World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
147
Citations
71395
World Ranking
321
National Ranking
189

Edo Berger 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 Edo Berger sits on this spectrum.

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 publications 1,469+

This scientist: 884 publications — 88th percentile

88% of scientists in this discipline score the same or lower.

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

Edo Berger 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 Edo Berger sits on this spectrum.

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 D-Index 185+

This scientist: 147 D-Index — 92nd percentile

92% of scientists in this discipline score the same or lower.

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

Overview

Edo Berger is affiliated with Harvard University in the United States and conducts research primarily within the field of Physics and Astronomy. Their scholarly output includes a significant focus on Astronomy and Astrophysics as well as contributions to Nuclear and High Energy Physics, Instrumentation, Computational Mechanics, and Biomedical Engineering.

Their research covers diverse topics including:

  • Gamma-ray bursts and supernovae
  • Pulsars and Gravitational Waves Research
  • Astrophysical Phenomena and Observations
  • Astrophysics and Cosmic Phenomena
  • Stellar, planetary, and galactic studies
  • Astronomy and Astrophysical Research
  • Astro and Planetary Science

Edo Berger's recent publications exemplify the scope of their work. Notable papers include:

  • "The Relational Dynamics of Space-Time" (2024), published in Spectrum Research Repository (Concordia University)
  • "A kilonova following a long-duration gamma-ray burst at 350 Mpc" (2022), published in Nature
  • "Impact of massive binary star and cosmic evolution on gravitational wave observations I: black hole-neutron star mergers" (2021), published in Monthly Notices of the Royal Astronomical Society
  • "A red giant orbiting a black hole" (2023), published in Monthly Notices of the Royal Astronomical Society
  • "An outflow powers the optical rise of the nearby, fast-evolving tidal disruption event AT2019qiz" (2020), published in Monthly Notices of the Royal Astronomical Society

Their frequent coauthors reflect a collaborative research approach. Key collaborators include:

  • R. Chornock
  • Sebastián Gómez
  • K. D. Alexander
  • T. Laskar
  • R. Margutti

Regarding venues for publication, Edo Berger commonly publishes in:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • The Astrophysical Journal Letters
  • Monthly Notices of the Royal Astronomical Society
  • Zenodo (CERN European Organization for Nuclear Research)

The extensive publication record and multidisciplinary topics suggest a broad engagement with theoretical and observational astrophysics, including phenomena involving gamma-ray bursts, gravitational waves, and cosmic events related to stellar and galactic systems.

Best Publications

  • The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample

    D. M. Scolnic;D. O. Jones;A. Rest;A. Rest;Y. C. Pan

  • The Complete Light-curve Sample of Spectroscopically Confirmed Type Ia Supernovae from Pan-STARRS1 and Cosmological Constraints from The Combined Pantheon Sample

    D. M. Scolnic;D. O. Jones;A. Rest;Y. C. Pan

  • BEAMING IN GAMMA-RAY BURSTS: EVIDENCE FOR A STANDARD ENERGY RESERVOIR

    D. A. Frail;S. R. Kulkarni;R. Sari;S. G. Djorgovski

  • 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

  • Short-Duration Gamma-Ray Bursts

    Edo Berger

  • 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 γ-ray burst at a redshift of z ≈ 8.2

    N. R. Tanvir;D. B. Fox;A. J. Levan;E. Berger

  • WHAT IS THE MOST PROMISING ELECTROMAGNETIC COUNTERPART OF A NEUTRON STAR BINARY MERGER

    B. D. Metzger;Edo Berger

  • Tidal Deformabilities and Radii of Neutron Stars from the Observation of GW170817

    Soumi De;Daniel Finstad;James Lattimer;Duncan Brown

  • The afterglow of GRB 050709 and the nature of the short-hard γ-ray bursts

    Derek B Fox;Derek B Fox;Dale A Frail;Paul Antony Price;Shrinivas R Kulkarni

  • An extremely luminous X-ray outburst at the birth of a supernova

    A. M. Soderberg;A. M. Soderberg;E. Berger;E. Berger;K. L. Page;P. Schady

  • Relativistic ejecta from X-ray flash XRF 060218 and the rate of cosmic explosions

    A. M. Soderberg;S. R. Kulkarni;E. Nakar;E. Berger

  • 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

  • A Photometric Redshift of z ~ 9.4 for GRB 090429B

    A. Cucchiara;A. Cucchiara;A. Cucchiara;A. J. Levan;D. B. Fox;N. R. Tanvir

  • 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

  • A Photometric Redshift of z ~ 9.4 for GRB 090429B

    A. Cucchiara;A. J. Levan;D. B. Fox;N. R. Tanvir

  • 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

Frequent Co-Authors

Ryan Chornock
Ryan Chornock Northwestern University
Raffaella Margutti
Raffaella Margutti Northwestern University
Wen-fai Fong
Wen-fai Fong Northwestern University
Alicia M. Soderberg
Alicia M. Soderberg Harvard University
Brian D. Metzger
Brian D. Metzger Columbia University
Ryan J. Foley
Ryan J. Foley University of California, Santa Cruz
Robert P. Kirshner
Robert P. Kirshner Harvard University
K. C. Chambers
K. C. Chambers University of Hawaii at Manoa
Marcelle Soares-Santos
Marcelle Soares-Santos Brandeis University
Nial R. Tanvir
Nial R. Tanvir University of Leicester

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