\begin{table}%t5
\caption{Magnitudes, parallaxes, corresponding masse and metallicity estimates of M-dwarf neighbors.\label{table:feh9pc}}
%\centerline
$$
{\begin{tabular}{llr@{~$\pm$~}lcl@{~$\pm$~}rl@{~$\pm$~}rlll}
      \hline\hline
Star & Spectral&\multicolumn{2}{c}{$V$}&source&\multicolumn{2}{c}{$K$}& \multicolumn{2}{c}{$\pi$}  & $M_{\star,V}$ & $M_{\star,K}$&[Fe/H]\\
        & type        &\multicolumn{2}{c}{[mag]} &$V^\dagger$&\multicolumn{2}{c}{[mag]} & \multicolumn{2}{c}{[mas]} &[$M_{\odot}$]   & [$M_{\odot}$] & [dex]\\
\hline
Gl15A           &M1     &8.10   &0.02 &M&4.02   &0.02   &280.30 &1.00   &0.450  &0.404  &$-$0.45\\
Gl48            &M3     &10.05  &0.01 &M&5.45   &0.02   &122.80 &1.20   &0.438  &0.471  &$+$0.04\\
Gl109           &M3     &10.60  &0.01 &M&5.96   &0.02   &132.40 &2.50   &0.354  &0.350  &$-$0.20\\
Gl205           &M1.5   &7.97   &0.01 &M&4.04   &0.26   &175.70 &1.20   &0.594  &0.602  &$-$0.09\\
LHS1805         &M3.5   &\multicolumn{2}{c}{11.71}      &G&6.64   &0.02   &132.10 &4.90   &0.257  &0.253  &$-$0.16\\
Gl251           &M3V    &10.02  &0.01 &M&5.28   &0.02   &181.30 &1.90   &0.346  &0.350  &$-$0.16\\
Gl273           &M3.5   &9.84   &0.01 &M&4.86   &0.02   &263.30 &1.40   &0.289  &0.291  &$-$0.16\\
Gl285           &M4.5   &11.21  &0.02 &M&5.70   &0.02   &168.60 &2.70   &0.262  &0.309  &$+$0.07\\
GJ1105          &M3.5   &12.01  &0.01 &M&6.88   &0.03   &120.80 &4.40   &0.249  &0.248  &$-$0.15\\
GJ2066          &M2     &10.12  &0.01 &M  &5.77   &0.02   &109.20 &1.80   &0.456  &0.459  &$-$0.14\\
Gl382           &M1.5   &9.26   &0.01 &M&5.01   &0.02   &128.00 &1.50   &0.526  &0.541  &$-$0.02\\
Gl388           &M3     &9.41   &0.02 &M&4.59   &0.02   &204.60 &2.80   &0.391  &0.423  &$+$0.05\\
Gl393           &M2     &9.66   &0.01 &M&5.31   &0.02   &138.30 &2.10   &0.454  &0.448  &$-$0.17\\
Gl402           &M4     &11.66  &0.01 &M&6.37   &0.02   &145.90 &3.80   &0.249  &0.260  &$-$0.06\\
Gl408           &M2.5   &10.04  &0.01 &M&\multicolumn{2}{c}{5.34$^\ddagger$}      &151.00 &1.60   &0.387  &0.372  &$-$0.24\\
Gl411           &M2     &7.49   &0.04 &M&3.25   &0.31   &392.40 &0.90   &0.435  &0.410  &$-$0.33\\
Gl412A          &M0.5   &8.82   &0.01 &M&4.77   &0.02   &206.90 &1.20   &0.458  &0.387  &$-$0.51\\
Gl424           &M0     &9.30   &0.01 &M&5.53   &0.02   &109.90 &1.10   &0.556  &0.502  &$-$0.47\\
Gl445           &M3.5   &10.84  &0.01 &M&5.95   &0.03   &185.50 &1.40   &0.270  &0.247  &$-$0.26\\
Gl450           &M1     &9.74   &0.03 &M&5.61   &0.02   &116.90 &1.40   &0.487  &0.462  &$-$0.29\\
Gl486           &M3.5   &11.38  &0.01 &M&6.36   &0.02   &121.80 &2.90   &0.305  &0.316  &$-$0.08\\
Gl514           &M0.5   &9.04   &0.01 &M&5.04   &0.03   &131.10 &1.30   &0.545  &0.526  &$-$0.23\\
LHS2784         &M3.5   &11.97  &0.02 &W&6.98   &0.02   &109.90 &3.20   &0.265  &0.261  &$-$0.19\\
Gl526           &M1.5   &8.48   &0.03 &M&4.42   &0.02   &184.10 &1.30   &0.527  &0.502  &$-$0.24\\
Gl555           &M4     &11.30  &0.02 &M&5.94   &0.03   &163.50 &2.80   &0.252  &0.284  &$+$0.01\\
Gl581           &M3     &10.55  &0.01 &M&5.84   &0.02   &159.50 &2.30   &0.324  &0.307  &$-$0.25\\
Gl625           &M1.5   &10.11  &0.01 &M&5.83   &0.02   &151.90 &1.10   &0.375  &0.323  &$-$0.48\\
Gl628           &M3.5   &10.07  &0.02 &M&5.08   &0.02   &234.50 &1.80   &0.294  &0.296  &$-$0.12\\
Gl687           &M3     &9.16   &0.02 &M&4.55   &0.02   &220.80 &0.90   &0.343  &0.401  &$+$0.11\\
Gl686           &M1     &9.60   &0.02 &M&5.57   &0.02   &123.00 &1.60   &0.486  &0.447  &$-$0.40\\
Gl701           &M1     &9.36   &0.01 &M&5.31   &0.02   &128.30 &1.40   &0.499  &0.481  &$-$0.30\\
GJ1230B         &M5     &\multicolumn{2}{c}{14.00}   &G&6.62   &0.02   &120.90 &7.20   &0.143  &0.281  &$+$0.15\\
Gl725A          &M3     &8.95   &0.01 &M&4.43   &0.02   &280.30 &3.60   &0.361  &0.334  &$-$0.31\\
Gl725B          &M3.5   &9.72   &0.01 &M&5.00   &0.02   &284.50 &5.00   &0.292  &0.250  &$-$0.34\\
Gl745A          &M1.5   &\multicolumn{2}{c}{10.76}   &G&6.52   &0.02   &115.90 &2.50   &0.373  &0.308  &$-$0.54\\
Gl745B          &M2     &\multicolumn{2}{c}{10.75}   &G&6.52   &0.02   &112.80 &2.40   &0.380  &0.317  &$-$0.52\\
Gl752A          &M2.5   &9.13   &0.01 &M&4.67   &0.02   &170.30 &1.40   &0.460  &0.484  &$-$0.02\\
Gl793           &M2.5   &10.63  &0.01 &M&5.93   &0.02   &125.60 &1.10   &0.376  &0.374  &$-$0.12\\
Gl809           &M0.5   &8.55   &0.02 &M&4.62   &0.02   &141.90 &0.80   &0.589  &0.577  &$-$0.16\\
Gl849           &M3.5   &10.37  &0.01 &M&5.59   &0.02   &114.00 &2.10   &0.410  &0.475  &$+$0.14\\
Gl860A          &M3     &\multicolumn{2}{c}{9.85}    &G&4.78   &0.03   &247.50 &1.50   &0.292  &0.322  &$-$0.04\\
Gl873           &M3.5   &10.05  &0.01 &M&5.30   &0.02   &198.10 &2.00   &0.300  &0.317  &$-$0.21\\
Gl876           &M4     &10.18  &0.01 &M&5.01   &0.02   &214.60 &0.20   &0.293  &0.334  &$+$0.03\\
Gl880           &M1.5   &8.70   &0.02 &M&4.52   &0.02   &145.30 &1.20   &0.569  &0.586  &$+$0.05\\
Gl896A          &M3.5   &\multicolumn{2}{c}{10.38}   &G&5.33   &0.02   &160.10 &2.80   &0.333  &0.387  &$+$0.08\\
Gl896B          &M4.5   &\multicolumn{2}{c}{12.40}   &G&6.26   &0.04   &160.10 &2.80   &0.186  &0.248  &$+$0.14\\
Gl908           &M1     &8.99   &0.01 &M&5.04   &0.02   &167.50 &1.50   &0.479  &0.421  &$-$0.52\\
\hline
\end{tabular}}
$$

$^\dagger$ M: Mermilliod et~al. (\cite{mermilliod97}), G: Gliese \& Jareiss (\cite{gliese91}), W: Weis (\cite{weis91}).\\
$^\ddagger$ $K$-band photometry given by Leggett (\cite{leggett92}) and transformed to 2MASS system using the relation given by Carpenter (\cite{carpenter01}).\\
The mass estimates use the listed photometry and the M/L relations of 
Delfosse et~al. (\cite{delfosse00}).\\
The $K$-band photometry originates from 2MASS and the parallaxes are adopted
from the compilation of Delfosse et~al. (2005, in prep.).
\end{table}