Table 6: Data of the proposed members of the $\beta $ Pic Association. Column 1: star identification; Cols. 2 and 3: equatorial coordinates; Cols. 4 and 5: proper motions; Col. 6: radial velocities and notes about duplicity; Col. 7: rotational velocities; Cols. 8 and 9: photometry; Col. 10: spectral types; Col. 11: Li equivalent widths; Col. 12: trigonometric parallaxes; Col. 13: kinematical parallaxes; Cols. 14 to 16: space velocities; Cols. 17 to 19: space positions; Col. 20: function F (see text); Col. 21: membership probabilities; Col. 22: notes.
Name $\alpha$ $\delta$ $\mu_{\alpha}$ $\mu_{\delta}$    $V_{\rm r}$ $V{\rm sin}~i$ VJ $V-I_{\rm C}$ SpT $E_{\rm Li}$ $\pi_{\rm tri}~~~$ $\pi_{\rm kin}$ (U,V,W)(X,Y,Z) FProb notes
  2000 2000   mas yr-1  km s-1       mÅ mas    mas km s-1pc     
HIP 10679 02 17 24.7 +28 44 31 86.7 -76.7   5.0$\pm $0.4 8     7.75 0.69 G2V 160 29.4$\pm $5.4 25.5 -12.3-16.2-8.6 -27.619.5-19.8 1.03 1.00 Z, s, N, H, 3
HD 14082 02 17 25.2 +28 44 43 84.3 -77.6   4.6$\pm $0.3 45     6.99 0.59 F5V 140 25.4$\pm $2.8 25.3 -11.7-16.4-8.8 -27.919.7-20.1 1.05 1.00 Z, N, H, 3
BD+30 397B 02 27 28.1 +30 58 41 79.5 -70.1   4.7$\pm $1.3   12.44 2.33 M2Ve 110   23.3 -12.5-16.4-7.9 -31.621.2-19.8 1.39 1.00 Z, s, 3, 5, 6
AG Tri 02 27 29.3 +30 58 25 79.5 -70.1   7.0$\pm $1.1 5   10.12 1.34 K6Ve 220 23.7$\pm $2.0 23.3 -14.2-15.3-8.9 -31.621.2-19.8 1.81 1.00 Z, s, H, 3, 4
BD+05 378 02 41 25.8 +05 59 19 82.3 -55.1 10.0 SB1 40   10.37 1.59 K6Ve 450 24.7$\pm $2.4 25.5 -11.9-15.9-6.6 -25.76.5-28.9 2.62 0.85 Z, S, 3, 7
HD 29391 04 37 36.1 -02 28 25 43.3 -64.2 21.0 95     5.22 0.34 F0V 0 33.6$\pm $0.9   -14.0-16.2-10.1 -24.3-8.2-15.2 1.95 0.90 Z, 2, 1
GJ 3305 04 37 37.5 -02 29 28 46.1 -64.8 20.1   10.59 1.98 M1Ve 120 33.6$\pm $0.9   -13.2-16.0-9.6 -24.3-8.2-15.2 1.01 0.90 Z, 9, 10, 11
V1005 Ori 04 59 34.8 +01 47 02 37.2 -93.9 18.7 14   10.05 1.84 M0Ve 270 37.5$\pm $2.6 41.5 -12.2-15.8-9.2 -21.0-6.7-9.7 0.53 0.90 S, H, 10, 13
CD-57 1054 05 00 47.1 -57 15 26 35.6 72.8 19.4$\pm $0.3 5.8 10.00 1.79 M0Ve 360 38.1$\pm $1.1   -10.8-16.7-9.2 -1.5-20.8-15.9 0.91 0.90 Z, S
HIP 23418 05 01 58.8 +09 59 00 17.2 -82.0 17.3 SB2   11.95* 2.46 M3Ve 0 31.2$\pm $8.6 29.1 -12.2-15.2-10.3 -32.0-5.9-11.1 1.77 0.90 Z, s, 3, 12, 8
HD 35850 05 27 04.7 -11 54 03 17.2 -49.3 22.8 SB2 50     6.56* 0.58 F7V 191 37.3$\pm $0.8   -13.2-17.1-9.9 -20.2-13.8-10.9 1.97 0.90 Z, N, H, 14
$\beta $ Pic 05 47 17.1 -51 04 00 4.7 82.0 20.2$\pm $0.4 139    3.77 0.16 A3V 0 51.9$\pm $0.5   -10.9-16.2-9.2 -3.3-16.2-9.8 0.55 0.90 Z, 1
AO Men 06 18 28.2 -72 02 42 -8.1 71.4 16.3 16.4   9.80 1.32 K4Ve 420 25.9$\pm $0.9   -9.8-16.3-8.8 7.5-33.2-18.3 1.45 0.90 Z, S, 21
HD 139084B 15 38 56.8 -57 42 19 -52.9 -106.0  0.1$\pm $2.0     14.80 2.90 M5Ve 460 25.2$\pm $1.1   -11.9-15.9-10.1 32.0-23.4-1.3 2.71 0.85 Z, S, 3
V343 Nor 15 38 57.6 -57 42 26 -52.9 -106.0  4.2$\pm $1.4 16.6  7.97 0.90 K0V 292 25.2$\pm $1.1   -8.6-18.3-10.2 32.0-23.4-1.3 2.85 0.80 Z, S
V824 Ara 17 17 25.5 -66 57 02 -21.8 -136.5   5.9 SB2 31     7.23* 0.84 G7IV 250 31.8$\pm $0.7   -8.1-17.5-9.3 24.7-17.4-8.8 2.43 0.85 Z, S, 15, 19
HD 155555C 17 17 31.3 -66 57 06 -21.8 -136.5  2.7$\pm1.8$ 6   12.82 2.73 M3Ve 20: 31.8$\pm $0.7   -10.6-15.8-8.4 24.7-17.4-8.8 1.11 0.90 Z, S, 20
CD-54 7336 17 29 55.1 -54 15 49 -7.0 -63.1  1.6$\pm $1.4 35.3  9.55 0.95 K1V 360   15.1 -7.1-16.5-8.7 59.7-25.5-12.5 1.14 0.85 S
HD 161460 17 48 33.8 -53 06 43 -3.9 -56.4  1.4 SB2 10.0  9.61* 0.91 K0IV 320   13.6 -6.8-16.6-8.3 67.1-25.4-16.2 1.34 0.80 S
HD 164249 18 03 03.4 -51 38 56 3.5 -86.5  0.5$\pm $0.4 20     7.01 0.53 F6V 107 21.3$\pm $0.9   -7.0-15.5-9.1 43.2-14.4-11.4 1.95 0.95 Z, H, 1
HD 164249B 18 03 04.1 -51 38 56 3.5 -86.5 -2.4$\pm $1.3   12.5:   M2Ve 70 21.3$\pm $0.9   -9.7-14.6-8.4 43.2-14.4-11.4 1.90 0.95  
V4046 Sgr 18 14 10.5 -32 47 33 2.1 -54.5 -6.9 SB2 13.8 10.94* 1.33 K6Ve 440   13.8 -8.1-16.2-8.4 72.0-0.4-9.1 1.13 0.90 16
GSC 7396-0759 18 14 22.1 -32 46 10 2.1 -54.5 -5.7 SB? 3.0 12.78 2.14 M1Ve 200   13.8 -6.9-16.2-8.6 72.0-0.4-9.2 0.99 0.85  
HD 168210 18 19 52.2 -29 16 32 2.8 -47.2 -7.0$\pm $2.6 114.7  8.89 0.78 G5V 290 13.3$\pm $1.4   -7.1-14.9-7.8 74.54.4-8.8 1.78 0.85 S
HD 172555 18 45 26.9 -64 52 15 32.7 -148.7   3.8 116     4.78 0.20 A6IV 0 34.2$\pm $0.7   -9.5-16.4-10.0 23.3-13.2-11.8 1.08 0.85 Z, H, 17
CD-64 1208 18 45 36.9 -64 51 48 32.7 -148.7  1.0$\pm $3.0 110.0   9.54 1.54 K5Ve 490 34.2$\pm $0.7   -11.8-15.2-8.8 23.3-13.1-11.8 2.04 0.95 Z
TYC 9073-0762 18 46 52.6 -62 10 36 18.1 -76.6  2.4$\pm $0.1 9.9 12.08 2.09 M1Ve 332   18.6 -9.3-15.2-9.5 44.2-22.1-21.2 1.01 0.90 S
TYC 7408-0054 18 50 44.5 -31 47 47 10.6 -77.8 -6.0$\pm $1.0 49.7 11.20 1.76 K7Ve 492   19.8 -7.0-16.6-8.1 49.03.4-12.0 1.95 0.90 S
PZ Tel 18 53 05.9 -50 10 49 16.6 -83.5 -3.4$\pm $0.7 69.0  8.29 0.85 G9IV 287 20.1$\pm $1.2   -10.6-15.4-7.9 45.2-11.1-17.6 2.34 0.95 Z, S
TYC 6872-1011 18 58 04.2 -29 53 05 16.1 -47.2 -4.9$\pm $1.0 33.8 11.78 1.80 M0Ve 483   12.8 -6.3-14.5-10.8 75.48.5-19.6 2.68 0.75 S
CD-26 13904 19 11 44.6 -26 04 09 18.9 -44.2 -8.1$\pm $0.3 9.8 10.27* 1.18 K4V 320   12.6 -8.7-14.6-10.4 75.115.0-21.6 2.50 0.85 S
$\eta$ Tel 19 22 51.2 -54 25 25 25.6 -83.0   0   D4.1" 330:   5.02 -0.02 A0V 0 21.0$\pm $0.7   -9.0-15.4-8.2 40.8-12.6-21.0 1.17 0.95 Z, 3, 18
HD 181327 19 22 58.9 -54 32 16 23.8 -81.8 -0.7 16     7.03 0.53 F6V 120 19.8$\pm $0.8   -9.9-16.0-7.9 43.3-13.4-22.3 1.75 0.90 Z, H, 1
AT MicN 20 41 51.1 -32 26 07 269.3 -365.7 -4.5 10.1 10.99* 2.99 M4Ve 0 97.8$\pm $4.7 105.1 -9.8-15.9-9.6 7.51.5-5.6 1.12 0.90 Z, S
AT MicS 20 41 51.1 -32 26 10 269.3 -365.7 -5.2 15.8 11.09* 3.03 M4Ve 0 97.8$\pm $4.7 105.1 -10.3-16.0-9.2 7.51.5-5.6 0.56 0.90 Z, S
AU Mic 20 45 09.5 -31 20 27 280.4 -360.1 -6.0$\pm $1.7 9.3  8.73 2.09 M1Ve 80 100.6$\pm $1.4   -11.3-16.7-9.6 7.81.7-6.0 1.15 0.90 Z, S
AZ Cap 20 56 02.7 -17 10 54 59.3 -63.0 -6.9 D2.2" 15.6 10.62* 1.49 K6Ve 420   21.6 -9.3-14.8-10.1 32.719.1-26.6 1.65 0.90 Z, S
CP-72 2713 22 42 49.0 -71 42 21 94.1 -54.4  8.6$\pm $0.5 7.5 10.60 1.73 K7Ve 440   27.3 -9.9-16.4-8.1 19.6-18.9-24.5 1.18 0.80 S
WW PsA 22 44 57.9 -33 15 02 183.1 -118.9  2.2 12.1 12.07 2.80 M4Ve 0 42.4$\pm $3.4 49.0 -10.7-15.5-9.8 9.32.1-18.0 0.86 0.95 Z, S
TX PsA 22 45 00.0 -33 15 26 183.1 -118.9  2.4 16.8 13.36 3.09 M5Ve 450   49.0 -10.7-15.4-10.0 9.32.1-18.0 1.18 0.90 Z, S
BD-13 6424 23 32 30.9 -12 15 52 138.1 -83.2  1.8$\pm $0.7 8.8 10.54 1.98 M0Ve 185   35.7 -10.6-15.7-10.1 4.210.4-25.7 1.00 0.90 S
possible members
HD 203 00 06 50.0 -23 06 27 97.3 -47.1  9.7$\pm $2.0 170.7   6.19 0.46 F3V 87 25.6$\pm $0.8   -10.4-14.5-13.3 4.55.8-38.4 4.53 0.45 Z, H
HD 199143 20 55 47.7 -17 06 51 59.2 -61.6 -4.5$\pm $2.1 127.5   7.35* 0.60 F7V 150 21.0$\pm $1.0   -7.8-13.9-11.8 33.719.7-27.3 3.72 0.60 Z, H
Data in italic were taken from the literature; (*) photometric data for SB2 or close visual binaries are corrected taken into account the companions (HIP 23418, CD-26 13904 and HD 199143 have faint visual companions at $\sim$ $1\hbox{$^{\prime\prime}$ }$); Z = proposed member by Zuckerman & Song (2004); s = within SACY definition, but in the Northern Hemisphere, and not observed by us; S = observed in the SACY program; H = photometry from Hipparcos; N = radial velocity and/or $V\sin~i$ from Nordström et al. (2004); (1) Zuckerman et al. (2001a); (2) Barbier-Brossat & Figon (2000); (3) Song et al. (2003); (4) Cutispoto et al. (2000); (5) Weis (1991b); (6) Ianna (1979); (7) Robertson & Hamilton (1987); (8) Koen et al. (2002) (9) Weis (1991a); (10) Gizis et al. (2002); (11) Feigelson et al. (2006); (12) Delfosse et al. (1999); (13) Favata et al. (1995); (14) Wichmann et al. (2003); (15) Strassmeier & Rice (2000); (16) Quast et al. (2000); (17) Erspamer & North (2003); (18) Gray & Garrison (1987); (19) Cutispoto (1998); (20) Eggen (1978); (21) Cutispoto et al. (1999).

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