SIMBAD references

Strong-lensing has developed into an important astrophysical tool for probing cosmology and galaxies (their structures, formations, and evolutions). Now several hundreds of strong-lens systems produced by massive galaxies have been discovered, which may form well-defined samples useful for statistical analyses. We aim to collect relatively complete lens-redshift data from various large systematic surveys of gravitationally lensed quasars and check the possibility of using these as a future supplement to other cosmological probes. We use the distribution of gravitationally-lensed image separations observed in the Cosmic Lens All-Sky Survey (CLASS), the PMN-NVSS Extragalactic Lens Survey (PANELS), the Sloan Digital Sky Survey (SDSS) and other surveys, considering a singular isothermal ellipsoid (SIE) model for galactic potentials as well as improved new measurements of the velocity dispersion function of galaxies based on the SDSS DR5 data and recent semi-analytical modeling of galaxy formation to constrain two dark-energy models (ΛCDM and constant w) under a flat universe assumption. We find that the current lens-redshift data yield a relatively weak constraint on the model parameter Ω_Λ=0.85^+0.11_–0.18 for the simplest cosmological constant model. However, by combing the redshift data with the cosmic macrowave background data, we obtain Ω_Λ=0.78^+0.02_–0.03; by combing the redshift data with the baryonic acoustic oscillation peak and the comic macrowave background data, we obtain a more stringent result: Ω_Λ=0.75^+0.02_–0.02. We obtain w←0.52 at 68.3% CL with the lens-redshift data for the constant w of a dynamical dark-energy model, therefore, the current quintessence dark-energy model is still included at 1σ and a super-negative equation of state is not necessarily favored by this strong lensing data. We notice that the joint data can also provide a good fit with Ω_x=0.80^+0.17_–0.17, w=-1.12^+0.57_–1.88 and Ω_x=0.71^+0.07_–0.07, w=-0.78^+0.22_–0.34, respectively, which agree with the flat Λ CDM model at 1σ.