Table 5: All galaxies from which we obtained $V_{\rm max}$. In the case of MS 1008-12 A12 = B8. For an identification see finding charts in Fig. 3. In some cases there was no [OII] line within the spectra and we used other emission lines.
Cluster ID mem Type Incl. $\delta$ $r_{\rm d}$ $V_{\rm max}$ EW ([OII]) MB
        [deg] [deg] [''] [km s-1] [Å] [mag]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
MS 1008-12 A8 yes +8 45 5 0.40 70 $\pm$ 30 72.8 -20.19
MS 1008-12 A12 yes +5 50 43 0.70 220 $\pm$ 59   -20.69
MS 1008-12 A15 yes +5 20 20 0.57 270 $\pm$ 126   -21.24
MS 1008-12 B1 yes +5 60 -9 1.35 130 $\pm$ 23   -20.15
MS 1008-12 B3 no +1 55 63 0.40 320 $\pm$ 129 5.1 -21.26
MS 1008-12 B5 yes +5 60 10 0.60 150 $\pm$ 26   -20.32
MS 1008-12 B8 yes +5 50 -17 0.70 240 $\pm$ 49   -20.69
MS 1008-12 B12 yes +5 50 8 0.60 160 $\pm$ 32   -20.52
MS 1008-12 B14 yes +5 52 -50 1.02 230 $\pm$ 68 15.7 -21.48
Cl 0303+17 B4 yes +3 20 -30 0.80 400 $\pm$ 135 5.1 -22.13
Cl 0303+17 B7 no +5 35 25 0.72 320 $\pm$ 62 19.4 -21.98
Cl 0413-65 A7 no +3 54 19 0.45 200 $\pm$ 26 12.3 -20.94
Cl 0413-65 A8 yes +8 65 -20 0.60 150 $\pm$ 18 39.5 -20.12
Cl 0413-65 A11 no +3 33 0 0.85 350 $\pm$ 96 10.3 -21.65
Cl 0413-65 A13 no +5 50 25 0.55 202 $\pm$ 29 14.1 -21.16
Cl 0413-65 A18 no +5 60 20 0.80 205 $\pm$ 38 36.1 -21.30
Cl 0413-65 B5 no +5 35 -5 0.95 300 $\pm$ 79 25.3 -21.53
Cl 0413-65 B6 yes +5 40 -15 0.25 165 $\pm$ 27 17.1 -20.41
Cl 0413-65 B11 yes +3 55 15 0.52 180 $\pm$ 23 11.4 -21.52
Cl 0413-65 B12 yes +5 43 -75 0.30 230 $\pm$ 130 7.2 -20.42
Cl 0413-65 B14 yes +3 63 -22 0.40 220 $\pm$ 27 4.5 -20.00


Source LaTeX | All tables | In the text