &0.888 &0.775 &$-$0.77 &0.09 &b \\ LHS~1841 &K &13.18 &0.03 &M &10.39 &0.02 &17.5 &3.3 &Y &0.571 &0.344 &$-$1.47 &0.06 &b\\ LHS~236 &sdK7 &13.10 &0.01 &M &9.85 &0.02 &18.2 &2.9 &Y &0.570 &0.423 &$-$1.32 &0.05 &b \\ LHS~2938 &K7 &10.67 &0.02 &M &7.76 &0.02 &19.0 &2.0 &H &0.885 &0.832 &$-$0.21 &0.11 &b\\ LHS~3084 &sdK &13.43 &0.03 &M &9.78 &0.02 &19.1 &2.9 &Y &0.513 &0.416 &$-$0.73 &0.05 &b\\ LHS~343 &sdK &13.82 &0.02 &M &10.66 &0.02 &18.6 &3.7 &Y &0.471 &0.284 &$-$1.74 &0.03 &b \\ LHS~467 &esdK7 &12.21 &0.03 &M &8.78 &0.02 &26.0 &3.6 &H &0.586 &0.479 &$-$1.10 &0.05 &b \\ LHS~5337 &M0 &11.15 &0.03 &M &7.47 &0.02 &34.5 &3.3 &H &0.647 &0.624 &$-$0.50 &0.06 &b\\ NLTT~45791 &M &\multicolumn{2}{c}{13.10} &N &8.23 &0.03 &34.57 &0.73 &G &0.398 &0.465 &$-$0.07 &0.05 &a \\ \hline \end{tabular}} $$ $^\dagger$ M: Mermilliod et~al. (\cite{mermilliod97}), G: Gliese \& Jareiss (\cite{gliese91}), N: Gould \& Chanam\'e (\cite{gould04}), T: Tycho Input Catalogue (Egret et~al. \cite{egret92}), S: Simbad database. Unfortunately their is no uncertainties on $V$-band photometry in the Gliese \& Jareiss catalogue.\\ $^{\dagger\dagger}$ H: ESA (\cite{esa97}), Y: van Altena et~al. (\cite{vanaltena95}), G: Gould \& Chanam\'e (\cite{gould04}).\\ $^\ddagger$ a: this paper, b: Woolf \& Wallerstein (\cite{woolf05}).\\ The $K$-band photometry is from 2MASS. The mass estimates use the listed photometry and the M/L relations of Delfosse et~al. (\cite{delfosse00}). \end{table}