Primary black hole spin in OJ287 as determined by the General Relativity centenary flare

M. J. Valtonen , S. Zola , S. Ciprini , A. Gopakumar , K. Matsumoto , K. Sadakane , M. Kidger , K. Gazeas

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K. Nilsson A. Berdyugin V. Piirola H. Jermak K. S. Baliyan F. Alicavus D. Boyd M. Campas Torrent F. Campos J. Carrillo Gomez D. B. Caton V. Chavushyan J. Dalessio B. Debski D. Dimitrov M. Drozdz H. Er A. Erdem A. Escartin Perez V. Fallah Ramazani A. V. Filippenko S. Ganesh F. Garcia F. Gomez Pinilla M. Gopinathan J. B. Haislip R. Hudec G. Hurst K. M. Ivarsen M. Jelinek A. Joshi M. Kagitani N. Kaur W. C. Keel A. P. LaCluyze B. C. Lee E. Lindfors J. Lozano de Haro J. P. Moore M. Mugrauer R. Naves Nogues A. W. Neely R. H. Nelson W. Ogloza S. Okano J. C. Pandey M. Perri P. Pihajoki G. Poyner J. Provencal T. Pursimo A. Raj D. E. Reichart R. Reinthal S. Sadegi T. Sakanoi J. L. Salto Gonzalez T. Schweyer M. Siwak F. C. Soldan Alfaro E. Sonbas I. Steele J. T. Stocke J. Strobl L. O. Takalo T. Tomov L. Tremosa Espasa J. R. Valdes J. Valero Perez F. Verrecchia J. R. Webb M. Yoneda M. Zejmo W. Zheng J. Telting J. Saario T. Reynolds A. Kvammen E. Gafton R. Karjalainen J. Harmanen P. Blay

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classification 🌌 astro-ph.HE

keywords blackholeopticaloutburstaccuracydecembergeneralmajor

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OJ287 is a quasi-periodic quasar with roughly 12 year optical cycles. It displays prominent outbursts which are predictable in a binary black hole model. The model predicted a major optical outburst in December 2015. We found that the outburst did occur within the expected time range, peaking on 2015 December 5 at magnitude 12.9 in the optical R-band. Based on Swift/XRT satellite measurements and optical polarization data, we find that it included a major thermal component. Its timing provides an accurate estimate for the spin of the primary black hole, chi = 0.313 +- 0.01. The present outburst also confirms the established general relativistic properties of the system such as the loss of orbital energy to gravitational radiation at the 2 % accuracy level and it opens up the possibility of testing the black hole no-hair theorem with a 10 % accuracy during the present decade.

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Primary black hole spin in OJ287 as determined by the General Relativity centenary flare

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