Properties of selected lens samples that enter the cosmology inference. The sample selection is only based on (i) lens and source existing spectroscopic redshift measurements; (ii) lensing analysis based on imaging data; (iii) LoS analysis. From left to right, the quantities are: lens redshift z_lens, background source redshift z_source, stellar velocity dispersion of the deflector σ_los^ap, half-light radius of the deflector R_eff, Einstein radius θ_E, R_eff/θ_E, lensing power-law slope γ_pl, lensing stellar velocity dispersion σ_SIS, relative over-density ζ_1/R, apparent axis ratio of light profile of the deflector q_light, and lensing information ℐ calculated under the choice of scaling parameters from Sheu et al. (2025). We demonstrate for the selected lenses, there is no significant difference from sample to sample in the parameter spaces of this plot, except for the distribution in redshifts and the difference in effective radius expected from the evolution of the size-mass relation (van Dokkum et al. 2010), see Section 6.6 for more information.