World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
121
Citations
63986
World Ranking
772
National Ranking
417

Mark Seibert 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 Mark Seibert 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: 423 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.

Mark Seibert 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 Mark Seibert 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: 121 D-Index — 79th percentile

79% of scientists in this discipline score the same or lower.

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

Overview

Mark Seibert is affiliated with the Carnegie Institution for Science in the United States. Their research primarily focuses on the field of Physics and Astronomy, with a substantive body of work spanning Astronomy and Astrophysics, Instrumentation, Artificial Intelligence, Radiological and Ultrasound Technology, and Biomedical Engineering.

The scientist's research topics encompass a range of subjects related to galactic and stellar phenomena. Key areas include galaxies' formation, evolution, and phenomena; stellar, planetary, and galactic studies; astronomy and astrophysical research; astrophysics and star formation studies; gamma-ray bursts and supernovae; astrophysical phenomena and observations; and geochemistry and geologic mapping.

Mark Seibert has published extensively, contributing to a number of notable academic journals and repositories. The frequent publication venues include:

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

The scientist's recent papers demonstrate engagement with large-scale surveys and detailed astrophysical analyses. Significant publications include:

  • "Galaxy And Mass Assembly (GAMA): Data Release 4 and the z < 0.1 total and z < 0.08 morphological galaxy stellar mass functions" (2022), published in Monthly Notices of the Royal Astronomical Society
  • "Metallicity, Ionization Parameter, and Pressure Variations of H ii Regions in the TYPHOON Spiral Galaxies: NGC 1566, NGC 2835, NGC 3521, NGC 5068, NGC 5236, and NGC 7793" (2022), published in The Astrophysical Journal
  • "Metallicity gradient of barred galaxies with TYPHOON" (2022), published in Monthly Notices of the Royal Astronomical Society
  • "A blue ring nebula from a stellar merger several thousand years ago" (2020), published in Nature
  • "The TYPHOON Stellar Population Synthesis Survey. I. The Young Stellar Population of the Great Barred Spiral NGC 1365" (2023), published in The Astrophysical Journal

Collaboration is a notable aspect of Mark Seibert's work, with frequent co-authors including Andrew Battisti, J. Rich, Barry F. Madore, Kathryn Grasha, and Qianhui Chen.

Best Publications

  • The Origin of the Mass--Metallicity Relation: Insights from 53,000 Star-Forming Galaxies in the SDSS

    C. A. Tremonti;T. M. Heckman;G. Kauffmann;J. Brinchmann

  • The Origin of the Mass-Metallicity Relation: Insights from 53,000 Star-forming Galaxies in the Sloan Digital Sky Survey

    Christy A. Tremonti;Christy A. Tremonti;Timothy M. Heckman;Guinevere Kauffmann;Jarle Brinchmann

  • Stellar Masses and Star Formation Histories for 10^5 Galaxies from the Sloan Digital Sky Survey

    Guinevere Kauffmann;Timothy M. Heckman;Simon D.M. White;Stephane Charlot

  • Stellar masses and star formation histories for 105 galaxies from the Sloan Digital Sky Survey

    Guinevere Kauffmann;Timothy M. Heckman;Simon D. M. White;Stéphane Charlot;Stéphane Charlot

  • The Dependence of Star Formation History and Internal Structure on Stellar Mass for 10^5 Low-Redshift Galaxies

    Guinevere Kauffmann;Timothy M. Heckman;Simon D.M. White;Stephane Charlot

  • UV Star Formation Rates in the Local Universe

    Samir Salim;R. Michael Rich;Stéphane Charlot;Jarle Brinchmann

  • The dependence of star formation history and internal structure on stellar mass for 105 low‐redshift galaxies

    Guinevere Kauffmann;Timothy M. Heckman;Simon D. M. White;Stéphane Charlot

  • The calibration and data products of GALEX

    Patrick Morrissey;Tim Conrow;Tom A. Barlow;Todd Small

  • Galaxy and Mass Assembly (GAMA): survey diagnostics and core data release

    S. P. Driver;D. T. Hill;L. S. Kelvin;A. S. G. Robotham

  • The GALEX Ultraviolet Atlas of Nearby Galaxies

    A. Gil de Paz;S. Boissier;B. F. Madore;M. Seibert

  • The GALEX Ultraviolet Atlas of Nearby Galaxies

    Armando Gil De Paz;Armando Gil De Paz;Samuel Boissier;Barry F. Madore;Barry F. Madore;Mark Seibert

  • The spitzer survey of stellar structure in galaxies (s^4g)

    Kartik Sheth;Kartik Sheth;Michael Regan;Joannah L. Hinz;Armando Gil de Paz

  • Galaxy and mass assembly (GAMA): End of survey report and data release 2

    J.. Liske;I.K.. Baldry;S.P.. Driver;S.P.. Driver;R.J.. Tuffs

  • Carnegie Hubble Program: A Mid-Infrared Calibration of the Hubble Constant

    Wendy L. Freedman;Barry F. Madore;Victoria Scowcroft;Chris Burns

  • The Detection of a Population of Submillimeter-Bright, Strongly Lensed Galaxies

    Mattia Negrello;R. Hopwood;G. De Zotti;A. Cooray

  • Dust attenuation in the nearby Universe: comparison between galaxies selected in the ultraviolet or in the infrared

    V. Buat;J. Iglesias-Paramo;M. Seibert;D. Burgarella

  • UV-optical colours as probes of early-type galaxy evolution

    S. Kaviraj;K. Schawinski;J. E. G. Devriendt;I. Ferreras

  • The UV-Optical Galaxy Color-Magnitude Diagram. I. Basic Properties

    Ted K. Wyder;D. Christopher Martin;David Schiminovich;Mark Seibert

  • Disk Accretion onto High-Mass Planets

    S. H. Lubow;M. Seibert;M. Seibert;P. Artymowicz

  • The Carnegie-Chicago Hubble Program. VIII. An Independent Determination of the Hubble Constant Based on the Tip of the Red Giant Branch

    Wendy L. Freedman;Barry F. Madore;Dylan Hatt;Taylor J. Hoyt

Frequent Co-Authors

Barry F. Madore
Barry F. Madore Carnegie Institution for Science
David Schiminovich
David Schiminovich Columbia University
Luciana Bianchi
Luciana Bianchi Johns Hopkins University
Timothy M. Heckman
Timothy M. Heckman Johns Hopkins University
Tom A. Barlow
Tom A. Barlow California Institute of Technology
Alexander S. Szalay
Alexander S. Szalay Johns Hopkins University
Young-Wook Lee
Young-Wook Lee Yonsei University
D. Christopher Martin
D. Christopher Martin California Institute of Technology
R. Michael Rich
R. Michael Rich University of California, Los Angeles
Todd Small
Todd Small California Institute of Technology

If you think any of the details on this page are incorrect, let us know.

Report an issue

We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:

Best Scientists Citing Mark Seibert

Trending Scientists

Recently Published Articles