activity
20162021
most citedRoboPol: AGN polarimetric monitoring data

58 citations · 135 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.EP202116 cited

Properties of slowly rotating asteroids from the Convex Inversion Thermophysical Model

A. Marciniak, J. Ďurech, V. Alí-Lagoa +73

Results from the TESS mission showed that previous studies strngly underestimated the number of slow rotators, revealing the importance of studying those asteroids. For most slowly…

astro-ph.HE202058 cited

RoboPol: AGN polarimetric monitoring data

D. Blinov, S. Kiehlmann, V. Pavlidou +29

We present uniformly reprocessed and re-calibrated data from the RoboPol programme of optopolarimetric monitoring of active galactic nuclei (AGN), covering observations between 201…

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…

astro-ph.EP201929 cited

Thermal properties of slowly rotating asteroids: Results from a targeted survey

A. Marciniak, V. Alí-Lagoa, T. G. Müller +51

Context. Earlier work suggests that slowly rotating asteroids should have higher thermal inertias than faster rotators because the heat wave penetrates deeper into the sub-surface.…

astro-ph.HE2018

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.EP201732 cited

Photometric survey, modelling, and scaling of long-period and low-amplitude asteroids

A. Marciniak, P. Bartczak, T. Müller +40

The available set of spin and shape modelled asteroids is strongly biased against slowly rotating targets and those with low lightcurve amplitudes. As a consequence of these select…