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20122020
most citedThe planets around NN Ser: still there

121 citations · 1.1k across the 29 of their papers we have counts for

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astro-ph.SR2020★ 31 cited

Spectroscopic and Photometric Periods of Six Ultracompact Accreting Binaries

Matthew J. Green, Thomas R. Marsh, Philip J. Carter +19

Ultracompact accreting binary systems each consist of a stellar remnant accreting helium-enriched material from a compact donor star. Such binaries include two related sub-classes,…

astro-ph.SR2017★ 118 cited

Testing the white dwarf mass-radius relationship with eclipsing binaries

S. G. Parsons, B. T. Gänsicke, T. R. Marsh +17

We present high precision, model independent, mass and radius measurements for 16 white dwarfs in detached eclipsing binaries and combine these with previously published data to te…

astro-ph.SR2017★ 33 cited

Using large spectroscopic surveys to test the double degenerate model for Type Ia supernovae

E. Breedt, D. Steeghs, T. R. Marsh +10

An observational constraint on the contribution of double degenerates to Type Ia supernovae requires multiple radial velocity measurements of ideally thousands of white dwarfs. Thi…

astro-ph.SR2017★ 28 cited

SDSS J105754.25+275947.5: a period-bounce eclipsing cataclysmic variable with the lowest-mass donor yet measured

M. J. McAllister, S. P. Littlefair, V. S. Dhillon +11

We present high-speed, multicolour photometry of the faint, eclipsing cataclysmic variable (CV) SDSS J105754.25+275947.5. The light from this system is dominated by the white dwarf…

astro-ph.SR2016★ 36 cited

Hunting For Eclipses: High Speed Observations of Cataclysmic Variables

Liam K Hardy, Martin J McAllister, Vik S Dhillon +12

We present new time-resolved photometry of 74 cataclysmic variables (CVs), 47 of which are eclipsing. 13 of these eclipsing systems are newly discovered. For all 47 eclipsing syste…

astro-ph.SR2016★ 22 cited

Using Gaussian processes to model light curves in the presence of flickering: the eclipsing cataclysmic variable ASASSN-14ag

M. J. McAllister, S. P. Littlefair, V. S. Dhillon +10

The majority of cataclysmic variable (CV) stars contain a stochastic noise component in their light curves, commonly referred to as flickering. This can significantly affect the mo…