Table 9: Clusters with both photometric and spectroscopic redshifts.
Cluster PDCS $\overline{z}_{\rm phot}$ $z_{{\rm spec}}$
V06 - 0.43 $0.3658 \pm 0.0009$
V13 P12 0.32 $0.2630 \pm 0.0020$ (1)
V17 - 0.32 $0.3965 \pm 0.0002$ (2)
V19 P23 0.19 $0.1290 \pm 0.0010$ (1)
V23 P20 0.34 $0.3371 \pm 0.0002$ (2)
V30 - 0.38 $0.3979 \pm 0.0002$ (2)
V36 P11 0.36 $0.3270 \pm 0.0030$ (1)
V48 P24 0.26 $0.2674 \pm 0.0002$ (2)
- P33 0.64 $0.6400 \pm 0.0040$
- P36 0.18 $0.2480 \pm 0.0020$
- P63 0.56 $0.6863 \pm 0.0003$
(1) From Holden et al. (1999).
(2) Redshift from SDSS data for a single galaxy that falls
into the brightest part of the ETS of the cluster.

Source LaTeX | All tables | In the text

Article Contents
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
List of tables
List of figures