Fig. 2.
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Histograms of the projected distance between 2D weak-lensing mass center and X-ray centroid (left), CAMIRA center (middle), galaxy map peak (right) for 23 CAMIRA clusters. The error bars indicate the statistical uncertainties. The best-fit model (red) consisting of the first and second Gaussian components is indicated by the cyan dashed, and green dotted curves, respectively.
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