A new LSST-pipeline-based reduction and multi-plane weak-lensing analysis measures the Hercules supercluster at 8.9 x 10^14 solar masses and attributes Abell 2147's inflated dynamical mass to a recent pericenter passage.
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LoVoCCS. III. Third Generation Pipeline & The Hercules Supercluster
A new LSST-pipeline-based reduction and multi-plane weak-lensing analysis measures the Hercules supercluster at 8.9 x 10^14 solar masses and attributes Abell 2147's inflated dynamical mass to a recent pericenter passage.