World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
76
Citations
23365
World Ranking
3307
National Ranking
1566

Todd J. Henry 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 Todd J. Henry 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: 424 publications — 42nd percentile

42% of scientists in this discipline score the same or lower.

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

Todd J. Henry 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 Todd J. Henry 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: 76 D-Index — 11th percentile

11% of scientists in this discipline score the same or lower.

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

Overview

Todd J. Henry is affiliated with Georgia State University in the United States and has contributed extensively to the field of Physics and Astronomy. Their research primarily revolves around stellar, planetary, and galactic studies, with a specific focus on astronomy and astrophysical research, astro and planetary science, and astrophysics and star formation studies.

Their scholarly output includes significant papers published across multiple respected venues. Notable recent publications include:

  • The First Habitable-zone Earth-sized Planet from TESS. I. Validation of the TOI-700 System, 2020, DSpace@MIT (Massachusetts Institute of Technology)
  • The Solar Neighborhood XLVIII: Nine Giant Planets Orbiting Nearby K Dwarfs, and the CHIRON Spectrograph's Radial Velocity Performance, 2021, The Astronomical Journal
  • A planet within the debris disk around the pre-main-sequence star AU Microscopii, 2020, Maryland Shared Open Access Repository (USMAI Consortium)
  • A 7 Day Multiwavelength Flare Campaign on AU Mic. I. High-time-resolution Light Curves and the Thermal Empirical Neupert Effect, 2023, The Astrophysical Journal
  • The Solar Neighborhood. XLIX. New Discoveries and Orbits of M-dwarf Multiples with Speckle Interferometry at SOAR, 2022, The Astronomical Journal

The scientist's frequent co-authors include Wei-Chun Jao, Eliot Halley Vrijmoet, Leonardo A. Paredes, Hodari-Sadiki James, and Jennifer G. Winters. Collaborative work with these individuals spans multiple projects and publications.

Todd J. Henry has published extensively in several key venues, notably:

  • The Astronomical Journal
  • arXiv (Cornell University)
  • UNC Libraries
  • The Astrophysical Journal
  • OPAL (Open@LaTrobe) (La Trobe University)

Their research engages with several subfields, including astronomy and astrophysics, instrumentation, atomic and molecular physics and optics, computational mechanics, and general health professions. The topics covered in their work are diverse but show a concentration on:

  • Stellar, planetary, and galactic studies
  • Astronomy and astrophysical research
  • Astro and planetary science
  • Astrophysics and star formation studies
  • Solar and space plasma dynamics
  • Adaptive optics and wavefront sensing
  • Astronomical observations and instrumentation

Best Publications

  • A SURVEY OF STELLAR FAMILIES: MULTIPLICITY OF SOLAR-TYPE STARS

    Deepak Raghavan;Harold A. McAlister;Todd J. Henry;David W. Latham

  • LSST Science Book, Version 2.0

    Paul A. Abell;Julius Allison;Scott F. Anderson

  • Stellar Diameters and Temperatures II. Main Sequence K & M Stars

    Tabetha S. Boyajian;Kaspar von Braun;Gerard van Belle;Harold A. McAlister

  • A Standard Stellar Spectral Sequence in the Red/Near-Infrared: Classes K5 to M9

    J. D. Kirkpatrick;Todd J. Henry;Donald W. McCarthy

  • Stellar Diameters and Temperatures. II. Main-sequence K- and M-stars

    Tabetha S. Boyajian;Kaspar Von Braun;Gerard Van Belle;Harold A. McAlister

  • The mass-luminosity relation for stars of mass 1.0 to 0.08 solar mass

    Todd J. Henry;Todd J. Henry;Donald W. Mccarthy

  • The Solar Neighborhood XVII: Parallax Results from the CTIOPI 0.9m Program -- Twenty New Members of the RECONS 10 Parsec Sample

    Todd J. Henry;Wei-Chun Jao;John P. Subasavage;Thomas D. Beaulieu

  • The Solar Neighborhood. XVII. Parallax Results from the CTIOPI 0.9 m Program: 20 New Members of the RECONS 10 Parsec Sample

    Todd J. Henry;Todd J. Henry;Wei-Chun Jao;Wei-Chun Jao;John P. Subasavage;John P. Subasavage;Thomas D. Beaulieu;Thomas D. Beaulieu

  • A Survey of Ca II H and K Chromospheric Emission in Southern Solar-Type Stars

    Todd J. Henry;David R. Soderblom;Robert A. Donahue;Sallie L. Baliunas

  • The High Angular Resolution Multiplicity of Massive Stars

    Brian D. Mason;William I. Hartkopf;Douglas R. Gies;Todd J. Henry

  • Toward Spectral Classification of L and T Dwarfs: Infrared and Optical Spectroscopy and Analysis

    T. R. Geballe;G. R. Knapp;S. K. Leggett;X. Fan

  • Infrared Photometry of Late-M, L, and T Dwarfs

    S. K. Leggett;David A. Golimowski;Xiaohui Fan;T. R. Geballe

  • A reappraisal of the habitability of planets around M dwarf stars.

    Jill C. Tarter;Peter R. Backus;Rocco L. Mancinelli;Jonathan M. Aurnou

  • A Re-appraisal of the Habitability of Planets Around M Dwarf Stars

    Jill C. Tarter;Peter R. Backus;Rocco L. Mancinelli;Jonathan M. Aurnou

  • The Missing Link: Early Methane ("T") Dwarfs in the Sloan Digital Sky Survey

    S. K. Leggett;T. R. Geballe;Xiaohui Fan

  • The solar neighborhood, 1: Standard spectral types (K5-M8) for northern dwarfs within eight parsecs

    Todd J. Henry;J. Davy Kirkpatrick;Douglas A. Simons

  • The Solar Neighborhood. II. The First List of Dwarfs with Spectral Types of M7 and Cooler

    J. Davy Kirkpatrick;Todd J. Henry;Douglas A. Simons

  • THE SOLAR NEIGHBORHOOD. XXXVII. THE MASS–LUMINOSITY RELATION FOR MAIN-SEQUENCE M DWARFS*

    G. F. Benedict;T. J. Henry;O. G. Franz;B. E. McArthur

  • The optical mass-luminosity relation at the end of the main sequence (0.08-0.20 M⊙)

    Todd J. Henry;Otto G. Franz;Lawrence H. Wasserman;G. Fritz Benedict

  • The missing link: Early methane ("T") dwarfs in the sloan digital Sky Survey

    S. K. Leggett;T. R. Geballe;Xiaohui Fan;Donald P. Schneider

Frequent Co-Authors

Nigel Hambly
Nigel Hambly University of Edinburgh
David R. Ciardi
David R. Ciardi California Institute of Technology
David W. Latham
David W. Latham Harvard University
Stephen R. Kane
Stephen R. Kane University of California, Riverside
T. ten Brummelaar
T. ten Brummelaar Georgia State University
Nils H. Turner
Nils H. Turner Georgia State University
Keivan G. Stassun
Keivan G. Stassun Vanderbilt University
Joshua Pepper
Joshua Pepper Lehigh University
Joshua N. Winn
Joshua N. Winn Princeton University

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