activity
20122026
most citedBK Lyncis: The Oldest Old Nova?... And a Bellwether for Cataclysmic-Variable Evolution

79 citations · 190 across the 9 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

Spectroscopic Analysis of the 2025 Eclipse of the Symbiotic Binary V1413 Aquilae

David Boyd, James Foster, Forrest Sims +12

We report on a coordinated campaign by amateur astronomers using a combination of high and low resolution spectroscopy to observe the 2025 eclipse of the symbiotic binary V1413 Aql…

astro-ph.SR2025

Photometry and Spectroscopy of the Symbiotic Binary V1413 Aquilae during the 2024 Eclipse

David Boyd, David Cejudo, James Foster +2

We report our photometric and spectroscopic observations and analysis of the 2024 eclipse of the symbiotic binary V1413 Aquilae. We found the system in a visually bright state and…

astro-ph.HE2022★ 17 cited

GRANDMA Observations of ZTF/Fink Transients during Summer 2021

V. Aivazyan, M. Almualla, S. Antier +80

We present our follow-up observations with GRANDMA of transient sources revealed by the Zwicky Transient Facility (ZTF). Over a period of six months, all ZTF triggers were examined…

astro-ph.SR2020

IM Normae: The Death Spiral of a Cataclysmic Variable?

Joseph Patterson, Jonathan Kemp, Berto Monard +18

We present a study of the orbital light curves of the recurrent nova IM Normae since its 2002 outburst. The broad "eclipses" recur with a 2.46 hour period, which increases on a tim…

astro-ph.SR2020★ 26 cited

The Spin-Period History of Intermediate Polars

Joseph Patterson, Enrique de Miguel, Jonathan Kemp +25

We report the detailed history of spin-period changes in five intermediate polars (DQ Herculis, AO Piscium, FO Aquarii, V1223 Sagittarii, and BG Canis Minoris) during the 30-60 yea…

astro-ph.SR2017★ 30 cited

IGR J19552+0044: A new asynchronous short period polar: "Filling the gap between intermediate and ordinary polars"

G. Tovmassian, D. Gonzalez-Buitrago, J. Thorstensen +23

Based on XMM--Newton X-ray observations IGR J19552+0044 appears to be either a pre-polar or an asynchronous polar. We conducted follow-up optical observations to identify the sourc…