Galaxy Evolution in a Pilot Survey up to
and CDM Halos
Figure 6
Diagram of the 4000 Å break amplitude plotted versus the equivalent width of [OII] for all the galaxies of our sample. The global parameters measured in the combined spectra are overplotted in different colors labeled by their redshifts. Individual errors are not shown; the bulk of individual spectra have typical errors of in D(4000) and in EQW([OII]).
