Table 2
List of objects.
Bellini | B − V | V | VQ |
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σHβ |
![]() |
σNa | Kaluzny | Period | Pvar | Vvar | Remark | |
|
|||||||||||||
1 | 69 263 | 0.36 | 18.33 | 1 | 227.5 | 12.7 | –5.7 | 9.2 | |||||
2 | 69 830 | 0.30 | 17.26 | 4 | 239.7 | 12.8 | 25.4 | 13.5 | |||||
3 | 81 157 | 0.22 | 17.23 | 1 | 210.6 | 34.9 | –55.7 | 12.8 | v | ||||
4 | 85 380 | 0.25 | 16.94 | 1 | 230.4 | 12.4 | –50.8 | 17.1 | |||||
5 | 87 731 | 0.48 | 16.37 | 4 | 254.5 | 14.0 | 26.0 | 14.9 | s | ||||
6 | 95 154 | 0.32 | 16.75 | 4 | 256.9 | 15.9 | 2.7 | 6.4 | s | ||||
7 | 95 702 | 0.11 | 17.93 | 1 | 191.2 | 27.6 | –49.1 | 20.7 | v | ||||
8 | 99 931 | 0.29 | 16.16 | 4 | 254.5 | 7.2 | 34.4 | 16.4 | |||||
9 | 100 977 | 0.39 | 16.73 | 1 | 239.7 | 12.0 | –43.4 | 13.7 | s | ||||
10 | 107 036 | 0.27 | 16.61 | 4 | 252.0 | 15.9 | 11.1 | 7.5 | s | ||||
11 | 107 122 | 0.32 | 17.87 | 1 | 202.9 | 16.6 | –47.0 | 15 | |||||
12 | 111 100 | 0.98 | 17.64 | 1 | 185.4 | 11.3 | –53.2 | 7.8 | lrs | ||||
13 | 113 098 | 0.35 | 17.20 | 4 | 248.9 | 13.4 | 13.5 | 9.9 | |||||
14 | 114 490 | 0.28 | 17.78 | 1 | 195.6 | 14.7 | –48.8 | 10 | |||||
15 | 118 163 | 0.45 | 17.65 | 1 | 205.5 | 32.0 | –32.3 | 11.6 | NV337 | 0.269 | EW? | v | |
16 | 121 450 | 1.06 | 18.76 | 4 | 279.6 | 31.8 | 0.0 | 0 | v | rs | |||
17 | 121 591 | 0.24 | 17.47 | 1 | 226.5 | 10.5 | –46.6 | 16.3 | |||||
18 | 124 330 | 0.49 | 16.07 | 1 | 81.2 | 66.1 | 0.0 | 0 | NV369 | 1.788 | ? | v | nm |
19 | 130 105 | 0.35 | 17.70 | 4 | 243.2 | 30.6 | 9.7 | 13.9 | NV401 | 0.354 | ? | v | |
20 | 131 682 | 0.47 | 16.68 | 1 | 197.9 | 10.2 | –52.1 | 10.7 | s | ||||
21 | 133 059 | 0.60 | 15.94 | 4 | 266.9 | 13.0 | 16.0 | 14.3 | |||||
22 | 135 321 | 0.99 | 18.83 | 1 | 232.6 | 10.4 | –20.6 | 27.3 | rs | ||||
23 | 137 605 | 1.19 | 17.73 | 4 | 241.4 | 17.0 | 12.7 | 11.3 | NV332 | 0.247 | EW | rs | |
24 | 140 758 | 0.33 | 17.32 | 1 | 242.6 | 12.4 | –30.9 | 10.6 | |||||
25 | 142 842 | 0.33 | 17.26 | 4 | 241.4 | 30.7 | 2.4 | 11.2 | |||||
26 | 143 829 | 0.43 | 17.08 | 1 | 244.3 | 5.3 | –27.1 | 25.2 | s | ||||
27 | 146 095 | 0.20 | 17.58 | 4 | 256.9 | 64.1 | –7.6 | 11.9 | v | ||||
28 | 146 967 | 1.10 | 17.98 | 1 | 262.7 | 35.6 | 13.1 | 45 | v | lrs | |||
29 | 148 727 | 0.03 | 17.18 | 4 | 246.3 | 17.4 | –4.1 | 15.8 | NV380 | 7.832 | ? | ||
30 | 149 714 | 0.22 | 16.94 | 1 | 230.5 | 14.6 | –49.7 | 12 | |||||
31 | 154 483 | 0.10 | 16.74 | 1 | 228.9 | 13.7 | –49.4 | 9.9 | |||||
32 | 155 556 | 0.85 | 15.08 | 4 | 249.6 | 13.7 | 1.2 | 9.7 | V216 | 23.737 | LT | rg | |
33 | 157 688 | 0.25 | 17.95 | 1 | 225.6 | 13.7 | –40.4 | 10.2 | |||||
34 | 159 485 | 0.35 | 18.40 | 4 | 263.9 | 11.6 | 0.0 | 0 | |||||
35 | 162 119 | 0.99 | 17.63 | 1 | 219.7 | 12.6 | –52.8 | 9.1 | rs | ||||
36 | 166 068 | 1.00 | 17.23 | 1 | 233.8 | 15.2 | –49.2 | 10.7 | s | rs | |||
37 | 167 555 | 1.03 | 16.38 | 4 | 272.3 | 15.5 | 15.3 | 13.9 | rs | ||||
38 | 171 825 | 0.51 | 16.63 | 4 | 253.2 | 14.7 | 6.4 | 15.1 | |||||
39 | 176 840 | 0.25 | 16.92 | 1 | 229.2 | 15.8 | –43.7 | 8.4 | |||||
40 | 177 256 | 0.57 | 15.69 | 4 | 237.3 | 17.6 | –2.4 | 9 | V259 | 19.120 | sp? | ||
41 | 179 912 | 0.32 | 16.44 | 1 | 229.8 | 23.0 | 0.0 | 0 | V239 | 1.189 | EA | v | |
42 | 180 526 | 0.97 | 17.78 | 4 | 250.4 | 16.2 | –35.0 | 11.6 | – | s | rs | ||
43 | 234 296 | 0.15 | 17.69 | 3 | 251.2 | 7.8 | 0.0 | 0 | |||||
44 | 234 998 | 0.39 | 18.20 | 2 | 237.4 | 24.5 | –2.1 | 15.5 | NV361 | 0.682 | EA | v | |
45 | 241 994 | 0.30 | 17.63 | 3 | 227.8 | 14.0 | 7.3 | 17.5 | |||||
46 | 244 408 | 0.41 | 17.01 | 2 | 248.0 | 28.9 | –12.3 | 14.8 | V208 | 0.306 | EW | v | |
47 | 249 955 | 0.49 | 16.51 | 2 | 222.0 | 13.4 | –13.9 | 15.7 | s | ||||
48 | 250 383 | 0.34 | 17.37 | 3 | 255.4 | 21.5 | 0.0 | 0 | v | ||||
49 | 253 226 | 1.02 | 17.73 | 3 | 237.8 | 9.3 | 0.0 | 0 | s | rs | |||
50 | 253 281 | 1.00 | 18.55 | 2 | 225.2 | 22.1 | –24.0 | 25.4 | v | rs | |||
51 | 258 274 | 0.49 | 16.88 | 2 | 206.9 | 27.0 | –21.3 | 17.3 | v | ||||
52 | 258 539 | 0.18 | 16.84 | 3 | 241.0 | 10.8 | 19.3 | 8.4 | s | ||||
53 | 262 766 | 0.94 | 14.10 | 2 | 246.1 | 18.4 | –11.3 | 22 | NV390 | 15.710 | ? | s | rg |
54 | 263 560 | 0.37 | 17.30 | 3 | 207.3 | 18.4 | 9.8 | 14.3 | v | ||||
55 | 265 591 | 0.29 | 17.29 | 2 | 219.1 | 19.7 | 0.0 | 0 | |||||
56 | 269 775 | 0.45 | 16.87 | 3 | 235.7 | 11.5 | 17.4 | 8 | s | ||||
57 | 274 338 | 0.18 | 16.98 | 2 | 237.3 | 6.8 | –13.1 | 17 | s | ||||
58 | 277 621 | 0.98 | 18.08 | 3 | 241.9 | 16.7 | –27.6 | 10.2 | s | rs | |||
59 | 279 427 | 0.29 | 17.80 | 2 | 239.7 | 30.5 | 31.7 | 16.7 | v | ||||
60 | 281 267 | 0.10 | 18.26 | 3 | 259.5 | 17.5 | 0.0 | 0 | |||||
61 | 287 148 | 0.28 | 17.33 | 3 | 230.0 | 15.0 | 16.0 | 11.2 | s | ||||
62 | 289 620 | 0.25 | 17.47 | 2 | 256.7 | 34.1 | 0.0 | 0 | v | ||||
63 | 293 439 | 0.58 | 17.24 | 2 | 243.9 | 31.9 | –7.7 | 16.9 | V212 | 2.467 | EA | v | |
64 | 297 708 | 0.39 | 17.77 | 2 | 238.5 | 26.6 | –18.1 | 14.5 | V207 | 0.276 | EW | v | |
65 | 297 731 | 0.22 | 16.56 | 3 | 256.5 | 22.6 | 15.7 | 11.3 | V209 | 0.834 | EA | v | |
66 | 302 520 | 0.28 | 17.15 | 3 | 230.9 | 8.6 | 0.0 | 0 | V205 | 0.369 | EA | ||
67 | 304 775 | 0.52 | 15.77 | 3 | 44.4 | 15.9 | 35.0 | 8.9 | nm | ||||
68 | 306 843 | 1.12 | 18.33 | 3 | 206.0 | 14.8 | 23.0 | 6.5 | lrs | ||||
69 | 311 900 | 0.64 | 15.12 | 2 | 228.5 | 17.0 | –11.9 | 11.1 | s | ||||
70 | 312 254 | 0.16 | 16.10 | 3 | 246.7 | 15.1 | 18.3 | 6.7 | NV374 | 3.311 | ? | ||
71 | 317 269 | 0.47 | 16.47 | 2 | 240.6 | 14.5 | –11.6 | 14 | s | ||||
72 | 319 396 | 0.22 | 16.01 | 2 | 241.9 | 17.0 | –12.7 | 11.1 | V192 | 1.376 | EA | ||
73 | 321 474 | 0.62 | 17.86 | 3 | 256.6 | 74.6 | 7.5 | 16.4 | NV363 | 0.824 | EA | v | to |
74 | 328 605 | 0.84 | 16.19 | 3 | 233.8 | 19.8 | 14.9 | 6.9 | NV379 | 7.104 | ? | v | rg |
Notes. Bellini – object’s number in Bellini et al. (2009). B − V-color index, not corrected for reddening. V – V-band magnitude. VQ – number of VIMOS quadrant. and σHβ – mean value and rms deviation of velocity calculated from Hβ.
and σNa – mean value and rms deviation of velocity calculated from the interstellar NaI D2 line (0 if the spectrum did not reach to the NaI doublet). Kaluzny – object’s number in Kaluzny et al. (2004). Period – photometric period in days. Pvar – type of photometric variability after Kaluzny et al. (2004): EA = Algol; EW = W UMa; LT = long term; SP = spotted. Vvar – flag for velocity variability: v = variable; s = suspected. Remarks: rs = red straggler; lrs = likely red straggler; rg = red giant; to = turnoff object; blank – object located to the left of main sequence and red giant branch (blue straggler, yellow straggler or hot subdwarf). The velocities are given in the heliocentric frame without corrections described in Sect. 3.3. The values of the corrections are 9.4, –3.4, –6.6 and 21.0 km s-1 for quadrants 1–4, respectively.
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