Galaxy Evolution in a Pilot Survey up to
and CDM Halos
Figure 4
Spectral fitting results with SSP models for the redshift bin. (a) Observed (thin black line) model (red line) and residuals for the absorption spectrum. Points indicate bad pixels and emission-line windows that were masked out during fitting. (b) Emission-line spectrum; (c) Total spectrum. SSPs do not model emission-lines.
