Table 7: Redshifts obtained from SDSS.
Cluster $\alpha_{\rm 2000}$ $\delta_{\rm 2000}$ z $\delta z$

(hh:mm:ss) ( $^{\circ}$ :':'')

Galaxy in V17 02:27:45 00:59:20 0.3965 0.0002

Galaxy in V23 02:28:33 00:57:18 0.3371 0.0002

Galaxy in V30 02:26:24 01:00:40 0.3979 0.0002

Galaxy in V48 02:25:23 01:08:50 0.2674 0.0002

**Table 7:** Redshifts obtained from SDSS.
Cluster	$\alpha_{\rm 2000}$	$\delta_{\rm 2000}$	z	$\delta z$
	(hh:mm:ss)	( $^{\circ}$ :':'')
Galaxy in V17	02:27:45	00:59:20	0.3965	0.0002
Galaxy in V23	02:28:33	00:57:18	0.3371	0.0002
Galaxy in V30	02:26:24	01:00:40	0.3979	0.0002
Galaxy in V48	02:25:23	01:08:50	0.2674	0.0002

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