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19982025
most citedMASTER optical detection of the first LIGO/Virgo neutron stars merging GW170817

261 citations · 2.2k across the 68 of their papers we have counts for

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68 papers

astro-ph.SR2025

Phase-resolved spectroscopic observations of the magnetic cataclysmic binary EF Eridani: Revealing complex magnetic accretion during a high state

Zwidofhela N. Khangale, Stephen B. Potter, David A. H. Buckley +1

We present high-resolution, phase-resolved spectroscopic observations of the polar EF Eri, obtained with SALT and the SAAO 1.9-m telescope during its recent emergence from a three-…

astro-ph.SR2025

A targeted search for binary white dwarf pulsars using Gaia and WISE

Ingrid Pelisoli, T. R. Marsh, G. Tovmassian +24

After its discovery in 2016, the white dwarf binary AR Scorpii (AR Sco) remained for several years the only white dwarf system to show pulsed radio emission associated with a fast-…

astro-ph.SR2025

A Link Between White Dwarf Pulsars and Polars: Multiwavelength Observations of the 9.36-Minute Period Variable Gaia22ayj

Antonio C. Rodriguez, Kareem El-Badry, Pasi Hakala +30

White dwarfs (WDs) are the most abundant compact objects, and recent surveys have suggested that over a third of WDs in accreting binaries host a strong (B 1 MG) magnetic…

astro-ph.HE2024

CSS161010: a luminous, fast blue optical transient with broad blueshifted hydrogen lines

Claudia P. Gutiérrez, Seppo Mattila, Peter Lundqvist +38

We present ultraviolet, optical and near-infrared photometric and optical spectroscopic observations of the luminous, fast blue optical transient (LFBOT), CSS161010:045834-081803 (…

astro-ph.SR2023★ 14 cited

Unveiling the white dwarf in J191213.72-441045.1 through ultraviolet observations

Ingrid Pelisoli, Snehalata Sahu, Maxim Lyutikov +7

J191213.72-441045.1 is a binary system composed of a white dwarf and an M-dwarf in a 4.03-hour orbit. It shows emission in radio, optical, and X-ray, all modulated at the white dwa…

astro-ph.SR2023

Rapid Evolution of the White Dwarf Pulsar AR Scorpii

Peter Garnavich, Stephen B. Potter, David A. H. Buckley +4

Analysis of AR Sco optical light curves spanning nine years show a secular change in the relative amplitudes of the beat pulse pairs generated by the two magnetic poles of its rota…