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Physics
Netherlands
2022

D-Index & Metrics

Physics

D-Index
110
Citations
43354
World Ranking
1169
National Ranking
24

Tom Oosterloo 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 Tom Oosterloo 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: 613 publications — 70th percentile

70% of scientists in this discipline score the same or lower.

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

Tom Oosterloo 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 Tom Oosterloo 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: 110 D-Index — 69th percentile

69% 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

  • 2022 - Research.com Physics in Netherlands Leader Award

Overview

Tom Oosterloo is affiliated with the Netherlands Institute for Radio Astronomy in the Netherlands. Their research primarily focuses on the domain of Physics and Astronomy, with a significant contribution to subfields including Astronomy and Astrophysics, Nuclear and High Energy Physics, Instrumentation, Computational Mechanics, and Aerospace Engineering.

Their scholarly output encompasses a diverse range of topics, notably:

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

Oosterloo has contributed to various journals and publication venues with notable frequency, including:

  • arXiv (Cornell University)
  • Astronomy and Astrophysics
  • Monthly Notices of the Royal Astronomical Society
  • Springer Link (Chiba Institute of Technology)
  • The Astrophysical Journal

Among the recent papers associated with Oosterloo's research are:

  • "Chromatic periodic activity down to 120 megahertz in a fast radio burst" (2021, Nature)
  • "Robust H i kinematics of gas-rich ultra-diffuse galaxies: hints of a weak-feedback formation scenario" (2020, Monthly Notices of the Royal Astronomical Society)
  • "No need for dark matter: resolved kinematics of the ultra-diffuse galaxy AGC 114905" (2021, arXiv (Cornell University))
  • "Apertif: Phased array feeds for the Westerbork Synthesis Radio Telescope. System overview and performance characteristics" (2022, The Caltech Institute Archives (California Institute of Technology))
  • "The baryonic specific angular momentum of disc galaxies" (2021, Springer Link (Chiba Institute of Technology))

Their frequent co-authors include:

  • R. Morganti
  • Elizabeth A. K. Adams
  • W. J. G. de Blok
  • J. M. van der Hulst
  • Kelley M. Hess

Best Publications

  • The ATLAS3D project – I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria

    Michele Cappellari;Eric Emsellem;Eric Emsellem;Eric Emsellem;Davor Krajnović;Richard M. Mcdermid

  • The ATLAS3D project – XX. Mass–size and mass–σ distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function

    Michele Cappellari;Richard M. McDermid;Katherine Alatalo;Leo Blitz

  • Astronomical Society of the Pacific Conference Series

    P. Serra;Raffaella Morganti;Thomas Oosterloo;K. Alatalo

  • The ATLAS3D project – III. A census of the stellar angular momentum within the effective radius of early‐type galaxies: unveiling the distribution of fast and slow rotators

    Eric Emsellem;Eric Emsellem;Michele Cappellari;Davor Krajnović;Katherine Alatalo

  • The HIPASS Catalogue - I. Data Presentation

    M. J. Meyer;M. A. Zwaan;R. L. Webster;L. Staveley-Smith

  • Cold gas accretion in galaxies

    R. Sancisi;F. Fraternali;T. Oosterloo;J. M. van der Hulst

  • Systematic variation of the stellar initial mass function in early-type galaxies

    Michele Cappellari;Richard M. McDermid;Katherine Alatalo;Leo Blitz

  • The ATLAS3D project XV: benchmark for early-type galaxies scaling relations from 260 dynamical models: mass-to-light ratio, dark matter, fundamental plane and mass plane

    Michele Cappellari;Nicholas Scott;Nicholas Scott;Katherine Alatalo;Leo Blitz

  • The HI Parkes All Sky Survey: southern observations, calibration and robust imaging

    D. G. Barnes;D. G. Barnes;L. Staveley-Smith;W. J. G. De Blok;T. Oosterloo

  • The HIPASS catalogue - I. Data presentation

    Martin J. Meyer;Martin J. Meyer;Martin A. Zwaan;Martin A. Zwaan;Rachel L. Webster;Lister Staveley-Smith

  • Cold gas accretion in galaxies

    Renzo Sancisi;Filippo Fraternali;Tom Oosterloo;Tom Oosterloo;Thijs van der Hulst

  • The 1000 Brightest HIPASS Galaxies: H I Properties

    B. S. Koribalski;L. Staveley-Smith;V. A. Kilborn;V. A. Kilborn;S. D. Ryder

  • The Atlas3D project -- XIII. Mass and morphology of HI in early-type galaxies as a function of environment

    Paolo Serra;Tom Oosterloo;Raffaella Morganti;Katherine Alatalo

  • The ATLAS3D project - II. Morphologies, kinemetric features and alignment between photometric and kinematic axes of early-type galaxies

    Davor Krajnović;Eric Emsellem;Eric Emsellem;Michele Cappellari;Katherine Alatalo

  • The ATLAS3D project - VII. A new look at the morphology of nearby galaxies: the kinematic morphology-density relation

    Michele Cappellari;Eric Emsellem;Eric Emsellem;Davor Krajnović;Richard M. McDermid

  • Discovery of an AGN-Driven Molecular Outflow in the Local Early-Type Galaxy NGC 1266

    Katherine Alatalo;Leo Blitz;Lisa M. Young;Timothy A. Davis

  • Advancing Astrophysics with the Square Kilometre Array (AASKA14)

    Tyler. L. Bourke;Robert Braun;Rob Fender;Federica Govoni

  • The ATLAS3D Project - XXX. Star formation histories and stellar population scaling relations of early-type galaxies

    Richard M. McDermid;Richard M. McDermid;Katherine Alatalo;Leo Blitz;Frédéric Bournaud

  • The ATLAS3D project - XIII. Mass and morphology of H I in early-type galaxies as a function of environment

    Paolo Serra;Tom Oosterloo;Tom Oosterloo;Raffaella Morganti;Raffaella Morganti;Katherine Alatalo

  • The ATLAS3D project – IV. The molecular gas content of early-type galaxies

    Lisa M. Young;Martin Bureau;Timothy A. Davis;Francoise Combes

Frequent Co-Authors

Raffaella Morganti
Raffaella Morganti Netherlands Institute for Radio Astronomy
Clive Tadhunter
Clive Tadhunter University of Sheffield
Richard M. McDermid
Richard M. McDermid Macquarie University
Michele Cappellari
Michele Cappellari University of Oxford
Marc Sarzi
Marc Sarzi Armagh Observatory
Martin Bureau
Martin Bureau University of Oxford
Sadegh Khochfar
Sadegh Khochfar University of Edinburgh
Roger L. Davies
Roger L. Davies University of Oxford
Harald Kuntschner
Harald Kuntschner European Southern Observatory
Pierre-Alain Duc
Pierre-Alain Duc University of Strasbourg

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