Fig. 3
CDFs (upper panels) and PDFs (lower panels) of the largest effective (left panels) and the median (right panels) Einstein radius for the mass functions of Press-Schechter, Tinker, Sheth & Tormen and Crocce as labelled in the panels. All distributions are based on the simulation of 1000 maxima with Mlim = 2×1014 M⊙ / h in the redshift interval of 0.5 ≤ z ≤ 1.0 on the full sky.
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