Table 3: Photometry and proper motion of the most obvious candidate members in the field of NGC 5385.
ID TYC 4558- $\alpha (J2000.0)$ $\delta (J2000.0)$ V (B-V) (U-B) $\mu_\alpha \cos \delta$ [mas/yr] $\mu_\delta$ [mas/yr]
1 1641 13:52:54.104 +76:09:59.63 11.29 0.50 0.18 -7.5 $\pm$ 1.9 11.7 $\pm$ 2.1
2 1385 13:52:08.976 +76:10:55.12 11.52 0.39 0.14 2.5 $\pm$ 2.0 -3.0 $\pm$ 2.1
3 457 13:51:58.757 +76:13:20.41 11.39 0.58 0.32 -44.6 $\pm$ 2.0 -6.6 $\pm$ 2.1
4 399 13:52:18.535 +76:10:45.58 11.31 0.68 0.39 -29.0 $\pm$ 2.3 13.8 $\pm$ 2.3
5 1797 13:51:49.975 +76:12:11.67 11.32 0.72 0.56 -23.6 $\pm$ 2.1 17.0 $\pm$ 2.2
6 1873 13:52:32.078 +76:08:07.41 11.78 0.64 0.33 -42.2 $\pm$ 2.2 26.8 $\pm$ 2.3
7 217 13:52:34.850 +76:11:10.84 11.77 1.04 1.03 -12.5 $\pm$ 2.3 6.5 $\pm$ 2.4


Source LaTeX | All tables | In the text