Fig. 6
Comparison between the theoretically expected general extreme value (GEV) distribution of the largest Einstein radius and the Einstein radius observed in the galaxy cluster MACS J0717.5+3745. The GEV distribution was fitted to the cumulative distribution of the largest Einstein radii extracted from 2000 mock realisations of the cluster population in the redshift range 0.5 ≤ z ≤ 1.0 (full sky).
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