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19952023
most citedA Massive Pulsar in a Compact Relativistic Binary

3.9k citations · 18.7k across the 302 of their papers we have counts for

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Showing 2021Show all

18 papers · 1 filter

astro-ph.SR2021★ 119 cited

Constraining the Evolution of Cataclysmic Variables via the Masses and Accretion Rates of their Underlying White Dwarfs

A. F. Pala, B. T. Gänsicke, D. Belloni +28

We report on the masses (), effective temperatures () and secular mean accretion rates () of 43 cataclysmic variable (CV) wh…

astro-ph.SR2021★ 2 cited

Three dimensional Doppler tomography

T. R. Marsh

Doppler tomography is a method to compute the emissivity distribution within the co-rotating frames of binary stars from observations of their emission line profiles at multiple or…

astro-ph.EP2021★ 11 cited

Velocity-imaging the rapidly precessing planetary disc around the white dwarf HE 1349-2305 using Doppler tomography

Christopher J. Manser, Erik Dennihy, Boris T. Gänsicke +11

The presence of planetary material in white dwarf atmospheres, thought to be accreted from a dusty debris disc produced via the tidal disruption of a planetesimal, is common. Appro…

astro-ph.SR2021★ 1 cited

The SNIa Runaway LP 398-9: Detection of Circumstellar Material and Surface Rotation

Vedant Chandra, Hsiang-Chih Hwang, Nadia L. Zakamska +12

A promising progenitor scenario for Type Ia supernovae (SNeIa) is the thermonuclear detonation of a white dwarf in a close binary system with another white dwarf. After the primary…

astro-ph.EP2021★ 48 cited

Relentless and Complex Transits from a Planetesimal Debris Disk

J. Farihi, J. J. Hermes, T. R. Marsh +11

This article reports quasi-continuous transiting events towards WD 1054-226 at d=36.2 pc and V=16.0 mag, based on simultaneous, high-cadence, multi-wavelength imaging photometry us…

astro-ph.SR2021★ 9 cited

Optical detection of the rapidly spinning white dwarf in V1460 Her

Ingrid Pelisoli, T. R. Marsh, R. P. Ashley +15

Accreting magnetic white dwarfs offer an opportunity to understand the interplay between spin-up and spin-down torques in binary systems. Monitoring of the white dwarf spin may rev…

astro-ph.SR2021★ 48 cited

Discovery and characterization of five new eclipsing AM CVn systems

J. van Roestel, T. Kupfer, M. J. Green +19

AM CVn systems are ultra-compact, helium-rich, accreting binaries with degenerate or semi-degenerate donors. We report the discovery of five new eclipsing AM CVn systems with orbit…

astro-ph.SR2021★ 40 cited

Found: a rapidly spinning white dwarf in LAMOST J024048.51+195226.9

Ingrid Pelisoli, T. R. Marsh, V. S. Dhillon +9

We present optical photometry of the cataclysmic variable LAMOST J024048.51+195226.9 taken with the high-speed, five-band CCD camera HiPERCAM on the 10.4 m Gran Telescopio Canarias…

astro-ph.IM2021★ 98 cited

HiPERCAM: a quintuple-beam, high-speed optical imager on the 10.4-m Gran Telescopio Canarias

V. S. Dhillon, N. Bezawada, M. Black +36

HiPERCAM is a portable, quintuple-beam optical imager that saw first light on the 10.4-m Gran Telescopio Canarias (GTC) in 2018. The instrument uses re-imaging optics and 4 dichroi…

astro-ph.HE2021★ 18 cited

Optical photometry of two transitional millisecond pulsars in the radio pulsar state

James G. Stringer, Rene P. Breton, Colin J. Clark +7

We present ULTRACAM multiband optical photometry of two transitional millisecond pulsars, PSR J1023+0038 and PSR J12274853, taken while both were in their radio pulsar states. T…

astro-ph.SR2021★ 11 cited

System parameters of three short period cataclysmic variable stars

J. F. Wild, S. P. Littlefair, R. P. Ashley +9

Using photometric ULTRACAM observations of three new short period cataclysmic variables, we model the primary eclipse lightcurves to extract the orbital separation, masses, and rad…

astro-ph.HE2021★ 23 cited

The Evolution of Rapid Optical/X-ray Timing Correlations in the Initial Hard State of MAXI J1820+070

J. A. Paice, P. Gandhi, T. Shahbaz +11

We report on a multi-epoch campaign of rapid optical/X-ray timing observations of the superbright 2018 outburst of MAXI J1820+070, a black hole low-mass X-ray binary system. The ob…

astro-ph.IM2021★ 3 cited

Processing GOTO data with the Rubin Observatory LSST Science Pipelines II: Forced Photometry and light curves

L. Makrygianni, J. Mullaney, V. Dhillon +45

We have adapted the Vera C. Rubin Observatory Legacy Survey of Space and Time (LSST) Science Pipelines to process data from the Gravitational-Wave Optical Transient Observer (GOTO)…

astro-ph.HE2021★ 69 cited

Measuring fundamental jet properties with multi-wavelength fast timing of the black hole X-ray binary MAXI J1820+070

A. J. Tetarenko, P. Casella, J. C. A. Miller-Jones +9

We present multi-wavelength fast timing observations of the black hole X-ray binary MAXI J1820+070 (ASASSN-18ey), taken with the Karl G. Jansky Very Large Array (VLA), Atacama Larg…

astro-ph.SR2021★ 19 cited

A test of the planet-star unipolar inductor for magnetic white dwarfs

N. Walters, J. Farihi, T. R. Marsh +7

Despite thousands of spectroscopic detections, only four isolated white dwarfs exhibit Balmer emission lines. The temperature inversion mechanism is a puzzle over 30 years old that…

astro-ph.EP2021★ 1 cited

TransitFit: combined multi-instrument exoplanet transit fitting for JWST, HST and ground-based transmission spectroscopy studies

J. J. C. Hayes, A. Priyadarshi, E. Kerins +19

We present TransitFit, a package designed to fit exoplanetary transit light-curves. TransitFit offers multi-epoch, multi-wavelength fitting of multi-telescope transit data. Transit…

astro-ph.SR2021★ 38 cited

Towards a volumetric census of close white dwarf binaries I.Reference samples

K. Inight, B. T. Gaensicke, E. Breedt +3

Close white dwarf binaries play an important role across a range of astrophysics, including thermonuclear supernovae, the Galactic low-frequency gravitational wave signal, and the…

astro-ph.SR2021★ 37 cited

Magnetic white dwarfs in post-common-envelope binaries

S. G. Parsons, B. T. Gänsicke, M. R. Schreiber +5

Magnitude-limited samples have shown that 20-25 per cent of cataclysmic variables contain white dwarfs with magnetic fields of Mega Gauss strength, in stark contrast to the approxi…