World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
85
Citations
24974
World Ranking
2607
National Ranking
1290

E. Baron 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 E. Baron 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: 440 publications — 46th percentile

46% of scientists in this discipline score the same or lower.

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

E. Baron 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 E. Baron 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: 85 D-Index — 31st percentile

31% of scientists in this discipline score the same or lower.

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

Overview

E. Baron is affiliated with the University of Oklahoma in the United States and has contributed extensively to the field of Physics and Astronomy, with a primary focus on Astronomy and Astrophysics. Their research spans several subfields, including Nuclear and High Energy Physics, Instrumentation, Molecular Biology, and Emergency Medicine. The scientist's main areas of investigation include Gamma-ray bursts and supernovae, Astrophysics and Cosmic Phenomena, Pulsars and Gravitational Waves Research, Astrophysical Phenomena and Observations, Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, and Neutrino Physics Research.

Among E. Baron's recent publications are the following papers:

  • SN 2018zd: an unusual stellar explosion as part of the diverse Type II Supernova landscape, 2020, Monthly Notices of the Royal Astronomical Society
  • Carnegie Supernova Project II: The Slowest Rising Type Ia Supernova LSQ14fmg and Clues to the Origin of Super-Chandrasekhar/03fg-like Events, 2020, The Astrophysical Journal
  • Carnegie Supernova Project: The First Homogeneous Sample of Super-Chandrasekhar-mass/2003fg-like Type Ia Supernovae, 2021, The Astrophysical Journal
  • Carnegie Supernova Project-II: Near-infrared Spectroscopy of Stripped-envelope Core-collapse Supernovae, 2022, The Astrophysical Journal
  • A Speed Bump: SN 2021aefx Shows that Doppler Shift Alone Can Explain Early Excess Blue Flux in Some Type Ia Supernovae, 2022, The Astrophysical Journal Letters

E. Baron frequently collaborates with a range of colleagues. Notable co-authors include:

  • C. Ashall
  • L. Galbany
  • M. Stritzinger
  • P. Hoêflich
  • M. M. Phillips

Their work appears regularly in several scientific journals and preprint platforms. Among the most frequent publication venues are:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Astronomy and Astrophysics
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal Letters

E. Baron's academic output reflects a consistent focus on understanding the complexities of supernovae and related astrophysical phenomena. The range of topics covered and breadth of collaboration illustrate engagement with multiple dimensions of contemporary astrophysical research.

Best Publications

  • The Dartmouth Stellar Evolution Database

    Aaron Dotter;Brian Chaboyer;Darko Jevremović;Veselin Kostov

  • The NextGen Model Atmosphere grid for $3000\le \Teff \le 10000\K$

    Peter H. Hauschildt;E. Baron

  • The NextGen Model Atmosphere Grid for 3000 ≤ Teff ≤ 10,000 K

    Peter H. Hauschildt;E. Baron

  • The NEXTGEN Model Atmosphere Grid. II. Spherically Symmetric Model Atmospheres for Giant Stars with Effective Temperatures between 3000 and 6800 K

    Peter H. Hauschildt;Jason Ferguson;E. Baron

  • Evidence for a Spectroscopic Sequence among Type Ia Supernovae

    Peter Nugent;Mark Phillips;E. Baron;David Branch

  • Evidence for a Spectroscopic Sequence Among SNe Ia

    Peter Nugent;Mark Phillips;E. Baron;David Branch

  • IN SEARCH OF THE PROGENITORS OF TYPE IA SUPERNOVAE

    David Branch;Mario Livio;L. R. Yungelson;Francesca R. Boffi

  • The ACS Survey of Galactic Globular Clusters. II. Stellar Evolution Tracks, Isochrones, Luminosity Functions, and Synthetic Horizontal-Branch Models*

    Aaron Dotter;Brian Chaboyer;Darko Jevremović;E. Baron;E. Baron

  • Parallel Implementation of the PHOENIX Generalized Stellar Atmosphere Program

    Peter H. Hauschildt;Peter H. Hauschildt;E. Baron

  • Comparative Direct Analysis of Type Ia Supernova Spectra. II. Maximum Light

    David Branch;Leeann Chau Dang;Nicholas Hall;Wesley Ketchum

  • A Comparative Study of the Absolute Magnitude Distributions of Supernovae

    Dean Richardson;David Branch;Darrin Casebeer;Jennifer Millard

  • Low‐luminosity Type II supernovae: spectroscopic and photometric evolution

    A Pastorello;A Pastorello;A Pastorello;L Zampieri;Massimo Turatto;Enrico Cappellaro

  • Type II supernovae in 12Mcirdot and 15Mcirdot stars: The equation of state and general relativity.

    E Baron;J Cooperstein;S Kahana

  • Synthetic Spectra of Hydrodynamic Models of Type Ia Supernovae

    Peter Nugent;Peter Nugent;E. Baron;David Branch;Adam Fisher

  • The collapse of white dwarfs to neutron stars

    S. E. Woosley;E. Baron

  • Supernovae and the nuclear equation of state at high densities

    E. Baron;E. Baron;J. Cooperstein;S. Kahana

  • Metallicity Effects in NLTE Model Atmospheres of Type IA Supernovae

    E. J. Lentz;E. Baron;D. Branch;P. H. Hauschildt

  • Direct Analysis of Spectra of Type Ib Supernovae

    David Branch;David Branch;S. Benetti;Daniel Kasen;E. Baron;E. Baron

  • Metallicity Effects in Non-LTE Model Atmospheres of Type Ia Supernovae

    Eric J. Lentz;E. Baron;David Branch;Peter H. Hauschildt

  • Comparative Direct Analysis of Type Ia Supernova Spectra. I. SN 1994D

    David Branch;E. Baron;Nicholas Hall;Mercy Melakayil

Frequent Co-Authors

Peter H. Hauschildt
Peter H. Hauschildt Universität Hamburg
Peter Nugent
Peter Nugent Lawrence Berkeley National Laboratory
Maximilian Stritzinger
Maximilian Stritzinger Aarhus University
Nidia Morrell
Nidia Morrell Carnegie Learning
Mark M. Phillips
Mark M. Phillips Carnegie Institution for Science
Nicholas B. Suntzeff
Nicholas B. Suntzeff Texas A&M University
Alexei V. Filippenko
Alexei V. Filippenko University of California, Berkeley
Mario Hamuy
Mario Hamuy University of Chile
Saurabh Jha
Saurabh Jha Rutgers, The State University of New Jersey
Robert P. Kirshner
Robert P. Kirshner Harvard University

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