World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
98
Citations
30750
World Ranking
1769
National Ranking
927

Dušan Kereš 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 Dušan Kereš 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: 202 publications — 4th percentile

4% of scientists in this discipline score the same or lower.

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

Dušan Kereš 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 Dušan Kereš 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: 98 D-Index — 53rd percentile

53% of scientists in this discipline score the same or lower.

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

Overview

Dušan Kereš is affiliated with the University of California, San Diego in the United States. Their research primarily spans the fields of physics and astronomy, with a significant focus on astronomy and astrophysics, instrumentation, and nuclear and high energy physics. Their work also crosses into related areas such as general health professions and computational mechanics.

The scientist has contributed extensively to topics within galaxies, star formation, and cosmic phenomena. Specific research interests include galaxies: formation, evolution, and phenomena; astrophysics and star formation studies; astronomy and astrophysical research; stellar, planetary, and galactic studies; astrophysics and cosmic phenomena; astrophysical phenomena and observations; as well as gamma-ray bursts and supernovae.

Dušan Kereš has published numerous papers, with several appearing in prominent scientific journals. Some recent papers include:

  • Properties of the circumgalactic medium in cosmic ray-dominated galaxy haloes, 2020, Monthly Notices of the Royal Astronomical Society
  • A dark matter profile to model diverse feedback-induced core sizes of ΛCDM haloes, 2020, Monthly Notices of the Royal Astronomical Society
  • Characterizing mass, momentum, energy, and metal outflow rates of multiphase galactic winds in the FIRE-2 cosmological simulations, 2021, Monthly Notices of the Royal Astronomical Society
  • No missing photons for reionization: moderate ionizing photon escape fractions from the FIRE-2 simulations, 2020, Monthly Notices of the Royal Astronomical Society
  • Virialization of the Inner CGM in the FIRE Simulations and Implications for Galaxy Disks, Star Formation, and Feedback, 2021, The Astrophysical Journal

The scientist has frequently collaborated with other researchers. Their most frequent coauthors are:

  • Philip F. Hopkins
  • Claude-André Faucher-Giguère
  • Eliot Quataert
  • Andrew Wetzel
  • Christopher C. Hayward

Dušan Kereš's work has been published predominantly in the following venues:

  • Monthly Notices of the Royal Astronomical Society
  • arXiv (Cornell University)
  • The Astrophysical Journal
  • The Astrophysical Journal Supplement Series
  • Nature Astronomy

Best Publications

  • A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies. I. Galaxy Mergers and Quasar Activity

    Philip F. Hopkins;Lars Hernquist;Thomas J. Cox;Dušan Kereš

  • Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation

    Philip F. Hopkins;Philip F. Hopkins;Dušan Kereš;José Oñorbe;Claude André Faucher-Giguère;Claude André Faucher-Giguère

  • FIRE-2 simulations: physics versus numerics in galaxy formation

    Philip F. Hopkins;Andrew Wetzel;Andrew Wetzel;Andrew Wetzel;Dušan Kereš;Claude André Faucher-Giguère

  • Gusty, gaseous flows of FIRE: Galactic winds in cosmological simulations with explicit stellar feedback

    Alexander L. Muratov;Dušan Kereš;Claude André Faucher-Giguère;Philip F. Hopkins

  • The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-frame Optical Spectroscopy for ~1500 H-selected Galaxies at 1.37 ? z ? 3.8

    Mariska Kriek;Alice E. Shapley;Naveen A. Reddy;Brian Siana

  • A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals

    Philip F. Hopkins;Thomas J. Cox;Dušan Kereš;Lars Hernquist

  • Reconciling dwarf galaxies with LCDM cosmology: Simulating a realistic population of satellites around a Milky Way-mass galaxy

    Andrew R. Wetzel;Philip F. Hopkins;Ji-hoon Kim;Claude-Andre Faucher-Giguere

  • RECONCILING DWARF GALAXIES WITH ΛCDM COSMOLOGY: SIMULATING A REALISTIC POPULATION OF SATELLITES AROUND A MILKY WAY–MASS GALAXY

    Andrew R. Wetzel;Andrew R. Wetzel;Andrew R. Wetzel;Philip F. Hopkins;Ji Hoon Kim;Ji Hoon Kim;Claude André Faucher-Giguère

  • Mergers and bulge formation in ΛCDM: Which mergers matter?

    Philip F. Hopkins;Kevin Bundy;Darren Croton;Lars Hernquist

  • The origin and evolution of the galaxy mass–metallicity relation

    Xiangcheng Ma;Philip F. Hopkins;Claude André Faucher-Giguère;Nick Zolman

  • The cosmic baryon cycle and galaxy mass assembly in the FIRE simulations

    Daniel Anglés-Alcázar;Claude André Faucher-Giguère;Dušan Kereš;Philip F. Hopkins

  • Dissipation and Extra Light in Galactic Nuclei. IV. Evolution in the Scaling Relations of Spheroids

    Philip F. Hopkins;Lars Hernquist;Thomas J. Cox;Dusan Keres

  • Forged in FIRE: cusps, cores and baryons in low-mass dwarf galaxies

    Jose Oñorbe;Jose Oñorbe;Michael Boylan-Kolchin;Michael Boylan-Kolchin;James S. Bullock;Philip F. Hopkins

  • The Baryonic Assembly of Dark Matter Halos

    Claude-André Faucher-Giguère;Dušan Kereš;Chung-Pei Ma

  • Moving mesh cosmology: tracing cosmological gas accretion

    Dylan Nelson;Mark Vogelsberger;Shy Genel;Debora Sijacki

  • The impact of baryonic physics on the structure of dark matter haloes: the view from the FIRE cosmological simulations

    T. K. Chan;D. Kereš;J. Oñorbe;P. F. Hopkins

  • SIMULATIONS OF THE MAGELLANIC STREAM IN A FIRST INFALL SCENARIO

    Gurtina Besla;Nitya Kallivayalil;L. Hernquist;R. P. van der Marel

  • Not so lumpy after all: modelling the depletion of dark matter subhaloes by Milky Way-like galaxies

    Shea Garrison-Kimmel;Andrew R. Wetzel;Andrew R. Wetzel;Andrew R. Wetzel;James S. Bullock;Philip F. Hopkins

  • WHAT DOES A SUBMILLIMETER GALAXY SELECTION ACTUALLY SELECT? THE DEPENDENCE OF SUBMILLIMETER FLUX DENSITY ON STAR FORMATION RATE AND DUST MASS

    Christopher C. Hayward;Dušan Kereš;Dušan Kereš;Patrik Jonsson;Desika Narayanan;Desika Narayanan

  • Mergers in Lambda-CDM: Uncertainties in Theoretical Predictions and Interpretations of the Merger Rate

    Philip F. Hopkins;Darren Croton;Kevin Bundy;Sadegh Khochfar

Frequent Co-Authors

Philip F. Hopkins
Philip F. Hopkins California Institute of Technology
Claude André Faucher-Giguère
Claude André Faucher-Giguère Northwestern University
Eliot Quataert
Eliot Quataert Princeton University
Norman Murray
Norman Murray University of Toronto
Michael Boylan-Kolchin
Michael Boylan-Kolchin The University of Texas at Austin
James S. Bullock
James S. Bullock University of California, Irvine
Romeel Davé
Romeel Davé University of Edinburgh
Lars Hernquist
Lars Hernquist Harvard University
Greg L. Bryan
Greg L. Bryan Columbia University
Alice E. Shapley
Alice E. Shapley University of California, Los Angeles

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