activity
20162024
most citedA new gamma-ray loud, eclipsing low-mass X-ray binary

48 citations · 170 across the 12 of their papers we have counts for

collaborators

12 papers

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.HE20233 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…

astro-ph.SR2023

Evidence of stellar oscillations in the post-common envelop binary candidate ASASSN-V J205543.90+240033.5

J. Takata, A. K. H. Kong, X. F. Wang +7

ASASSN-V J205543.90+240033.5 (ASJ2055) is a possible post-common envelope binary system. Its optical photometric data shows an orbital variation about ~days and a fast period…

astro-ph.HE202311 cited

A comparison of millisecond pulsar populations between globular clusters and the Galactic field

Jongsu Lee, C. Y. Hui, J. Takata +4

We have performed a systematic study of the rotational, orbital and X-ray properties of millisecond pulsars (MSPs) in globular clusters (GCs) and compared their nature with those o…

astro-ph.SR20228 cited

Searching for cataclysmic variable stars in unidentified X-ray sources

J. Takata, X. F. Wang, A. K. H. Kong +6

We carry out a photometric search for new cataclysmic variable stars (CVs), with the goal of identification for candidates of AR~Scorpii-type binary systems. We select GAIA sources…