Light bending by the cosmological constant

We revisit the question of whether cosmological constant $\Lambda$ affects gravitational bending light, by numerical integration geodesic equations for a Swiss cheese model consisting point mass and compensated vacuole, in Friedmann-Robertson-Walker background. find that there is virtually no dependence light on not already accounted angular diameter distances standard lensing equations, plus small modifications arise because restricted to finite region covered hole. The residual $10^{13}\,M_{\odot}$ lens at level 1 part $10^7$, even this might be changes hole size evolution as photon crosses. therefore conclude need modification presence constant.