World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
83
Citations
20282
World Ranking
2798
National Ranking
1373

Margaret Meixner 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 Margaret Meixner 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: 488 publications — 54th percentile

54% of scientists in this discipline score the same or lower.

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

Margaret Meixner 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 Margaret Meixner 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: 83 D-Index — 26th percentile

26% 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

  • 2014 - Fellow of the American Association for the Advancement of Science (AAAS)

Overview

Margaret Meixner is affiliated with the Space Telescope Science Institute in the United States. Their research spans various domains within physics and astronomy, with a focus on subfields such as astronomy and astrophysics, instrumentation, aerospace engineering, molecular biology, and atomic and molecular physics and optics.

Their work covers a range of main topics including stellar, planetary, and galactic studies; astrophysics and star formation studies; astronomy and astrophysical research; gamma-ray bursts and supernovae; astrophysical phenomena and observations; astro and planetary science; and galaxies relating to formation, evolution, and phenomena.

Meixner has published extensively, contributing to venues such as The Astrophysical Journal, arXiv (Cornell University), Journal of Astronomical Telescopes Instruments and Systems, Monthly Notices of the Royal Astronomical Society, and Astronomy and Astrophysics.

Recent papers authored or co-authored by Meixner include:

  • The Mid-infrared Instrument for JWST and Its In-flight Performance, 2023, Publications of the Astronomical Society of the Pacific
  • The Core Human Microbiome: Does It Exist and How Can We Find It? A Critical Review of the Concept, 2022, Nutrients
  • Capillary electrophoresis-mass spectrometry for the direct analysis of glyphosate: method development and application to beer beverages and environmental studies, 2020, Analytical and Bioanalytical Chemistry
  • The CO-dark molecular gas mass in 30 Doradus, 2020, Monthly Notices of the Royal Astronomical Society
  • METAL: The Metal Evolution, Transport, and Abundance in the Large Magellanic Cloud Hubble Program. II. Variations of Interstellar Depletions and Dust-to-gas Ratio within the LMC, 2021, The Astrophysical Journal

Frequent co-authors collaborating with Meixner include:

  • Olivia Jones
  • Alec S. Hirschauer
  • Omnarayani Nayak
  • Nolan Habel
  • Laura Lenkić

Meixner's work falls predominantly within the fields of physics and astronomy, with a significant number of publications (157) contributing to these fields. The scientist's research output demonstrates involvement in both interdisciplinary and specialized areas, such as instrumentation and molecular biology, reflecting a diverse approach to scientific inquiry.

Among awards received, Meixner was named a Fellow of the American Association for the Advancement of Science (AAAS) in 2014.

Best Publications

  • Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE) I: Overview and Initial Results

    Margaret Meixner;Karl D. Gordon;Remy Indebetouw;Joseph L. Hora

  • Spitzer Survey of the Large Magellanic Cloud: Surveying the Agents of a Galaxy's Evolution (SAGE). I. Overview and Initial Results

    Margaret Meixner;Karl D. Gordon;Remy Indebetouw;Joseph L. Hora

  • Herschel Detects a Massive Dust Reservoir in Supernova 1987A

    M. Matsuura;E. Dwek;M. Meixner;M. Otsuka

  • Surveying the Agents of Galaxy Evolution in the Tidally Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). II. Cool Evolved Stars

    Martha L. Boyer;Sundar Srinivasan;Jacco Th. van Loon;Iain McDonald

  • An hst snapshot survey of proto-planetary nebulae candidates: two types of axisymmetric reflection nebulosities

    Toshiya Ueta;Margaret Meixner;Matthew Bobrowsky

  • Surveying the Agents of Galaxy Evolution in the Tidally-Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview

    Karl D. Gordon;Margaret Meixner;Marilyn Meade;Barbara A. Whitney

  • Massive-Star Supernovae as Major Dust Factories

    Ben E. K. Sugerman;Barbara Ercolano;M. J. Barlow;A. G. G. M. Tielens

  • 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

  • Non-standard grain properties, dark gas reservoir, and extended submillimeter excess, probed by Herschel in the Large Magellanic Cloud

    F. Galliano;S. Hony;J.-P. Bernard;C. Bot

  • Spitzer SAGE survey of the Large Magellanic Cloud III: star formation and ~1000 new candidate young stellar objects

    B.A. Whitney;M. Sewilo;R. Indebetouw;T.P. Robitaille

  • Anatomy of the Photodissociation Region in the Orion Bar

    A. G. G. M. Tielens;M. M. Meixner;P. P. van der Werf;J. Bregman

  • Spitzer SAGE Survey of the Large Magellanic Cloud. II. Evolved Stars and Infrared Color-Magnitude Diagrams

    R.D. Blum;J.R. Mould;K.A. Olsen;J.A. Frogel

  • Spitzer SAGE Infrared Photometry of Massive Stars in the Large Magellanic Cloud

    A. Z. Bonanos;D. L. Massa;M. Sewilo;D. J. Lennon

  • Dust Production and Particle Acceleration in Supernova 1987A Revealed with ALMA

    R. Indebetouw;R. Indebetouw;M. Matsuura;E.L.I. Dwek;Giovanna Zanardo

  • Dust and Gas in the Magellanic Clouds from the HERITAGE Herschel Key Project. I. Dust Properties and Insights into the Origin of the Submm Excess Emission

    Karl D. Gordon;Julia Roman-Duval;Caroline Bot;Margaret Meixner

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

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

  • Surveying the Agents of Galaxy Evolution in the Tidally Stripped, Low Metallicity Small Magellanic Cloud (SAGE-SMC). I. Overview

    K. D. Gordon;M. Meixner;M. R. Meade;B. Whitney;B. Whitney

  • Spitzer Survey of the Large Magellanic Cloud, Surveying the Agents of a Galaxy's Evolution (SAGE). IV. Dust Properties in the Interstellar Medium

    Jean Philippe Bernard;William T. Reach;Deborah Paradis;Margaret Meixner

  • The HERSCHEL Inventory of The Agents of Galaxy Evolution in the Magellanic Clouds, a Herschel Open Time Key Program

    M. Meixner;M. Meixner;P. Panuzzo;J. Roman-Duval;C. Engelbracht;C. Engelbracht

  • The Mid-Infrared Instrument for the James Webb Space Telescope I: Introduction

    G. H. Rieke;G. S. Wright;T. Boeker;J. Bouwman

Frequent Co-Authors

Remy Indebetouw
Remy Indebetouw National Radio Astronomy Observatory
Joseph L. Hora
Joseph L. Hora Smithsonian Institution
Brian Babler
Brian Babler University of Wisconsin–Madison
William T. Reach
William T. Reach Universities Space Research Association
Akiko Kawamura
Akiko Kawamura National Institutes of Natural Sciences
Charles W. Engelbracht
Charles W. Engelbracht University of Arizona
M. J. Barlow
M. J. Barlow University College London
Toshikazu Onishi
Toshikazu Onishi Osaka Metropolitan University
Barbara A. Whitney
Barbara A. Whitney University of Wisconsin–Madison

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