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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 98 1766 1680 6 6 413 33046

Ezequiel Treister publications per year

The chart shows the history of publications by Ezequiel Treister between 2002 and 2026, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Ezequiel Treister published across 25 years, from 2002 to 2026, averaging 18.6 papers a year. Output peaked at 41 publications in 2017. 24 of the 465 publications appeared in the last two years.

No. of publications
10 20 30 40
Bar chart. Horizontal axis: year, 2002 to 2026. Vertical axis: number of publications, 0 to 41. Peak 41 publications in 2017. 2002: 2 publications 2003: 7 publications 2004: 17 publications 2005: 17 publications 2006: 19 publications 2007: 11 publications 2008: 10 publications 2009: 19 publications 2010: 23 publications 2011: 27 publications 2012: 23 publications 2013: 18 publications 2014: 13 publications 2015: 23 publications 2016: 27 publications 2017: 41 publications 2018: 23 publications 2019: 22 publications 2020: 17 publications 2021: 21 publications 2022: 32 publications 2023: 12 publications 2024: 17 publications 2025: 22 publications 2026: 2 publications
2002 2026

465 publications in total across all disciplines

View publications per year as a table
Ezequiel Treister: publications per year, 2002 to 2026
Year Publications
2002 2
2003 7
2004 17
2005 17
2006 19
2007 11
2008 10
2009 19
2010 23
2011 27
2012 23
2013 18
2014 13
2015 23
2016 27
2017 41
2018 23
2019 22
2020 17
2021 21
2022 32
2023 12
2024 17
2025 22
2026 2
Total 465
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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.

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, 403–422 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: 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.

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
323–342 162
343–362 155
363–382 156
383–402 134
403–422 145 413
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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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.

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, 98–99 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: 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.

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
88–89 155
90–91 134
92–93 137
94–95 102
96–97 112
98–99 110 98
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

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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