Based on observations obtained at the ESO Very Large Telescope (VLT) as part of the Large Programme 166.A-0162 (the ESO Distant Cluster Survey).

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Full Table 4 is only available in electronic form at the CDS via anoymous ftp to cdsarc.u-strasbg.fr (130.79.125.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/427/397

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... hyperz

http://webast.obs-mip.fr/hyperz/

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... IRAF

IRAF is distributed by the National Optical Astronomy Observatories, which are operated by the Association of Universities for Research in Astronomy, Inc., under cooperative agreement with the National Science Foundation.

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... Cl 1040

When computing the success rate, galaxies in Cl 1054-12A and Cl 1054-12B have been considered together, since the separation in redshift (0.0195) is far too small to be separated by any photometric-redshift technique. The lower success rate in Cl 1040 is due to a higher contamination from back- and fore-ground galaxies.

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