activity
20162026
most citedOptical spectroscopy and demographics of redback millisecond pulsar binaries

117 citations · 592 across the 33 of their papers we have counts for

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40 papers · 1 filter

astro-ph.HE2026

Sharpening the Mass Measurement of PSR J1048+2339 via High-Cadence Photometry

Kwan-Lok Li, Ka-Yui Au, Lupin C. C. Lin +3

Neutron stars are among the densest objects in the universe, and the mass measurements are crucial to the understanding of their equation of state. Pulsars in tight binaries can be…

astro-ph.HE2025

Two Possible Optical--X-Ray Anti-Correlations of PSR J1023+0038

Ka-Yui Au, Kwan-Lok Li, Albert K. H. Kong +3

X-ray emission is generally believed to be one of the major heating sources for the optical modulation in redback pulsar binaries as we have seen similar phenomena in many low mass…

astro-ph.HE2025★ 3 cited

What determines the -ray luminosities of classical novae?

Peter Craig, Elias Aydi, Laura Chomiuk +25

Classical novae in the Milky Way have now been well-established as high-energy GeV -ray sources. In novae with main-sequence companions, this emission is believed to result from…

astro-ph.HE2024

Autoregressive Search of Gravitational Waves: Denoising

Sangin Kim, C. Y. Hui, Jianqi Yan +5

Because of the small strain amplitudes of gravitational-wave (GW) signals, unveiling them in the presence of detector/environmental noise is challenging. For visualizing the signal…

astro-ph.HE2023

Chandra Observation of NGC 1559: Eight Ultraluminous X-ray Sources Including a Compact Binary Candidate

Chen-Hsun Ma, Kwan-Lok Li, You-Hua Chu +1

Despite the 30-year history of ultra-luminous X-ray sources (ULXs) studies, issues like the majority of their physical natures (i.e., neutron stars, stellar-mass black holes, or in…

astro-ph.HE2023★ 3 cited

Influences of dynamical disruptions on the evolution of pulsars in globular clusters

Kwangmin Oh, C. Y. Hui, Jongsuk Hong +5

By comparing the physical properties of pulsars hosted by core-collapsed (CCed) and non-core-collapsed (Non-CCed) globular clusters (GCs), we find that pulsars in CCed GCs rotate s…