World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
80
Citations
25367
World Ranking
3007
National Ranking
1458

B. Scott Gaudi 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 B. Scott Gaudi 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: 330 publications — 23rd percentile

23% of scientists in this discipline score the same or lower.

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

B. Scott Gaudi 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 B. Scott Gaudi 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: 80 D-Index — 19th percentile

19% of scientists in this discipline score the same or lower.

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

Overview

B. Scott Gaudi is affiliated with The Ohio State University in the United States. Their primary field of study is Physics and Astronomy, with extensive work in related subfields including Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Atomic and Molecular Physics, and Optics, as well as Computational Mechanics.

Their research covers a range of topics, prominently featuring stellar, planetary, and galactic studies. Other significant topics include Astrophysics and Star Formation Studies, Astronomy and Astrophysical Research, Astro and Planetary Science, Gamma-ray bursts and supernovae, Adaptive optics and wavefront sensing, and Astronomical Observations and Instrumentation.

Gaudi has contributed to a number of influential publications. Recent notable papers include:

  • The Habitable Exoplanet Observatory (HabEx) Mission Concept Study Final Report, 2020, arXiv (Cornell University)
  • On the Probability That a Rocky Planet's Composition Reflects Its Host Star, 2021, The Planetary Science Journal
  • Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet, 2021, The Astronomical Journal
  • KELT-9 b's Asymmetric TESS Transit Caused by Rapid Stellar Rotation and Spin-Orbit Misalignment, 2020, The Astronomical Journal
  • Eating Planets for Lunch and Dinner: Signatures of Planet Consumption by Evolving Stars, 2020, The Astrophysical Journal

Their publications frequently appear in several key scientific venues, including:

  • The Astronomical Journal
  • Monthly Notices of the Royal Astronomical Society
  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Astronomy and Astrophysics

Gaudi collaborates regularly with various researchers. Frequent co-authors include:

  • David W. Latham
  • Ji Wang
  • Keivan G. Stassun
  • Yossi Shvartzvald
  • Richard W. Pogge

Best Publications

  • SDSS-III: MASSIVE SPECTROSCOPIC SURVEYS OF THE DISTANT UNIVERSE, THE MILKY WAY, AND EXTRA-SOLAR PLANETARY SYSTEMS

    Daniel J. Eisenstein;Daniel J. Eisenstein;David H. Weinberg;Eric Agol;Hiroaki Aihara

  • Achieving Better Than 1 Minute Accuracy in the Heliocentric and Barycentric Julian Dates

    Jason Eastman;Robert Siverd;B. Scott Gaudi

  • EXOFAST: A Fast Exoplanetary Fitting Suite in IDL

    Jason Eastman;B. Scott Gaudi;Eric Agol

  • Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing

    B. S. Gaudi;D. P. Bennett;A. Udalski;A. Gould

  • Microlens OGLE-2005-BLG-169 Implies Cool Neptune-Like Planets are Common

    A. Gould;A. Udalski;D. An;D. P. Bennett

  • Accurate Empirical Radii and Masses of Planets and Their Host Stars with Gaia Parallaxes

    Keivan G. Stassun;Keivan G. Stassun;Karen A. Collins;Karen A. Collins;B. Scott Gaudi;B. Scott Gaudi

  • KELT-1b: A Strongly Irradiated, Highly Inflated, Short Period, 27 Jupiter-mass Companion Transiting a mid-F Star

    Robert J. Siverd;Thomas G. Beatty;Joshua Pepper;Jason D. Eastman

  • FREQUENCY OF SOLAR-LIKE SYSTEMS AND OF ICE AND GAS GIANTS BEYOND THE SNOW LINE FROM HIGH-MAGNIFICATION MICROLENSING EVENTS IN 2005-2008

    A. Gould;Subo Dong;B. S. Gaudi;A. Udalski

  • Periodic Flux Variability of Stars due to the Reflex Doppler Effect Induced by Planetary Companions

    Abraham Loeb;Abraham Loeb;B. Scott Gaudi

  • A Jovian-Mass Planet in Microlensing Event OGLE-2005-BLG-071

    A. Udalski;M. Jaroszyński;B. Paczyński;M. Kubiak

  • Prospects for the characterization and confirmation of transiting exoplanets via the rossiter-mclaughlin effect

    B. Scott Gaudi;Joshua Nathan Winn

  • OGLE-2003-BLG-262: FINITE-SOURCE EFFECTS FROM A POINT-MASS LENS

    Jaiyul Yoo;D. L. DePoy;A. Gal-Yam;B. S. Gaudi

  • KELT-1b: A STRONGLY IRRADIATED, HIGHLY INFLATED, SHORT PERIOD, 27 JUPITER-MASS COMPANION TRANSITING A MID-F STAR

    Robert J. Siverd;Thomas G. Beatty;Joshua Pepper;Jason D. Eastman;Jason D. Eastman

  • OGLE-2005-BLG-071Lb, THE MOST MASSIVE M DWARF PLANETARY COMPANION?

    Subo Dong;Andrew Gould;Andrzej Udalski;Jay Anderson

  • State of the Field: Extreme Precision Radial Velocities*

    Debra A. Fischer;Guillem Anglada-Escude;Guillem Anglada-Escude;Pamela Arriagada;Roman V. Baluev

  • MOA-2011-BLG-293Lb: A test of pure survey microlensing planet detections

    J. C. Yee;Y. Shvartzvald;A. Gal-Yam;I. A. Bond

  • A COLD NEPTUNE-MASS PLANET OGLE-2007-BLG-368Lb: COLD NEPTUNES ARE COMMON

    T. Sumi;D. P. Bennett;I. A. Bond;A. Udalski

  • FIRST MICROLENS MASS MEASUREMENT: PLANET PHOTOMETRY OF EROS BLG-2000-5

    Jin H. An;M. D. Albrow;M. D. Albrow;J.-P. Beaulieu;J. A. R. Caldwell

  • Predictions of the WFIRST Microlensing Survey. I. Bound Planet Detection Rates

    Matthew T. Penny;B. Scott Gaudi;Eamonn Kerins;Nicholas J. Rattenbury

  • Detection of Rotation in a Binary Microlens: PLANET Photometry of MACHO 97-BLG-41*

    M. D. Albrow;J.-P. Beaulieu;J.-P. Beaulieu;J. A. R. Caldwell;M. Dominik

Frequent Co-Authors

Keivan G. Stassun
Keivan G. Stassun Vanderbilt University
Joshua Pepper
Joshua Pepper Lehigh University
Carlos Allende Prieto
Carlos Allende Prieto University of La Laguna
Richard W. Pogge
Richard W. Pogge The Ohio State University
Leslie Hebb
Leslie Hebb Hobart and William Smith Colleges
Donald P. Schneider
Donald P. Schneider Pennsylvania State University
David W. Latham
David W. Latham Harvard University
Jennifer L. Marshall
Jennifer L. Marshall Texas A&M University
Dmitry Bizyaev
Dmitry Bizyaev New Mexico State University
Lars A. Buchhave
Lars A. Buchhave Technical University of Denmark

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