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1 Introduction
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2 Target selection and observations
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3 Data reduction
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4 Galaxy redshifts
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5 Completeness, success rate and potential selection biases
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6 Cluster redshifts and velocity dispersions
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7 Cluster substructure
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8 Discussion
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9 Summary
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Appendix A: Quantitative comparison of the performance
of the two sky subtraction methods
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References
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