Table of redshifts vs object ID in photometric catalog. These are free for use in any publication with the provision that they are referenced as Glazebrook et al., 1998, in preparation.
The redshift histogram shows an interesting spike
at z=0.585 which probably corresponds to a foreground cluster. 225 R<24
sources were observed spectroscopically at once. Spectral identifications
go as deep as R=24, though the completenss is rather low at the limit due
to an aperture-seeing mismatch.
Here is a plot of redshift vs R magnitude.
The spectra are available for download. Again please reference as above.
The original AAT prime focus images are available, as well as astrometrically corrected images (with WCS headers) of the STIS and WFPC field.