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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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astro-ph.HE2022★ 39 cited

The TRAPUM L-band survey for pulsars in Fermi-LAT gamma-ray sources

C. J. Clark, R. P. Breton, E. D. Barr +35

More than 100 millisecond pulsars (MSPs) have been discovered in radio observations of gamma-ray sources detected by the Fermi Large Area Telescope (LAT), but hundreds of pulsar-li…

astro-ph.GA2022

First detection of the outer edge of an AGN accretion disc: Very fast multiband optical variability of NGC 4395 with GTC/HiPERCAM and LT/IO:O

I. M. McHardy, M. Beard, E. Breedt +11

We present fast (~200s sampling) ugriz photometry of the low mass AGN NGC 4395 with the Liverpool Telescope, followed by very fast (3s sampling) us, gs, rs, is and zs simultaneous…

astro-ph.SR2022★ 4 cited

Limiting the accretion disk light in two mass transferring hot subdwarf binaries

Kunal Deshmukh, Thomas Kupfer, Pasi Hakala +6

We report the results from follow-up observations of two Roche-lobe filling hot subdwarf binaries with white dwarf companions predicted to have accretion disks. ZTF J213056.71+4420…

astro-ph.SR2022★ 24 cited

Two decades of optical timing of the shortest-period binary star system HM Cancri

James Munday, T. R. Marsh, Mark Hollands +15

The shortest-period binary star system known to date, RX J0806.3+1527 (HM Cancri), has now been observed in the optical for more than two decades. Although it is thought to be a do…

astro-ph.SR2022★ 54 cited

white dwarfs within 40 pc III: spectroscopic observations of new candidates in the southern hemisphere

Mairi W. O'Brien, P. -E. Tremblay, N. P. Gentile Fusillo +31

We present a spectroscopic survey of 248 white dwarf candidates within 40 pc of the Sun; of these 244 are in the southern hemisphere. Observations were performed mostly with the Ve…

astro-ph.SR2022★ 19 cited

A dense star in a 51-minute orbital period eclipsing binary

Kevin B. Burdge, Kareem El-Badry, Thomas R. Marsh +24

In over a thousand known cataclysmic variables (CVs), where a white dwarf is accreting from a hydrogen-rich star, only a dozen have orbital periods below 75 minutes. One way to ach…

astro-ph.SR2022★ 6 cited

The C/N ratio from FUV spectroscopy as a constraint upon the past evolution of HS0218+3229

O. Toloza, Boris T. Gaensicke, Laura M. Guzman-Rincon +8

Some white dwarfs accreting from non-degenerate companions show anomalous carbon and nitrogen abundances in the photospheres of their stellar components which have been postulated…

astro-ph.SR2022★ 10 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.SR2022★ 17 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…

astro-ph.SR2022★ 5 cited

Two substellar survivor candidates; one found and one missing

N. Walters, J. Farihi, T. R. Marsh +4

This study presents observations of two possible substellar survivors of post-main sequence engulfment, currently orbiting white dwarf stars. Infrared and optical spectroscopy of G…

astro-ph.SR2022★ 12 cited

Circular Polarimetry of Suspect Wind-accreting Magnetic pre-Polars

Pasi Hakala, Steven G. Parsons, Thomas R. Marsh +4

We present results from a circular polarimetric survey of candidate detached magnetic white dwarf - M dwarf binaries obtained using the Nordic Optical Telescope, La Palma. We obtai…

astro-ph.HE2022★ 2 cited

A tentative 114-minute orbital period challenges the ultra-compact nature of the X-ray binary 4U 1812-12

M. Armas Padilla, P. Rodríguez-Gil, T. Muñoz-Darias +7

We present a detailed time-resolved photometric study of the ultra-compact X-ray binary candidate 4U 1812-12. The multicolor light curves obtained with HiPERCAM on the 10.4-m Gran…

astro-ph.HE2022★ 24 cited

A 62-minute orbital period black widow binary in a wide hierarchical triple

Kevin B. Burdge, Thomas R. Marsh, Jim Fuller +30

Over a dozen millisecond pulsars are ablating low-mass companions in close binary systems. In the original "black widow", the 8-hour orbital period eclipsing pulsar PSR J1959+2048…

astro-ph.HE2022★ 2 cited

X-ray observation of the Roche-lobe filling white dwarf plus hot subdwarf system ZTF J213056.71+442046.5

S. Mereghetti, N. La Palombara, T. Kupfer +9

ZTF J213056.71+442046.5 is the prototype of a small class of recently discovered compact binaries composed of a white dwarf and a hot subdwarf that fills its Roche-lobe. Its orbita…

astro-ph.SR2022★ 21 cited

Characterising eclipsing white dwarf M dwarf binaries from multi-band eclipse photometry

Alex J. Brown, Steven G. Parsons, Stuart P. Littlefair +10

With the prevalence of wide-field, time-domain photometric sky surveys, the number of eclipsing white dwarf systems being discovered is increasing dramatically. An efficient method…

astro-ph.HE2022★ 31 cited

Measuring the mass of the black widow PSR J1555-2908

M. R. Kennedy, R. P. Breton, C. J. Clark +8

Accurate measurements of the masses of neutron stars are necessary to test binary evolution models, and to constrain the neutron star equation of state. In pulsar binaries with no…