World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
129
Citations
62487
World Ranking
583
National Ranking
18

Thierry Contini 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 Thierry Contini 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: 529 publications — 60th percentile

60% of scientists in this discipline score the same or lower.

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

Thierry Contini 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 Thierry Contini 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: 129 D-Index — 85th percentile

85% of scientists in this discipline score the same or lower.

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

Overview

Thierry Contini is affiliated with the Research Institute in Astrophysics and Planetology in France. Their research primarily falls within the field of Physics and Astronomy, with a focus on Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, General Health Professions, and Atomic and Molecular Physics, and Optics.

The scientist's main research topics include:

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

Thierry Contini has contributed to numerous scholarly publications, including the following recent papers:

  • The MUSE Hubble Ultra Deep Field Survey, 2020, Astronomy and Astrophysics
  • The MUSE Hubble Ultra Deep Field surveys: Data release II, 2022, Astronomy and Astrophysics
  • The star formation burstiness and ionizing efficiency of low-mass galaxies, 2022, Monthly Notices of the Royal Astronomical Society
  • The MUSE Extremely Deep Field: The cosmic web in emission at high redshift, 2021, Astronomy and Astrophysics
  • Possible signatures of a cold-flow disk from muse using a z ~ to 1 galaxy-quasar pair toward SDSS J1422-0001, 2024, OPAL (Open@LaTrobe) (La Trobe University)

Thierry Contini frequently collaborates with several scientists in related fields. Notable frequent co-authors include:

  • N. Bouché
  • Johan Richard
  • Joop Schaye
  • Leindert Boogaard
  • Roland Bacon

The scientist's work appears in a range of publication venues, with multiple contributions to:

  • Astronomy and Astrophysics
  • arXiv (Cornell University)
  • Monthly Notices of the Royal Astronomical Society
  • HAL (Le Centre pour la Communication Scientifique Directe)
  • OPAL (Open@LaTrobe) (La Trobe University)

Best Publications

  • Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

    Y. Peng;S. J. Lilly;K. Kovac;M. Bolzonella

  • Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function

    Ying-jie Peng;Simon J. Lilly;Katarina Kovač;Micol Bolzonella

  • Accurate photometric redshifts for the CFHT Legacy Survey calibrated using the VIMOS VLT Deep Survey

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

  • 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

  • zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field

    S.J. Lilly;O. Le Fevre;A. Renzini;G. Zamorani

  • COSMOS Photometric Redshifts with 30-bands for 2-deg2

    O. Ilbert;P. Capak;M. Salvato;H. Aussel

  • zCOSMOS: A Large VLT/VIMOS Redshift Survey Covering 0 < z < 3 in the COSMOS Field*

    S. J. Lilly;O. Le Fèvre;A. Renzini;G. Zamorani

  • The VIMOS VLT Deep Survey - First epoch VVDS-Deep survey: 11564 spectra with 17.5<=IAB<=24, and the redshift distribution over 0< z <=5

    O. Le Fevre;G. Vettolani;B. Garilli;L. Tresse

  • The MUSE second-generation VLT instrument

    R. Bacon;M. Accardo;L. Adjali;H. Anwand

  • A test of the nature of cosmic acceleration using galaxy redshift distortions

    L. Guzzo;M. Pierleoni;B. Meneux;E. Branchini

  • Combined CO & Dust Scaling Relations of Depletion Time and Molecular Gas Fractions with Cosmic Time, Specific Star Formation Rate and Stellar Mass

    R. Genzel;L.J. Tacconi;D. Lutz;A. Saintonge

  • The zCOSMOS 10k-Bright Spectroscopic Sample

    Simon J. Lilly;Vincent Le Brun;Christian Maier;Vincenzo Mainieri

  • The VIMOS VLT deep survey. First epoch VVDS-deep survey: 11 564 spectra with 17.5 ≤ IAB ≤ 24, and the redshift distribution over 0 ≤ z ≤ 5

    O. Le Fèvre;G. Vettolani;B. Garilli;L. Tresse

  • PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions

    L. J. Tacconi;R. Genzel;A. Saintonge;F. Combes

  • COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS

    R. Genzel;L. J. Tacconi;D. Lutz;A. Saintonge

  • zCOSMOS - 10k-bright spectroscopic sample. The bimodality in the Galaxy Stellar Mass Function: exploring its evolution with redshift

    L. Pozzetti;M. Bolzonella;E. Zucca;G. Zamorani

  • Improved constraints on the expansion rate of the Universe up to z ∼ 1.1 from the spectroscopic evolution of cosmic chronometers

    M. Moresco;A. Cimatti;R. Jimenez;L. Pozzetti

  • The Herschel* PEP/HerMES luminosity function - I. Probing the evolution of PACS selected Galaxies to z ≃ 4

    C. Gruppioni;F. Pozzi;G. Rodighiero;I. Delvecchio

  • 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

  • The VIMOS VLT Deep Survey: Public release of 1599 redshifts to IAB<=24 across the Chandra Deep Field South

    O. Le Fevre;G. Vettolani;S. Paltani;L. Tresse

Frequent Co-Authors

S. Bardelli
S. Bardelli National Institute for Astrophysics
A. Iovino
A. Iovino National Institute for Astrophysics
Elena Zucca
Elena Zucca National Institute for Astrophysics
H. J. McCracken
H. J. McCracken Institut d'Astrophysique de Paris
Lucia Pozzetti
Lucia Pozzetti National Institute for Astrophysics
A. Cappi
A. Cappi National Institute for Astrophysics
D. Maccagni
D. Maccagni National Institute for Astrophysics
Lidia Tasca
Lidia Tasca Aix-Marseille University
Christian Marinoni
Christian Marinoni Aix-Marseille University
Karina Caputi
Karina Caputi University of Groningen

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