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researcher

W. Fong

114 papers hereh-index 5811k citations219 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author14
  • middle author71
  • last author6

Across the 91 of 114 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE89
  • astro-ph.GA10
  • astro-ph.IM6
  • astro-ph.CO5
  • astro-ph2
  • astro-ph.SR2
same name
  • W. Fong — 37 papers, h 15
  • W. Fong — 17 papers, h 6
  • W. Fong — 10 papers, h 9
  • W. Fong — 9 papers, h 4
  • W. Fong — 2 papers, h 2
  • W. Fong — 2 papers, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20062025
most citedThe Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models

1k citations · 13.7k across the 113 of their papers we have counts for

collaborators
Showing 2014Show all

3 papers · 1 filter

astro-ph.HE2014★ 80 cited

Possible Detection of the Stellar Donor or Remnant for the Type Iax Supernova 2008ha

Ryan J. Foley, Curtis McCully, Saurabh W. Jha +5

Type Iax supernovae (SNe Iax) are thermonuclear explosions that are related to SNe Ia, but are physically distinct. The most important differences are that SNe Iax have significant…

astro-ph.SR2014★ 167 cited

A luminous, blue progenitor system for a type-Iax supernova

Curtis McCully, Saurabh W. Jha, Ryan J. Foley +6

Type-Iax supernovae (SN Iax) are stellar explosions that are spectroscopically similar to some type-Ia supernovae (SN Ia) at maximum light, except with lower ejecta velocities. The…

astro-ph.CO2014★ 20 cited

GRB 140515A at z=6.33: Constraints on the End of Reionization From a Gamma-ray Burst in a Low Hydrogen Column Density Environment

R. Chornock, E. Berger, D. B. Fox +3

We present the discovery and subsequent spectroscopy with Gemini-North of the optical afterglow of the Swift gamma-ray burst (GRB) 140515A. The spectrum exhibits a well-detected co…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.