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Physics
Australia
2023

D-Index & Metrics

Physics

D-Index
122
Citations
57030
World Ranking
754
National Ranking
17

Michael A. Dopita 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 Michael A. Dopita 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: 687 publications — 77th percentile

77% of scientists in this discipline score the same or lower.

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

Michael A. Dopita 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 Michael A. Dopita 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: 122 D-Index — 80th percentile

80% 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

  • 2023 - Research.com Physics in Australia Leader Award
  • 2022 - Research.com Physics in Australia Leader Award

Overview

Michael A. Dopita was affiliated with the Australian National University in Australia. Their academic work focused primarily on the fields of Physics and Astronomy, with a substantial emphasis on Astronomy and Astrophysics.

The main subfields of study in their research included:

  • Astronomy and Astrophysics
  • Instrumentation
  • Statistical and Nonlinear Physics
  • Global and Planetary Change
  • Atomic and Molecular Physics, and Optics

Their research topics covered a range of areas such as:

  • Stellar, planetary, and galactic studies
  • Astrophysics and Star Formation Studies
  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Gamma-ray bursts and supernovae
  • Astrophysical Phenomena and Observations
  • Scientific Research and Discoveries

Dopita contributed to several frequent publication venues throughout their career, including:

  • Monthly Notices of the Royal Astronomical Society
  • UNC Libraries
  • The Astrophysical Journal
  • OPAL (Open@LaTrobe) (La Trobe University)
  • Astronomy and Astrophysics

Their published works included numerous papers, with notable recent publications such as:

  • The survey for ionization in neutral gas galaxies. II. The star formation rate density of the local universe (2024, OPAL (Open@LaTrobe) (La Trobe University))
  • What drives the redshift evolution of strong emission line ratios? (2020, Monthly Notices of the Royal Astronomical Society)
  • On the origin of nitrogen at low metallicity (2021, Monthly Notices of the Royal Astronomical Society)
  • The Black Hole-Galaxy Connection: Interplay between Feedback, Obscuration, and Host Galaxy Substructure (2022, The Astrophysical Journal)
  • Helium and nitrogen enrichment in massive main-sequence stars: mechanisms and implications for the origin of WNL stars (2020, Monthly Notices of the Royal Astronomical Society)

Dopita collaborated frequently with several co-authors during their career, including:

  • Brent Groves
  • Lisa J. Kewley
  • Ralph S. Sutherland
  • L. Binette
  • A.B. Roy

Best Publications

  • Cooling Functions for Low-Density Astrophysical Plasmas

    Ralph S. Sutherland;Michael A. Dopita

  • Theoretical Modeling of Starburst Galaxies

    Lisa Kewley;Michael Dopita;Ralph Sutherland;Charlene Heisler

  • Measurements* of the Cosmological Parameters Ω and Λ from the First Seven Supernovae at z ≥ 0.35

    Saul Perlmutter;Saul Perlmutter;S. Gabi;S. Gabi;G. Goldhaber;G. Goldhaber;Ariel Goobar;Ariel Goobar;Ariel Goobar

  • Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35

    S. Perlmutter;S. Gabi;G. Goldhaber;D. E. Groom

  • Using Strong Lines to Estimate Abundances in Extragalactic HII Regions and Starburst Galaxies

    L. J. Kewley;M. A. Dopita

  • Using Strong Lines to Estimate Abundances in Extragalactic H II Regions and Starburst Galaxies

    Lisa J. Kewley;Michael A. Dopita

  • The MAPPINGS III Library of Fast Radiative Shock Models

    Mark G. Allen;Brent A. Groves;Michael A. Dopita;Ralph S. Sutherland

  • A γ-ray burst at a redshift of z ≈ 8.2

    N. R. Tanvir;D. B. Fox;A. J. Levan;E. Berger

  • Spectral Signatures of Fast Shocks. II. Optical Diagnostic Diagrams

    Michael A. Dopita;Ralph S. Sutherland

  • Abundances of the heavy elements in the Magellanic Clouds. III - Interpretation of results

    Stephen C. Russell;Michael A. Dopita

  • Spectral Signatures of Fast Shocks. I. Low-Density Model Grid

    Michael A. Dopita;Ralph S. Sutherland

  • A Photometric Redshift of z ~ 9.4 for GRB 090429B

    A. Cucchiara;A. Cucchiara;A. Cucchiara;A. J. Levan;D. B. Fox;N. R. Tanvir

  • Optical Classification of Southern Warm Infrared Galaxies

    Lisa Kewley;Charlene Heisler;Michael Dopita;Stuart Lumsden

  • A Photometric Redshift of z ~ 9.4 for GRB 090429B

    A. Cucchiara;A. J. Levan;D. B. Fox;N. R. Tanvir

  • An H I Aperture Synthesis Mosaic of the Large Magellanic Cloud

    Sungeun Kim;Lister Staveley-Smith;Michael A. Dopita;Ken C. Freeman

  • THEORETICAL EVOLUTION OF OPTICAL STRONG LINES ACROSS COSMIC TIME

    Lisa J. Kewley;Lisa J. Kewley;Michael A. Dopita;Michael A. Dopita;Claus Leitherer;Romeel Davé

  • The Hubble Space Telescope Wide Field Camera 3 Early Release Science data: Panchromatic Faint Object Counts for 0.2-2 microns wavelength

    Rogier A. Windhorst;Seth H. Cohen;Nimish P. Hathi;Patrick J. McCarthy

  • New Strong Line Abundance Diagnostics for \HII Regions: Effects of $\kappa$-Distributed Electron Energies and New Atomic Data

    Michael A. Dopita;Ralph S. Sutherland;David C. Nicholls;Lisa J. Kewley

  • Radiative shock-wave theory. II - High-velocity shocks and thermal instabilities

    L. Binette;M. A. Dopita;I. R. Tuohy

  • Evidence for a Non-Uniform Initial Mass Function in the Local Universe

    Gerhardt R. Meurer;O.I. Wong;J.H. Kim;D.J. Hanish

Frequent Co-Authors

Lisa J. Kewley
Lisa J. Kewley Australian National University
Brent Groves
Brent Groves University of Western Australia
Rogier A. Windhorst
Rogier A. Windhorst Arizona State University
Robert W. O'Connell
Robert W. O'Connell University of Virginia
Joseph Silk
Joseph Silk Johns Hopkins University
Howard E. Bond
Howard E. Bond Pennsylvania State University
Alistair R. Walker
Alistair R. Walker National Optical-Infrared Astronomy Research Lab
Daniela Calzetti
Daniela Calzetti University of Massachusetts Amherst
Kenneth C. Freeman
Kenneth C. Freeman Australian National University
Lister Staveley-Smith
Lister Staveley-Smith University of Western Australia

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