Fig. 10
The distribution with redshift of sizes, surface luminosities, and dynamical masses
of the galaxy sample. We show the half-luminosity radii
log Re (top), effective surface
brightness log Ie (middle), and
dynamical mass log Mdyn (bottom) as a
function of redshift for cluster (left) and field
(right) galaxies. Black and red points show spectroscopic types 1
and 2, respectively. Crosses and circles show galaxies with HST and VLT photometry,
respectively. The solid green lines show the mean values in 0.1 redshift bins with
the errors. The dotted lines show the averages obtained by weighting each galaxy
with the inverse of its selection value. The blue lines show the mean luminosity
evolution derived from Fig. 17:
for cluster galaxies and
for the field.
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