All Tables

Table 1: Cluster candidates selected for observations.
Table 2: Identified groups with a significance of at least 99% as obtained by at least one of the employed methods. The ones in bold face are the ones we interpret as causing the cluster detection as discussed in the text. The meaning of the missing $\sigma _v$ 's is described in the text.
Table A.1: Redshifts obtained in the EISJ0045-2923 field. Here and in the following tables an attached ":'' represents a less secure redshift as described in the text, and an "e'' represents that the galaxy has one or more emission lines. The galaxies with redshifts in bold face are the ones considered members of the cluster.
Table A.2: Redshifts obtained in the EISJ0046-2925 field.
Table A.3: Redshifts obtained in the EISJ0052-2923 field.
Table A.4: Redshifts obtained in the EISJ2237-3932 field.
Table A.5: Redshifts obtained in the EISJ2241-3949 field.
Table A.6: Redshifts obtained in the EISJ2243-4013 field.
Table A.7: Redshifts obtained in the EISJ2243-4025 field.
Table A.8: Redshifts obtained in the EISJ2244-3955 field.
Table A.9: Redshifts obtained in the EISJ2245-3952 field.
Table A.10: Redshifts obtained in the EISJ2246-4012A field.