Table 4: Number of stellar sources (N^*) detected in each filter and relative limiting magnitudes at the 10 $\sigma$ , 5 $\sigma$ , 3 $\sigma$ and 95% completeness level.
Filter N^* Mag 10 $\sigma$ Mag 5 $\sigma$ Mag 3 $\sigma$ Mag (C=95%)

Rc/162 141 400 21.8 22.6 23.2 21.3

Ic/Iwp 141 000 21.0 21.7 22.3 21.0

z+/61 79 000 18.7 19.6 20.2 18.8

H $\alpha$ /7 72 500 17.5 19.8 20.4 18.0

H $\alpha$ /12 84 200 17.8 19.9 20.8 18.4

856-nm 76 700 18.6 19.4 20.0 18.0

914-nm 80 400 18.9 19.5 20.1 18.0

**Table 4:** Number of stellar sources (N^*) detected in each filter and relative limiting magnitudes at the 10 $\sigma$ , 5 $\sigma$ , 3 $\sigma$ and 95% completeness level.
Filter	N^*	Mag 10 $\sigma$	Mag 5 $\sigma$	Mag 3 $\sigma$	Mag (C=95%)
Rc/162	141 400	21.8	22.6	23.2	21.3
Ic/Iwp	141 000	21.0	21.7	22.3	21.0
z+/61	79 000	18.7	19.6	20.2	18.8
H $\alpha$ /7	72 500	17.5	19.8	20.4	18.0
H $\alpha$ /12	84 200	17.8	19.9	20.8	18.4
856-nm	76 700	18.6	19.4	20.0	18.0
914-nm	80 400	18.9	19.5	20.1	18.0

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