Table 2: The calculated optical depths ( $\tau _{\rm GL}$ and $\tau ^p_{\rm L}$ for 3 gravitational lensed objects). The used parameters are: $\Omega _0=0.3,\ \Omega _{\rm L}=0.05$ , F=0.15. $\tau _{\rm GL}$ is the optical depth for macrolensing for quasars located at the same redshifts as the gravitational lensed objects.
Object z $\tau _{\rm GL}$ $\tau ^p_{\rm L}$

MG J0414+0534 2.64 0.013652 0.1151256

QSO 2237+0305 1.695 0.006635 0.0626277

BAL QSO H1413+117 AT 2.56 0.013049 0.1112457

**Table 2:** The calculated optical depths ( $\tau _{\rm GL}$ and $\tau ^p_{\rm L}$ for 3 gravitational lensed objects). The used parameters are: $\Omega _0=0.3,\ \Omega _{\rm L}=0.05$ , F=0.15. $\tau _{\rm GL}$ is the optical depth for macrolensing for quasars located at the same redshifts as the gravitational lensed objects.
Object	z	$\tau _{\rm GL}$	$\tau ^p_{\rm L}$
MG J0414+0534	2.64	0.013652	0.1151256
QSO 2237+0305	1.695	0.006635	0.0626277
BAL QSO H1413+117 AT	2.56	0.013049	0.1112457

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