Table 4: Magnification factors $\mu$ from the lensing models of A1835 and AC114 predicted for various source redshifts $z_{\rm s}$ . The values of $\mu$ are dimensionless magnification factors, and not in magnitudes.
Object $z_{\rm s}=0.5$ $z_{\rm s}=1.$ $z_{\rm s}=2.$ $z_{\rm s}=3.$ $z_{\rm s}=7.$

A1835-#1 1.13 1.21 1.26 1.28 1.33

A1835-#2 1.38 1.71 1.95 2.05 2.32

A1835-#3 1.24 1.43 1.54 1.59 1.72

A1835-#4 1.25 1.45 1.57 1.62 1.76

A1835-#10 1.19 1.33 1.42 1.45 1.54

A1835-#11 1.14 1.23 1.28 1.30 1.35

A1835-#17 1.14 1.23 1.28 1.30 1.36

AC114-#1 1.49 2.24 2.87 3.15 4.03

**Table 4:** Magnification factors $\mu$ from the lensing models of A1835 and AC114 predicted for various source redshifts $z_{\rm s}$ . The values of $\mu$ are dimensionless magnification factors, and not in magnitudes.
Object	$z_{\rm s}=0.5$	$z_{\rm s}=1.$	$z_{\rm s}=2.$	$z_{\rm s}=3.$	$z_{\rm s}=7.$
A1835-#1	1.13	1.21	1.26	1.28	1.33
A1835-#2	1.38	1.71	1.95	2.05	2.32
A1835-#3	1.24	1.43	1.54	1.59	1.72
A1835-#4	1.25	1.45	1.57	1.62	1.76
A1835-#10	1.19	1.33	1.42	1.45	1.54
A1835-#11	1.14	1.23	1.28	1.30	1.35
A1835-#17	1.14	1.23	1.28	1.30	1.36
AC114-#1	1.49	2.24	2.87	3.15	4.03

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