\begin{table}%t3
\par
\caption{\label{tab:uma_mem_data}The sample of UMa group members.}
%\centerline
 {
\begin{tabular}{lllrccccccccc}
\hline\hline
Object&Spectral type&\multicolumn{1}{c}{$V$}&\multicolumn{1}{c}{$\pi$}      &\multicolumn{2}{c}{\citetalias{Montes01b}}    &\multicolumn{3}{c}{\citetalias{King03}}&\citetalias{Fuhrmann04}&\multicolumn{3}{c}{Sub-sample}\\
&&&\multicolumn{1}{c}{[mas]}&pec. vel.&rad. vel.&kin.&phot.&final       &&&&\\
\hline\\[-3.2mm]
HD  11131          &G1V     & $6.727\pm0.005$$^1$&  42.35 $\pm$ 0.87$^3$& Y & Y &?   &Y?&Y?  &Y&{\it M01k}&&\\
HD  24916       A  &K4V     & $8.033\pm0.018$    &  63.41 $\pm$ 2.00& Y & Y &N?  &? &N?  & &{\it M01k}&&\\
HD  26923          &G0IV    & $6.314\pm0.005$$^1$&  47.20 $\pm$ 1.08& Y & Y &Y?  &Y &Y?  &Y&{\it M01k}&&\\
HD  28495          &G0V     & $7.748\pm0.023$    &  36.32 $\pm$ 1.07& N & Y &Y   &Y &Y   & &&{\it K03k}&{\it K03f}\\
HD  38393          &F7V     & $3.586\pm0.0044$   & 111.49 $\pm$ 0.60& Y & Y &?/Y?&Y?&Y?  & &{\it M01k}&&\\
HD  39587          &G0V     & $4.396\pm0.005$$^1$& 115.43 $\pm$ 1.08&   &   &Y   &Y &Y   &Y&&{\it K03k}&{\it K03f}\\
HD  41593          &K0V     & $6.762\pm0.005$$^1$&  64.71 $\pm$ 0.91& Y & Y &N?/?&Y &N?/?&Y&{\it M01k}&&\\
HD  59747          &G5V     & $7.677\pm0.005$$^1$&  50.80 $\pm$ 1.29& Y & Y &Y   &Y?&Y   &Y&{\it M01k}&{\it K03k}&{\it K03f}\\
HD  71974       A  &G5V     & $7.265\pm0.011$    &  34.83 $\pm$ 1.37& Y & N &Y   &Y?&Y   & &&{\it K03k}&{\it K03f}\\
HD  95650          &M0      & $9.508\pm0.024$    &  85.76 $\pm$ 1.36& N & Y &Y   &Y?&Y   & &&{\it K03k}&{\it K03f}\\
HD  238087         &K5      & $9.975\pm0.030$    &  35.24 $\pm$ 1.24& Y & Y &Y?  &? &?   & &{\it M01k}&&\\
HD  109011         &K2V     & $8.069\pm0.015$    &  42.13 $\pm$ 3.11&   &   &Y   &Y &Y   & &&{\it K03k}&{\it K03f}\\
HD  109647         &K0V     & $8.503\pm0.020$    &  38.08 $\pm$ 1.11& Y & Y &Y   &Y &Y   & &{\it M01k}&{\it K03k}&{\it K03f}\\
HD  110463         &K3V     & $8.256\pm0.018$    &  43.06 $\pm$ 0.82& Y & Y &Y   &Y &Y   & &{\it M01k}&{\it K03k}&{\it K03f}\\
HD  112196         &F8V     & $6.985\pm0.015$    &  29.19 $\pm$ 1.60& Y & Y &N?/?&? &N?/?& &{\it M01k}&&\\
HD  115043         &G1Va    & $6.814\pm0.011$    &  38.92 $\pm$ 0.67& Y & Y &Y   &Y &Y   & &{\it M01k}&{\it K03k}&{\it K03f}\\
HD  238224         &K5      & $9.642\pm0.022$    &  39.84 $\pm$ 1.44& Y & Y &Y   &? &Y?  & &{\it M01k}&{\it K03k}&\\
HD  152863      A  &G5III   & $6.066\pm0.008$    &   7.14 $\pm$ 0.67& Y & Y &?   &Y?&?   & &{\it M01k}&&\\
HD  155674      A  &K0      & $8.903\pm0.087$    &  47.14 $\pm$ 1.88& Y & Y &?   &? &?   & &{\it M01k}&&\\
HD  155674      B  &K8      & $9.304\pm0.054$    &  47.86 $\pm$ 3.11& Y & Y &?   &? &?   & &{\it M01k}&&\\
HD  167389         &F8      & $7.383\pm0.010$    &  29.91 $\pm$ 0.59& Y & Y &N?  &? &N?/?& &{\it M01k}&&\\
HD  171746      A  &G2V     & $6.924\pm0.071$$^2$&  29.23 $\pm$ 1.54& N & Y &Y   &Y?&Y   & &&{\it K03k}&{\it K03f}\\
HD  171746      B  &G2V     & $7.009\pm0.071$$^2$&  29.23 $\pm$ 1.54&   &   &Y   &Y?&Y   & &&{\it K03k}&{\it K03f}\\
HD  184960         &F7V     & $5.714\pm0.006$    &  39.08 $\pm$ 0.47& Y & Y &?/Y?&? &?/Y?& &{\it M01k}&&\\
HD  205435         &G8III   & $3.986\pm0.006$    &  26.20 $\pm$ 0.51& Y & Y &?/Y?&? &?   & &{\it M01k}&&\\
\hline
\end{tabular}}
\medskip
\par
The table gives the spectral type {(2)}, the $V$ band magnitude {(3)} derived from the {\em Hipparcos} system using the conversion of \citet{Bessell00} in most cases, the parallax $\pi$ {(4)}, Eggen's peculiar velocity criterion {(5)} and Eggen's cluster radial velocity criterion {(6)} as applied by \citetalias{Montes01b}, the kinematic $UVW$ criterion {(7)},  photometric criterion {(8)}, and  final membership according to \citetalias{King03} {(9)}, and the spectroscopic membership following \citetalias{Fuhrmann04} {(10)}. The last column indicates the membership of the sub-samples {\it M01k}, {\it K03k}, and {\it K03f} as described in the text in detail. Most astrometric and photometric measurements are taken from the {\em Hipparcos} catalogue \citep{Perryman97}. Exceptions are indicated in the footnote below.\\
$^1$ \citetalias{Fuhrmann04}. 
$^2$ Based on values in the {\em Hipparcos} system given by \citet{Fabricius00}. See Sect.~\ref{sect:mult} for more details. 
$^3$ According to \citetalias{Fuhrmann04}, the parallax of the primary HD~11171 is adopted.
\end{table}