Reanalysis of the binary neutron star mergers GW170817 and GW190425 using numerical-relativity calibrated waveform models

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B. D. Metzger, T. A. Thompson and E. Quataert, “A magnetar origin for the kilonova ejecta in GW170817,” Astrophys. J. 856

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S. Z. Li, L. D. Liu, Y. W. Yu and B. Zhang, “What Powered the Optical Transient AT2017gfo Associated with GW170817?,” Astrophys. J. Lett. 861

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