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Fig. 10.


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HST/ACS COSMOS field reconstructions along known X-ray clusters from the XMM-Newton survey. Top left: Kaiser–Squires (with a Gaussian smoothing of σ = 1 arcmin). Top right: sample from the posterior distribution. Bottom left: mean of the posterior distribution. Bottom right: standard deviation of the posterior distribution (over 400 samples, shown in the clipped range [0, 0.035]).

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