Table B.1.
Properties of the candidates in our sample for which Mieske et al. (2007) confirmed the membership to the Centaurus cluster.
CCOS | RA | DEC | V0 | (V-R)0 | vr | CLASSi′ | g′0 | r′0 | i′0 | (g′−i′)0 | (r′−i′)0 | (g′−r′)0 |
---|---|---|---|---|---|---|---|---|---|---|---|---|
(hh:mm:ss) | (° ′ ″) | (mag) | (mag) | (km s−1) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag) | ||
J1248.79-4117.15 | 12:48:47.6 | -41:17:09.9 | 21.1 | 0.5 | 2882±54 | 0.983 | 21.521±0.007 | 20.873±0.004 | 20.508±0.003 | 1.013 | 0.364 | 0.648 |
J1248.74-4118.58 | 12:48:44.7 | -41:18:35.3 | 21.76 | 0.44 | 2189±114 | 0.609 | 22.037±0.010 | 21.570±0.006 | 21.333±0.007 | 0.704 | 0.238 | 0.466 |
J1248.76-4118.70 | 12:48:45.5 | -41:18:42.4 | 21.77 | 0.55 | 2828±45 | 0.982 | 22.087±0.010 | 21.432±0.005 | 21.098±0.005 | 0.989 | 0.334 | 0.655 |
J1248.97-4120.01 | 12:48:58.2 | -41:19:59.7 | 22.12 | 0.52 | 2962±98 | 0.979 | 22.111±0.011 | 21.461±0.006 | 21.141±0.006 | 0.970 | 0.320 | 0.650 |
J1248.74-4118.95 | 12:48:44.1 | -41:18:57.1 | 22.17 | 0.53 | 3213±53 | 0.983 | 22.390±0.013 | 21.796±0.007 | 21.550±0.008 | 0.840 | 0.246 | 0.594 |
J1248.70-4118.23 | 12:48:42.0 | -41:18:14.4 | 22.18 | 0.48 | 2822±55 | 0.979 | 22.177±0.011 | 21.455±0.006 | 21.100±0.005 | 1.077 | 0.354 | 0.723 |
J1248.91-4117.70 | 12:48:54.6 | -41:17:42.4 | 22.29 | 0.43 | 2909±120 | 0.979 | 22.536±0.015 | 22.000±0.008 | 21.727±0.009 | 0.809 | 0.273 | 0.536 |
J1248.99-4118.08 | 12:48:59.6 | -41:18:04.7 | 22.31 | 0.53 | 2806±75 | 0.984 | 22.528±0.015 | 21.943±0.008 | 21.680±0.009 | 0.848 | 0.263 | 0.585 |
Notes. The columns report the name of the source (CCOS), the coordinates (RA and DEC), the extinction-corrected V magnitude (V0), the extinction-corrected color index (V-R)0, and the radial velocity (vr) obtained by Mieske et al. (2007). The last columns show the stellarity index (CLASSi′), extinction-corrected magnitudes (g′0, r′0, and i′0), and colors ((g′−i′)0, (r′−i′)0, and (g′−r′)0) obtained in this work.
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