most citedSpitzer Observations of the Predicted Eddington Flare from Blazar OJ 287

70 citations · 119 across the 3 of their papers we have counts for

collaborators

9 papers

astro-ph.HE202143 cited

Explaining temporal variations in the jet position angle of the blazar OJ 287 using its binary black hole central engine model

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

The bright blazar OJ 287 is the best-known candidate for hosting a supermassive black hole binary system. It inspirals due to the emission of nanohertz gravitational waves (GWs). O…

astro-ph.HE202070 cited

Spitzer Observations of the Predicted Eddington Flare from Blazar OJ 287

Seppo Laine, Lankeswar Dey, Mauri Valtonen +25

Binary black hole (BH) central engine description for the unique blazar OJ 287 predicted that the next secondary BH impact-induced bremsstrahlung flare should peak on 2019 July 31.…

astro-ph.IM202049 cited

MSTAR -- a fast parallelised algorithmically regularised integrator with minimum spanning tree coordinates

Antti Rantala, Pauli Pihajoki, Matias Mannerkoski +2

We present the novel algorithmically regularised integration method MSTAR for high accuracy () integrations of N-body systems using minimum spanning tree c…

astro-ph.GA2019

Gravitational Waves from the Inspiral of Supermassive Black Holes in Galactic-scale Simulations

Matias Mannerkoski, Peter H. Johansson, Pauli Pihajoki +2

We study the orbital evolution and gravitational wave (GW) emission of supermassive black hole (SMBH) binaries formed in gas-free mergers of massive early-type galaxies using the h…

astro-ph.IM2019

Barycentric interpolation on Riemannian and semi-Riemannian spaces

Pauli Pihajoki, Matias Mannerkoski, Peter H. Johansson

Interpolation of data represented in curvilinear coordinates and possibly having some non-trivial, typically Riemannian or semi-Riemannian geometry is an ubiquitous task in all of…

astro-ph.HE2019

Accretion Disk Parameters determined from the great 2015 flare of OJ 287

Mauri J. Valtonen, Staszek Zola, Pauli Pihajoki +17

In the binary black hole model of OJ 287 the secondary black hole orbits a much more massive primary, and impacts on the primary accretion disk at predictable times. We update the…