World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
128
Citations
61043
World Ranking
600
National Ranking
331

Richard W. Pogge 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 Richard W. Pogge 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: 864 publications — 87th percentile

87% of scientists in this discipline score the same or lower.

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

Richard W. Pogge 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 Richard W. Pogge 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: 128 D-Index — 84th percentile

84% 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

  • 2012 - Fellow of the American Association for the Advancement of Science (AAAS)

Overview

Richard W. Pogge is affiliated with The Ohio State University in the United States. Their primary research falls within the broad field of Physics and Astronomy, with a specific focus on Astronomy and Astrophysics, Instrumentation, Atomic and Molecular Physics and Optics, Computational Mechanics, and Nuclear and High Energy Physics.

Their research covers multiple topics, including stellar, planetary, and galactic studies, astronomy and astrophysical research, gamma-ray bursts and supernovae, astrophysics and star formation studies, galaxies in terms of formation, evolution, and phenomena, astro and planetary science, and adaptive optics and wavefront sensing.

Frequent coauthors collaborating with Richard W. Pogge include:

  • Jennifer C. Yee
  • Yossi Shvartzvald
  • Andrew Gould
  • Michael D. Albrow
  • Cheongho Han

The scientist has published extensively in notable venues. The most frequent publication platforms include:

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

Among recent scholarly papers authored or coauthored by Richard W. Pogge are:

  • The COS Legacy Archive Spectroscopy Survey (CLASSY) Treasury Atlas, 2022, The Astrophysical Journal Supplement Series
  • Improving helium abundance determinations with Leo P as a case study, 2021, Journal of Cosmology and Astroparticle Physics
  • To TDE or not to TDE: the luminous transient ASASSN-18jd with TDE-like and AGN-like qualities, 2020, Monthly Notices of the Royal Astronomical Society
  • Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet, 2021, The Astronomical Journal
  • (Title not provided), 2022, Warwick Research Archive Portal (University of Warwick)

They have also contributed to book publications, including the title Interstellar and Intergalactic Medium published in 2021 by Cambridge University Press.

Richard W. Pogge was recognized with the designation of Fellow of the American Association for the Advancement of Science (AAAS) in 2012.

Best Publications

  • CENTRAL MASSES AND BROAD-LINE REGION SIZES OF ACTIVE GALACTIC NUCLEI. II. A HOMOGENEOUS ANALYSIS OF A LARGE REVERBERATION-MAPPING DATABASE

    Bradley M Peterson;Laura Ferrarese;K M Gilbert;K M Gilbert;S Kaspi;S Kaspi

  • The Man Behind the Curtain: X-rays Drive the UV through NIR Variability in the 2013 AGN Outburst in NGC 2617

    B. J. Shappee;J. L. Prieto;D. Grupe;C. S. Kochanek

  • THE MAN BEHIND THE CURTAIN: X-RAYS DRIVE THE UV THROUGH NIR VARIABILITY IN THE 2013 ACTIVE GALACTIC NUCLEUS OUTBURST IN NGC 2617

    B. J. Shappee;J. L. Prieto;D. Grupe;C. S. Kochanek

  • The spectra of narrow-line Seyfert 1 galaxies.

    D. E. Osterbrock;R. W. Pogge

  • Supermassive Black Holes in Active Galactic Nuclei. II. Calibration of the M-sigma Relationship for AGNs

    Christopher A. Onken;Laura Ferrarese;David Merritt;Bradley M. Peterson

  • The Low-luminosity End of the Radius-Luminosity Relationship for Active Galactic Nuclei

    Misty C. Bentz;Kelly D. Denney;Catherine J. Grier;Aaron J. Barth

  • Supermassive black holes in active galactic nuclei. II. Calibration of the black hole mass-velocity dispersion relationship for active galactic nuclei

    Christopher A. Onken;Laura Ferrarese;David Merritt;David Merritt;Bradley M. Peterson

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

    Amir Aghamousa;Jessica Aguilar;Steve Ahlen

  • The Radius-Luminosity Relationship For Active Galactic Nuclei: The Effect of Host-Galaxy Starlight On Luminosity Measurements. II. The Full Sample of Reverberation-Mapped AGNs

    Misty C. Bentz;Misty C. Bentz;Bradley M. Peterson;Hagai Netzer;Richard W. Pogge

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

    Amir Aghamousa;Francisco Prada;Ginevra Favole;Klaus Honscheid

  • The Frequency of Barred Spiral Galaxies in the Near-IR

    Paul B. Eskridge;Jay A. Frogel;Richard W. Pogge;Alice C. Quillen

  • The Frequency of Barred Spiral Galaxies in the Near-Infrared*

    Paul B. Eskridge;Jay A. Frogel;Richard W. Pogge;Alice C. Quillen

  • Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing

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

  • OGLE-2003-BLG-262: Finite-Source Effects from a Point-Mass Lens

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

  • The Radius-Luminosity Relationship for Active Galactic Nuclei: The Effect of Host-Galaxy Starlight on Luminosity Measurements

    Misty C. Bentz;Bradley M. Peterson;Richard W. Pogge;Marianne Vestergaard

  • Supermassive Black Holes in Active Galactic Nuclei. I. The Consistency of Black Hole Masses in Quiescent and Active Galaxies

    Laura Ferrarese;Laura Ferrarese;Richard W. Pogge;Richard W. Pogge;Bradley M. Peterson;Bradley M. Peterson;David Merritt

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

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

  • Reverberation Mapping Measurements of Black Hole Masses in Six Local Seyfert Galaxies

    K. D. Denney;B. M. Peterson;R. W. Pogge;A. Adair

  • 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

  • The Kilodegree Extremely Little Telescope (KELT): A Small Robotic Telescope for Large‐Area Synoptic Surveys

    Joshua Pepper;Richard W. Pogge;D. L. DePoy;J. L. Marshall

Frequent Co-Authors

Andrew Gould
Andrew Gould The Ohio State University
Andrzej Udalski
Andrzej Udalski University of Warsaw
Michał K. Szymański
Michał K. Szymański University of Warsaw
Igor Soszyński
Igor Soszyński University of Warsaw
David P. Bennett
David P. Bennett Goddard Space Flight Center
Darren L. DePoy
Darren L. DePoy Texas A&M University
Keith Horne
Keith Horne University of St Andrews
Krzysztof Ulaczyk
Krzysztof Ulaczyk University of Warwick
Fumio Abe
Fumio Abe Nagoya University
Yoshitaka Itow
Yoshitaka Itow Nagoya University

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