World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
105
Citations
30704
World Ranking
1404
National Ranking
123

C. De Breuck 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 C. De Breuck 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: 536 publications — 61st percentile

61% of scientists in this discipline score the same or lower.

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

C. De Breuck 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 C. De Breuck 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: 105 D-Index — 63rd percentile

63% of scientists in this discipline score the same or lower.

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

Overview

C. De Breuck is affiliated with the European Southern Observatory in Germany. Their research primarily spans the field of Physics and Astronomy, with a focus on Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Atmospheric Science, and Spectroscopy. Their scientific contributions are published extensively across renowned venues, demonstrating engagement with a broad spectrum of astrophysical research.

The scientist's frequent publication venues include:

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

Research topics central to C. De Breuck's work consist of:

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

Frequent collaborators in their research include:

  • M. D. Lehnert
  • J. Vernet
  • Manuel Aravena
  • A. Lundgren
  • M. Béthermin

Selected recent papers authored or co-authored by C. De Breuck are:

  • The Complete Redshift Distribution of Dusty Star-forming Galaxies from the SPT-SZ Survey, 2020, The Astrophysical Journal
  • A massive stellar bulge in a regularly rotating galaxy 1.2 billion years after the Big Bang., 2021, Apollo (University of Cambridge)
  • Quasar feedback survey: multiphase outflows, turbulence, and evidence for feedback caused by low power radio jets inclined into the galaxy disc, 2022, Monthly Notices of the Royal Astronomical Society
  • Megaparsec-scale structure around the protocluster core SPT2349-56 at z = 4.3, 2020, Monthly Notices of the Royal Astronomical Society
  • High molecular gas content and star formation rates in local galaxies that host quasars, outflows, and jets, 2020, Monthly Notices of the Royal Astronomical Society

The body of work by C. De Breuck reflects extensive involvement in studies related to the formation and evolution of galaxies, the behavior and characteristics of star-forming regions, as well as investigations into various astrophysical phenomena through advanced instrumentation and observational techniques.

Best Publications

  • The LABOCA Survey of the Extended Chandra Deep Field South

    A. Weiss;A. Kovacs;K. Coppin;T.R. Greve

  • Distant radio galaxies and their environments

    George Miley;Carlos De Breuck

  • The Large Apex Bolometer Camera Survey of the Extended Chandra Deep Field South

    A. Weiß;A. Kovács;K. Coppin;T. R. Greve

  • Intense star formation within resolved compact regions in a galaxy at z = 2.3

    A.M. Swinbank;I. Smail;S. Longmore;A.I. Harris

  • Protoclusters associated with z > 2 radio galaxies - I. Characteristics of high redshift protoclusters

    B. P. Venemans;H. J. A. Röttgering;G. K. Miley;W. J. M. Van Breugel;W. J. M. Van Breugel

  • The Massive Hosts of Radio Galaxies Across Cosmic Time

    Nick Seymour;Daniel Stern;Carlos De Breuck;Joel Vernet

  • ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies

    A. Weiss;C. De Breuck;D. P. Marrone;J. D. Vieira

  • An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: The Redshift Distribution and Evolution of Submillimeter Galaxies

    James Simpson;Mark Swinbank;Ian Smail;Dave Alexander

  • An ALMA survey of sub-millimetre Galaxies in the Extended Chandra Deep Field South: the far-infrared properties of SMGs

    A. M. Swinbank;J. M. Simpson;Ian Smail;C. M. Harrison

  • Dusty starburst galaxies in the early Universe as revealed by gravitational lensing

    J. D. Vieira;D. P. Marrone;S. C. Chapman;S. C. Chapman;C. De Breuck

  • ALMA redshifts of millimeter-selected galaxies from the SPT survey: The redshift distribution of dusty star-forming galaxies

    A. Weiß;C. De Breuck;D. P. Marrone;J. D. Vieira

  • Evidence for powerful AGN winds at high redshift: dynamics of galactic outflows in radio galaxies during the “Quasar Era”

    N. P. H. Nesvadba;M. D. Lehnert;C. De Breuck;A. M. Gilbert

  • AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: SOURCE CATALOG AND MULTIPLICITY

    J. A. Hodge;A. Karim;I. Smail;A. M. Swinbank

  • An ALMA survey of submillimetre galaxies in the Extended Chandra Deep Field South: high-resolution 870 μm source counts

    A. Karim;A. M. Swinbank;J. A. Hodge;I. R. Smail

  • The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

    M. Pierre;F. Pacaud;C. Adami;S. Alis

  • The Most Distant Structure of Galaxies Known: A Protocluster at z = 4.1*

    B. P. Venemans;J. D. Kurk;G. K. Miley;H. J. A. Röttgering

  • The XXL Survey - I. Scientific motivations − XMM-Newton observing plan − Follow-up observations and simulation programme

    M. Pierre;F. Pacaud;C. Adami;S. Alis;S. Alis

  • Galaxy Clusters around radio-loud AGN at 1.3 < z < 3.2 as seen by Spitzer

    D. Wylezalek;A. Galametz;D. Stern;J. Vernet

  • An ALMA survey of submillimeter galaxies in the Extended Chandra Deep Field South : the redshift distribution and evolution of submillimeter galaxies.

    J. M. Simpson;A. M. Swinbank;Ian Smail;D. M. Alexander

  • Optical and Near-Infrared Imaging of Ultra-Steep-Spectrum Radio Sources: The K-z Diagram of Radio-selected and Optically Selected Galaxies*

    Carlos De Breuck;Wil van Breugel;S. A. Stanford;S. A. Stanford;Huub Röttgering

Frequent Co-Authors

Rob Ivison
Rob Ivison European Southern Observatory
Scott Chapman
Scott Chapman Dalhousie University
Thomas R. Greve
Thomas R. Greve University College London
Achim Weiss
Achim Weiss Max Planck Society
Daniel P. Marrone
Daniel P. Marrone University of Arizona
Karl M. Menten
Karl M. Menten Max Planck Society
Helmut Dannerbauer
Helmut Dannerbauer University of La Laguna
Joaquin Vieira
Joaquin Vieira University of Illinois at Urbana-Champaign
Ian Smail
Ian Smail Durham University
Fabian Walter
Fabian Walter Max Planck Society

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