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Table 1.

Main features of the Cluster-1, Cluster-2, and Cluster-3 mocks.

Cluster proprieties
Cluster-1 Cluster-2 Cluster-3
58 58 58 SUBHALOS

Ngal(Out SR) 80 (80) 200 (22) 200 (22)

NDH 0 0 910

xgal)sys [″] 0.0 0.01 0.01

58 69 69 IMAGES

xim)st [″] 0.2 0.2 0.2

xim)sys [″] 0.0 0.01 0.01

8.66 12.53 13.75 RES.

0.08 0.09 0.09

Notes. The number of galaxies with and without a measured velocity dispersion is given by and Ngal, respectively. For the latter, the number of galaxies, in BAYESLENS, that in principle are free to scatter around the best-fit σ-mag scaling relation is quoted in brackets. The systematic uncertainty assumed on galaxy positions is (Δxgal)sys. The quantity is the total number of observed multiple images, while (Δxim)st and (Δxim)sys are the statistical and systematic isotropic errors assumed on their positions. In the last two lines, the total chi-square and the rms displacement between the measured and model-predicted image positions are listed.

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