Notes. The table shows the lens and source redshifts z_l and z_s, the Einstein radius θ_E in arcseconds, the effective radius R_eff in arcseconds, the stellar mass in log M_*/M_⊙ (for SL2S lenses adjusted for the comparison), the slit width and length in arcseconds for SL2S systems, the fiber radius R_fib in arcseconds for SLACS and BELLS lenses, the measured velocity dispersion within the aperture σ_ap in , the atmospheric seeing FWHM in arcseconds, the derived mass slope γ (Sect. 4.2), and the survey name of the lens system. The lines indicate a change of redshift bin. All values, except the mass slope, for the SLACS and BELLS lenses are from Chen et al. (2019). For the BELLS lenses, the atmospheric seeing is not available for the lens systems used here, so we took the average seeing of those BELLS lenses with values for the seeing. The SL2S slit sizes, velocity dispersions, and seeings are from Sonnenfeld et al. (2013a); Sonnenfeld et al. (2015). For systems with more than one velocity dispersion, we took the median of the velocity dispersion values weighted by their signal-to-noise ratio.