output
19992026
most citedA massive binary black-hole system in OJ287 and a test of general relativity

416 citations

Showing astro-ph.HEShow all

6 papers · 1 filter

astro-ph.HE2018★ 124 cited

Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using its General Relativity Centenary Flare: Improved Orbital Parameters

Lankeswar Dey, M. J. Valtonen, A. Gopakumar +5

Results from regular monitoring of relativistic compact binaries like PSR 1913+16 are consistent with the dominant (quadrupole) order emission of gravitational waves (GWs). We show…

astro-ph.HE2017★ 81 cited

Stochastic modeling of multiwavelength variability of the classical BL Lac object OJ 287 on timescales ranging from decades to hours

A. Goyal, L. Stawarz, S. Zola +109

We present the results of our power spectral density analysis for the BL Lac object OJ\,287, utilizing the {\it Fermi}-LAT survey at high-energy -rays, {\it Swift}-XRT in X-rays…

astro-ph.HE2017★ 12 cited

Rapid Optical Variations Correlated with X-rays in the 2015 Second Outburst of V404 Cygni (GS 2023338)

Mariko Kimura, Taichi Kato, Keisuke Isogai +24

We present optical multi-colour photometry of V404 Cyg during the outburst from December, 2015 to January, 2016 together with the simultaneous X-ray data. This outburst occurred le…

astro-ph.HE2016★ 86 cited

Repetitive Patterns in Rapid Optical Variations in the Nearby Black-hole Binary V404 Cygni

Mariko Kimura, Keisuke Isogai, Taichi Kato +65

How black holes accrete surrounding matter is a fundamental, yet unsolved question in astrophysics. It is generally believed that matter is absorbed into black holes via accretion…

astro-ph.HE2016★ 149 cited

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

M. J. Valtonen, S. Zola, S. Ciprini +87

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 majo…

astro-ph.HE2009★ 37 cited

Swift X-ray and UV monitoring of the Classical Nova V458 Vul (Nova Vul 2007)

J. -U. Ness, J. J. Drake, A. P. Beardmore +18

We describe the highly variable X-ray and UV emission of V458 Vul (Nova Vul 2007), observed by Swift between 1 and 422 days after outburst. Initially bright only in the UV, V458 Vu…