**Table 1:** Cluster candidates selected for observations.
ID	Field^a	$\alpha_{J2000}$	$\delta_{J2000}$	$z_{\rm MF}$	$\Lambda_{\rm cl, org}$
1	EISJ0044-2950A	00 44 58.6	-29 50 49.5	0.3	23.1
2	EISJ0045-2944	00 45 00.8	-29 44 57.7	0.4	35.5
3	EISJ0047-2942	00 47 23.0	-29 42 59.0	0.4	30.4
4	EISJ0048-2928	00 48 25.8	-29 28 50.1	0.4	36.6
5	EISJ0049-2920	00 49 31.3	-29 20 34.1	0.3	35.7
6	EISJ2236-3935	22 36 02.9	-39 35 33.7	0.3	44.5
7	EISJ2236-4026	22 36 47.6	-40 26 17.4	0.4	44.0
8	EISJ2236-4014	22 36 52.6	-40 14 53.0	0.4	37.4
9	EISJ2237-4000	22 37 11.4	-40 00 16.1	0.3	31.3
10	EISJ2238-3934	22 38 03.4	-39 34 50.4	0.3	41.8
11	EISJ2239-3954	22 39 18.4	-39 54 34.9	0.3	62.5
12	EISJ2240-4021	22 40 07.8	-40 21 08.0	0.3	41.2
13	EISJ2241-4006	22 41 26.7	-40 06 24.7	0.3	32.6
14	EISJ2241-3932	22 41 31.3	-39 32 10.4	0.4	44.5
15	EISJ2243-4010A	22 43 01.9	-40 10 24.8	0.3	39.1
16	EISJ2243-3952	22 43 19.4	-39 52 41.2	0.3	50.9
17	EISJ2243-3959	22 43 29.4	-39 59 33.5	0.3	45.0
18	EISJ2243-4010B	22 43 42.7	-40 10 30.4	0.3	32.4
-^b	EISJ2243-4008	22 43 47.4	-40 08 47.0	0.3	34.3
19	EISJ2243-3947	22 43 56.1	-39 47 28.8	0.4	48.6
20	EISJ2244-4008	22 44 21.8	-40 08 21.6	0.4	31.1
21	EISJ2244-4019	22 44 28.4	-40 19 46.5	0.3	38.3
22	EISJ2246-4012B	22 46 48.5	-40 12 48.2	0.4	39.5
23	EISJ2248-4015	22 48 54.8	-40 15 18.8	0.3	36.2

^a Here we have added a ``J'' in the name to conform with international standards. The EIS identification is the same except for this ``J''; ^b overlaps with EISJ2243-4014B and separate observations were not carried out.

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