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Mark Seibert

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 121 772 730 417 389 423 63986

Mark Seibert publications per year

The chart shows the history of publications by Mark Seibert between 1999 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Mark Seibert published across 27 years, from 1999 to 2025, averaging 16 papers a year. Output peaked at 52 publications in 2007. 5 of the 431 publications appeared in the last two years.

No. of publications
10 20 30 40 50
Bar chart. Horizontal axis: year, 1999 to 2025. Vertical axis: number of publications, 0 to 52. Peak 52 publications in 2007. 1999: 1 publication 2000: 1 publication 2001: 3 publications 2002: 6 publications 2003: 4 publications 2004: 27 publications 2005: 31 publications 2006: 21 publications 2007: 52 publications 2008: 10 publications 2009: 31 publications 2010: 24 publications 2011: 34 publications 2012: 33 publications 2013: 25 publications 2014: 16 publications 2015: 22 publications 2016: 23 publications 2017: 12 publications 2018: 16 publications 2019: 12 publications 2020: 12 publications 2021: 3 publications 2022: 5 publications 2023: 2 publications 2024: 3 publications 2025: 2 publications
1999 2025

431 publications in total across all disciplines

View publications per year as a table
Mark Seibert: publications per year, 1999 to 2025
Year Publications
1999 1
2000 1
2001 3
2002 6
2003 4
2004 27
2005 31
2006 21
2007 52
2008 10
2009 31
2010 24
2011 34
2012 33
2013 25
2014 16
2015 22
2016 23
2017 12
2018 16
2019 12
2020 12
2021 3
2022 5
2023 2
2024 3
2025 2
Total 431
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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.

No. of scientists
50 100 150
Bar chart with 70 bars. Horizontal axis: publications, 103–122 to 1,469+. Vertical axis: number of scientists, 0 to 162. Most scientists, 162, have 323–342 publications. The last bar groups every scientist with 1,469 publications or more. The highlighted bar, 423–442 publications, is where this scientist sits. 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
103–122 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.

View publications distribution as a table
Number of Physics scientists by publication count, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
Publications Scientists This scientist
103–122 7
123–142 10
143–162 31
163–182 35
183–202 53
203–222 81
223–242 85
243–262 112
263–282 114
283–302 126
303–322 136
323–342 162
343–362 155
363–382 156
383–402 134
403–422 145
423–442 147 423
443–462 131
463–482 131
483–502 116
503–522 106
523–542 103
543–562 87
563–582 84
583–602 94
603–622 70
623–642 76
643–662 60
663–682 54
683–702 60
703–722 48
723–742 64
743–762 48
763–782 37
783–802 43
803–822 34
823–842 36
843–862 32
863–882 32
883–902 31
903–922 25
923–942 15
943–962 24
963–982 13
983–1,002 21
1,003–1,022 21
1,023–1,042 16
1,043–1,062 9
1,063–1,082 19
1,083–1,102 11
1,103–1,122 17
1,123–1,142 11
1,143–1,162 7
1,163–1,182 4
1,183–1,202 10
1,203–1,222 8
1,223–1,242 16
1,243–1,262 4
1,263–1,282 10
1,283–1,302 5
1,303–1,322 7
1,323–1,342 4
1,343–1,362 8
1,363–1,382 6
1,383–1,402 7
1,403–1,422 3
1,423–1,442 4
1,443–1,462 4
1,463–1,468 3
1,469+ 100
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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.

No. of scientists
50 100 150
Bar chart with 59 bars. Horizontal axis: D-Index, 70–71 to 185+. Vertical axis: number of scientists, 0 to 167. Most scientists, 167, have 80–81 D-Index. The last bar groups every scientist with 185 D-Index or more. The highlighted bar, 120–121 D-Index, is where this scientist sits. 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
70–71 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.

View D-Index distribution as a table
Number of Physics scientists by D-index, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
D-Index Scientists This scientist
70–71 76
72–73 110
74–75 143
76–77 153
78–79 144
80–81 167
82–83 167
84–85 166
86–87 132
88–89 155
90–91 134
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116
102–103 97
104–105 103
106–107 87
108–109 90
110–111 67
112–113 78
114–115 75
116–117 67
118–119 69
120–121 60 121
122–123 59
124–125 53
126–127 42
128–129 41
130–131 33
132–133 32
134–135 45
136–137 19
138–139 24
140–141 28
142–143 31
144–145 22
146–147 20
148–149 12
150–151 16
152–153 24
154–155 23
156–157 15
158–159 15
160–161 11
162–163 17
164–165 12
166–167 11
168–169 9
170–171 9
172–173 11
174–175 4
176–177 8
178–179 5
180–181 3
182–183 4
184 4
185+ 99
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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

External Links

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Rob Ivison

Rob Ivison

European Southern Observatory

Publications: 326

Simon P. Driver

Simon P. Driver

University of Western Australia

Publications: 279

Anton M. Koekemoer

Anton M. Koekemoer

Space Telescope Science Institute

Publications: 241

Joss Bland-Hawthorn

Joss Bland-Hawthorn

University of Sydney

Publications: 217

Loretta Dunne

Loretta Dunne

Cardiff University

Publications: 199

Maarten Baes

Maarten Baes

Ghent University

Publications: 195

Luca Cortese

Luca Cortese

University of Western Australia

Publications: 189

Sarah Brough

Sarah Brough

University of New South Wales

Publications: 186

Andrew M. Hopkins

Andrew M. Hopkins

Macquarie University

Publications: 176

Asantha Cooray

Asantha Cooray

University of California, Irvine

Publications: 173

Sebastián F. Sánchez

Sebastián F. Sánchez

National Autonomous University of Mexico

Publications: 172

G. de Zotti

G. de Zotti

National Institute for Astrophysics

Publications: 170

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Matt J. Jarvis

University of Oxford

Publications: 165

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Eric F. Bell

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Publications: 165

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Romeel Davé

University of Edinburgh

Publications: 157

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Cardiff University

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