Non-parametric weak-lensing mass profiles of CLASH clusters imply nearly flat circular velocities, while cluster offsets from galaxy scaling relations hinge on uncertain gas extrapolations.
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Mass models of galaxy clusters from a non-parametric weak-lensing reconstruction
Non-parametric weak-lensing mass profiles of CLASH clusters imply nearly flat circular velocities, while cluster offsets from galaxy scaling relations hinge on uncertain gas extrapolations.