Stacked cluster dynamical masses overestimate the true mean mass by about 20% at the virial radius, and this can be corrected with two simulation-calibrated factors.
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Dynamical analysis of stacked samples of asymmetric, non-static, self-gravitating systems
Stacked cluster dynamical masses overestimate the true mean mass by about 20% at the virial radius, and this can be corrected with two simulation-calibrated factors.