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The SAMI galaxy survey : the cluster redshift survey, target selection and cluster properties

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Figure

Table 1. Clusters selected for SAMI observations. Clusters are ordered in increasing mass (per the caustic estimate)
Figure 1. Colour–magnitude diagrams for the SAMI-CRS clusters with VST/ATLAS photometry
Table 2. Summary of the SAMI-CRS and archival 2dF/AAOmega data.
Figure 3. Upper left panel: an example of a single Gaussian fit (red line) to the profile (black crosses) at column 1485, centred around row 860 for one of the2by the 2flat-fields
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