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Table 5.

Global cluster properties measured from our strong lensing mass model.

Cluster Nsys Nimg rmsmodel θE (z = 4) M(θ <  θE(z = 4)) σmodel σdynamics
[″] [″] [1014 M] [km s−1] [km s−1]
A2744 29 (29) 83 (83) 0.67 23.9 0.62 ± 0.04 1394 ± 37 1357 ± 138
A370 45 (39) 137 (122) 0.78 39.5 2.53 ± 0.03 1976 ± 50 1789 ± 109
MACS0257 25 (25) 81 (78) 0.78 28.1 1.10 ± 0.02 1487 ± 30 1633 ± 164
MACS0329 9 (8) 24 (21) 0.53 29.9 1.56 ± 0.08 1621 ± 68 1231 ± 130
MACS0416 71 (71) 198 (198) 0.58 29.9 1.05 ± 0.04 1559 ± 25 1277 ± 93
Bullet 15 (5) 40 (15) 0.39 25.8 0.73 ± 0.02 1601 ± 90 1283 ± 273
MACS0940 7 (7) 22 (22) 0.23 10.9 0.17 ± 0.01 859 ± 291 856 ± 192
MACS1206 37 (36) 113 (110) 0.52 31.5 1.76 ± 0.06 1603 ± 69 1842 ± 184
RXJ1347 36 (35) 121 (119) 0.84 38.6 2.75 ± 0.02 1684 ± 48 1097 ± 121
SMACS2031 13 (13) 46 (45) 0.33 26.1 0.76 ± 0.05 1683 ± 24 1531 ± 210
SMACS2131 10 (10) 28 (29) 0.79 24.4 1.08 ± 0.05 1270 ± 40 1378 ± 408
MACS2214 15 (15) 46 (46) 0.41 22.5 0.99 ± 0.02 1578 ± 60 1359 ± 224

Total 312 (293) 939 (888)

Notes. From left to right: number of multiply-imaged systems, total number of multiple images, global rms of the model, Einstein radius at z = 4, total enclosed mass within the Einstein radius, global velocity dispersion measured from the lens model or the cluster dynamics. Numbers in boldface are confirmed with spectroscopy.

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