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Table 1

Summary of the results of the strong lensing analysis of all 12 MACS clusters by Zitrin et al. (2011) relevant for this work.

MACS z θ eff a r eff Massb
(arcsec) (kpc) (1014 M)

J0717.5+3745 0.546 55 ± 3 353
J0257.1-2325 0.505 39 ± 2 241
J2129.4-0741 0.589 37 ± 2 246
J0744.8+3927 0.698 31 ± 2 222
J0025.4-1222 0.584 30 ± 2 199
J0647.7+7015 0.591 28 ± 2 187
J1149.5+2223 0.544 27 ± 3 173
J0018.5+1626 0.545 24 ± 2 154
J2214.9-1359 0.503 23 ± 2 142
J1423.8+2404 0.543 20 ± 2 128
J0454.1-0300 0.538 83
J0911.2+1746 0.505 68

Notes. The clusters are ordered by effective Einstein radius. Part of the data is based on the work of Ebeling et al. (2007).

(a)

The estimation of the effective Einstein radius assumes a source redshift of zs = 2.0.

(b)

Mass enclosed within the critical curve in 1014 M.

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