World's Best Scientists 2026 revealed!
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Michael T. Murphy

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 82 2869 2725 72 70 368 22077

Michael T. Murphy publications per year

The chart shows the history of publications by Michael T. Murphy between 1985 and 2026, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Michael T. Murphy published across 42 years, from 1985 to 2026, averaging 9.9 papers a year. Output peaked at 33 publications in 2021. 8 of the 417 publications appeared in the last two years.

No. of publications
10 20 30
Bar chart. Horizontal axis: year, 1985 to 2026. Vertical axis: number of publications, 0 to 33. Peak 33 publications in 2021. 1985: 1 publication 1986: 0 publications 1987: 1 publication 1988: 0 publications 1989: 0 publications 1990: 0 publications 1991: 0 publications 1992: 0 publications 1993: 0 publications 1994: 0 publications 1995: 0 publications 1996: 0 publications 1997: 1 publication 1998: 1 publication 1999: 2 publications 2000: 2 publications 2001: 8 publications 2002: 6 publications 2003: 11 publications 2004: 13 publications 2005: 13 publications 2006: 8 publications 2007: 27 publications 2008: 24 publications 2009: 20 publications 2010: 20 publications 2011: 14 publications 2012: 16 publications 2013: 18 publications 2014: 20 publications 2015: 14 publications 2016: 17 publications 2017: 13 publications 2018: 12 publications 2019: 21 publications 2020: 25 publications 2021: 33 publications 2022: 23 publications 2023: 14 publications 2024: 11 publications 2025: 7 publications 2026: 1 publication
1985 2026

417 publications in total across all disciplines

View publications per year as a table
Michael T. Murphy: publications per year, 1985 to 2026
Year Publications
1985 1
1986 0
1987 1
1988 0
1989 0
1990 0
1991 0
1992 0
1993 0
1994 0
1995 0
1996 0
1997 1
1998 1
1999 2
2000 2
2001 8
2002 6
2003 11
2004 13
2005 13
2006 8
2007 27
2008 24
2009 20
2010 20
2011 14
2012 16
2013 18
2014 20
2015 14
2016 17
2017 13
2018 12
2019 21
2020 25
2021 33
2022 23
2023 14
2024 11
2025 7
2026 1
Total 417
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Michael T. Murphy 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 T. Murphy 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, 363–382 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: 368 publications — 31st percentile

31% 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
363–382 156 368
383–402 134
403–422 145
423–442 147
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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Michael T. Murphy 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 T. Murphy 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, 82–83 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: 82 D-Index — 24th percentile

24% 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 82
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
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

Michael T. Murphy is affiliated with Swinburne University of Technology in Australia. Their academic work primarily spans the field of Physics and Astronomy, focusing notably on subfields such as Astronomy and Astrophysics, Instrumentation, Atomic and Molecular Physics and Optics, Nuclear and High Energy Physics, and Computational Mechanics.

Their research interests cover multiple topics including Stellar, planetary, and galactic studies, Astronomy and Astrophysical Research, Galaxies: Formation, Evolution, Phenomena, Astrophysics and Star Formation Studies, Cosmology and Gravitation Theories, Astro and Planetary Science, and Gamma-ray bursts and supernovae.

They have published extensively, contributing to prominent journals and platforms. Frequent publication venues for their work include:

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

Michael T. Murphy has collaborated frequently with several researchers, with notable co-authors including:

  • S. Cristiani
  • C. J. A. P. Martins
  • Tobias M. Schmidt
  • P. Molaro
  • N. J. Nunes

Selected recent papers illustrate the scope of their research interests and contributions:

  • ESPRESSO at VLT (2020), Astronomy and Astrophysics
  • Precision measures of the primordial abundance of deuterium (2024), OPAL (Open@LaTrobe) (La Trobe University)
  • High-precision wavelength calibration of astronomical spectrographs with laser frequency combs (2024), OPAL (Open@LaTrobe) (La Trobe University)
  • Cosmic dynamics in the era of Extremely Large Telescopes (2024), OPAL (Open@LaTrobe) (La Trobe University)
  • MUSE Analysis of Gas around Galaxies (MAGG) - II: metal-enriched halo gas around z ∼ 1 galaxies (2020), Monthly Notices of the Royal Astronomical Society

The range of publications and collaborations indicates involvement in both observational and instrumental aspects of astronomy, including calibration techniques and cosmic structure studies. The scientist's work integrates developments in instrumentation with astrophysical applications, contributing to both fundamental and applied research domains within the broader field of Physics and Astronomy.

Best Publications

  • Further Evidence for Cosmological Evolution of the Fine Structure Constant

    J. K. Webb;M. T. Murphy;V. V. Flambaum;V. A. Dzuba

  • Laser Frequency Combs for Astronomical Observations

    Tilo Steinmetz;Tobias Wilken;Constanza Araujo-Hauck;Ronald Holzwarth

  • Further evidence for a variable fine‐structure constant from Keck/HIRES QSO absorption spectra

    M. T. Murphy;M. T. Murphy;J. K. Webb;Victor V. Flambaum

  • Indications of a Spatial Variation of the Fine Structure Constant

    J. K. Webb;J. A. King;M. T. Murphy;V. V. Flambaum

  • Possible evidence for a variable fine structure constant from QSO absorption lines: Motivations, analysis and results

    M. T. Murphy;J. K. Webb;Victor V. Flambaum;V. A. Dzuba

  • Precision measures of the primordial abundance of deuterium

    Ryan J. Cooke;Max Pettini;Regina A. Jorgenson;Michael T. Murphy

  • High‐precision wavelength calibration of astronomical spectrographs with laser frequency combs

    Michael T. Murphy;Thomas Udem;Ronald Holzwarth;Andreas Sizmann

  • ESPRESSO at VLT - On-sky performance and first results

    F. Pepe;S. Cristiani;R. Rebolo;R. Rebolo;N. C. Santos

  • Deuterium abundance in the most metal-poor damped Lyman alpha system: converging on Ωb,0h2

    Max Pettini;Berkeley J. Zych;Michael T. Murphy;Michael T. Murphy;Antony M. Lewis

  • Deuterium Abundance in the Most Metal-Poor Damped Lyman alpha System: Converging on Omega_baryons

    Max Pettini;Antony Lewis;Berkeley J Zych;Michael T Murphy

  • Cosmic dynamics in the era of Extremely Large Telescopes

    Jochen Liske;Andrea Grazian;Eros Vanzella;Miroslava Dessauges

  • Spatial variation in the fine-structure constant – new results from VLT/UVES

    Julian A. King;John K. Webb;Michael T. Murphy;Victor V. Flambaum

  • Signatures of Cool Gas Fueling a Star-Forming Galaxy at Redshift 2.3

    N. Bouché;N. Bouché;M. T. Murphy;G. G. Kacprzak;C. Péroux

  • New perspectives on strong z ≃ 0.5 Mg II absorbers: Are halo mass and equivalent width anticorrelated?

    Nicolas Bouché;Michael T. Murphy;Céline Péroux;István Csabai

  • New perspectives on strong z=0.5 MgII absorbers: are halo-mass and equivalent width anti-correlated?

    Nicolas Bouche;Michael T. Murphy;Celine Peroux;Istvan Csabai

  • Halo Gas Cross Sections And Covering Fractions of MgII Absorption Selected Galaxies

    G. G. Kacprzak;C. W. Churchill;C. C. Steidel;M. T. Murphy

  • Halo Gas and Galaxy Disk Kinematics Derived from Observations and LCDM Simulations of MgII Absorption Selected Galaxies at Intermediate Redshift

    G. G. Kacprzak;C. W. Churchill;D. Ceverino;C. C. Steidel

  • Strong Limit on a Variable Proton-to-Electron Mass Ratio from Molecules in the Distant Universe

    Michael T. Murphy;Victor V. Flambaum;Sébastien Muller;Christian Henkel

  • The Giant Gemini GMOS survey of zem > 4.4 quasars – I. Measuring the mean free path across cosmic time

    Gábor Worseck;Gábor Worseck;J. Xavier Prochaska;J. Xavier Prochaska;John M. O'Meara;George D. Becker

  • The health of adult Britain 1841-1994.

    Jhon Charlton;Mike Murphy

Frequent Co-Authors

Victor V. Flambaum
Victor V. Flambaum University of New South Wales
Sandro D'Odorico
Sandro D'Odorico European Southern Observatory
Sara L. Ellison
Sara L. Ellison University of Victoria
Luca Pasquini
Luca Pasquini European Southern Observatory
Lex Kaper
Lex Kaper University of Amsterdam
Paolo Molaro
Paolo Molaro National Institute for Astrophysics
Charles C. Steidel
Charles C. Steidel California Institute of Technology
Jochen Liske
Jochen Liske Universität Hamburg
Martin G. Haehnelt
Martin G. Haehnelt University of Cambridge
J. Xavier Prochaska
J. Xavier Prochaska University of California, Santa Cruz

External Links

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Best Scientists Citing Michael T. Murphy

J. Xavier Prochaska

J. Xavier Prochaska

University of California, Santa Cruz

Publications: 112

Pasquier Noterdaeme

Pasquier Noterdaeme

University of Chile

Publications: 100

Raghunathan Srianand

Raghunathan Srianand

Inter-University Centre for Astronomy and Astrophysics

Publications: 94

Patrick Petitjean

Patrick Petitjean

Institut d'Astrophysique de Paris

Publications: 77

Victor V. Flambaum

Victor V. Flambaum

University of New South Wales

Publications: 63

Donald G. York

Donald G. York

University of Chicago

Publications: 63

Scott A. Diddams

Scott A. Diddams

University of Colorado Boulder

Publications: 62

Joseph F. Hennawi

Joseph F. Hennawi

University of California, Santa Barbara

Publications: 58

Sara L. Ellison

Sara L. Ellison

University of Victoria

Publications: 51

Hongzheng Chen

Hongzheng Chen

Zhejiang University

Publications: 50

Adam J. Burgasser

Adam J. Burgasser

University of California, San Diego

Publications: 48

Johan P. U. Fynbo

Johan P. U. Fynbo

University of Copenhagen

Publications: 46

Rafael Rebolo

Rafael Rebolo

Spanish National Research Council

Publications: 45

Ronald Holzwarth

Ronald Holzwarth

Max Planck Society

Publications: 44

Paolo Molaro

Paolo Molaro

National Institute for Astrophysics

Publications: 42

C. Ledoux

C. Ledoux

European Southern Observatory

Publications: 42

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