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Galaxy cluster mass reconstruction project I Methods and first results on galaxy based techniques

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Figure

Figure 1. Cluster mass functions for the mock HOD light-cone (blackdashed line) and the selected sample (red solid line)
Table 1. Summary of the participating cluster mass estimation methods. Listed is an acronymidentifying the method, an indication of the scheme used to undertake member galaxy selectionand an indication of the method used to convert this membership list to
Table 2. Values of the constantsof the relation log (amethods that utilize the group/cluster ve-locity dispersion
Figure 3. Recovered versus true mass when the group/cluster membership is not known. The black dotted line represents the 1:1 relation
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