Table 1: Log of the observations with WFC@INT.
Date Field $t_{{\rm exp}}$ (s) Seeing Airmass

$B_{\rm H}$ band

99-10-13 F0028+0515 10 000 1.6'' 1.8-1.1

99-10-14 F0027+0555 10 000 1.6'' 1.2-1.1

99-10-13 F0228+0115 10 000 1.7'' 1.4-1.2

99-10-14 F0226+0106 10 000 1.1'' 1.6-1.1

$R_{{\rm H}}$ band

99-10-12 F0028+0515 3600 1.4'' 1.8-1.2

99-10-14 F0027+0555 4200 1.6'' 1.9-1.2

99-10-12 F0228+0115 4800 1.2'' 1.7-1.3

99-10-13 F0226+0106 6000 1.4'' 1.5-1.1

**Table 1:** Log of the observations with WFC@INT.
Date	Field	$t_{{\rm exp}}$ (s)	Seeing	Airmass
$B_{\rm H}$ band
99-10-13	F0028+0515	10 000	1.6''	1.8-1.1
99-10-14	F0027+0555	10 000	1.6''	1.2-1.1
99-10-13	F0228+0115	10 000	1.7''	1.4-1.2
99-10-14	F0226+0106	10 000	1.1''	1.6-1.1
$R_{{\rm H}}$ band
99-10-12	F0028+0515	3600	1.4''	1.8-1.2
99-10-14	F0027+0555	4200	1.6''	1.9-1.2
99-10-12	F0228+0115	4800	1.2''	1.7-1.3
99-10-13	F0226+0106	6000	1.4''	1.5-1.1

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