Evidence for X-Ray Emission in Excess to the Jet-afterglow Decay 3.5 yr after the Binary Neutron Star Merger GW 170817: A New Emission Component
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E. Berger | B. Metzger | S. Bernuzzi | J. Zrake | A. MacFadyen | R. Chornock | D. Radice | V. Villar | M. Nicholl | B. Margalit | R. Margutti | O. Gottlieb | G. Hosseinzadeh | W. Fong | P. Blanchard | K. Alexander | T. Eftekhari | C. Kilpatrick | C. Guidorzi | D. Coppejans | G. Terreran | J. Bright | A. Hajela | D. Matthews | L. Sironi | I. Heywood | Y. Cendes | T. Laskar | D. Giannios | R. Duran | V. Nedora | S. Gomez | F. Broekgaarden | A. Kathirgamaraju | X. Xie | J. Rastinejad | A. McDowell | A. Macfadyen