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Home All issues Volume 500 / No 2 (June III 2009) A&A, 500 2 (2009) 735-747 Full HTML
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Table 1:

Spectroscopic sample in the Leo I field.
ID $\alpha$ (J2000) $\delta$ (J2000) B-V V v $\Delta v$ S/N Other
          km s-1 km s-1    
1 10:08:28.43 +12:15:54.1 1.39 19.62 268.2 1.5 57  
2 10:08:16.47 +12:15:59.5 1.48 19.59 264.5 3.2 46  
3 10:08:36.41 +12:16:02.2 1.46 19.89 261.9 5.7 37  
4 10:08:17.58 +12:16:15.7 1.61 19.55 267.0 0.9 42  
5 10:08:19.45 +12:16:34.1 1.10 20.28 268.6 3.2 32 B8391
6 10:08:40.46 +12:16:38.0 1.35 19.78 273.5 0.4 36 B25113
7 10:08:31.00 +12:16:40.6 1.32 19.85 282.4 3.1 58 B18214
8 10:08:03.62 +12:16:46.4 1.50 19.74 301.0 7.4 59  
9 10:08:32.56 +12:16:54.9 1.19 20.45 290.7 1.5 33  
10 10:08:08.79 +12:17:05.9 1.07 20.00 304.3 2.2 90  
11 10:08:10.61 +12:17:08.0 1.20 20.05 262.2 6.8 62 B4173
12 10:08:49.42 +12:17:14.8 1.18 20.44 281.2 2.5 18  
13 10:08:34.90 +12:17:17.8 1.16 20.01 287.8 6.8 38  
14 10:08:39.66 +12:17:19.9 1.37 19.68 258.4 3.7 44 K195
15 10:08:57.38 +12:17:20.8 1.18 20.44 280.3 6.6 34 K833
16 10:08:55.47 +12:17:21.9 1.26 20.14 274.2 10.9 43  
17 10:08:11.82 +12:17:29.4 1.05 20.31 260.0 0.6 51  
18 10:08:29.89 +12:17:31.7 1.30 19.67 262.8 4.8 43  
19 10:08:07.52 +12:17:34.6 1.25 20.16 269.6 7.4 52  
20 10:08:14.21 +12:17:36.1 1.11 19.90 247.6 32.2 67 B5496
21 10:08:15.40 +12:17:38.3 1.43 19.48 266.1 3.0 37  
22 10:08:46.36 +12:17:41.3 1.33 20.32 261.9 2.9 30  
23 10:08:20.50 +12:17:45.0 1.61 19.64 263.7 0.3 50  
24 10:08:06.29 +12:17:45.3 1.28 20.16 269.9 7.1 49 B3135
25 10:08:50.70 +12:17:46.9 1.15 20.31 270.5 6.7 35 K677
26 10:07:55.77 +12:17:55.2 1.14 20.48 277.3 6.0 47  
27 10:08:01.84 +12:17:56.6 1.43 19.82 275.4 5.4 61 B2488
28 10:08:45.25 +12:17:57.8 1.28 20.08 248.9 5.5 52  
29 10:08:38.58 +12:18:21.0 0.94 19.71 274.5 8.3 41  
30 10:08:56.58 +12:18:22.4 1.13 20.22 271.1 0.3 30  
31 10:08:34.85 +12:18:22.6 1.24 19.98 256.2 0.1 47  
32 10:08:15.96 +12:18:25.3 1.17 20.25 282.9 3.0 34  
33 10:07:57.28 +12:18:26.1 1.40 19.74 284.3 7.5 69  
34 10:08:44.09 +12:18:29.0 1.13 19.66 278.8 9.5 42  
35 10:08:47.87 +12:18:29.9 1.46 19.70 248.8 8.0 39  
36 10:08:36.01 +12:18:32.6 1.30 19.58 254.0 0.6 45  
37 10:07:59.36 +12:18:35.7 1.60 19.75 273.9 6.3 54  
38 10:08:58.70 +12:18:37.1 1.44 19.85 257.2 8.2 46  
39 10:08:41.92 +12:18:39.7 1.16 20.22 250.4 7.8 31 B25820
40 10:08:51.73 +12:18:45.7 1.28 20.23 278.9 3.0 49  
41 10:08:20.21 +12:18:46.6 1.41 19.62 258.0 0.1 27  
42 10:08:33.75 +12:18:47.0 1.26 19.23 275.4 0.0 50  
43 10:08:24.22 +12:18:53.3 1.38 19.93 259.0 2.4 42  
44 10:08:40.60 +12:19:02.8 1.25 19.66 276.9 2.7 48  
45 10:08:30.67 +12:19:30.0 1.00 20.34 259.4 4.6 39  
46 10:08:21.15 +12:19:43.6 1.52 19.72 270.8 1.0 35  
47 10:08:39.42 +12:20:05.9 1.16 19.74 271.2 3.8 51  
48 10:08:37.29 +12:20:12.2 1.24 19.88 270.7 1.3 43 K351
49 10:08:13.35 +12:20:13.8 1.27 19.64 292.2 2.9 55  
50 10:08:22.17 +12:20:14.9 1.38 19.15 289.8 0.9 59  
51 10:08:28.41 +12:20:29.6 1.51 19.61 267.6 2.1 64 K137
52 10:08:14.96 +12:20:43.9 1.47 19.58 266.6 2.9 50  
53 10:08:19.17 +12:20:48.9 1.38 19.87 255.3 2.0 38 B8203
54 10:08:18.24 +12:20:54.6 1.27 20.02 268.0 0.7 31  
101 10:07:51.18 +12:17:36.6 1.52 19.56 49.6 8.5 72  
102 10:08:05.23 +12:18:13.5 1.05 19.96 -27.9 5.5 52  
103 10:08:53.43 +12:18:27.4 1.36 19.88 90.4 8.7 55  
Notes. v is the heliocentric radial velocity and $\Delta v$ the absolute semi-difference in radial velocity of the individual spectra. The last column gives the identification of stars in common with Bosler et al. (2007) and Koch et al. (2007b).

Source LaTeX | All tables | In the text

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