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Wen-fai Fong

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 86 2538 2413 1258 1173 322 24996

Wen-fai Fong publications per year

The chart shows the history of publications by Wen-fai Fong between 2006 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Wen-fai Fong published across 20 years, from 2006 to 2025, averaging 19.5 papers a year. Output peaked at 53 publications in 2019. 36 of the 389 publications appeared in the last two years.

No. of publications
10 20 30 40 50
Bar chart. Horizontal axis: year, 2006 to 2025. Vertical axis: number of publications, 0 to 53. Peak 53 publications in 2019. 2006: 1 publication 2007: 0 publications 2008: 2 publications 2009: 1 publication 2010: 5 publications 2011: 7 publications 2012: 17 publications 2013: 25 publications 2014: 14 publications 2015: 15 publications 2016: 23 publications 2017: 49 publications 2018: 26 publications 2019: 53 publications 2020: 44 publications 2021: 21 publications 2022: 22 publications 2023: 28 publications 2024: 12 publications 2025: 24 publications
2006 2025

389 publications in total across all disciplines

View publications per year as a table
Wen-fai Fong: publications per year, 2006 to 2025
Year Publications
2006 1
2007 0
2008 2
2009 1
2010 5
2011 7
2012 17
2013 25
2014 14
2015 15
2016 23
2017 49
2018 26
2019 53
2020 44
2021 21
2022 22
2023 28
2024 12
2025 24
Total 389
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Wen-fai Fong publication distribution in Physics in 2026

The chart shows the distribution of publications by all Research.com ranked scientists in the field of Physics in 2026. The highlighted bar marks where Wen-fai Fong sits on this spectrum.

No. of scientists
50 100 150
Bar chart with 70 bars. Horizontal axis: publications, 103–122 to 1,469+. Vertical axis: number of scientists, 0 to 162. Most scientists, 162, have 323–342 publications. The last bar groups every scientist with 1,469 publications or more. The highlighted bar, 303–322 publications, is where this scientist sits. 103–122 publications: 7 scientists 123–142 publications: 10 scientists 143–162 publications: 31 scientists 163–182 publications: 35 scientists 183–202 publications: 53 scientists 203–222 publications: 81 scientists 223–242 publications: 85 scientists 243–262 publications: 112 scientists 263–282 publications: 114 scientists 283–302 publications: 126 scientists 303–322 publications: 136 scientists 323–342 publications: 162 scientists 343–362 publications: 155 scientists 363–382 publications: 156 scientists 383–402 publications: 134 scientists 403–422 publications: 145 scientists 423–442 publications: 147 scientists 443–462 publications: 131 scientists 463–482 publications: 131 scientists 483–502 publications: 116 scientists 503–522 publications: 106 scientists 523–542 publications: 103 scientists 543–562 publications: 87 scientists 563–582 publications: 84 scientists 583–602 publications: 94 scientists 603–622 publications: 70 scientists 623–642 publications: 76 scientists 643–662 publications: 60 scientists 663–682 publications: 54 scientists 683–702 publications: 60 scientists 703–722 publications: 48 scientists 723–742 publications: 64 scientists 743–762 publications: 48 scientists 763–782 publications: 37 scientists 783–802 publications: 43 scientists 803–822 publications: 34 scientists 823–842 publications: 36 scientists 843–862 publications: 32 scientists 863–882 publications: 32 scientists 883–902 publications: 31 scientists 903–922 publications: 25 scientists 923–942 publications: 15 scientists 943–962 publications: 24 scientists 963–982 publications: 13 scientists 983–1,002 publications: 21 scientists 1,003–1,022 publications: 21 scientists 1,023–1,042 publications: 16 scientists 1,043–1,062 publications: 9 scientists 1,063–1,082 publications: 19 scientists 1,083–1,102 publications: 11 scientists 1,103–1,122 publications: 17 scientists 1,123–1,142 publications: 11 scientists 1,143–1,162 publications: 7 scientists 1,163–1,182 publications: 4 scientists 1,183–1,202 publications: 10 scientists 1,203–1,222 publications: 8 scientists 1,223–1,242 publications: 16 scientists 1,243–1,262 publications: 4 scientists 1,263–1,282 publications: 10 scientists 1,283–1,302 publications: 5 scientists 1,303–1,322 publications: 7 scientists 1,323–1,342 publications: 4 scientists 1,343–1,362 publications: 8 scientists 1,363–1,382 publications: 6 scientists 1,383–1,402 publications: 7 scientists 1,403–1,422 publications: 3 scientists 1,423–1,442 publications: 4 scientists 1,443–1,462 publications: 4 scientists 1,463–1,468 publications: 3 scientists 1,469+ publications: 100 scientists
103–122 publications 1,469+

This scientist: 322 publications — 21st percentile

21% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 1,469 publications or more.

View publications distribution as a table
Number of Physics scientists by publication count, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
Publications Scientists This scientist
103–122 7
123–142 10
143–162 31
163–182 35
183–202 53
203–222 81
223–242 85
243–262 112
263–282 114
283–302 126
303–322 136 322
323–342 162
343–362 155
363–382 156
383–402 134
403–422 145
423–442 147
443–462 131
463–482 131
483–502 116
503–522 106
523–542 103
543–562 87
563–582 84
583–602 94
603–622 70
623–642 76
643–662 60
663–682 54
683–702 60
703–722 48
723–742 64
743–762 48
763–782 37
783–802 43
803–822 34
823–842 36
843–862 32
863–882 32
883–902 31
903–922 25
923–942 15
943–962 24
963–982 13
983–1,002 21
1,003–1,022 21
1,023–1,042 16
1,043–1,062 9
1,063–1,082 19
1,083–1,102 11
1,103–1,122 17
1,123–1,142 11
1,143–1,162 7
1,163–1,182 4
1,183–1,202 10
1,203–1,222 8
1,223–1,242 16
1,243–1,262 4
1,263–1,282 10
1,283–1,302 5
1,303–1,322 7
1,323–1,342 4
1,343–1,362 8
1,363–1,382 6
1,383–1,402 7
1,403–1,422 3
1,423–1,442 4
1,443–1,462 4
1,463–1,468 3
1,469+ 100
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Wen-fai Fong D-index placement in Physics in 2026

The chart shows the D-index (discipline H-index) distribution of Physics scientists ranked by Research.com in 2026. The highlighted bar marks where Wen-fai Fong sits on this spectrum.

No. of scientists
50 100 150
Bar chart with 59 bars. Horizontal axis: D-Index, 70–71 to 185+. Vertical axis: number of scientists, 0 to 167. Most scientists, 167, have 80–81 D-Index. The last bar groups every scientist with 185 D-Index or more. The highlighted bar, 86–87 D-Index, is where this scientist sits. 70–71 D-Index: 76 scientists 72–73 D-Index: 110 scientists 74–75 D-Index: 143 scientists 76–77 D-Index: 153 scientists 78–79 D-Index: 144 scientists 80–81 D-Index: 167 scientists 82–83 D-Index: 167 scientists 84–85 D-Index: 166 scientists 86–87 D-Index: 132 scientists 88–89 D-Index: 155 scientists 90–91 D-Index: 134 scientists 92–93 D-Index: 137 scientists 94–95 D-Index: 102 scientists 96–97 D-Index: 112 scientists 98–99 D-Index: 110 scientists 100–101 D-Index: 116 scientists 102–103 D-Index: 97 scientists 104–105 D-Index: 103 scientists 106–107 D-Index: 87 scientists 108–109 D-Index: 90 scientists 110–111 D-Index: 67 scientists 112–113 D-Index: 78 scientists 114–115 D-Index: 75 scientists 116–117 D-Index: 67 scientists 118–119 D-Index: 69 scientists 120–121 D-Index: 60 scientists 122–123 D-Index: 59 scientists 124–125 D-Index: 53 scientists 126–127 D-Index: 42 scientists 128–129 D-Index: 41 scientists 130–131 D-Index: 33 scientists 132–133 D-Index: 32 scientists 134–135 D-Index: 45 scientists 136–137 D-Index: 19 scientists 138–139 D-Index: 24 scientists 140–141 D-Index: 28 scientists 142–143 D-Index: 31 scientists 144–145 D-Index: 22 scientists 146–147 D-Index: 20 scientists 148–149 D-Index: 12 scientists 150–151 D-Index: 16 scientists 152–153 D-Index: 24 scientists 154–155 D-Index: 23 scientists 156–157 D-Index: 15 scientists 158–159 D-Index: 15 scientists 160–161 D-Index: 11 scientists 162–163 D-Index: 17 scientists 164–165 D-Index: 12 scientists 166–167 D-Index: 11 scientists 168–169 D-Index: 9 scientists 170–171 D-Index: 9 scientists 172–173 D-Index: 11 scientists 174–175 D-Index: 4 scientists 176–177 D-Index: 8 scientists 178–179 D-Index: 5 scientists 180–181 D-Index: 3 scientists 182–183 D-Index: 4 scientists 184 D-Index: 4 scientists 185+ D-Index: 99 scientists
70–71 D-Index 185+

This scientist: 86 D-Index — 32nd percentile

32% of scientists in this discipline score the same or lower.

The last bar groups every scientist with 185 D-Index or more.

View D-Index distribution as a table
Number of Physics scientists by D-index, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
D-Index Scientists This scientist
70–71 76
72–73 110
74–75 143
76–77 153
78–79 144
80–81 167
82–83 167
84–85 166
86–87 132 86
88–89 155
90–91 134
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116
102–103 97
104–105 103
106–107 87
108–109 90
110–111 67
112–113 78
114–115 75
116–117 67
118–119 69
120–121 60
122–123 59
124–125 53
126–127 42
128–129 41
130–131 33
132–133 32
134–135 45
136–137 19
138–139 24
140–141 28
142–143 31
144–145 22
146–147 20
148–149 12
150–151 16
152–153 24
154–155 23
156–157 15
158–159 15
160–161 11
162–163 17
164–165 12
166–167 11
168–169 9
170–171 9
172–173 11
174–175 4
176–177 8
178–179 5
180–181 3
182–183 4
184 4
185+ 99
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Overview

Wen-fai Fong is affiliated with Northwestern University in the United States. Their academic work is primarily situated within the field of Physics and Astronomy, with a strong focus on subfields such as Astronomy and Astrophysics, Nuclear and High Energy Physics, Instrumentation, Biomedical Engineering, and Atomic and Molecular Physics, and Optics.

The researcher's publication record features a concentration on topics including Gamma-ray bursts and supernovae, Pulsars and Gravitational Waves Research, Astrophysical Phenomena and Observations, Stellar, planetary, and galactic studies, Astrophysics and Cosmic Phenomena, Astronomy and Astrophysical Research, and Adaptive optics and wavefront sensing.

Fong has contributed to frequent publication venues including arXiv (Cornell University), The Astrophysical Journal, The Astrophysical Journal Letters, Monthly Notices of the Royal Astronomical Society, and Nature Astronomy.

They have collaborated frequently with several researchers, including C. D. Kilpatrick, Anya E. Nugent, J. X. Prochaska, Tarraneh Eftekhari, and Jillian Rastinejad.

Recent papers authored or co-authored by Wen-fai Fong include:

  • A kilonova following a long-duration gamma-ray burst at 350 Mpc (2022, Nature)
  • Characterizing the Fast Radio Burst Host Galaxy Population and its Connection to Transients in the Local and Extragalactic Universe (2022, The Astronomical Journal)
  • Heavy-element production in a compact object merger observed by JWST (2023, Nature)
  • Short GRB Host Galaxies. I. Photometric and Spectroscopic Catalogs, Host Associations, and Galactocentric Offsets (2022, The Astrophysical Journal)
  • The Demographics, Stellar Populations, and Star Formation Histories of Fast Radio Burst Host Galaxies: Implications for the Progenitors (2023, The Astrophysical Journal)

Best Publications

  • A gravitational-wave standard siren measurement of the Hubble constant

    B. P. Abbott;R. Abbott;T. D. Abbott;F. Acernese;F. Acernese

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models

    P. S. Cowperthwaite;E. Berger;V. A. Villar;B. D. Metzger

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

    P. S. Cowperthwaite;E. Berger;V. A. Villar;B. D. Metzger

  • A Decade of Short-duration Gamma-ray Burst Broad-band Afterglows: Energetics, Circumburst Densities, and Jet Opening Angles

    Wen-fai Fong;Edo Berger;Raffaella Margutti;B. Ashley Zauderer

  • An r-process Kilonova Associated with the Short-hard GRB 130603B

    Edo Berger;W Fong;R Chornock

  • A Decade of Short-duration Gamma-ray Burst Broadband Afterglows: Energetics, Circumburst Densities, and jet Opening Angles

    W. Fong;E. Berger;R. Margutti;R. Margutti;B. A. Zauderer

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart

    M. Soares-Santos;D. E. Holz;J. Annis;R. Chornock

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Discovery of the Optical Counterpart Using the Dark Energy Camera

    M. Soares-Santos;M. Soares-Santos;D. E. Holz;J. Annis;R. Chornock

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South

    R. Chornock;E. Berger;D. Kasen;P. S. Cowperthwaite

  • The combined ultraviolet, optical, and near-infrared light curves of the kilonova associated with the binary neutron star merger gw170817: unified data set, analytic models, and physical implications

    V. A. Villar;J. Guillochon;E. Berger;B. D. Metzger

  • The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications

    V. Ashley Villar;James Guillochon;Edo Berger;Brian D. Metzger

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. VI. Radio Constraints on a Relativistic Jet and Predictions for Late-time Emission from the Kilonova Ejecta

    K. D. Alexander;E. Berger;Wen-fai Fong;P. K.G. Williams

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. V. Rising X-ray Emission from an Off-Axis Jet

    Raffaella Margutti;E. Berger;W. Fong;C. Guidorzi

  • The binary neutron star event ligo/virgo gw170817 a hundred and sixty days after merger: Synchrotron emission across the electromagnetic spectrum

    Raffaella Margutti;K. D. Alexander;X. Xie;L. Sironi

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. V. Rising X-Ray Emission from an Off-axis Jet

    Raffaella Margutti;E. Berger;Wen-fai Fong;C. Guidorzi

  • Hubble Space Telescope Observations of Short Gamma-Ray Burst Host Galaxies: Morphologies, Offsets, and Local Environments

    Wen-fai Fong;Edo Berger;Derek B. Fox

  • The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. IV. Detection of Near-infrared Signatures of r-process Nucleosynthesis with Gemini-South

    R. Chornock;E. Berger;D. Kasen;D. Kasen;P. S. Cowperthwaite;P. S. Cowperthwaite

  • The Locations of Short Gamma-Ray Bursts as Evidence for Compact Object Binary Progenitors

    Wen-Fai Fong;Edo Berger

  • Localization and broadband follow-up of the gravitational-wave transient GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • Hubble Space Telescope Observations of Short GRB Host Galaxies: Morphologies, Offsets and Local Environments

    Wen-fai Fong;E. Berger;D. Fox

Frequent Co-Authors

Edo Berger
Edo Berger Harvard University
Raffaella Margutti
Raffaella Margutti Northwestern University
Ryan Chornock
Ryan Chornock Northwestern University
Brian D. Metzger
Brian D. Metzger Columbia University
Ryan J. Foley
Ryan J. Foley University of California, Santa Cruz
Marcelle Soares-Santos
Marcelle Soares-Santos Brandeis University
Daniel E. Holz
Daniel E. Holz University of Chicago
Nial R. Tanvir
Nial R. Tanvir University of Leicester
Nathan Smith
Nathan Smith University of Arizona
Joshua A. Frieman
Joshua A. Frieman University of Chicago

External Links

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