\begin{table}%t3
\caption {\label{Tab:SecuAcc}Proper motion $\mu$, parallax $\pi$ (from Hipparcos, \citealt{vanLeeuwen07}) and secular acceleration (SA) $\dot{v}_{{\rm r}}(t)$ for the M~dwarfs sample, with the highest SA stars in the lower part of the table for comparison (not in our sample).}
%\centering
\par
\begin{tabular}{lrrrr}
\hline
\hline Star&
\multicolumn{1}{c}{$\mu_{\alpha}$}&
\multicolumn{1}{c}{$\mu_{\delta}$}&
\multicolumn{1}{c}{$\pi$}&
\multicolumn{1}{c}{$\dot{v}_{{\rm r}}(t)$}\\
&
\multicolumn{1}{c}{{[}mas/yr{]}}&
\multicolumn{1}{c}{{[}mas/yr{]}}&
\multicolumn{1}{c}{{[}mas{]}}&
\multicolumn{1}{c}{{[}m/s/yr{]}}\\
\hline
%\input{star.hip.pm.tex}%&
Barnard   &  --798.58~$\pm$~1.72 & 10328.12~$\pm$~1.22 & 548.31~$\pm$~1.51 &  4.497~$\pm$~0.012\\
GJ~1      &  5634.68~$\pm$~0.86 & --2337.71~$\pm$~0.71 & 230.42~$\pm$~0.90 &  3.711~$\pm$~0.015\\
GJ~27.1   &   485.57~$\pm$~2.81 &  --223.13~$\pm$~2.11 &  41.69~$\pm$~2.80 &  0.157~$\pm$~0.011\\
GJ~118    &   978.61~$\pm$~2.27 &   633.21~$\pm$~2.64 &  85.87~$\pm$~1.99 &  0.364~$\pm$~0.008\\
GJ~160.2  &    51.90~$\pm$~1.24 &  --780.04~$\pm$~1.57 &  43.25~$\pm$~1.61 &  0.325~$\pm$~0.012\\
GJ~173    &  --225.75~$\pm$~1.94 &  --192.57~$\pm$~1.88 &  90.10~$\pm$~1.74 &  0.022~$\pm$~0.000\\
GJ~180    &   408.07~$\pm$~2.49 &  --642.82~$\pm$~2.06 &  82.52~$\pm$~2.40 &  0.161~$\pm$~0.005\\
GJ~190    &   502.99~$\pm$~1.32 & --1399.76~$\pm$~1.52 & 107.85~$\pm$~2.10 &  0.471~$\pm$~0.009\\
GJ~218    &   768.13~$\pm$~1.39 &  --123.17~$\pm$~1.54 &  66.54~$\pm$~1.43 &  0.209~$\pm$~0.005\\
GJ~229    &  --137.09~$\pm$~0.50 &  --713.66~$\pm$~0.81 & 173.81~$\pm$~0.99 &  0.070~$\pm$~0.000\\
GJ~263    &  --123.73~$\pm$~3.68 &  --814.92~$\pm$~2.87 &  62.41~$\pm$~3.16 &  0.250~$\pm$~0.013\\
GJ~357    &   136.67~$\pm$~1.53 &  --989.13~$\pm$~1.41 & 110.82~$\pm$~1.92 &  0.207~$\pm$~0.004\\
GJ~377    & --1096.84~$\pm$~2.11 &   647.29~$\pm$~2.63 &  61.39~$\pm$~2.55 &  0.607~$\pm$~0.025\\
GJ~422    & --2466.98~$\pm$~2.87 &  1180.09~$\pm$~2.17 &  78.91~$\pm$~2.60 &  2.178~$\pm$~0.072\\
GJ~433    &   --72.51~$\pm$~1.49 &  --851.92~$\pm$~0.88 & 112.58~$\pm$~1.44 &  0.149~$\pm$~0.002\\
GJ~477    &  --101.39~$\pm$~2.28 &  --697.57~$\pm$~1.75 &  52.67~$\pm$~3.05 &  0.217~$\pm$~0.013\\
GJ~510    &  --452.04~$\pm$~2.55 &  --104.79~$\pm$~1.55 &  59.72~$\pm$~2.43 &  0.083~$\pm$~0.003\\
GJ~620    &  --348.40~$\pm$~2.35 &  --675.73~$\pm$~1.87 &  60.83~$\pm$~2.06 &  0.218~$\pm$~0.007\\
GJ~637    &  --480.59~$\pm$~1.17 &  --529.12~$\pm$~1.86 &  62.97~$\pm$~1.99 &  0.186~$\pm$~0.006\\
GJ~682    &  --708.98~$\pm$~2.55 &  --937.40~$\pm$~1.88 & 196.90~$\pm$~2.15 &  0.161~$\pm$~0.002\\
GJ~739    &   153.46~$\pm$~2.91 &  --495.17~$\pm$~1.98 &  70.95~$\pm$~2.56 &  0.087~$\pm$~0.003\\
GJ~817    &  --918.58~$\pm$~3.68 & --2038.13~$\pm$~2.50 &  52.16~$\pm$~2.92 &  2.202~$\pm$~0.123\\
GJ~821    &   713.47~$\pm$~2.82 & --1994.64~$\pm$~0.95 &  82.18~$\pm$~2.17 &  1.255~$\pm$~0.033\\
GJ~842    &   888.07~$\pm$~1.31 &  --125.56~$\pm$~1.16 &  83.43~$\pm$~1.77 &  0.222~$\pm$~0.005\\
GJ~855    &   587.72~$\pm$~2.17 &  --376.75~$\pm$~1.32 &  52.22~$\pm$~2.17 &  0.214~$\pm$~0.009\\
GJ~891    &   717.43~$\pm$~3.40 &    22.12~$\pm$~2.69 &  62.17~$\pm$~3.27 &  0.190~$\pm$~0.010\\
GJ~911    &   --42.36~$\pm$~3.32 &   128.87~$\pm$~2.44 &  41.22~$\pm$~2.64 &  0.010~$\pm$~0.001\\
GJ~1009   &    62.95~$\pm$~2.45 &  --196.98~$\pm$~2.46 &  55.62~$\pm$~2.32 &  0.018~$\pm$~0.001\\
GJ~1046   &  1395.67~$\pm$~1.72 &   547.16~$\pm$~2.52 &  71.06~$\pm$~3.23 &  0.727~$\pm$~0.033\\
GJ~1100   &   118.29~$\pm$~2.67 &  --498.47~$\pm$~1.30 &  34.57~$\pm$~2.79 &  0.174~$\pm$~0.014\\
GJ~3020   &   --44.73~$\pm$~4.05 &  --237.17~$\pm$~3.70 &  43.89~$\pm$~4.39 &  0.030~$\pm$~0.003\\
GJ~3082   &   104.14~$\pm$~2.04 &   311.53~$\pm$~1.81 &  60.38~$\pm$~1.81 &  0.041~$\pm$~0.001\\
GJ~3098   &  --589.19~$\pm$~1.86 &  --887.83~$\pm$~1.24 &  55.98~$\pm$~1.91 &  0.466~$\pm$~0.016\\
GJ~3671   &  --603.54~$\pm$~1.64 &  --296.43~$\pm$~1.36 &  56.38~$\pm$~2.04 &  0.184~$\pm$~0.007\\
GJ~3759   &  --391.22~$\pm$~1.50 &  --411.01~$\pm$~1.71 &  58.94~$\pm$~2.40 &  0.126~$\pm$~0.005\\
GJ~3916   &  --332.19~$\pm$~2.90 &  --352.83~$\pm$~2.62 &  66.21~$\pm$~3.18 &  0.082~$\pm$~0.004\\
GJ~3973   &    --9.48~$\pm$~2.45 &  --221.00~$\pm$~1.72 &  54.86~$\pm$~2.18 &  0.020~$\pm$~0.001\\
GJ~4106   &    31.55~$\pm$~4.63 &  --104.82~$\pm$~3.59 &   9.05~$\pm$~3.70 &  0.030~$\pm$~0.012\\
GJ~4293   &   198.08~$\pm$~2.42 &  --113.57~$\pm$~2.08 &  39.90~$\pm$~3.04 &  0.030~$\pm$~0.002\\
HG~7-15   &   176.02~$\pm$~2.85 &     5.73~$\pm$~1.79 &  26.80~$\pm$~2.05 &  0.027~$\pm$~0.002\\
Prox~Cen  & --3775.75~$\pm$~1.63 &   765.54~$\pm$~2.01 & 771.64~$\pm$~2.60 &  0.442~$\pm$~0.002\\
\hline
%\input{highSAstar.hip.pm.tex}%&
GJ~451~A  &  4003.98~$\pm$~0.37 & --5813.62~$\pm$~0.23 & 109.99~$\pm$~0.41 & 10.411~$\pm$~0.039\\
GJ~9511~B &  --999.75~$\pm$~1.29 & --3542.60~$\pm$~1.13 &  35.14~$\pm$~1.48 &  8.861~$\pm$~0.373\\
GJ~9511~A &  --997.47~$\pm$~1.20 & --3543.55~$\pm$~1.03 &  34.65~$\pm$~1.28 &  8.988~$\pm$~0.332\\
GJ~191    &  6505.08~$\pm$~0.98 & --5730.84~$\pm$~0.96 & 255.66~$\pm$~0.91 &  6.756~$\pm$~0.024\\
GJ~9371   &   264.99~$\pm$~2.23 & --3157.36~$\pm$~2.30 &  42.79~$\pm$~2.70 &  5.391~$\pm$~0.340\\
\hline
\end{tabular}
\end{table}