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D-Index & Metrics

Physics

D-Index
86
Citations
30469
World Ranking
2519
National Ranking
1251

Massimo Stiavelli 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 Massimo Stiavelli 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: 302 publications — 18th percentile

18% of scientists in this discipline score the same or lower.

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

Massimo Stiavelli 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 Massimo Stiavelli 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: 86 D-Index — 32nd percentile

32% of scientists in this discipline score the same or lower.

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

Research.com Recognitions

  • 2018 - Fellow of the American Association for the Advancement of Science (AAAS)

Overview

Massimo Stiavelli is affiliated with the Space Telescope Science Institute in the United States. Their research primarily falls within the field of Physics and Astronomy, with a specialized focus on Astronomy and Astrophysics, Instrumentation, Computational Mechanics, Nuclear and High Energy Physics, as well as Control and Systems Engineering.

The main topics covered by their work include:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Gamma-ray bursts and supernovae
  • Stellar, planetary, and galactic studies
  • Astrophysics and Star Formation Studies
  • Astrophysical Phenomena and Observations
  • Astronomical Observations and Instrumentation

Stiavelli has published extensively in several scientific venues. The most frequent publication venues are:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • The Astrophysical Journal Letters
  • Astronomy and Astrophysics
  • Journal of Astronomical Telescopes Instruments and Systems

Their recent papers include the following:

  • "Enhanced Subkiloparsec-scale Star Formation: Results from a JWST Size Analysis of 341 Galaxies at 5 < z < 14" (2024), The Astrophysical Journal
  • "Physical Characterization of Early Galaxies in the Webb's First Deep Field SMACS J0723.3-7327" (2023), The Astrophysical Journal Letters
  • "The Puzzling Properties of the MACS1149-JD1 Galaxy at z = 9.11" (2023), The Astrophysical Journal Letters
  • "Diverse Oxygen Abundance in Early Galaxies Unveiled by Auroral Line Analysis with JWST" (2024), The Astrophysical Journal
  • "Uncovering a Massive z ∼ 7.7 Galaxy Hosting a Heavily Obscured Radio-loud Active Galactic Nucleus Candidate in COSMOS-Web" (2024), The Astrophysical Journal Letters

Stiavelli collaborates frequently with a number of researchers, including:

  • Takahiro Morishita
  • Tommaso Treu
  • Michele Trenti
  • Guido Roberts-Borsani
  • Nicha Leethochawalit

In 2018, Massimo Stiavelli was recognized as a Fellow of the American Association for the Advancement of Science (AAAS).

Best Publications

  • The Great Observatories Origins Deep Survey: Initial Results From Optical and Near-Infrared Imaging

    M. Giavalisco

  • The James Webb Space Telescope

    Jonathan P. Gardner;John C. Mather;Mark Clampin;Rene Doyon

  • The Great Observatories Origins Deep Survey: Initial results from optical and near-infrared imaging

    M. Giavalisco;H. C. Ferguson;H. C. Ferguson;A. M. Koekemoer;M. Dickinson;M. Dickinson

  • The Hubble Ultra Deep Field

    Steven V. W. Beckwith;Steven V. W. Beckwith;Massimo Stiavelli;Anton M. Koekemoer;John A. R. Caldwell;John A. R. Caldwell

  • 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

  • PASSIVELY EVOLVING EARLY-TYPE GALAXIES AT 1.4 z 2.5 IN THE HUBBLE ULTRA DEEP FIELD

    E. Daddi;A. Renzini;N. Pirzkal;Andrea Cimatti

  • 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 HUBBLE ULTRA DEEP FIELD FROM ULTRA-DEEP WFC3/IR OBSERVATIONS*

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

  • 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

  • Spiral Galaxies with WFPC2. II. The Nuclear Properties of 40 Objects

    C. M. Carollo;M. Stiavelli;M. Stiavelli;J. Mack

  • WFPC2 Observations of the Hubble Deep Field South

    Stefano Casertano;Stefano Casertano;Duília de Mello;Mark Dickinson;Henry C. Ferguson

  • 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

  • The changing Lya optical depth in the range 6<z<9 from MOSFIRE spectroscopy of Y-dropouts

    T. Treu;K. B. Schmidt;M. Trenti;L. D. Bradley

  • THE SPECTRAL ENERGY DISTRIBUTIONS OF z ∼ 8 GALAXIES FROM THE IRAC ULTRA DEEP FIELDS: EMISSION LINES, STELLAR MASSES, AND SPECIFIC STAR FORMATION RATES AT 650 MYR*

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

  • The Hubble Ultra Deep Field

    S. V. W. Beckwith;J. Caldwell;M. Clampin;G. de Marchi

Frequent Co-Authors

Michele Trenti
Michele Trenti University of Melbourne
Tommaso Treu
Tommaso Treu University of California, Los Angeles
Rychard Bouwens
Rychard Bouwens Leiden University
Henry C. Ferguson
Henry C. Ferguson Space Telescope Science Institute
Pascal Oesch
Pascal Oesch University of Geneva
Nino Panagia
Nino Panagia Space Telescope Science Institute
Garth D. Illingworth
Garth D. Illingworth University of California, Santa Cruz
Claudia Scarlata
Claudia Scarlata University of Minnesota
C. M. Carollo
C. M. Carollo ETH Zurich
Rogier A. Windhorst
Rogier A. Windhorst Arizona State University

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