Measured isotropic (top sub-panel in each panel) and anisotropic (bottom sub-panel in each panel, note the varying y-axis scale) shear signal around red (left) and blue (right) lenses in the NGVSLenS fields. From top to bottom: decreasing stellar mass bins as indicated. For better readability the anisotropic signal has been scaled by r. The best-fitting NFW shear profile constrained within 45 kpc/h₇₀ <  r <  200 kpc/h₇₀ is shown by the curve for the isotropic signal. For (f − f₄₅)ΔΣ the curves show models computed from the best-fit isotropic model and the best-fit f_h for the solid curve, and f_h ∈ { + 1, 0, −1} for the dotted curves, respectively. The best-fit f_h has been constrained from (f − f₄₅)ΔΣ and ΔΣ within 45 kpc/h₇₀ <  r <  r_200c (range indicated by vertical lines), where r_200c has been estimated from the isotropic signal. The corresponding figures for the other surveys are shown in Appendix C.