[1] | Walsh D, Carswell R F and Weymann R J 1979 Nature 279 381 | 0957 + 561 A, B: twin quasistellar objects or gravitational lens?
[2] | Yang L, Xu L X and Yang W Q 2015 Chin. Phys. Lett. 32 059801 | Constraining Equation of State of Dark Matter: Including Weak Gravitational Lensing
[3] | Biesiada M 2006 Phys. Rev. D 73 023006 | Strong lensing systems as a probe of dark energy in the universe
[4] | Cao S, Biesiada M, Gavazzi R, Piorkowska A and Zhu Z H 2015 Astrophys. J. 806 185 | COSMOLOGY WITH STRONG-LENSING SYSTEMS
[5] | Biesiada M, Piorkowska A and Malec B 2010 Mon. Not. R. Astron. Soc. 406 1055 | Cosmic equation of state from strong gravitational lensing systems
[6] | Cao S and Zhu Z H 2012 J. Cosmol. Astropart. Phys. 03 016 | Constraints on cosmological models from strong gravitational lensing systems
[7] | Wang N and Xu L 2013 Mod. Phys. Lett. A 28 1350057 | STRONG GRAVITATIONAL LENSING AND ITS COSMIC CONSTRAINTS
[8] | Zhu Z H 2000 Mod. Phys. Lett. A 15 1023 | GRAVITATIONAL LENSING STATISTICS AS A PROBE OF DARK ENERGY
[9] | Zhu Z H 2000 Int. J. Mod. Phys. D 9 591 | GRAVITATIONAL LENSING STATISTICAL PROPERTIES IN GENERAL FRW COSMOLOGIES WITH DARK ENERGY COMPONENT(S): ANALYTIC RESULTS
[10] | Chae K H 2003 Mon. Not. R. Astron. Soc. 346 746 | The Cosmic Lens All-Sky Survey: statistical strong lensing, cosmological parameters, and global properties of galaxy populations
[11] | Mitchell J L et al 2005 Astrophys. J. 622 81 | Improved Cosmological Constraints from Gravitational Lens Statistics
[12] | Treu T, Koopmans L V, Bolton A S et al 2006 Astrophys. J. 640 662 | The Sloan Lens ACS Survey. II. Stellar Populations and Internal Structure of Early‐Type Lens Galaxies
[13] | Koopmans L V E, Bolton A, Ture T et al 2009 Astrophys. J. 703 L51 | THE STRUCTURE AND DYNAMICS OF MASSIVE EARLY-TYPE GALAXIES: ON HOMOLOGY, ISOTHERMALITY, AND ISOTROPY INSIDE ONE EFFECTIVE RADIUS
[14] | Kochanek C S 1996 Astrophys. J. 466 638 | Is There a Cosmological Constant?
[15] | Ofek E O, Rix H W and Maoz D 2003 Mon. Not. R. Astron. Soc. 343 639 | The redshift distribution of gravitational lenses revisited: constraints on galaxy mass evolution
[16] | Chae K H and Mao S 2003 Astrophys. J. 599 L61 | Limits on the Evolution of Galaxies from the Statistics of Gravitational Lenses
[17] | Chae K H et al 2004 Astrophys. J. 607 L71 | Constraints on Scalar-Field Dark Energy from the Cosmic Lens All-Sky Survey Gravitational Lens Statistics
[18] | Li X, Cao S, Zheng X, Biesiada M and Zhu Z H 2015 arXiv:1510.03494[astro-ph.CO] |
[19] | Liao K, Li Z, Cao C, Biesiada M, Zheng X and Zhu Z H 2015 arXiv:1511.01318[astro-ph.CO] |
[20] | Chen Y, Geng C, Cao S, Huang Y and Zhu Z 2015 J. Cosmol. Astropart. Phys. 2015 02010 | Constraints on a φCDM model from strong gravitational lensing and updated Hubble parameter measurements
[21] | Eisenstein D J et al 2011 Astron. J. 142 72 | SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS
[22] | Brownstein et al 2012 Astrophys. J. 744 41 | THE BOSS EMISSION-LINE LENS SURVEY (BELLS). I. A LARGE SPECTROSCOPICALLY SELECTED SAMPLE OF LENS GALAXIES AT REDSHIFT ∼0.5
[23] | Ruff A et al 2011 Astrophys. J. 727 96 | THE SL2S GALAXY-SCALE LENS SAMPLE. II. COSMIC EVOLUTION OF DARK AND LUMINOUS MASS IN EARLY-TYPE GALAXIES
[24] | Sonnenfeld A et al 2013 Astrophys. J. 777 98 | THE SL2S GALAXY-SCALE LENS SAMPLE. IV. THE DEPENDENCE OF THE TOTAL MASS DENSITY PROFILE OF EARLY-TYPE GALAXIES ON REDSHIFT, STELLAR MASS, AND SIZE
[25] | Grillo C, Lombardi M et al 2008 Astron. Astrophys. 477 397 | Cosmological parameters from strong gravitational lensing and stellar dynamics in elliptical galaxies
[26] | Jørgensen I, Franx M and Kjærgard P 1995 Mon. Not. R. Astron. Soc. 273 1097 | Multicolour CCD surface photometry for E and S0 galaxies in 10 clusters
[27] | Jørgensen I, Franx M and Kjærgard P 1995 Mon. Not. R. Astron. Soc. 276 1341 | Spectroscopy for E and S0 galaxies in nine clusters
[28] | Lewis A and Bridle S 2002 Phys. Rev. D 66 103511 | Cosmological parameters from CMB and other data: A Monte Carlo approach
[29] | Ade P A R et al 2015 arXiv:1502.01589v2[astro-ph.CO] |