\begin{table}%tA.1
\caption{\label{tabA1}Spectral-type reference stars and radial velocity standards (marked with~*).}
%\centering
\par
\begin{tabular}{llcccccl}
\hline \hline  
HD/GJ & SpT & $V_{\rm r} \pm \sigma_{V_{\rm r}}$  & Ref$_{\rm v}$ & $v \sin i$ & 
Ref$_{\rm r}$ & $S \pm \sigma_{\rm S}$ & Observing run \\
   &              &          (km s$^{-1}$)            &             & (km s$^{-1}$) &
               &   &           \\
\hline
212754   & F7 V   & --17.8 $\pm$ 1.2 & a & 7.9 $\pm$ 0.7 & j & 0.142 $\pm$ 0.001 & 4, 5 \\
43587  * & F9 V   & ~~4.6 $\pm$ 0.1 & b & ...           &   & 0.158 $\pm$ 0.001 & 5, 6 \\
84737  * & G0.5 V & ~~6.0 $\pm$ 1.1 & b & 2.8 $\pm$ 0.8 & j & 0.144 $\pm$ 0.000 & 10 \\
10307    & G2 V   & ...             &   & 2.1 $\pm$ 0.5 & k & 0.152 $\pm$ 0.003 & 7 \\
193664   & G3 V   & ~--4.7 $\pm$ 1.2 & a & ...           &   & 0.161 $\pm$ 0.004 & 7 \\
25680    & G5 V   & ~24.0 $\pm$ 0.1 & c & 7.0 $\pm$ 0.7 & j & 0.281 $\pm$ 0.000 & 5, 7 \\
31966    & G5 V   & --18.1 $\pm$ 0.1 & c & ...           &   & ...               & 5 \\
71148  * & G5 V   & --31.0 $\pm$ 0.7 & b & ...           &   & 1.570 $\pm$ 0.000 & 10 \\
159222 * & G5 V   & --50.5 $\pm$ 1.2 & b & ...           &   & 0.164 $\pm$ 0.002 & 1, 4, 11 \\
182488 * & G8 V   & --21.5           & d & 0.6 $\pm$ 0.5 & k & 0.155 $\pm$ 0.008 & 1, 4, 11 \\
48432    & K0 III & ~17.9 $\pm$ 0.2 & e & ${<}1.0$        & e & 0.120 $\pm$ 0.000 & 5, 6 \\
62509  * & K0 III & ~~3.2 $\pm$ 0.3 & b & 1.7 $\pm$ 0.5 & k & 0.140 $\pm$ 0.019 & 3 \\
100696 * & K0 III & ~~0.2 $\pm$ 0.5 & b & 1.2 $\pm$ 1.0 & l & ...               & 10 \\
197989   & K0 III & --10.6 $\pm$ 0.5 & a & 2.0 $\pm$ 0.5 & k & 0.104 $\pm$ 0.001 & 1, 2, 4, 7, 8, 11 \\
3651   * & K0 V   & --32.8 $\pm$ 0.8 & b & 2.2 $\pm$ 0.5 & k & 0.191 $\pm$ 0.001 & 2, 3, 4, 5, 7 \\
97004    & K0 V   & ~~5.4 $\pm$ 0.1 & c & ...           &   & ...               & 10 \\
112758   & K0 V   & ~--4.1 $\pm$ 1.2 & a & ...           &   & 0.206 $\pm$ 0.000 & 10 \\
136442 * & K0 V   & --45.6 $\pm$ 0.8 & b & ...           &   & ...               & 10 \\
185144   & K0 V   & ~26.7 $\pm$ 0.1 & c & 0.6 $\pm$ 0.5 & k & 0.195 $\pm$ 0.003 & 11 \\
201651   & K0 V   & --13.7 $\pm$ 1.2 & a & ...           &   & ...               & 4, 7, 8 \\
92588  * & K1 IV  & ~43.5 $\pm$ 0.3 & f & ${<}1.0$        & e & ...               & 9, 10 \\
10476  * & K1 V   & --33.9 $\pm$ 0.9 & b & 0.6 $\pm$ 0.5 & k & 0.192 $\pm$ 0.001 & 1, 5 \\
12929  * & K2 III & --14.6 $\pm$ 0.2 & g & 1.8 $\pm$ 0.5 & k & 0.118 $\pm$ 0.002 & 5 \\
124897 * & K2 III & ~--5.3 $\pm$ 0.3 & g & 3.3 $\pm$ 0.5 & k & 0.144 $\pm$ 0.012 & 6, 10 \\
161096 * & K2 III & --12.5 $\pm$ 0.3 & g & 2.5 $\pm$ 0.5 & k & 0.103 $\pm$ 0.002 & 1, 4, 11 \\
201196   & K2 IV  & --34.8 $\pm$ 0.2 & e & ${<}1.0$        & e & ...               & 1, 5 \\
4628   * & K2 V   & --10.1 $\pm$ 0.4 & f & 0.0 $\pm$ 0.5 & h & 0.223 $\pm$ 0.001 & 2, 5, 8, 12 \\
136713   & K2 V   & ~--6.0 $\pm$ 0.1 & c & 3.8 $\pm$ 5.7 & m & ...               & 6 \\
166620   & K2 V   & ~~6.9 $\pm$ 0.1 & h & 0.0 $\pm$ 0.4 & h & 0.193 $\pm$ 0.001 & 1, 2, 4, 6, 7, 9, 10, 11 \\
16160    & K3 V   & ~25.8 $\pm$ 0.1 & c & 1.0 $\pm$ 1.0 & h & 0.221 $\pm$ 0.002 & 8 \\
219134   & K3/4 V & --18.6 $\pm$ 0.1 & c & 2.1 $\pm$ 0.5 & k & 0.229 $\pm$ 0.003 & 1, 2, 4, 5, 11 \\
29139  * & K5 III & ~54.2 $\pm$ 0.2 & g & 2.0 $\pm$ 1.0 & e & ...               & 4, 6, 7 \\
154363   & K5 V   & ~34.1 $\pm$ 0.1 & c & 3.7 $\pm$ 5.9 &   & 0.197 $\pm$ 0.001 & 1, 6, 10 \\
201091   & K5 V   & ~~7.0 $\pm$ 0.1 & h & 0.0 $\pm$ 0.8 & h & 0.613 $\pm$ 0.006 & 1, 4, 5, 6, 7, 8, 10, 11 \\
GJ 910   & K5 V   & ~~2.0           & i & 0.0 $\pm$ 0.0 & m & ...               & 7 \\
151877   & K7 V   & ~~2.0 $\pm$ 0.1 & c & 0.0 $\pm$ 0.0 & m & ...               & 1 \\
201092   & K7 V   & ~~7.2 $\pm$ 0.1 & h & 1.7 $\pm$ 0.6 & h & 0.922 $\pm$ 0.011 & 1, 4, 5, 6, 7, 8, 10, 11 \\
GJ 466   & M0 V   & ~--5.0 $\pm$ 5.0 & a & ...           &   & ...               & 10 \\
147379   & M0 V   & --18.8 $\pm$ 0.1 & c & 4.2 $\pm$ 6.2 & m & 1.761 $\pm$ 0.160 & 11 \\
GJ 720A  & M0 V   & --25.0 $\pm$ 2.5 & a & 6.3 $\pm$ 1.7 & m & ...               & 7 \\
GJ 16    & M0/1 V & ...             &   & ...           &   & ...               & 8 \\
GJ 806   & M1.5 V & --24.7 $\pm$ 0.1 & c & 1.9 $\pm$ 0.7 & n & ...               & 11 \\
18884  * & M2 III & --26.1 $\pm$ 0.3 & g & ...           &   & 0.331 $\pm$ 0.004 & 8 \\
115521 * & M2 III & --28.6 $\pm$ 2.3 & g & ...           &   & ...               & 6, 10 \\
95735    & M2 V   & --84.7 $\pm$ 0.1 & c & 0.0 $\pm$ 0.0 & n & 0.392 $\pm$ 0.009 & 6, 10 \\
GJ 687B\tablefootmark{\dag} & M3.5 V & --28.8 $\pm$ 0.1 & c & ...     &   & ...               & 6, 10 \\
\hline 
\end{tabular}
\tablefoot {\tablefoottext{\dag}{The radial velocity given for GJ~687B is that of GJ~687A.}}
\tablebib {a~\citet{duf95}, WEB (Wilson Evans Batten Catalogue);
b~\citet{bar86}; c~\citet{nid02}; d~{\it ELODIE};\index{ELODIE} e~\citet{dem99}; f~\citet{bea79};
g~\citet{udr99}; h~\citet{ben84}; i~\citet{dye54}; j~\citet{sod82}, \citet{sod89};
k~\citet{fek97}; l~\citet{dem00}; m~\citet{tok92}; n~\citet{mar92}.}
\end{table}