activity
20022020
most citedSuperhumps in Cataclysmic Binaries. XXV. q_crit, epsilon(q), and Mass-Radius

239 citations · 2k across the 68 of their papers we have counts for

collaborators

68 papers

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.SR2019★ 16 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. X: The Tenth Year (2017)

Taichi Kato, Keisuke Isogai, Yasuyuki Wakamatsu +67

Continuing the project described by Kato et al. (2009, PASJ, 61, S395, arXiv/0905.1757), we collected times of superhump maxima for 102 SU UMa-type dwarf novae observed mainly duri…

astro-ph.SR2018★ 11 cited

Orbital Period Increase in ES Ceti

Enrique de Miguel, Joseph Patterson, Jonathan Kemp +5

We report a long-term study of the eclipse times in the 10-minute helium binary ES Ceti. The binary period increases rapidly, with P/P-dot = 6.2x10^6 yr. This is consistent with th…

astro-ph.SR2017★ 8 cited

Orbital Period Changes in WZ Sagittae

Joseph Patterson, Geoffrey Stone, Jonathan Kemp +19

We report a long-term (1961-2017) study of the eclipse times in the dwarf nova WZ Sagittae, in an effort to learn its rate of orbital-period change. Some wiggles with a time scale…

astro-ph.SR2017★ 34 cited

Survey of Period Variations of Superhumps in SU UMa-Type Dwarf Novae. IX: The Ninth Year (2016-2017)

Taichi Kato, Keisuke Isogai, Franz-Josef Hambsch +76

Continuing the project described by Kato et al. (2009, arXiv:0905.1757), we collected times of superhump maxima for 127 SU UMa-type dwarf novae observed mainly during the 2016--201…

astro-ph.SR2016★ 14 cited

A 16-Year Photometric Campaign on the Eclipsing Novalike Variable DW Ursae Majoris

D. R. S. Boyd, E. de Miguel, J. Patterson +29

We present an analysis of photometric observations of the eclipsing novalike variable DW UMa made by the CBA consortium between 1999 and 2015. Analysis of 372 new and 260 previousl…