Galaxy Evolution in a Pilot Survey up to
and CDM Halos
Figure 7
Composite spectra of galaxies with emission-lines: (a) blue half; (b) red half; and (c) reddest. Spectra have been normalized in the wavelength range Å and shifted for clarity. The S/N ratios of the continuum in the wavelength range Å are given in Tables 7, 8, and 12.Note the probable contamination of blue spectra by Seyferts (conventionally defined as galaxies with ; [30]).
