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R. H. Nelson

Researcher at Herzberg Institute of Astrophysics

Publications -  26
Citations -  409

R. H. Nelson is an academic researcher from Herzberg Institute of Astrophysics. The author has contributed to research in topics: Light curve & Radial velocity. The author has an hindex of 7, co-authored 26 publications receiving 344 citations.

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Primary Black Hole Spin in OJ 287 as Determined by the General Relativity Centenary Flare

Mauri Valtonen, +98 more
TL;DR: In this paper, a quasi-periodic quasar with roughly 12-year optical cycles displays prominent outbursts that are predictable in a binary black hole model, and the model predicted a major optical outburst in 2015 December.
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Primary black hole spin in OJ287 as determined by the General Relativity centenary flare

TL;DR: In this article, the authors found that the outburst did occur within the expected time range, peaking on 2015 December 5 at magnitude 12.9 in the optical R-band, based on Swift/XRT satellite measurements and optical polarization data.
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Authenticating the presence of a relativistic massive black hole binary in OJ 287 using its general relativity centenary flare: improved orbital parameters

Lankeswar Dey, +113 more
TL;DR: In this article, it was shown that even the effects of certain hereditary contributions to GW emission are required to predict impact flare timings of OJ 287, and they developed an approach that incorporated this effect into the BBH model for OJ287.
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DN Bootis: A low mass-ratio W UMa-type contact binary

TL;DR: In this article, photoelectric BVR light curves and radial velocity curves were obtained for the HIPPARCOS discovery DN Boo at the TUG 1 National Observatory of Turkey (TUG) and Dominion Astrophysical Observatory (DAO), respectively, to determine physical nature of the variable.
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A Search for QPOs in the Blazar OJ287: Preliminary Results from the 2015/2016 Observing Campaign

Stanisław Zoła, +97 more
TL;DR: In this paper, the authors analyse the light curve in the R band of the blazar OJ287, gathered during the 2015/2016 observing season, and search for quasi-periodic oscillations (QPOs) using several methods over a wide range of timescales.