ID | LHS | V | R | I | J | H | ![]() |
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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