Abstract

AbstractWe present a new type of observation relating the gravitational wave emission of supermassive black hole mergers to their electromagnetic counterparts. This dual emission involves variability of a relativistic jet arising from the spin‐orbit precession of the supermassive black hole binary at its base. (© 2013 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

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