World's Best Scientists 2026 revealed!

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Physics

D-Index
138
Citations
109497
World Ranking
429
National Ranking
13

Stephane Charlot 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 Stephane Charlot 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: 403 publications — 38th percentile

38% of scientists in this discipline score the same or lower.

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

Stephane Charlot 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 Stephane Charlot 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: 138 D-Index — 88th percentile

88% of scientists in this discipline score the same or lower.

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

Overview

Stephane Charlot is affiliated with the Institut d'Astrophysique de Paris in France. Their research primarily spans the field of Physics and Astronomy, with a strong focus on Astronomy and Astrophysics and related subfields such as Instrumentation, Atomic and Molecular Physics and Optics, Computational Mechanics, and Electrical and Electronic Engineering.

The scientist's main research topics include:

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

Stephane Charlot has a significant publication record, frequently publishing in venues such as:

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

Frequent co-authors of Charlot include:

  • Andrew J. Bunker
  • R. Maiolino
  • Stefano Carniani
  • Chris J. Willott
  • Jacopo Chevallard

The following recent papers highlight some of the research work associated with Charlot's field of interest:

  • "The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope," 2022, published in Astronomy and Astrophysics
  • "Spectroscopic confirmation of four metal-poor galaxies at z = 10.3-13.2," 2023, published in Nature Astronomy
  • "JADES NIRSpec Spectroscopy of GN-z11: Lyman-α emission and possible enhanced nitrogen abundance in a z = 10.60 luminous galaxy," 2023, published in Astronomy and Astrophysics
  • "A small and vigorous black hole in the early Universe," 2024, published in Nature
  • "The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z ∼ 8," 2022, published in Monthly Notices of the Royal Astronomical Society

Best Publications

  • Stellar population synthesis at the resolution of 2003

    G. Bruzual;Stephane Charlot

  • The Host Galaxies of AGN

    Guinevere Kauffmann;Timothy M. Heckman;Christy Tremonti;Jarle Brinchmann

  • The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS

    C. A. Tremonti;T. M. Heckman;G. Kauffmann;J. Brinchmann

  • The host galaxies of active galactic nuclei

    Guinevere Kauffmann;Timothy M. Heckman;Christy Tremonti;Jarle Brinchmann

  • The Origin of the Mass-Metallicity Relation: Insights from 53,000 Star-forming Galaxies in the Sloan Digital Sky Survey

    Christy A. Tremonti;Christy A. Tremonti;Timothy M. Heckman;Guinevere Kauffmann;Jarle Brinchmann

  • The physical properties of star-forming galaxies in the low-redshift universe

    J. Brinchmann;S. Charlot;S. Charlot;S. D. M. White;C. Tremonti;C. Tremonti

  • Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey

    Guinevere Kauffmann;Timothy M. Heckman;Simon D.M. White;Stephane Charlot

  • Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey

    Guinevere Kauffmann;Timothy M. Heckman;Simon D. M. White;Stéphane Charlot;Stéphane Charlot

  • A SIMPLE MODEL FOR THE ABSORPTION OF STARLIGHT BY DUST IN GALAXIES

    Stéphane Charlot;Stéphane Charlot;S. Michael Fall

  • The Dependence of Star Formation History and Internal Structure on Stellar Mass for 10^5 Low-Redshift Galaxies

    Guinevere Kauffmann;Timothy M. Heckman;Simon D.M. White;Stephane Charlot

  • Accurate photometric redshifts for the CFHT legacy survey calibrated using the VIMOS VLT deep survey

    O. Ilbert;O. Ilbert;S. Arnouts;H. J. Mccracken;M. Bolzonella

  • UV Star Formation Rates in the Local Universe

    Samir Salim;R. Michael Rich;Stéphane Charlot;Jarle Brinchmann

  • The dependence of star formation history and internal structure on stellar mass for 105 low‐redshift galaxies

    Guinevere Kauffmann;Timothy M. Heckman;Simon D. M. White;Stéphane Charlot

  • The environmental dependence of the relations between stellar mass, structure, star formation and nuclear activity in galaxies

    Guinevere Kauffmann;Simon D. M. White;Timothy M. Heckman;Brice Ménard

  • GOODS–Herschel: an infrared main sequence for star-forming galaxies

    D. Elbaz;M. Dickinson;H. S. Hwang;T. Díaz-Santos

  • Present-Day Growth of Black Holes and Bulges: the SDSS Perspective

    Timothy M. Heckman;Guinevere Kauffmann;Jarle Brinchmann;Stephane Charlot

  • A simple model to interpret the ultraviolet, optical and infrared emission from galaxies

    Elisabete Da Cunha;Stéphane Charlot;David Elbaz

  • The ages and metallicities of galaxies in the local universe

    Anna Gallazzi;Stéphane Charlot;Jarle Brinchmann;Simon D. M. White

  • The host galaxies of radio-loud AGN: mass dependencies, gas cooling and AGN feedback

    P. N. Best;G. Kauffmann;T. M. Heckman;J. Brinchmann

  • Present-Day Growth of Black Holes and Bulges: The Sloan Digital Sky Survey Perspective

    Timothy M. Heckman;Guinevere Kauffmann;Jarle Brinchmann;Stéphane Charlot

Frequent Co-Authors

H. J. McCracken
H. J. McCracken Institut d'Astrophysique de Paris
A. Cappi
A. Cappi National Institute for Astrophysics
S. Bardelli
S. Bardelli National Institute for Astrophysics
A. Iovino
A. Iovino National Institute for Astrophysics
Lucia Pozzetti
Lucia Pozzetti National Institute for Astrophysics
Christian Marinoni
Christian Marinoni Aix-Marseille University
Paolo Ciliegi
Paolo Ciliegi National Institute for Astrophysics
D. Maccagni
D. Maccagni National Institute for Astrophysics
Elena Zucca
Elena Zucca National Institute for Astrophysics
Luigi Guzzo
Luigi Guzzo University of Milan

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