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J2102+6015: a potential distant multimessenger?

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arxiv 2301.12283 v3 pith:L6G6WTGX submitted 2023-01-28 astro-ph.CO gr-qc

Leonid I. Gurvits , Sándor Frey , Máté Krezinger , Oleg Titov , Tao An , Yingkang Zhang , Alexander G. Polnarev , Krisztina É. Gabányi
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Krisztina Perger Alexey Melnikov
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classification astro-ph.COgr-qc
keywords consideredj2102propertiessourceastrometricbinaryblackbriefly
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We present and briefly discuss results of several studies of the source J2102+6015 with tentatively defined redshift z=4:575 which demonstrates unusual properties in imaging and astrometric VLBI observations. Its properties might be considered as indications on the supermassive black hole binary which can be considered as a so far rare example of a high-redshift source of known electromagnetic and, possibly, predictable gravitational wave emissions.

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