Table 2: Coordinates and areas of INT pointings and PDCS fields.
Field $\alpha_{{2000}}$ $\delta_{{2000}}$ Area (sq. deg.)

$B_{\rm H}$ $R_{{\rm H}}$

F0028+0515 00:28:50 05:15:20 0.277 0.284

F0027+0555 00:27:25 05:55:35 0.296 0.321

F0228+0115 02:28:05 01:15:30 0.285 0.303

F0226+0106 02:26:25 01:06:20 0.325 0.294

V₄ I₄

PDCS $0^{{\rm h}}$ 00:29:11 05:31:55 1.074 0.970

PDCS $2^{{\rm h}}$ 02:28:33 00:55:45 1.120 0.927

**Table 2:** Coordinates and areas of INT pointings and PDCS fields.
Field	$\alpha_{{2000}}$	$\delta_{{2000}}$	Area (sq. deg.)
			$B_{\rm H}$	$R_{{\rm H}}$
F0028+0515	00:28:50	05:15:20	0.277	0.284
F0027+0555	00:27:25	05:55:35	0.296	0.321
F0228+0115	02:28:05	01:15:30	0.285	0.303
F0226+0106	02:26:25	01:06:20	0.325	0.294
			V₄	I₄
PDCS $0^{{\rm h}}$	00:29:11	05:31:55	1.074	0.970
PDCS $2^{{\rm h}}$	02:28:33	00:55:45	1.120	0.927

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