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Ish: The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VIII. A Comparison to Cosmological Short-duration Gamma-Ray Bursts

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2. No velocity-kicks are required to explain large-distance offsets of Ca-rich supernovae and short-GRBs

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3. Optical superluminal motion measurement in the neutron-star merger GW170817

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