World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
74
Citations
15952
World Ranking
3490
National Ranking
306

Clive Tadhunter 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 Clive Tadhunter 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: 392 publications — 36th percentile

36% of scientists in this discipline score the same or lower.

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

Clive Tadhunter 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 Clive Tadhunter 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: 74 D-Index — 7th percentile

7% of scientists in this discipline score the same or lower.

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

Overview

Clive Tadhunter is affiliated with the University of Sheffield in the United Kingdom. Their research primarily focuses on the field of Physics and Astronomy, with a strong emphasis on Astronomy and Astrophysics as well as related subfields such as Instrumentation and Nuclear and High Energy Physics. Their work also extends into areas like Computer Vision and Pattern Recognition and Computational Mechanics.

The scientist's research topics broadly cover the formation, evolution, and phenomena of galaxies, as well as astrophysical processes and observations. Specific topics include:

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

Tadhunter has contributed extensively to academic journals, regularly publishing in the following venues:

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

Their recent papers illustrate a focus on quasars, active galactic nuclei (AGN), and galaxy interactions, including:

  • "The diverse cold molecular gas contents, morphologies, and kinematics of type-2 quasars as seen by ALMA" (2021) in Astronomy and Astrophysics
  • "AGN-driven outflows and the AGN feedback efficiency in young radio galaxies" (2020) in Astronomy and Astrophysics
  • "Galaxy interactions are the dominant trigger for local type 2 quasars" (2023) in Monthly Notices of the Royal Astronomical Society
  • "Taking snapshots of the jet-ISM interplay: The case of PKS 0023-26" (2021) in Astronomy and Astrophysics
  • "Multiphase characterization of AGN winds in five local type-2 quasars" (2023) in Astronomy and Astrophysics

Frequent co-authors with whom Clive Tadhunter has collaborated include:

  • R. Morganti
  • C. Ramos Almeida
  • Tom Oosterloo
  • L. R. Holden
  • P. S. Bessiere

Tadhunter's academic output reflects a sustained engagement with observational and theoretical aspects of extragalactic astrophysics, with particular attention to phenomena such as AGN feedback mechanisms and galaxy interaction processes. Their contributions extend to instrumentation techniques supporting these astrophysical explorations.

Best Publications

  • Fast outflows in compact radio sources: evidence for AGN-induced feedback in the early stages of radio source evolution

    J. Holt;C. N. Tadhunter;R. Morganti

  • Fast neutral outflows in powerful radio galaxies : a major source of feedback in massive galaxies

    Raffaella Morganti;Raffaella Morganti;CN Tadhunter;Thomas Oosterloo;Thomas Oosterloo

  • The radio structures of southern 2-Jy radio sources

    R. Morganti;N. E. B. Killeen;C. N. Tadhunter

  • AGN outflows and feedback twenty years on

    C. M. Harrison;T. Costa;C. N. Tadhunter;A. Flütsch

  • The fast molecular outflow in the Seyfert galaxy IC 5063 as seen by ALMA

    Raffaella Morganti;Tom Oosterloo;J. B. Raymond Oonk;J. B. Raymond Oonk;Wilfred Frieswijk

  • Optical spectroscopy of a complete sample of southern 2-Jy radio sources

    C. N. Tadhunter;R. Morganti;S. di Serego Alighieri;R. A. E. Fosbury

  • Anisotropic ionizing radiation in NGC5252

    Clive Tadhunter;Zlatan Tsvetanov

  • The fast molecular outflow in the Seyfert galaxy IC5063 as seen by ALMA

    Raffaella Morganti;Tom Oosterloo;J. B. R. Oonk;Wilfred Frieswijk

  • Jet acceleration of the fast molecular outflows in the Seyfert galaxy IC 5063

    C. Tadhunter;R. Morganti;R. Morganti;M. Rose;J. B. R. Oonk

  • Spectroscopy of the near-nuclear regions of Cygnus A: estimating the mass of the supermassive black hole

    Clive Tadhunter;Alessandro Marconi;David Axon;Karen Wills

  • Emission-line activity in radio galaxies⋆

    A. Robinson;L. Binette;R. A. E. Fosbury;C. N. Tadhunter

  • Radio AGN in the local universe: unification, triggering and evolution

    Clive Tadhunter

  • The co-evolution of the obscured quasar PKS 1549-79 and its host galaxy : evidence for a high accretion rate and warm outflow

    J. Holt;C. Tadhunter;R. Morganti;R. Morganti;M. Bellamy

  • Starbursts and the triggering of the activity in nearby powerful radio galaxies

    C. Tadhunter;T. G. Robinson;R. M. González Delgado;K. Wills

  • The nature of the optical–radio correlations for powerful radio galaxies

    Clive Tadhunter;Raffaella Morganti;Andrew Robinson;Robert Dickson

  • HI absorption in radio galaxies: effect of orientation or interstellar medium?

    R. Morganti;T. A. Oosterloo;C. N. Tadhunter;G. van Moorsel

  • H i absorption in radio galaxies: effect of orientation or interstellar medium?

    R. Morganti;T. A. Oosterloo;C. N. Tadhunter;G. van Moorsel

  • The nebular contribution to the extended UV continua of powerful radio galaxies

    R. Dickson;C. Tadhunter;M. Shaw;N. Clark

  • The origin of the UV excess in powerful radio galaxies: spectroscopy and polarimetry of a complete sample of intermediate‐redshift radio galaxies

    C. Tadhunter;R. Dickson;R. Morganti;T. G. Robinson

  • PKS 2250—41 and the role of jet-cloud interactions in powerful radio galaxies

    M. Villar-Martín;C. Tadhunter;R. Morganti;D. Axon

Frequent Co-Authors

Raffaella Morganti
Raffaella Morganti Netherlands Institute for Radio Astronomy
Tom Oosterloo
Tom Oosterloo Netherlands Institute for Radio Astronomy
David Axon
David Axon University of Sussex
William B. Sparks
William B. Sparks Space Telescope Science Institute
Elaine M. Sadler
Elaine M. Sadler University of Sydney
Christopher P. O'Dea
Christopher P. O'Dea University of Manitoba
Anton M. Koekemoer
Anton M. Koekemoer Space Telescope Science Institute
Stefi A. Baum
Stefi A. Baum University of Manitoba
P. T. O'Brien
P. T. O'Brien University of Leicester
George K. Miley
George K. Miley Leiden University

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