\begin{table}%T1
\caption{Spectra obtained with the FOCES echelle spectrograph at the Calar Alto 
2.2~m telescope in August 2001 (top section), and with the UVES echelle 
spectrograph at the ESO VLT telescope in March 2001 (bottom section). Columns 
are mostly self-explanatory. Parallaxes (mas), their errors $\sigma$, and proper 
motions (mas/y) are taken from the H{\sc ipparcos} catalogue (ESA \cite{ES97}).  
$N$ and $t_{\rm exp}$ refer to the number of spectra taken and the total exposure 
time (s).} \label{obs} 
%\centerline
{
\begin{tabular}{lrrrrrrrrrrrl}
\hline\hline\noalign{\smallskip}
~~~~~HD  &  HIP~~  & $\alpha(2000)~~$ & $\delta(2000)~~$ &  $V$~~ &   $B-V$~ & 
  $\pi$~~~ & $\sigma(\pi)$ & $\mu(\alpha)$~ & $\mu(\delta)$~ & $N$ & $t_{\rm exp}$ \\
\noalign{\smallskip}\hline\noalign{\smallskip}
HD 133621  &  73440  &  15 00 27.71  &  +71 45 54.9  &  6.64  &  0.631  &  29.67  &  0.78  &  --405.35  &    80.73  &  3  &  1350 & SB1 \\
HD 134113  &  74033  &  15 07 46.81  &  +08 52 47.7  &  8.26  &  0.575  &  15.40  &  1.37  &  --518.99  &   --57.02  &  3  &  3600 & SB1 \\
HD 140283  &  76976  &  15 43 03.76  & --10 55 57.9  &  7.20  &  0.484  &  17.44  &  0.56  & --1115.54  &  --302.77  &  3  &   300 & \\
HD 141335  &  77122  &  15 44 52.06  &  +62 51 36.0  &  8.95  &  0.580  &  11.53  &  0.78  &  --255.74  &   128.23  &  3  &  5400 & SB2 \\
HD 142267  &  77801  &  15 53 12.19  &  +13 11 52.8  &  6.07  &  0.598  &  57.27  &  0.88  &  --150.56  &  --562.69  &  3  &   900 & \\
HD 144061  &  78217  &  15 58 21.13  &  +70 53 37.8  &  7.26  &  0.654  &  34.35  &  1.08  &   --59.70  &   253.89  &  3  &  1800 & \\
HD 148816  &  80837  &  16 30 28.71  &  +04 10 53.8  &  7.27  &  0.545  &  24.34  &  0.90  &  --432.73  & --1392.34  &  3  &  2700 & \\
BD+68\degr~901  &  82896  &  16 56 24.27  &  +68 01 28.3  &  8.70  &  0.659  &  19.73  &  0.70  &   --73.74  &   263.02  &  3  &  5400 & em \\
HD 157089  &  84905  &  17 21 07.15  &  +01 26 32.6  &  6.95  &  0.571  &  25.88  &  0.95  &  --165.01  &   269.80  &  3  &  1350 & \\
HD 157466  &  85007  &  17 22 27.61  &  +24 52 47.4  &  6.88  &  0.526  &  33.54  &  0.84  &    62.67  &  --160.22  &  3  &  1800 & \\
HD 158226  &  85378  &  17 26 43.44  &  +31 04 37.2  &  8.48  &  0.626  &  14.51  &  0.93  &  --361.74  &    74.09  &  3  &  4500 & \\
G170-56    &  86321  &  17 38 15.73  &  +18 33 27.3  &  9.77  &  0.480  &   8.93  &  1.48  &  --188.07  &  --205.58  &  2  &  3600 & \\
HD 160933  &  86184  &  17 36 40.03  &  +69 34 16.5  &  6.33  &  0.596  &  23.53  &  0.54  &   --53.74  &  --217.54  &  3  &   900 & \\
HD 160693  &  86431  &  17 39 37.24  &  +37 11 08.7  &  8.39  &  0.576  &  18.32  &  0.78  &  --497.69  &  --819.78  &  2  &  3000 & \\
HD 170357  &  90393  &  18 26 38.02  &  +46 04 59.8  &  8.27  &  0.619  &  14.37  &  0.73  &  --348.79  &   199.92  &  3  &  4500 & \\
HD 171620  &  91058  &  18 34 30.56  &  +34 24 54.6  &  7.55  &  0.511  &  19.12  &  0.69  &   196.35  &   191.26  &  4  &  4200 & \\
HD 173084  &  91395  &  18 38 23.87  &  +67 07 33.9  &  7.70  &  0.635  &  19.11  &  0.59  &  --133.33  &   183.71  &  3  &  3600 & SB2 \\
G142-2     &  93445  &  19 01 51.11  &  +16 03 51.0  & 10.38  &  0.655  &   9.72  &  1.65  &  --146.98  &  --302.79  &  3  &  5400 & \\
HD 182807  &  95492  &  19 25 25.87  &  +24 54 51.5  &  6.19  &  0.528  &  36.05  &  0.73  &  --177.20  &  --631.08  &  3  &   900 & \\
HD 184448  &  96077  &  19 32 02.61  &  +50 10 51.0  &  8.05  &  0.659  &  19.16  &  0.63  &   --90.99  &   292.17  &  3  &  2700 & \\
HD 184855  &  96427  &  19 36 15.58  &  +04 45 57.0  &  9.18  &  0.660  &  13.51  &  1.34  &    10.75  &  --216.08  &  3  &  5400 & SB1 \\
HD 186379  &  97023  &  19 43 06.97  &  +24 35 55.0  &  6.87  &  0.567  &  22.10  &  0.82  &    87.13  &  --271.16  &  3  &  1560 & \\
G261-10    &  96780  &  19 40 17.42  &  +79 43 07.9  & 10.34  &  0.700  &  10.55  &  1.09  &   191.72  &   188.90  &  3  &  4600 & SB2 \\
HD 198300  & 102523  &  20 46 35.63  &  +59 51 12.0  &  8.54  &  0.653  &  17.52  &  1.21  &  --132.08  &  --289.23  &  3  &  3600 & \\
HD 200580  & 103987  &  21 04 07.55  &  +02 59 43.4  &  7.31  &  0.547  &  17.83  &  1.29  &  --272.98  &  --368.63  &  3  &  3600 & VB \\
HD 204155  & 105888  &  21 26 42.81  &  +05 26 32.1  &  8.49  &  0.572  &  13.02  &  1.11  &    167.09  &  --246.66  &  3  &  5100 & \\
G188-22    & 107294  &  21 43 57.28  &  +27 23 25.4  & 10.05  &  0.480  &   9.19  &  1.70  &  --238.75  &  --159.67  &  4  &  7200 & \\
HD 208906  & 108490  &  21 58 41.08  &  +29 48 48.8  &  6.95  &  0.501  &  34.12  &  0.70  &  --361.74  &  --386.30  &  3  &  1320 & \\
HD 210631  & 109563  &  22 11 39.23  &  +06 11 35.8  &  8.45  &  0.594  &  13.78  &  1.18  &   234.28  &    67.75  &  3  &  3600 & SB1 \\
G242-4     & 111549  &  22 35 53.16  &  +76 29 31.1  &  9.39  &  0.540  &   9.82  &  1.13  &  --214.74  &   158.14  &  3  &  5400 & \\
HD 215257  & 112229  &  22 43 50.63  &  +03 53 09.7  &  7.41  &  0.515  &  23.66  &  0.97  &   150.64  &   331.61  &  3  &  3300 & \\
HD 218209  & 113989  &  23 05 05.15  &  +68 25 00.0  &  7.49  &  0.646  &  33.65  &  0.59  &   592.20  &   162.21  &  3  &  1800 & \\
G217-8     & 115704  &  23 26 32.30  &  +60 37 42.4  & 10.49  &  0.469  &   8.85  &  1.43  &   455.75  &    40.74  &  7  & 12~600 & SB1 \\
HD 221876  & 116441  &  23 35 42.62  &  +20 34 51.4  &  9.10  &  0.560  &  13.28  &  1.19  &  --131.09  &  --116.74  &  3  &  4500 & \\
HD 221950  & 116495  &  23 36 23.35  &  +02 06 07.5  &  5.68  &  0.449  &  32.27  &  0.84  &  --104.50  &    62.11  &  3  &  1000 & SB2\\
HD 224930  &    171  &  00 02 09.65  &  +27 05 04.2  &  5.80  &  0.690  &  80.63  &  3.03  &   778.59  &  --918.72  &  3  &   780 & \hspace{-3mm} SB1,em \\
G69-8      &   3054  &  00 38 47.63  &  +31 01 09.5  &  9.04  &  0.630  &  16.48  &  1.19  &  --245.89  &   --58.42  &  4  &  6600 & \\
HD 10443   &   7929  &  01 41 56.28  &  +01 54 10.7  &  8.88  &  0.540  &  14.66  &  1.40  &  --131.30  &  --155.61  &  1  &  3600 & SB1 \\
\noalign{\smallskip}\hline\noalign{\smallskip}
HD 29907   &  21609  &  04 38 21.37  &  --65 25 08.5  &  9.85  &  0.639  &  17.00  &  0.70  &   732.93  &  1249.38  & 3 & 3600 & SB1 \\ 
HD 31128   &  22632  &  04 52 09.80  &  --27 03 50.7  &  9.13  &  0.497  &  15.55  &  0.57  &   165.38  &   --27.80  & 3 & 1500 &  \\
HD 34328   &  24316  &  05 13 04.20  &  --59 38 48.8  &  9.43  &  0.503  &  14.55  &  0.58  &   935.43  &   515.36  & 3 & 1800 &  \\
HD 59392   &  36269  &  07 28 03.10  &  --38 00 38.9  &  9.71  &  0.473  &   6.66  &  0.54  &   159.61  &  --270.15  & 3 & 2400 &  \\
CD--52\degr~2174 &  38526  &  07 53 21.16  &  --52 39 13.6  &  9.50  &  0.490  &   9.43  &  1.70  &    83.83  &    25.14  & 3 & 2100 & SB2 \\    
HD 74000   &  42592  &  08 40 50.59  &  --16 20 38.3  &  9.67  &  0.431  &   7.26  &  0.50  &   351.79  &  --484.80  & 3 & 2100 &  \\
BD--3\degr~2525 &  44124  &  08 59 09.91  &  --04 01 31.4  &  9.66  &  0.481  &  12.37  &  0.55  &   345.31  &  --581.46  & 3 & 2400 & SB2 \\
CD--51\degr~4628 &  50382  &  10 17 14.49  &  --52 29 18.7  & 10.06  &  0.447  &   7.68  &  1.43  &   408.35  &     3.50  & 3 & 3600 &  \\  
HD 97320   &  54641  &  11 11 00.51  &  --65 25 36.0  &  8.16  &  0.484  &  17.77  &  0.56  &   159.19  &  --201.28  & 3 &  720 &  \\
HD 99383   &  55790  &  11 25 49.93  &  --38 52 18.5  &  9.07  &  0.480  &  10.99  &  0.55  &  --124.33  &   173.91  & 3 & 1200 & SB2 \\
HD 102200  &  57360  &  11 45 34.18  &  --46 03 45.4  &  8.75  &  0.434  &  12.45  &  0.50  &    60.31  &  --109.97  & 3 &  900 &  \\
BD--4\degr~3208 &  59109  &  12 07 15.24  &  --05 43 59.6  & 10.00  &  0.413  &   5.75  &  0.48  &  --278.43  &  --228.07  & 3 & 3300 &  \\
HD 122196  &  68464  &  14 01 02.45  &  --38 03 02.5  &  8.73  &  0.463  &   9.77  &  0.53  &  --452.86  &   --82.55  & 3 & 1200 &  \\
HD 140283  &  76976  &  15 43 03.76  &  --10 55 57.9  &  7.20  &  0.484  &  17.44  &  0.56  & --1115.54  &  --302.77  & 3 &  300 &  \\
\hline
\end{tabular}}
\par
\medskip
{Comments: SB1 = known (single-lined) binaries, SB2 = double-lined 
spectra, VB = visual binary, em = \ion{Ca}{ii}~H+K cores in emission.\\ SB1 
binary identifications refer to orbital solutions of Latham et al. 
(\cite{LS02}), except HD~224930 (Underhill \cite{U63}) and HD~29907 (Lindgren 
\& Ardeberg \cite{LA96}). SB2 detections are from our own spectra, except 
HD~99383 (Nissen et al. \cite{NP02}).} 
\end{table}