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Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational-Wave Event S190521g.
Graham, M J; Ford, K E S; McKernan, B; Ross, N P; Stern, D; Burdge, K; Coughlin, M; Djorgovski, S G; Drake, A J; Duev, D; Kasliwal, M; Mahabal, A A; van Velzen, S; Belecki, J; Bellm, E C; Burruss, R; Cenko, S B; Cunningham, V; Helou, G; Kulkarni, S R; Masci, F J; Prince, T; Reiley, D; Rodriguez, H; Rusholme, B; Smith, R M; Soumagnac, M T.
Phys Rev Lett ; 124(25): 251102, 2020 Jun 26.
Article in English | MEDLINE | ID: mdl-32639755

ABSTRACT

We report the first plausible optical electromagnetic counterpart to a (candidate) binary black hole merger. Detected by the Zwicky Transient Facility, the electromagnetic flare is consistent with expectations for a kicked binary black hole merger in the accretion disk of an active galactic nucleus [B. McKernan, K. E. S. Ford, I. Bartos et al., Astrophys. J. Lett. 884, L50 (2019)AJLEEY2041-821310.3847/2041-8213/ab4886] and is unlikely [

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