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S. S. Meyer

D-Index & Metrics

Physics

D-Index
126
Citations
179142
World Ranking
629
National Ranking
349

S. S. Meyer 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 S. S. Meyer 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: 459 publications — 49th percentile

49% of scientists in this discipline score the same or lower.

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

S. S. Meyer 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 S. S. Meyer 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: 126 D-Index — 83rd percentile

83% of scientists in this discipline score the same or lower.

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

Overview

S. S. Meyer is affiliated with the University of Chicago in the United States, contributing extensively to the field of Physics and Astronomy with a focus on several specialized subfields.

The main areas of their research include:

  • Cosmology and Gravitation Theories
  • Astrophysics and Cosmic Phenomena
  • Dark Matter and Cosmic Phenomena
  • Radio Astronomy Observations and Technology
  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Particle Detector Development and Performance

Their work spans across important subfields such as:

  • Astronomy and Astrophysics
  • Nuclear and High Energy Physics
  • Instrumentation
  • Electrical and Electronic Engineering
  • Orthopedics and Sports Medicine

They have published a significant number of scientific papers, with recent papers including:

  • "The Solar Orbiter EUI instrument: The Extreme Ultraviolet Imager" (2020), Astronomy and Astrophysics
  • "Measurements of the E-mode polarization and temperature-E-mode correlation of the CMB from SPT-3G 2018 data" (2021), Physical review. D/Physical review. D.
  • "The SPTpol Extended Cluster Survey" (2020), The Astrophysical Journal Supplement Series
  • "The POEMMA (Probe of Extreme Multi-Messenger Astrophysics) Observatory" (2020), Institutional Research Information System University of Turin (University of Turin)
  • "Measurements of B-mode polarization of the cosmic microwave background from 500 square degrees of SPTpol data" (2020), Physical review. D/Physical review. D.

Their frequent co-authors are:

  • B. A. Benson
  • L. E. Bleem
  • N. W. Halverson
  • W. L. Holzapfel
  • C. L. Chang

They have published regularly in journals and venues such as:

  • arXiv (Cornell University)
  • Physical review. D/Physical review. D.
  • The Astrophysical Journal
  • The Astrophysical Journal Supplement Series
  • Monthly Notices of the Royal Astronomical Society

In addition to journal articles, S. S. Meyer has authored books published by Berliner Kommentare, including two editions of "BNatSchG" released in 2021 and 2024.

Best Publications

  • First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Determination of cosmological parameters

    D. N. Spergel;L. Verde;H. V. Peiris;E. Komatsu

  • FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION

    Eiichiro Komatsu;J. Dunkley;J. Dunkley;M. R. Nolta;C. L. Bennett

  • SEVEN-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE (WMAP *) OBSERVATIONS: COSMOLOGICAL INTERPRETATION

    Eiichiro Komatsu;K. M. Smith;J. Dunkley;C. L. Bennett

  • Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation

    E. Komatsu;J. Dunkley;M. R. Nolta;C. L. Bennett

  • Wilkinson Microwave Anisotropy Probe (WMAP) three year results: implications for cosmology

    D. N. Spergel;R. Bean;R. Bean;O. Doré;O. Doré;M. R. Nolta;M. R. Nolta

  • Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology

    D. N. Spergel;R. Bean;O. Doré;M. R. Nolta

  • The Microwave Anisotropy Probe* Mission

    C. L. Bennett;M. Bay;M. Halpern;G. Hinshaw

  • First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Preliminary Maps and Basic Results

    C. L. Bennett;M. Halpern;G. Hinshaw;N. Jarosik

  • First year Wilkinson Microwave Anisotropy Probe (WMAP) observations: Preliminary maps and basic results

    C. L. Bennett;M. Halpern;G. Hinshaw;N. Jarosik

  • Nine-year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Parameter Results

    G. Hinshaw;D. Larson;E. Komatsu;David N. Spergel;David N. Spergel

  • Structure in the COBE differential microwave radiometer first year maps

    G. F. Smoot;C. L. Bennett;A. Kogut;E. L. Wright

  • Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data

    J. Dunkley;E. Komatsu;M. R. Nolta;D. N. Spergel

  • Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results

    G. Hinshaw;J. L. Weiland;R. S. Hill;N. Odegard

  • First-Year Wilkinson Microwave Anisotropy Probe (WMAP)* Observations: Foreground Emission

    C. L. Bennett;R. S. Hill;G. Hinshaw;M. R. Nolta

  • Nine-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Final Maps and Results

    C. L. Bennett;D. Larson;J. L. Weiland;N. Jarosik

  • FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE * OBSERVATIONS: LIKELIHOODS AND PARAMETERS FROM THE WMAP DATA

    J. Dunkley;J. Dunkley;Eiichiro Komatsu;M. R. Nolta;D. N. Spergel

  • Three-year Wilkinson Microwave Anisotropy Probe (WMAP) observations: temperature analysis

    G. Hinshaw;M. R. Nolta;C. L. Bennett;R. Bean

  • Five-Year Wilkinson Microwave Anisotropy Probe Observations: Data Processing, Sky Maps, and Basic Results

    G. Hinshaw;J. L. Weiland;R. S. Hill;N. Odegard

  • Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Power Spectra and WMAP-Derived Parameters

    D. Larson;J. Dunkley;G. Hinshaw;Eiichiro Komatsu

  • Three Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Polarization Analysis

    L. Page;G. Hinshaw;E. Komatsu;M. R. Nolta

Frequent Co-Authors

Adrian T. Lee
Adrian T. Lee University of California, Berkeley
C. L. Chang
C. L. Chang Argonne National Laboratory
John E. Carlstrom
John E. Carlstrom University of Chicago
Matt Dobbs
Matt Dobbs McGill University
Joaquin Vieira
Joaquin Vieira University of Illinois at Urbana-Champaign
N. W. Halverson
N. W. Halverson University of Colorado Boulder
Jeff McMahon
Jeff McMahon University of Chicago
W. L. Holzapfel
W. L. Holzapfel University of California, Berkeley
Christian L. Reichardt
Christian L. Reichardt University of Melbourne
T. M. Crawford
T. M. Crawford University of Chicago

External Links

Personal website of S. S. Meyer

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Best Scientists Citing S. S. Meyer

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European Southern Observatory

Publications: 290

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H. K. Eriksen

H. K. Eriksen

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National Institute for Astrophysics

Publications: 264

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Sapienza University of Rome

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Publications: 256

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