World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
102
Citations
75055
World Ranking
1517
National Ranking
797

Tod R. Lauer 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 Tod R. Lauer 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.

Tod R. Lauer 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 Tod R. Lauer 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: 102 D-Index — 59th percentile

59% of scientists in this discipline score the same or lower.

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

Overview

Tod R. Lauer is affiliated with the National Science Foundation in the United States and has an extensive research record in physics and astronomy. Their work encompasses a broad range of topics within this field, including stellar, planetary, and galactic studies, as well as detailed investigations into astrophysical phenomena and planetary science exploration.

Their research contributions span multiple specialized subfields such as astronomy and astrophysics, instrumentation, nuclear and high energy physics, atomic and molecular physics and optics, and geophysics. This multidisciplinary approach has enabled a comprehensive understanding of various astronomical and physical systems.

Tod R. Lauer has published numerous papers in prominent scientific venues. These include frequent contributions to arXiv (Cornell University) with 12 papers, The Astrophysical Journal with 11 publications, The Planetary Science Journal with 8, Zenodo (CERN European Organization for Nuclear Research) accounting for 4 papers, and The Astrophysical Journal Letters with 3 publications.

The following recent papers illustrate the scope of their research:

  • New Horizons Observations of the Cosmic Optical Background, 2021, The Astrophysical Journal
  • Anomalous Flux in the Cosmic Optical Background Detected with New Horizons Observations, 2022, The Astrophysical Journal Letters

Other relevant recent research papers associated with their work or closely related areas include:

  • Gravitational Test beyond the First Post-Newtonian Order with the Shadow of the M87 Black Hole, 2020, Physical Review Letters
  • JWST Reveals a Possible z ∼ 11 Galaxy Merger in Triply Lensed MACS0647-JD, 2023, The Astrophysical Journal Letters
  • The Image of the M87 Black Hole Reconstructed with PRIMO, 2023, The Astrophysical Journal Letters

Throughout their career, Tod R. Lauer has collaborated extensively. Frequent coauthors include J. R. Spencer, S. A. Stern, H. A. Weaver, Marc Postman, and K. N. Singer. These collaborations reflect a strong engagement with research teams in planetary science, astrophysics, and observational instrumentation.

Their research topics cover diverse areas including:

  • Stellar, planetary, and galactic studies
  • Astronomy and astrophysical research
  • Astrophysical phenomena and observations
  • Astro and planetary science
  • Planetary science and exploration
  • Galaxies: formation, evolution, phenomena
  • Gamma-ray bursts and supernovae

Best Publications

  • The Demography of Massive Dark Objects in Galaxy Centres

    John Magorrian;Scott Tremaine;Douglas Richstone;Ralf Bender

  • The Demography of massive dark objects in galaxy centers

    John Magorrian;Scott Tremaine;Scott Tremaine;Douglas Richstone;Ralf Bender

  • A Relationship between Nuclear Black Hole Mass and Galaxy Velocity Dispersion

    Karl Gebhardt;Ralf Bender;Gary Bower;Alan Dressler

  • THE SLOPE OF THE BLACK HOLE MASS VERSUS VELOCITY DISPERSION CORRELATION

    Scott Tremaine;Karl Gebhardt;Ralf Bender;Gary Bower

  • First M87 Event Horizon Telescope Results. I. The Shadow of the Supermassive Black Hole

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • The M-σ and M-L Relations in Galactic Bulges, and Determinations of Their Intrinsic Scatter

    Kayhan Gültekin;Douglas D.O. Richstone;Karl Gebhardt;Tod Lauer

  • First M87 Event Horizon Telescope Results. IV. Imaging the Central Supermassive Black Hole

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • The M-sigma and M-L Relations in Galactic Bulges and Determinations of their Intrinsic Scatter

    Kayhan Gultekin;Douglas O. Richstone;Karl Gebhardt;Tod R. Lauer

  • Overview of the DESI Legacy Imaging Surveys.

    Arjun Dey;David J. Schlegel;Dustin Lang;Robert Blum

  • First M87 Event Horizon Telescope Results. VI. The Shadow and Mass of the Central Black Hole

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • First M87 Event Horizon Telescope Results. V. Physical Origin of the Asymmetric Ring

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • The centers of early-type galaxies with HST. IV. Central parameter relations

    S. M. Faber;Scott Tremaine;Edward A. Ajhar;Yong Ik Byun;Yong Ik Byun

  • First M87 Event Horizon Telescope Results. II. Array and Instrumentation

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • First M87 Event Horizon Telescope Results. III. Data Processing and Calibration

    Kazunori Akiyama;Antxon Alberdi;Walter Alef

  • The Centers of Early-Type Galaxies with HST.I.An Observational Survey

    Tod R. Lauer;Edward A. Ajhar;Yong Ik Byun;Alan Dressler

  • The DESI Experiment Part I: Science,Targeting, and Survey Design

    Amir Aghamousa;Jessica Aguilar;Steve Ahlen

  • The DESI Experiment Part I: Science,Targeting, and Survey Design

    Amir Aghamousa;Francisco Prada;Ginevra Favole;Klaus Honscheid

  • Black Hole Mass Estimates from Reverberation Mapping and from Spatially Resolved Kinematics

    Karl Gebhardt;Karl Gebhardt;John Kormendy;Luis C. Ho;Ralf Bender

  • The Centers of Early-Type Galaxies with HST. V. New WFPC2 Photometry

    Tod R. Lauer;S. M. Faber;Karl Gebhardt;Douglas Richstone

  • Overview of the DESI legacy imaging surveys

    Arjun Dey;David J. Schlegel;Dustin Lang;Dustin Lang;Robert Blum

Frequent Co-Authors

Douglas O. Richstone
Douglas O. Richstone University of Michigan–Ann Arbor
Karl Gebhardt
Karl Gebhardt The University of Texas at Austin
John Kormendy
John Kormendy The University of Texas at Austin
Harold A. Weaver
Harold A. Weaver Johns Hopkins University Applied Physics Laboratory
Carl J. Grillmair
Carl J. Grillmair California Institute of Technology
Ross A. Beyer
Ross A. Beyer Ames Research Center
Marc Postman
Marc Postman Space Telescope Science Institute
William B. McKinnon
William B. McKinnon Washington University in St. Louis
Luis C. Ho
Luis C. Ho Peking University
Paul M. Schenk
Paul M. Schenk Lunar and Planetary Institute

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