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Table 2:

Photometric data and absolute magnitudes based on the parallaxes in Table 1.

ID
LHS V   R   I   J    H    $K_{\rm s}$    M(J)       M(K)      
1 1047 11.481 10.271 8.711 7.22 6.71 6.39 8.49   (-0.14,+0.14) 7.66   (-0.14,+0.14)
2 1050 12.612 11.462 10.042 8.62 8.07 7.81 8.33   (-0.08, +0.09) 7.52   (-0.08, +0.09)
3 1104 12.543 11.353 10.343 8.93 8.35 8.10 6.97   (-0.12, +0.12) 6.13   (-0.12, +0.12)
4 1475 10.483 9.503 8.713 7.43 6.80 6.59 6.31   (-0.17, +0.19) 5.48   (-0.17, +0.19)
5 228 15.534 14.425 13.254 12.02 11.52 11.3 8.89   (-0.10, +0.11) 8.17   (-0.10, +0.11)
6 1923 18.094 15.915 13.944 11.92 11.38 11.09 10.14   (-0.08, +0.08) 9.31   (-0.08, +0.08)
7 243 16.096 14.806 13.126 11.51 11.04 10.74 9.58   (-0.06, +0.07) 8.81   (-0.06, +0.07)
8 1976 11.383 10.313 9.413 8.06 7.48 7.24 6.08   (-0.26, +0.29) 5.26   (-0.26, +0.29)
9 2065 18.967 16.787 14.497 11.21 10.47 9.94 11.42   (-0.09, +0.09) 10.1   (-0.09, +0.09)
10 306 14.198 12.808 11.058 9.36 8.76 8.50 9.00   (-0.44, +0.56) 8.14   (-0.44, +0.56)
11 2472 12.812 11.612 10.122 8.70 8.19 7.87 8.43   (-0.09, +0.09) 7.6   (-0.09, +0.09)
12 326 14.939 13.999 13.059 11.93 11.43 11.23 7.06   (-0.74, +1.14) 6.36   (-0.74, +1.14)
13 334 18.0210 16.7010 15.1310 13.75 13.25 13.04 10.47   (-0.35, +0.42) 9.77   (-0.35, +0.42)
14 2632 19.154 16.805 14.764 12.23 11.58 11.21 10.86   (-0.09, +0.10) 9.84   (-0.09, +0.10)
15 ... 14.523 13.353 11.883 9.48 8.91 8.61 9.31   (-0.11, +0.12) 8.44   (-0.11, +0.12)
16 2686 14.1611 12.8811 11.1811 9.58 9.00 8.69 9.51   (-0.10, +0.11) 8.62   (-0.10, +0.11)
17 2719 ... 14.845 13.095 11.28 10.77 10.48 9.12   (-0.19, +0.21) 8.33   (-0.19, +0.21)
18 360 15.229 14.299 13.419 12.39 11.85 11.62 8.64   (-0.34, +0.40) 7.87   (-0.34, +0.40)
19 369 12.962 11.752 10.252 8.74 8.19 7.98 7.93   (-0.12, +0.13) 7.17   (-0.12, +0.13)
20 2924 19.5812 17.285 15.2112 11.99 11.23 10.74 11.62   (-0.14, +0.15) 10.3   (-0.14, +0.15)
21 3343 11.683 10.423 9.323 7.85 7.25 7.00 7.02   (-0.07, +0.07) 6.17   (-0.07, +0.07)
22 3445 11.593 10.313 9.163 7.58 7.03 6.81 6.31   (-0.09, +0.09) 5.54   (-0.09, +0.09)
23 3482 9.793 8.713 7.823 6.88 6.22 6.04 6.06   (-0.11, +0.11) 5.22   (-0.11, +0.11)
24 3494 13.413 11.413 9.763 7.79 7.19 6.85 9.58   (-0.04, +0.04) 8.64   (-0.04, +0.04)
25 528 11.763 10.563 9.523 8.06 7.38 7.18 6.86   (-0.09, +0.09) 5.98   (-0.09, +0.09)
26 3872 13.873 12.433 11.203 9.65 9.09 8.81 7.69   (-0.23, +0.26) 6.85   (-0.23, +0.26)
27 535 12.453 11.203 10.103 8.62 8.10 7.92 8.05   (-0.08, +0.08) 7.34   (-0.08, +0.08)

References. (1) Kilkenny et al. (2007); (2) Bessell (1990); (3) Weis (1996); (4) TOPP see text (5) GSC2.3 transformation see text (6) Dawson & Forbes (1989); (7) Costa et al. (2005); (8) Jao et al. (2005); (9) Costa et al. (2006); (10) Jao et al. (2008); (11) Weistrop (1979); (12) Dahn et al. (2002).

Notes. All infrared magnitudes come from the 2MASS catalogue. Absolute magnitude uncertainties include both parallax and apparent magnitude errors.


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