The Astrophysical Journal Letters (Jan 2023)

Quasi-simultaneous Optical Flux and Polarization Variability of the Binary Super Massive Black Hole Blazar OJ 287 from 2015 to 2023: Detection of an Anticorrelation in Flux and Polarization Variability

  • Alok C. Gupta,
  • Pankaj Kushwaha,
  • Mauri J. Valtonen,
  • Sergey S. Savchenko,
  • Svetlana G. Jorstad,
  • Ryo Imazawa,
  • Paul J. Wiita,
  • Minfeng Gu,
  • Alan P. Marscher,
  • Zhongli Zhang,
  • Rumen Bachev,
  • G. A. Borman,
  • Haritma Gaur,
  • T. S. Grishina,
  • V. A. Hagen-Thorn,
  • E. N. Kopatskaya,
  • V. M. Larionov,
  • E. G. Larionova,
  • L. V. Larionova,
  • D. A. Morozova,
  • T. Nakaoka,
  • A. Strigachev,
  • Yulia V. Troitskaya,
  • I. S. Troitsky,
  • M. Uemura,
  • A. A. Vasilyev,
  • Z. R. Weaver,
  • A. V. Zhovtan

DOI
https://doi.org/10.3847/2041-8213/acfd2e
Journal volume & issue
Vol. 957, no. 1
p. L11

Abstract

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We study the optical flux and polarization variability of the binary black hole blazar OJ 287 using quasi-simultaneous observations from 2015 to 2023 carried out using telescopes in the USA, Japan, Russia, Crimea, and Bulgaria. This is one of the most extensive quasi-simultaneous optical flux and polarization variability studies of OJ 287. OJ 287 showed large amplitude, ∼3.0 mag flux variability, large changes of ∼37% in degree of polarization, and a large swing of ∼215° in the angle of the electric vector of polarization. During the period of observation, several flares in flux were detected. Those flares are correlated with a rapid increase in the degree of polarization and swings in electric vector of polarization angle. A peculiar behavior of anticorrelation between flux and polarization degree, accompanied by a nearly constant polarization angle, was detected from JD 2,458,156 to JD 2,458,292. We briefly discuss some explanations for the flux and polarization variations observed in OJ 287.

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