Table 3: Completeness and limiting magnitudes.
Field $m_{{\rm c}}$ $m_{{\rm lim}}$

B R B R

F0028+0515 24.4 21.8 26.0 23.1

F0027+0555 24.5 22.9 26.2 24.2

F0228+0115 24.4 22.3 25.8 23.8

F0226+0106 23.4 21.3 24.7 23.3

V I V I

PDCS $0^{{\rm h}}$ 23.5 21.0 24.8 22.8

PDCS $2^{{\rm h}}$ 23.5 21.2 25.1 23.3

**Table 3:** Completeness and limiting magnitudes.
Field	$m_{{\rm c}}$	$m_{{\rm lim}}$
	B	R	B	R
F0028+0515	24.4	21.8	26.0	23.1
F0027+0555	24.5	22.9	26.2	24.2
F0228+0115	24.4	22.3	25.8	23.8
F0226+0106	23.4	21.3	24.7	23.3
	V	I	V	I
PDCS $0^{{\rm h}}$	23.5	21.0	24.8	22.8
PDCS $2^{{\rm h}}$	23.5	21.2	25.1	23.3

Source LaTeX | All tables | In the text

	1 Introduction
	2 Observations and galaxy catalogs
	3 Detecting clusters with the VGCF
	4 The cluster catalog
	5 Color analysis of cluster candidates
	6 Discussion of the VGCF and PDCS cluster detections
	7 Summary
	References
	Online Material