All Tables

Table 1: Observation log of our MOS- and imaging data.
Table 2: MOS targets in the field of MS 1008-12 observed with Setup A ( $\rm PA=+55^{\circ }$ ) and Setup B ( $\rm PA=-58^{\circ }$ ). There are 7 objects which have been observed in both setups: A3 = B14, A4 = B15, A6 = B6, A8 = B19, A12 = B8, A15 = B11 and A17 = B10. For identification of galaxies see finding chart in Fig. 3.
Table 3: MOS targets in the field of Cl 0303+17 observed with Setup A ( $\rm PA=+45^{\circ }$ ) and Setup B ( $\rm PA=-45^{\circ }$ ). A11 = B6.
Table 4: MOS targets in the field of Cl 0413-65 observed with Setup A ( $\rm PA=-45^{\circ }$ ) and Setup B ( $\rm PA=+45^{\circ }$ ). A11 = B9.
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.
Table 6: Measured rotation velocities $V_{\rm rot}$ as function of projected distance (Pos) to the galaxies' centers (Pos = 0) for MS 1008-12. Galaxies are indicated by their ID with the measured emission line, respectively. See Fig. 4 for comparison.
Table 7: Measured rotation velocities $V_{\rm rot}$ as function of projected distance (Pos) to the galaxies' centers (Pos = 0) for MS 1008-12. Galaxies are indicated by their ID with the measured emission line, respectively. See Fig. 4 for comparison.
Table 8: Measured rotation velocities $V_{\rm rot}$ as function of projected distance (Pos) to the galaxies' centers (Pos = 0) for MS 1008-12. Galaxies are indicated by their ID with the measured emission line, respectively. See Fig. 4 for comparison.
Table 9: Measured rotation velocities $V_{\rm rot}$ as function of projected distance (Pos) to the galaxies' centers (Pos = 0) for Cl 0303+17. Galaxies are indicated by their ID with the measured emission line, respectively. See Fig. 5 for comparison.
Table 10: Measured rotation velocities $V_{\rm rot}$ as function of projected distance (Pos) to the galaxies' centers (Pos = 0) for Cl 0413-65. Galaxies are indicated by their ID with the measured emission line, respectively. See Fig. 6 for comparison.
Table 11: Measured rotation velocities $V_{\rm rot}$ as function of projected distance (Pos) to the galaxies' centers (Pos = 0) for Cl 0413-65. Galaxies are indicated by their ID with the measured emission line, respectively. See Fig. 6 for comparison.