World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
98
Citations
33046
World Ranking
1766
National Ranking
6

Ezequiel Treister 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 Ezequiel Treister 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: 413 publications — 40th percentile

40% of scientists in this discipline score the same or lower.

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

Ezequiel Treister 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 Ezequiel Treister 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

Ezequiel Treister is affiliated with the Pontificia Universidad Católica de Chile in Chile. Their research focuses primarily within the broad field of Physics and Astronomy, with specific attention to several subfields including Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, General Health Professions, and Computational Mechanics.

Their scientific work covers various main topics, featuring extensively on Galaxies: Formation, Evolution, Phenomena; Astrophysical Phenomena and Observations; Astronomy and Astrophysical Research; Gamma-ray bursts and supernovae; Astrophysics and Star Formation Studies; Stellar, planetary, and galactic studies; and Astrophysics and Cosmic Phenomena.

Frequent collaborators in their research include:

  • F. E. Bauer
  • Cláudio Ricci
  • C. M. Urry
  • Michael Koss
  • Daniel Stern

They have published numerous articles in several prominent scientific journals. The principal venues for these publications are:

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

Recent publications include:

  • MAGNUM survey: Compact jets causing large turmoil in galaxies, 2021, Astronomy and Astrophysics
  • BASS. XXII. The BASS DR2 AGN Catalog and Data, 2022, The Astrophysical Journal Supplement Series
  • GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies, 2021, arXiv (Cornell University)
  • A hard X-ray view of luminous and ultra-luminous infrared galaxies in GOALS - I. AGN obscuration along the merger sequence, 2021, Monthly Notices of the Royal Astronomical Society
  • Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies, 2021, The Astrophysical Journal

Best Publications

  • The Nuclear Spectroscopic Telescope Array (NuSTAR) Mission

    Fiona A. Harrison;William W. Craig;Finn E. Christensen;Charles J. Hailey

  • THE NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY (NuSTAR) HIGH-ENERGY X-RAY MISSION

    Fiona A. Harrison;William W. Craig;William W. Craig;Finn E. Christensen;Charles J. Hailey

  • The green valley is a red herring: Galaxy Zoo reveals two evolutionary pathways towards quenching of star formation in early-and late-type galaxies

    Kevin Schawinski;C. Megan Urry;Brooke D. Simmons;Lucy F Fortson

  • The XMM-Newton Wide-Field Survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous AGN

    M. Brusa;F. Civano;A. Comastri;T. Miyaji

  • Ly-alpha Emission-Line Galaxies at z = 3.1 in the Extended Chandra Deep Field South

    C. Gronwall;R. Ciardullo;T. Hickey;E. Gawaiser

  • Major Galaxy Mergers Only Trigger the Most Luminous AGN

    E. Treister;K. Schawinski;C. M. Urry;B. D. Simmons

  • The Space Density of Compton Thick AGN and the X-ray Background

    E. Treister;C. Megan Urry;Shanil Virani

  • THE CHANDRA COSMOS LEGACY SURVEY: OVERVIEW AND POINT SOURCE CATALOG

    F. Civano;F. Civano;S. Marchesi;S. Marchesi;S. Marchesi;A. Comastri;M. C. Urry

  • Ly Alpha-Emitting Galaxies at z=3.1: L* Progenitors Experiencing Rapid Star Formation

    Eric Gawiser;Harold Francke;Kamson Lai;Kevin Schawinski

  • Lyα Emission-Line Galaxies at z = 3.1 in the Extended Chandra Deep Field-South

    Caryl Gronwall;Robin Ciardullo;Thomas Hickey;Eric Gawiser

  • The Multiwavelength Survey by Yale-Chile (MUSYC): Survey Design and Deep Public UBVRIz' Images and Catalogs of the Extended Hubble Deep Field South

    E. Gawiser;P. G. van Dokkum;D. Herrera

  • The Fall of AGN and the Rise of Star-Forming Galaxies: A Close Look at the Chandra Deep Field X-ray Number Counts

    F. E. Bauer;D. M. Alexander;W. N. Brandt;D. P. Schneider

  • MAJOR GALAXY MERGERS ONLY TRIGGER THE MOST LUMINOUS ACTIVE GALACTIC NUCLEI

    E. Treister;K. Schawinski;C. M. Urry;B. D. Simmons

  • Lyα-Emitting Galaxies at z = 3.1: L* Progenitors Experiencing Rapid Star Formation*

    Eric Gawiser;Harold Francke;Harold Francke;Kamson Lai;Kevin Schawinski

  • The fall of active galactic nuclei and the rise of star-forming galaxies: A close look at the Chandra Deep Field X-ray number counts

    F. E. Bauer;F. E. Bauer;D. M. Alexander;W. N. Brandt;D. P. Schneider

  • The Space Density of Compton-Thick Active Galactic Nucleus and the X-Ray Background

    E. Treister;E. Treister;C. Megan Urry;Shanil Virani

  • The XMM-Newton wide-field survey in the COSMOS field (XMM-COSMOS): demography and multiwavelength properties of obscured and unobscured luminous active galactic nuclei

    M. Brusa;F. Civano;A. Comastri;T. Miyaji;T. Miyaji

  • The multiwavelength survey by Yale-Chile (MUSYC): Survey design and deep public UBVRIz′ images and catalogs of the extended Hubble Deep Field-South

    Eric Gawiser;Pieter G. Van Dokkum;David Herrera;José Maza

  • BAT AGN Spectroscopic Survey - V. X-ray properties of the Swift/BAT 70-month AGN catalog

    Claudio Ricci;Benny Trakhtenbrot;Michael J. Koss;Yoshihiro Ueda

  • The nuclear spectroscopic telescope array (NuSTAR) high-energy X-ray mission

    Kristin K. Madsen;Fiona A. Harrison;Hongjun An;Steven E. Boggs

Frequent Co-Authors

Franz E. Bauer
Franz E. Bauer Pontificia Universidad Católica de Chile
C. Megan Urry
C. Megan Urry Yale University
Michael Koss
Michael Koss ETH Zurich
Andrea Comastri
Andrea Comastri National Institute for Astrophysics
Fiona A. Harrison
Fiona A. Harrison California Institute of Technology
Eric Gawiser
Eric Gawiser Rutgers, The State University of New Jersey
Daniel Stern
Daniel Stern California Institute of Technology
Poshak Gandhi
Poshak Gandhi University of Southampton
Francesca Civano
Francesca Civano Harvard University

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