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J2102+6015: a potential distant multimessenger?

Published online by Cambridge University Press:  11 September 2023

Leonid I. Gurvits Open the ORCID record for Leonid I. Gurvits [Opens in a new window] ,
Sándor Frey Open the ORCID record for Sándor Frey [Opens in a new window] ,
Máté Krezinger Open the ORCID record for Máté Krezinger [Opens in a new window] ,
Oleg Titov Open the ORCID record for Oleg Titov [Opens in a new window] ,
Tao An Open the ORCID record for Tao An [Opens in a new window] ,
Yingkang Zhang ,
Alexander G. Polnarev ,
Krisztina É. Gabányi Open the ORCID record for Krisztina É. Gabányi [Opens in a new window] ,
Krisztina Perger Open the ORCID record for Krisztina Perger [Opens in a new window]  and
Alexey Melnikov Open the ORCID record for Alexey Melnikov [Opens in a new window]
Leonid I. Gurvits
Affiliation:
Joint Institute for VLBI ERIC, Oude Hoogeveensedijk 4, 7991 PD Dwingeloo, The Netherlands Aerospace Faculty, Delft University of Technology, Kluyverweg 1, 2629 HS Delft, The Netherlands
Sándor Frey
Affiliation:
Konkoly Observatory, ELKH Research Centre for Astronomy and Earth Sciences (MTA Centre of Excellence), Konkoly Thege Miklós út 15-17, H-1121, Budapest, Hungary Institute of Physics and Astronomy, ELTE Eötvös Loránd University, Pázmány Péter sétány 1/A, H-1117, Budapest, Hungary
Máté Krezinger
Affiliation:
Konkoly Observatory, ELKH Research Centre for Astronomy and Earth Sciences (MTA Centre of Excellence), Konkoly Thege Miklós út 15-17, H-1121, Budapest, Hungary Department of Astronomy, Institute of Physics and Astronomy, ELTE Eötvös Loránd University, Pázmány Péter sétány 1/A, H-1117, Budapest, Hungary
Oleg Titov
Affiliation:
Geoscience Australia, PO Box 378, Canberra 2601, Australia
Tao An
Affiliation:
Shanghai Astronomical Observatory, CAS, 80 Nandan Road, Shanghai 200030, China
Yingkang Zhang
Affiliation:
Shanghai Astronomical Observatory, CAS, 80 Nandan Road, Shanghai 200030, China
Alexander G. Polnarev
Affiliation:
Queen Mary University of London, London E1 4NS, United Kingdom
Krisztina É. Gabányi
Affiliation:
Konkoly Observatory, ELKH Research Centre for Astronomy and Earth Sciences (MTA Centre of Excellence), Konkoly Thege Miklós út 15-17, H-1121, Budapest, Hungary Department of Astronomy, Institute of Physics and Astronomy, ELTE Eötvös Loránd University, Pázmány Péter sétány 1/A, H-1117, Budapest, Hungary ELKH-ELTE Extragalactic Astrophysics Research Group, Eötvös Loránd University, Pázmány Péter sétány 1/A, H-1117, Budapest, Hungary
Krisztina Perger
Affiliation:
Konkoly Observatory, ELKH Research Centre for Astronomy and Earth Sciences (MTA Centre of Excellence), Konkoly Thege Miklós út 15-17, H-1121, Budapest, Hungary
Alexey Melnikov
Affiliation:
Institute of Applied Astronomy, Russian Academy of Sciences, Kutuzova Embankment 10, St. Petersburg 191187, Russia
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Abstract

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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.

Keywords

SMBH binaryAGNVLBImultimessenger
Type
Contributed Paper
Information
Proceedings of the International Astronomical Union , Volume 17 , Symposium S375: The Multimessenger Chakra of Blazar Jets , December 2021 , pp. 86 - 90
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Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2023. Published by Cambridge University Press on behalf of International Astronomical Union

References

Frey, S., An, T., Gabányi, K., Gurvits, L., Krezinger, M., Melnikov, A., Mohan, P., Paragi, Z., Perger, K., Shu, F., Titov, O., de Vicente, P., & Zhang, Y. 2023, J2102+6015: an Intriguing Radio-loud Active Galactic Nucleus in the Early Universe. PoS, EVN2022(022), arXiv.2301.07355.Google Scholar
Frey, S., Titov, O., Melnikov, A. E., de Vicente, P., & Shu, F. 2018, High-resolution radio imaging of two luminous quasars beyond redshift 4.5. A&A, 618, A68.Google Scholar
Gabányi, K. É., Belladitta, S., Frey, S., Orosz, G., Gurvits, L. I., Rozgonyi, K., An, T., Cao, H., Paragi, Z., & Perger, K. 2023, Very long baseline interferometry observations of the high-redshift blazar candidate J0141-5427. PASA, 40, e004.CrossRefGoogle Scholar
Ivanov, P. B., Papaloizou, J. C. B., Paardekooper, S. J., & Polnarev, A. G. 2015, The evolution of a binary in a retrograde circular orbit embedded in an accretion disk. A&A, 576, A29.Google Scholar
Ivanov, P. B., Papaloizou, J. C. B., & Polnarev, A. G. 1999, The evolution of a supermassive binary caused by an accretion disc. MNRAS, 307(1), 79–90.CrossRefGoogle Scholar
Krezinger, M., Perger, K., Gabányi, K. É., Frey, S., Gurvits, L. I., Paragi, Z., An, T., Zhang, Y., Cao, H., & Sbarrato, T. 2022, Radio-loud Quasars above Redshift 4: Very Long Baseline Interferometry (VLBI) Imaging of an Extended Sample. ApJS, 260(2), 49.CrossRefGoogle Scholar
Perger, K., Zhang, Y., Frey, S., An, T., Gabányi, K., Gurvits, L., Hwang, C.-Y., Koptelova, E., Paragi, Z., & Wang, A. 2023, High-resolution Imaging of Two Radio Quasars at the End of the Reionization Epoch. PoS, EVN2022(024), arXiv:2301.09947.Google Scholar
Sowards-Emmerd, D., Romani, R. W., Michelson, P. F., & Ulvestad, J. S. 2004, Blazar Counterparts for 3EG Sources at -40° <Decl.< 0°: Pushing South through the Bulge. ApJ, 609(2), 564–575.CrossRefGoogle Scholar
Titov, O., Frey, S., Melnikov, A., Shu, F., Xia, B., Gonzalez, J., Tercero, B., Gurvits, L. I., de Witt, A., McCallum, J., Kharinov, M., Zimovsky, V., & Krezinger, M. 2023, Astrometric Apparent Motion of High-Redshift Radio Sources. AJ, 165(69), 12.CrossRefGoogle Scholar
Zhang, Y., An, T., Frey, S., Gabányi, K. É., & Sotnikova, Y. 2022, Radio Jet Proper-motion Analysis of Nine Distant Quasars above Redshift 3.5. ApJ, 937(1), 19.CrossRefGoogle Scholar
Zhang, Y., An, T., Frey, S., Yang, X., Krezinger, M., Titov, O., Melnikov, A., de Vicente, P., Shu, F., & Wang, A. 2021, J2102+6015: a young radio source at z = 4.575. MNRAS, 507(3), 3736–3744.CrossRefGoogle Scholar