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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 152 284 272 166 159 855 71764

Tommaso Treu publications per year

The chart shows the history of publications by Tommaso Treu between 1998 and 2026, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Tommaso Treu published across 29 years, from 1998 to 2026, averaging 34.6 papers a year. Output peaked at 75 publications in 2022. 58 of the 1,002 publications appeared in the last two years.

No. of publications
25 50 75
Bar chart. Horizontal axis: year, 1998 to 2026. Vertical axis: number of publications, 0 to 75. Peak 75 publications in 2022. 1998: 4 publications 1999: 4 publications 2000: 3 publications 2001: 11 publications 2002: 13 publications 2003: 26 publications 2004: 22 publications 2005: 14 publications 2006: 19 publications 2007: 25 publications 2008: 27 publications 2009: 34 publications 2010: 28 publications 2011: 37 publications 2012: 45 publications 2013: 39 publications 2014: 40 publications 2015: 62 publications 2016: 51 publications 2017: 53 publications 2018: 50 publications 2019: 53 publications 2020: 53 publications 2021: 45 publications 2022: 75 publications 2023: 55 publications 2024: 56 publications 2025: 55 publications 2026: 3 publications
1998 2026

1,002 publications in total across all disciplines

View publications per year as a table
Tommaso Treu: publications per year, 1998 to 2026
Year Publications
1998 4
1999 4
2000 3
2001 11
2002 13
2003 26
2004 22
2005 14
2006 19
2007 25
2008 27
2009 34
2010 28
2011 37
2012 45
2013 39
2014 40
2015 62
2016 51
2017 53
2018 50
2019 53
2020 53
2021 45
2022 75
2023 55
2024 56
2025 55
2026 3
Total 1,002
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Tommaso Treu 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 Tommaso Treu 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, 843–862 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: 855 publications — 87th percentile

87% 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
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 32 855
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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Tommaso Treu 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 Tommaso Treu 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, 152–153 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: 152 D-Index — 93rd percentile

93% 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
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 24 152
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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Research.com Recognitions

  • 2007 - Fellow of Alfred P. Sloan Foundation

Overview

Tommaso Treu is affiliated with the University of California, Los Angeles in the United States. Their research primarily focuses on Physics and Astronomy, with a significant body of work in Astronomy and Astrophysics, Instrumentation, Atomic and Molecular Physics, and Optics, as well as contributions to Nuclear and High Energy Physics and Computational Mechanics.

Their research topics span a variety of areas including:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Gamma-ray bursts and supernovae
  • Stellar, planetary, and galactic studies
  • Adaptive optics and wavefront sensing
  • Astrophysical Phenomena and Observations
  • Cosmology and Gravitation Theories

Key recent publications by Tommaso Treu include:

  • The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans, 2022, The Astrophysical Journal
  • Early Results from GLASS-JWST. III. Galaxy Candidates at z ∼9-15*, 2022, The Astrophysical Journal Letters

Other notable papers associated with Treu's research network include:

  • STRIDES: a 3.9 per cent measurement of the Hubble constant from the strong lens system DES J0408−5354, 2020, Monthly Notices of the Royal Astronomical Society
  • The brightest galaxies at cosmic dawn, 2023, Monthly Notices of the Royal Astronomical Society
  • Dark matter haloes of massive elliptical galaxies at z ∼ 0.2 are well described by the Navarro-Frenk-White profile, 2021, Monthly Notices of the Royal Astronomical Society

Tomaso Treu regularly publishes in the following venues:

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

Frequent collaborators include Takahiro Morishita, Guido Roberts-Borsani, Michele Trenti, M. Castellano, and Simon Birrer, reflecting recurring partnerships in research projects and publications.

In recognition of their contributions to the field, Tommaso Treu was named a Fellow of the Alfred P. Sloan Foundation in 2007.

Best Publications

  • Tensions between the early and late Universe

    Licia Verde;Tommaso Treu;Adam G. Riess;Adam G. Riess

  • H0LiCOW – XIII. A 2.4 per cent measurement of H0 from lensed quasars: 5.3σ tension between early- and late-Universe probes

    Kenneth C. Wong;Sherry H. Suyu;Sherry H. Suyu;Sherry H. Suyu;Geoff C. F. Chen;Cristian E. Rusu;Cristian E. Rusu

  • The Low-luminosity End of the Radius-Luminosity Relationship for Active Galactic Nuclei

    Misty C. Bentz;Kelly D. Denney;Catherine J. Grier;Aaron J. Barth

  • Tensions between the Early and the Late Universe

    L. Verde;T. Treu;A.G. Riess

  • CAN MINOR MERGING ACCOUNT FOR THE SIZE GROWTH OF QUIESCENT GALAXIES? NEW RESULTS FROM THE CANDELS SURVEY

    Andrew B. Newman;Richard S. Ellis;Kevin Bundy;Tommaso Treu

  • The Lick AGN Monitoring Project: Broad-Line Region Radii and Black Hole Masses from Reverberation Mapping of Hbeta

    Misty C. Bentz;Jonelle L. Walsh;Aaron J. Barth;Nairn Baliber;Nairn Baliber

  • The Sloan Lens ACS Survey. III. The Structure and Formation of Early-Type Galaxies and Their Evolution since z ≈ 1

    Leon V. E. Koopmans;Tommaso Treu;Adam S. Bolton;Adam S. Bolton;Scott Burles

  • Strong Lensing by Galaxies

    Tommaso Treu

  • The Sloan Lens ACS Survey. I. A large spectroscopically selected sample of massive early-type lens galaxies

    Adam S. Bolton;Adam S. Bolton;Scott Burles;Leon V. E. Koopmans;Tommaso Treu;Tommaso Treu

  • THE SLOAN LENS ACS SURVEY. X. STELLAR, DYNAMICAL, AND TOTAL MASS CORRELATIONS OF MASSIVE EARLY-TYPE GALAXIES

    M. W. Auger;T. Treu;A. S. Bolton;R. Gavazzi;R. Gavazzi

  • Constraints on the equation of state of dark energy and the Hubble constant from stellar ages and the CMB

    Raul Jimenez;Licia Verde;Tommaso Treu;Daniel Stern

  • H0LiCOW - V. New COSMOGRAIL time delays of HE 0435-1223: H0 to 3.8 per cent precision from strong lensing in a flat ΛCDM model

    V. Bonvin;F. Courbin;S. H. Suyu;S. H. Suyu;S. H. Suyu;P. J. Marshall

  • A wide field Hubble Space Telescope study of the cluster CL0024+16 at z=0.4. I: morphological distributions to 5 Mpc radius

    T. Treu;R.S. Ellis;J.-P. Kneib;A. Dressler

  • The Sloan Lens ACS Survey. IV. The Mass Density Profile of Early-Type Galaxies out to 100 Effective Radii

    Raphaël Gavazzi;Tommaso Treu;Jason D. Rhodes;Léon V. E. Koopmans

  • Massive Dark Matter Halos and Evolution of Early-Type Galaxies to z ~ 1

    Tommaso Treu;Tommaso Treu;Léon V.E. Koopmans

  • The lick agn monitoring project: Broad-line region radii and black hole masses from reverberation mapping of Hβ

    Misty C. Bentz;Jonelle L. Walsh;Aaron J. Barth;Nairn Baliber;Nairn Baliber

  • The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample

    Adam S. Bolton;Scott Burles;Leon V. E. Koopmans;Tommaso Treu

  • The Structure & Dynamics of Massive Early-type Galaxies: On Homology, Isothermality and Isotropy inside one Effective Radius

    L.V.E. Koopmans;A. Bolton;T. Treu;O. Czoske

  • A Wide-Field Hubble Space Telescope Study of the Cluster Cl 0024+16 at z = 0.4. I. Morphological Distributions to 5 Mpc Radius

    Tommaso Treu;Richard S. Ellis;Jean-Paul Kneib;Alan Dressler

  • The Initial Mass Function of Early-Type Galaxies

    Tommaso Treu;Tommaso Treu;Matthew W. Auger;Leon V. E. Koopmans;Raphael Gavazzi;Raphael Gavazzi

Frequent Co-Authors

Christopher D. Fassnacht
Christopher D. Fassnacht University of California, Davis
Michele Trenti
Michele Trenti University of Melbourne
Richard S. Ellis
Richard S. Ellis University College London
Aaron J. Barth
Aaron J. Barth University of California, Irvine
Jong-Hak Woo
Jong-Hak Woo Seoul National University
Raphael Gavazzi
Raphael Gavazzi Institut d'Astrophysique de Paris
Massimo Stiavelli
Massimo Stiavelli Space Telescope Science Institute
Léon V. E. Koopmans
Léon V. E. Koopmans University of Groningen
Matthew A. Malkan
Matthew A. Malkan University of California, Los Angeles
Misty C. Bentz
Misty C. Bentz Georgia State University

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