activity
20162023
most citedUsing Gaussian processes to model light curves in the presence of flickering: the eclipsing cataclysmic variable ASASSN-14ag

22 citations · 98 across the 8 of their papers we have counts for

collaborators

8 papers

astro-ph.SR2023

TIC 378898110: A Bright, Short-Period AM CVn Binary in TESS

Matthew J. Green, J. J. Hermes, Brad N. Barlow +22

AM CVn-type systems are ultracompact, helium-accreting binary systems which are evolutionarily linked to the progenitors of thermonuclear supernovae and are expected to be strong G…

astro-ph.SR202317 cited

A rotating white dwarf shows different compositions on its opposite faces

Ilaria Caiazzo, Kevin B. Burdge, Pier-Emmanuel Tremblay +35

White dwarfs, the extremely dense remnants left behind by most stars after their death, are characterised by a mass comparable to that of the Sun compressed into the size of an Ear…

astro-ph.SR202310 cited

An Eclipsing 47 minute Double White Dwarf Binary at 400 pc

James Munday, P. -E. Tremblay, J. J. Hermes +20

We present the discovery of the eclipsing double white dwarf (WD) binary WDJ 022558.21-692025.38 that has an orbital period of 47.19 min. Following identification with the Transiti…

astro-ph.SR202322 cited

Photometric follow-up of 43 new eclipsing white dwarf plus main-sequence binaries from the ZTF survey

Alex J. Brown, Steven G. Parsons, Jan van Roestel +12

Wide-field time-domain photometric sky surveys are now finding hundreds of eclipsing white dwarf plus M dwarf binaries, a population encompassing a wealth of information and potent…

astro-ph.SR202210 cited

Multi-colour optical light curves of the companion star to the millisecond pulsar PSR J2051-0827

V. S. Dhillon, M. R. Kennedy, R. P. Breton +16

We present simultaneous, multi-colour optical light curves of the companion star to the black-widow pulsar PSR J2051-0827, obtained approximately 10 years apart using ULTRACAM and…

astro-ph.SR202217 cited

Long-term photometric monitoring and spectroscopy of the white dwarf pulsar AR Scorpii

Ingrid Pelisoli, T. R. Marsh, S. G. Parsons +14

AR Scorpii (AR Sco) is the only radio-pulsing white dwarf known to date. It shows a broad-band spectrum extending from radio to X-rays whose luminosity cannot be explained by therm…