Table 1: 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 IPPARCOS catalogue (ESA 1997). N and $t_{\rm exp}$ refer to the number of spectra taken and the total exposure time (s).

     HD		 HIP   $\alpha(2000)~~$ $\delta(2000)~~$ V   B-V  $\pi$    $\sigma(\pi)$ $\mu(\alpha)$  $\mu(\delta)$  N $t_{\rm exp}$  
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$^\circ $ 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 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
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$^\circ $ 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$^\circ $ 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$^\circ $ 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$^\circ $ 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  
Comments: SB1 = known (single-lined) binaries, SB2 = double-lined spectra, VB = visual binary, em = Ca II H+K cores in emission.
SB1 binary identifications refer to orbital solutions of Latham et al. (2002), except HD 224930 (Underhill 1963) and HD 29907 (Lindgren & Ardeberg 1996). SB2 detections are from our own spectra, except HD 99383 (Nissen et al. 2002).

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