142 citations · 1.1k across the 29 of their papers we have counts for
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Polarimetric evidence of a white dwarf pulsar in the binary system AR Scorpii
D. A. H. Buckley, P. J. Meintjes, S. B. Potter +2
The variable star AR Sco was recently discovered to pulse in brightness every 1.97 min from ultraviolet wavelengths into the radio regime. The system is composed of a cool, low-mas…
PTF1 J082340.04+081936.5: A hot subdwarf B star with a low mass white dwarf companion in an 87 minute orbit
Thomas Kupfer, Jan van Roestel, Jared Brooks +19
We present the discovery of the hot subdwarf B star (sdB) binary PTF1 J082340.04+081936.5. The system has an orbital period P min (0.060761584(10) days), ma…
The OmegaWhite Survey for short period variable stars II: An overview of results from the first four years
Ruxandra Toma, Gavin Ramsay, Sally MacFarlane +7
OmegaWhite is a wide-field, high cadence, synoptic survey targeting fields in the southern Galactic plane, with the aim of discovering short period variable stars. Our strategy is…