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This page illustrates some of the differences between the old photometric/spec/HI tables, and the most recent (final) ones, available here

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Legend:

Original INT cat = the old photometry table with available redshifts at the time
Marcs_table = the new master tables
New HI = revised optical counterparts for HI detections
OLD HI = the HI table ww used to design the spectroscopic observations (old)
z in HI range = redshifts in the range 0.16 < z < 0.22
Possible HI groups = galaxies near or within an HI detection

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