Fig. 16

Consistency of the shapes of the
profiles of the passive (solid red line) and SF (dashed blue line) cluster galaxy
populations. The profile for the SF galaxy population has been multiplied by 3.7 to
allow for a direct comparison with the profile of the passive galaxy population. The
hatched (orange) region indicates the 1σ confidence level of the
profile of the passive population (that for the SF population is not shown, but it is
much larger).
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