A
Albert K. H. Kong
Researcher at National Tsing Hua University
Publications - 109
Citations - 2466
Albert K. H. Kong is an academic researcher from National Tsing Hua University. The author has contributed to research in topics: Pulsar & Luminosity. The author has an hindex of 30, co-authored 109 publications receiving 2122 citations. Previous affiliations of Albert K. H. Kong include University of Oxford & Massachusetts Institute of Technology.
Papers
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Revealing a new black widow binary 4FGL J0336.0+7502
TL;DR: In this paper, a promising candidate as a black widow millisecond pulsar binary, 4FGL J0336.0+7502, was identified within the 95% error region of the LAT source, and an optical counterpart with a clear periodicity at P(orb) = 3.718178(9) hours using the Bohyunsan 1.8m Telescope, Lulin One-meter Telescope, Canada-France-Hawaii Telescope, and Gemini-North.
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NuSTAR and Swift observations of Swift J1357.2-0933 during an early phase of its 2017 outburst
TL;DR: In this paper, the authors present a detailed spectral analysis of the very faint X-ray transient and black hole system, Swift J1357.2-0933, during an early, low-hard state of its 2017 outburst.
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Discovery of a Redback Millisecond Pulsar Candidate: 3FGL J0212.1+5320
Kwan-Lok Li,Albert K. H. Kong,Xian Hou,Xian Hou,Jirong Mao,Jay Strader,Laura Chomiuk,Evangelia Tremou +7 more
TL;DR: In this paper, Chandra detects a bright X-ray source (i.e., F(0.5-7keV) = 1.4e-12 erg/cm^2/s), which has a low-mass optical counterpart (M 64% of the Roche-lobe).
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Bayesian analysis on the X-ray spectra of the binary neutron star merger GW170817
TL;DR: In this article, a Bayesian time-resolved spectral analysis of the X-ray afterglow datasets of GW170817/GRB17017A was presented.
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X-ray spectral evolution of PSR J2032+4127 during the 2017 periastron passage
Partha Sarathi Pal,Pak-Hin Thomas Tam,Y. D. Cui,Kwan-Lok Li,Albert K. H. Kong,Albert K. H. Kong,Can Güngör +6 more
TL;DR: In this paper, Chandra, XMM-Newton, Nuclear Spectroscopic Telescope Array Mission (NuSTAR), and Swift observations of PSR J2032+4127 taken before, during, and after the periastron on 2017 November 13.