World's Best Scientists 2026 revealed!
Martin A.T. Groenewegen

Martin A.T. Groenewegen

D-Index & Metrics

Physics

D-Index
80
Citations
24211
World Ranking
3015
National Ranking
15

Martin A.T. Groenewegen 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 Martin A.T. Groenewegen 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: 465 publications — 50th percentile

50% of scientists in this discipline score the same or lower.

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

Martin A.T. Groenewegen 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 Martin A.T. Groenewegen 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: 80 D-Index — 19th percentile

19% of scientists in this discipline score the same or lower.

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

Overview

Martin A.T. Groenewegen is affiliated with the Royal Observatory of Belgium in Belgium and has contributed extensively to the field of Physics and Astronomy. The primary focus of their work lies in Astronomy and Astrophysics, with significant attention to related subfields such as Instrumentation, Computational Mechanics, Nuclear and High Energy Physics, and Spectroscopy.

Their research spans several topics within the broad area of astrophysical studies. Key topics covered in their publications include:

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

Martin A.T. Groenewegen has authored publications in the following frequent venues:

  • Astronomy and Astrophysics
  • Monthly Notices of the Royal Astronomical Society
  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Zenodo (CERN European Organization for Nuclear Research)

Their recent papers reflect a focus on resolved stellar populations, star formation history, and the properties and spatial structure of the Large Magellanic Cloud. Selected recent publications include:

  • Constraining the thermally pulsing asymptotic giant branch phase with resolved stellar populations in the Large Magellanic Cloud, 2020, Monthly Notices of the Royal Astronomical Society
  • DEATHSTAR: Nearby AGB stars with the Atacama Compact Array, 2020, Astronomy and Astrophysics
  • The VMC survey - XLIII. The spatially resolved star formation history across the Large Magellanic Cloud, 2021, Monthly Notices of the Royal Astronomical Society
  • The VMC survey - XLVIII. Classical cepheids unveil the 3D geometry of the LMC, 2022, Monthly Notices of the Royal Astronomical Society
  • The VMC Survey - XLII. Near-infrared period-luminosity relations for RR Lyrae stars and the structure of the Large Magellanic Cloud, 2021, Monthly Notices of the Royal Astronomical Society

Frequent collaborators of Martin A.T. Groenewegen include:

  • Jacco Th. van Loon
  • Richard de Grijs
  • Maria-Rosa L. Cioni
  • V. D. Ivanov
  • J. M. Oliveira

Best Publications

  • Evolution of asymptotic giant branch stars II. Optical to far-infrared isochrones with improved TP-AGB models

    P. Marigo;L. Girardi;A. Bressan;M. A. T. Groenewegen

  • Theoretical isochrones in several photometric systems I. Johnson-Cousins-Glass, HST/WFPC2, HST/NICMOS, Washington, and ESO Imaging Survey filter sets

    L Girardi;G Bertelli;A Bressan;C Chiosi

  • The Gaia-ESO Public Spectroscopic Survey

    G. Gilmore;S. Randich;M. Asplund;J. Binney

  • A New Generation of PARSEC-COLIBRI Stellar Isochrones Including the TP-AGB Phase

    Paola Marigo;Léo Girardi;Alessandro Bressan;Philip Rosenfield

  • New theoretical yields of intermediate mass stars

    L.B. van den Hoek;Martin Groenewegen

  • Star counts in the Galaxy - Simulating from very deep to very shallow photometric surveys with the TRILEGAL code

    L Girardi;Martin Groenewegen;E Hatziminaoglou;E Hatziminaoglou;L da Costa

  • The VMC Survey - I. Strategy and First Data

    M.-R.L. Cioni;M.-R.L. Cioni;G. Clementini;L. Girardi;R. Guandalini

  • Theoretical isochrones in several photometric systems

    L. Girardi;G. Bertelli;A. Bressan;C. Chiosi

  • The global gas and dust budget of the Large Magellanic Cloud: AGB stars and supernovae, and the impact on the ISM evolution

    M. Matsuura;M. J. Barlow;A. A. Zijlstra;P. A. Whitelock

  • Revised bolometric corrections and interstellar extinction coefficients for the ACS and WFPC2 photometric systems

    L. Girardi;J. Dalcanton;B. Williams;R. de Jong

  • ESO imaging survey - Deep public survey: Multi-color optical data for the Chandra Deep Field South

    S. Arnouts;B. Vandame;C. Benoist;M. A. T. Groenewegen

  • The influence of chemical composition on the properties of Cepheid stars. II - The iron content ⋆

    M. Romaniello;F. Primas;M. Mottini;S. Pedicelli

  • Stellar populations in the Galactic bulge - Modelling the Galactic bulge with TRILEGAL

    E. Vanhollebeke;M. A. T. Groenewegen;M. A. T. Groenewegen;L. Girardi

  • `Thermal' SiO radio line emission towards M-type AGB stars: a probe of circumstellar dust formation and dynamics

    D. Gonzalez Delgado;H. Olofsson;F. Kerschbaum;F. L. Schoeier

  • Post-AGB stars with hot circumstellar dust: binarity of the low-amplitude pulsators

    Hans Van Winckel;Tom Lloyd Evans;Maryline Briquet;Peter De Cat

  • Near‐infrared photometry of carbon stars★

    Patricia A. Whitelock;Michael W. Feast;Freddy Marang;M. A. T. Groenewegen

  • The winds of O-stars. I - An analysis of the UV line profiles with the SEI method

    M. A. T. Groenewegen;H. J. G. L. M. Lamers

  • A Stubbornly Large Mass of Cold Dust in the Ejecta of Supernova 1987A

    Mikako Matsuura;E. Dwek;M. J. Barlow;B. Babler

  • Luminosities and mass-loss rates of SMC and LMC AGB stars and red supergiants

    M. A. T. Groenewegen;G. C. Sloan;I. Soszyński;E. A. Petersen;E. A. Petersen

  • A purely geometric distance to the binary star Atlas, a member of the Pleiades

    N Zwahlen;P North;Y Debernardi;L Eyer

Frequent Co-Authors

Albert A. Zijlstra
Albert A. Zijlstra University of Manchester
M. J. Barlow
M. J. Barlow University College London
Marcella Marconi
Marcella Marconi National Institute for Astrophysics
Rob Ivison
Rob Ivison European Southern Observatory
Giuseppe Bono
Giuseppe Bono University of Rome Tor Vergata
Walter Kieran Gear
Walter Kieran Gear Cardiff University
José Cernicharo
José Cernicharo Spanish National Research Council
Kenji Bekki
Kenji Bekki University of Western Australia
Léo Girardi
Léo Girardi National Institute for Astrophysics
Alessandro Bressan
Alessandro Bressan International School for Advanced Studies

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