  For 18 well-observed gravitationally lensed QSOs, we compare new
non-parametric mass profiles for the lensing galaxies with stellar-population
models derived from published HST photometry. The large volume of parameter
space searched -- with respect to the possible star formation histories --
allows us to infer robust estimates and uncertainties for the stellar masses.
The most interesting results are: (1) the transition from little or no dark
matter in the inner regions (<r_e) to dark matter dominating on the ~5r_e scale
(~20 kpc) is clearly seen in massive ellipticals; (2) Such a trend is not seen
in lower-mass galaxies, so that the stellar content dominates the mass budget
out to ~5r_e; (3) the radial gradient in the dark-matter fraction for these
intermediate redshift galaxies agrees with published data on nearby galaxies.
This result can help reconcile the discrepancies found in recent estimates of
dark matter in elliptical galaxies using different techniques (e.g. Planetary
nebulae versus X-ray). The observed trend suggests the stellar component in
massive galaxies extends further out in terms of the dark matter scale radius.
