Open Access

Table 2.

Distribution of the objects in the reliable spectroscopic sample.

QF ≥ 3 MUSE VIMOS DEIMOS CNN
Total 432 11 47
Stars 31 0 0
Foreground 42 1 5
Background 146 1 7
Cluster members 213 9 35 110

C.M. mF160W ≤ 21 85 9 35 24

Notes. For completeness, photometric cluster members identified by a CNN are also reported (see Sect. 3.1).

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