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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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iPTF16fnl: A Faint and Fast Tidal Disruption Event in an E+A Galaxy

TL;DR: In this article, ground-based and Swift observations of iPTF16fnl, a likely tidal disruption event (TDE) discovered by the intermediate Palomar Transient Factory (iPTF) survey at 666 Mpc, were presented.
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GROWTH on S190425z: Searching Thousands of Square Degrees to Identify an Optical or Infrared Counterpart to a Binary Neutron Star Merger with the Zwicky Transient Facility and Palomar Gattini-IR

Michael W. Coughlin, +84 more
TL;DR: In this article, the authors performed a dedicated follow-up campaign with the Zwicky Transient Facility (ZTF) and Palomar Gattini-IR telescopes.
Journal ArticleDOI

iPTF16fnl: a faint and fast tidal disruption event in an E+A galaxy

TL;DR: In this paper, ground-based and Swift observations of iPTF16fnl, a likely tidal disruption event (TDE) discovered by the intermediate Palomar Transient Factory (iPTF) survey at 66.6 Mpc, were presented.
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A tidal disruption event coincident with a high-energy neutrino.

Robert Stein, +64 more
TL;DR: In this paper, the authors presented the likely association of a radio-emitting tidal disruption event, AT2019dsg, with a second high-energy neutrino, which was identified as part of a systematic search for optical counterparts to high-energetic neutrinos with the Zwicky Transient Facility.
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GROWTH on S190814bv: Deep Synoptic Limits on the Optical/Near-infrared Counterpart to a Neutron Star–Black Hole Merger

Igor Andreoni, +59 more
TL;DR: In this paper, the authors used a photometric redshift catalog and radiative transfer simulations of NSBH mergers to constrain the ejecta mass of S190814bv to be $M_\mathrm{ej} < 0.04$~$M_{\odot}$ at polar viewing angles, or if the opacity is $\kappa < 2$~cm$^2$g$^{-1}$.