activity
20092026
most citedVariability and stability in blazar jets on time scales of years: Optical polarization monitoring of OJ287 in 2005-2009

113 citations · 378 across the 10 of their papers we have counts for

collaborators

11 papers

astro-ph.HE2026

Multi-band optical photometric variability of the blazar OJ 287 from 2015 to 2025

Alok C. Gupta, Karan Dogra, Mark Kidger +101

We present the most densely sampled multi-band optical photometric observations of the peculiar BL Lacertae object OJ 287 from 2015 to 2025 with a focus on its optical activity on…

astro-ph.GA2023

Revisiting Blueshift Interpretation In Light Of Recent Discovery Of Multiple Systems Of Quasars

Justin Singh, Shirin Haque

This study investigates the anomalies associated with redshifts from emission lines in certain quasar candidates and the viability of a blueshift interpretation instead. The sample…

astro-ph.GA2020★ 4 cited

Relativistic Effects on Triple Black Holes: Burrau's Problem Revisited

Ariel Chitan, Aleksandr Mylläri, Shirin Haque

We explore, using numerical simulations, the influence of mass and distance on the evolution of triple black hole systems. Following in the direction of Burrau's famous 3,4,5 probl…

astro-ph.HE2020★ 70 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.SR2019★ 2 cited

A Fractal Analysis of Magnetograms within Active Regions

Brandon Rajkumar, Shirin Haque

The magnetograms of sixteen Active Regions, observed during June - November 2015, were obtained from the Joint Science Operations Center and used to determine the fractal dimension…

astro-ph.HE2018

High accuracy measurement of gravitational wave back-reaction in the OJ287 black hole binary

Mauri J. Valtonen, L. Dey, R. Hudec +16

Blazar OJ287 exhibits large thermal flares at least twice every 12 years. The times of these flares have been predicted successfully using the model of a quasi-Keplerian eccentric…