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Physics

D-Index
82
Citations
26030
World Ranking
2842
National Ranking
1394

Stacy S. McGaugh 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 Stacy S. McGaugh 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: 299 publications — 17th percentile

17% of scientists in this discipline score the same or lower.

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

Stacy S. McGaugh 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 Stacy S. McGaugh 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: 82 D-Index — 24th percentile

24% of scientists in this discipline score the same or lower.

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

Overview

Stacy S. McGaugh is affiliated with Case Western Reserve University in the United States. Their research primarily focuses on the fields of Physics and Astronomy, with significant contributions to subfields such as Astronomy and Astrophysics, Instrumentation, Atomic and Molecular Physics, Nuclear and High Energy Physics, and Statistical and Nonlinear Physics.

The scientist's main research topics include:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Stellar, planetary, and galactic studies
  • Cosmology and Gravitation Theories
  • Astrophysics and Star Formation Studies
  • Pulsars and Gravitational Waves Research
  • Astronomical Observations and Instrumentation

McGaugh has published extensively, with recent papers including:

  • Predictions and Outcomes for the Dynamics of Rotating Galaxies, 2020, Galaxies
  • Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing, 2024, The Astrophysical Journal Letters
  • Cold gas disks in main-sequence galaxies at cosmic noon: Low turbulence, flat rotation curves, and disk-halo degeneracy, 2023, Astronomy and Astrophysics
  • Tracing the Dynamical Mass in Galaxy Disks Using H i Velocity Dispersion and Its Implications for the Dark Matter Distribution in Galaxies, 2020, The Astrophysical Journal
  • Stellar Mass-to-light Ratios: Composite Bulge+Disk Models and the Baryonic Tully-Fisher Relation, 2022, The Astronomical Journal

Frequent publication venues for Stacy S. McGaugh include:

  • arXiv (Cornell University)
  • Astronomy and Astrophysics
  • The Astrophysical Journal
  • The Astronomical Journal
  • The Astrophysical Journal Letters

The scientist has collaborated extensively with several co-authors, including:

  • James M. Schombert
  • Federico Lelli
  • Pengfei Li
  • Tobias Mistele
  • Marcel S. Pawlowski

Best Publications

  • Modified Newtonian dynamics as an alternative to dark matter

    Robert H. Sanders;Stacy S. McGaugh

  • The Baryonic Tully-Fisher Relation

    Stacy McGaugh;Jim Schombert;Greg Bothun;Erwin de Blok

  • H II region abundances - Model oxygen line ratios

    Stacy S. McGaugh

  • The Baryonic Tully-Fisher Relation.

    S. S. McGaugh;J. M. Schombert;G. D. Bothun;W. J. G. de Blok

  • Modified Newtonian Dynamics (MOND):Observational Phenomenology and Relativistic Extensions

    Benoît Famaey;Benoît Famaey;Stacy S. McGaugh;Stacy S. McGaugh

  • Mass Density Profiles of LSB Galaxies

    W.J.G. de Blok;Stacy S. McGaugh;Albert Bosma;Vera C. Rubin

  • Mass Density Profiles of Low Surface Brightness Galaxies

    W. J. G. de Blok;Stacy S. McGaugh;Albert Bosma;Vera C. Rubin

  • Radial Acceleration Relation in Rotationally Supported Galaxies.

    Stacy S. McGaugh;Federico Lelli;James M. Schombert

  • SPARC: MASS MODELS FOR 175 DISK GALAXIES WITH SPITZER PHOTOMETRY AND ACCURATE ROTATION CURVES

    Federico Lelli;Stacy S. McGaugh;James M. Schombert

  • THE BARYONIC TULLY-FISHER RELATION OF GALAXIES WITH EXTENDED ROTATION CURVES AND THE STELLAR MASS OF ROTATING GALAXIES

    Stacy S. McGaugh

  • The dark and visible matter content of low surface brightness disc galaxies

    W. J. G. de Blok;Stacy S. McGaugh

  • The Baryonic Tully-Fisher Relation of Gas Rich Galaxies as a Test of LCDM and MOND

    Stacy McGaugh

  • High-Resolution Rotation Curves of Low Surface Brightness Galaxies. II. Mass Models

    W. J. G. de Blok;Stacy S. McGaugh;Vera C. Rubin

  • H i observations of low surface brightness galaxies: probing low-density galaxies

    W. J. G. de Blok;S. S. McGaugh;J. M. van der Hulst

  • Mass Models for Low Surface Brightness Galaxies with High-Resolution Optical Velocity Fields

    Rachel Kuzio de Naray;Rachel Kuzio de Naray;Stacy S. McGaugh;W. J. G. de Blok

  • Testing the Dark Matter Hypothesis with Low Surface Brightness Galaxies and Other Evidence

    Stacy McGaugh;Erwin de Blok

  • Testing the dark matter hypothesis with low surface brightness galaxies and other evidence

    Stacy S. McGaugh;Stacy S. McGaugh;W. J. G. de Blok;W. J. G. de Blok

  • One Law To Rule Them All: The Radial Acceleration Relation of Galaxies

    Federico Lelli;Federico Lelli;Stacy S. McGaugh;James M. Schombert;Marcel S. Pawlowski;Marcel S. Pawlowski

  • THE BARYONIC TULLY-FISHER RELATION OF GAS-RICH GALAXIES AS A TEST OF ΛCDM AND MOND

    Stacy S. McGaugh

  • Star formation thresholds in low surface brightness galaxies

    J. M. Van Der Hulst;E. D. Skillman;T. R. Smith;G. D. Bothun

Frequent Co-Authors

Elias Brinks
Elias Brinks University of Hertfordshire
Chris Impey
Chris Impey University of Arizona
Pierre-Alain Duc
Pierre-Alain Duc University of Strasbourg
Pavel Kroupa
Pavel Kroupa University of Bonn
Helmut Jerjen
Helmut Jerjen Australian National University
Rodrigo A. Ibata
Rodrigo A. Ibata University of Strasbourg
David Merritt
David Merritt Rochester Institute of Technology
Sandro D'Odorico
Sandro D'Odorico European Southern Observatory
Edward W. Olszewski
Edward W. Olszewski University of Arizona
Francoise Combes
Francoise Combes Collège de France

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