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20042022
most citedSW Sextantis stars: the dominant population of CVs with orbital periods between 3-4 hours

90 citations · 190 across the 29 of their papers we have counts for

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astro-ph.SR2022

Investigating the low-flux states in six Intermediate Polars

Ava E. Covington, Aarran W. Shaw, Koji Mukai +30

We present optical photometry of six intermediate polars that exhibit transitions to a low-flux state. For four of these systems, DW Cnc, V515 And, V1223 Sgr and RX J2133.7+5107, w…

astro-ph.SR2020

The Unusual Eruption of the Extragalactic Classical Nova M31N 2017-09a

Christopher Lloyd, Lewis M. Cook, Seiichiro Kiyota +10

M31N 2017-09a is a classical nova and was observed for some 160 days following its initial eruption, during which time it underwent a number of bright secondary outbursts. The ligh…

astro-ph.SR2020

International observational campaign of the 2014 eclipse of EE Cep

D. Pieńkowski, C. Gałan, T. Tomov +64

Context. EE Cep is one of few eclipsing binary systems with a dark, dusty disk around an invisible object similar to ε Aur. The system is characterized by grey and asymmetric eclip…

astro-ph.SR201916 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.SR201918 cited

Precise Measures of Orbital Period, Before and After Nova Eruption for QZ Aurigae

Bradley E. Schaefer, David Boyd, Geoffrey C. Clayton +7

For the ordinary classical nova QZ Aurigae (which erupted in 1964), we report 1317 magnitudes from 1912--2016, including four eclipses detected on archival photographic plates from…

astro-ph.SR2018

Photometry and spectrophotometry of the Herbig Ae star RR Tauri

David Boyd

Multicolour broadband photometry and flux calibrated low resolution spectroscopy between 2014 and 2018 are used to investigate the behaviour of the highly variable Herbig Ae star R…