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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 g0 r0 i0 (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 (g0, r0, and i0), and colors ((g′−i′)0, (r′−i′)0, and (g′−r′)0) obtained in this work.

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