World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
95
Citations
31199
World Ranking
1936
National Ranking
50

Michele Trenti 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 Michele Trenti 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: 364 publications — 31st percentile

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

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

Michele Trenti 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 Michele Trenti 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: 95 D-Index — 49th percentile

49% of scientists in this discipline score the same or lower.

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

Overview

Michele Trenti is affiliated with the University of Melbourne in Australia and works in the field of Physics and Astronomy. Their research interests span several subfields of study, including Astronomy and Astrophysics, Instrumentation, Aerospace Engineering, Atomic and Molecular Physics and Optics, and Computational Mechanics.

The scientist's academic work covers a range of topics such as Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, Phenomena, Gamma-ray Bursts and Supernovae, Stellar, Planetary, and Galactic Studies, Astrophysical Phenomena and Observations, Adaptive Optics and Wavefront Sensing, and Astrophysics and Star Formation Studies.

Among recent publications, Michele Trenti has contributed to papers including:

  • Early Results from GLASS-JWST. III. Galaxy Candidates at z ∼9-15, 2022, The Astrophysical Journal Letters
  • The GLASS-JWST Early Release Science Program. I. Survey Design and Release Plans, 2022, The Astrophysical Journal
  • The brightest galaxies at cosmic dawn, 2023, Monthly Notices of the Royal Astronomical Society
  • A highly magnified star at redshift 6.2, 2022, Nature
  • Early Results from GLASS-JWST. XIX. A High Density of Bright Galaxies at z ≈ 10 in the A2744 Region, 2023, The Astrophysical Journal Letters

Michele Trenti frequently publishes in the following venues:

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

The scientist collaborates regularly with several co-authors, including Tommaso Treu, Takahiro Morishita, Guido Roberts-Borsani, Maruša Bradač, and Nicha Leethochawalit.

Best Publications

  • UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields

    R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Trenti

  • UV luminosity functions at redshifts z ∼ 4 to z ∼ 10: 10,000 galaxies from HST legacy fields

    R.J. Bouwens;R.J. Bouwens;G.D. Illingworth;P.A. Oesch;P.A. Oesch;M. Trenti

  • UV Luminosity Functions from 132 z~7 and z~8 Lyman-Break Galaxies in the ultra-deep HUDF09 and wide-area ERS WFC3/IR Observations

    R. J. Bouwens;G. D. Illingworth;P. A. Oesch;I. Labbe

  • Ultraviolet Luminosity Functions from 132 z ~ 7 and z ~ 8 Lyman-break Galaxies in the Ultra-deep HUDF09 and Wide-area Early Release Science WFC3/IR Observations

    R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;I. Labbé

  • Discovery of z~8 Galaxies in the HUDF from ultra-deep WFC3/IR Observations

    R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Stiavelli

  • UV-continuum Slopes at z ~ 4-7 from the HUDF09+ERS+CANDELS Observations: Discovery of a Well-defined UV Color-Magnitude Relationship for z ≥ 4 Star-forming Galaxies

    R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P.A. Oesch;M. Franx

  • DISCOVERY OF z ∼ 8 GALAXIES IN THE HUBBLE ULTRA DEEP FIELD FROM ULTRA-DEEP WFC3/IR OBSERVATIONS*

    R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Stiavelli

  • UV-CONTINUUM SLOPES OF >4000 z ∼ 4-8 GALAXIES FROM THE HUDF/XDF, HUDF09, ERS, CANDELS-SOUTH, AND CANDELS-NORTH FIELDS

    R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;I. Labbé

  • The Most Luminous z~9-10 Galaxy Candidates yet Found: The Luminosity Function, Cosmic Star-Formation Rate, and the First Mass Density Estimate at 500 Myr

    P. A. Oesch;R. J. Bouwens;G. D. Illingworth;I. Labbe

  • Cosmic Variance and Its Effect on the Luminosity Function Determination in Deep High-z Surveys

    M. Trenti;M. Stiavelli;M. Stiavelli

  • A candidate redshift z ≈ 10 galaxy and rapid changes in that population at an age of 500 Myr

    R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;I. Labbe;P. A. Oesch

  • Very blue UV-continuum slopes of low luminosity z~7 galaxies from WFC3/IR: Evidence for extremely low metallicities?

    R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Trenti

  • Structure and Morphologies of z~7-8 Galaxies from ultra-deep WFC3/IR Imaging of the HUDF

    P.A. Oesch;R.J. Bouwens;C.M. Carollo;G.D. Illingworth

  • A Remarkably Luminous Galaxy at z=11.1 Measured with Hubble Space Telescope Grism Spectroscopy

    P.A. Oesch;G. Brammer;P.G. van Dokkum;G.D. Illingworth

  • z ∼ 7 GALAXIES IN THE HUDF: FIRST EPOCH WFC3/IR RESULTS*

    P. A. Oesch;R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;C. M. Carollo

  • LOWER-LUMINOSITY GALAXIES COULD REIONIZE THE UNIVERSE: VERY STEEP FAINT-END SLOPES TO THE UV LUMINOSITY FUNCTIONS AT z ⩾ 5-8 FROM THE HUDF09 WFC3/IR OBSERVATIONS*

    R. J. Bouwens;R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Trenti

  • Probing the Dawn of Galaxies at z ~{} 9-12 : New Constraints from HUDF12/XDF and CANDELS data

    P. A. Oesch;R. J. Bouwens;G. D. Illingworth;I. Labbé

  • The HST eXtreme Deep Field (XDF): Combining All ACS and WFC3/IR Data on the HUDF Region into the Deepest Field Ever

    G. D. Illingworth;D. Magee;P. A. Oesch;R. J. Bouwens

  • UV Luminosity Functions at redshifts z~4 to z~10: 11000 Galaxies from HST Legacy Fields

    R. J. Bouwens;G. D. Illingworth;P. A. Oesch;M. Trenti

  • Gravitational N-body Simulations

    M. Trenti;P. Hut

Frequent Co-Authors

Tommaso Treu
Tommaso Treu University of California, Los Angeles
Rychard Bouwens
Rychard Bouwens Leiden University
Massimo Stiavelli
Massimo Stiavelli Space Telescope Science Institute
Pascal Oesch
Pascal Oesch University of Geneva
Garth D. Illingworth
Garth D. Illingworth University of California, Santa Cruz
Ivo Labbe
Ivo Labbe Swinburne University of Technology
Gabriel B. Brammer
Gabriel B. Brammer University of Copenhagen
Masami Ouchi
Masami Ouchi University of Tokyo
Keiichi Umetsu
Keiichi Umetsu Institute of Astronomy and Astrophysics, Academia Sinica
Daniel P. Stark
Daniel P. Stark University of Arizona

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