  We improve strong lensing constraints on cosmological parameters in light of
the new measurement of the velocity dispersion function of early-type galaxies
based on the SDSS DR5 data and recent semi-analytical modeling of galaxy
formation. Using both the number statistics of the CLASS statistical sample and
the image separation distribution of the CLASS and the PANELS radio-selected
lenses, we find the cosmological matter density $\Om = 0.25^{+0.12}_{-0.08}$
(68% CL) assuming evolutions of galaxies predicted by a semi-analytical model
of galaxy formation and $\Om = 0.26^{+0.12}_{-0.08}$ assuming no evolution of
galaxies for a flat cosmology with an Einstein cosmological constant. For a
flat cosmology with a generalized dark energy, we find the non-evolving dark
energy equation of state $w_x < -1.2$ ($w_x < -0.5$) at the 68% CL (95% CL).
