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Fig. 9.


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Comparison of the probability of cluster detection given the input data and the detection method with respect to the S/N. The ratio of detection corresponds the number of samples above 5σ over the total number of samples. The S/N was computed by dividing the maximum κ value of the NFW profile by the noise in the κ field. We considered clusters at redshift zh = 0.5 and concentration c = 1 varying the halo mass.

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