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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 85 2571 2445 225 216 345 36090

Martin Bureau publications per year

The chart shows the history of publications by Martin Bureau between 1996 and 2026, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Martin Bureau published across 31 years, from 1996 to 2026, averaging 12.3 papers a year. Output peaked at 34 publications in 2012. 19 of the 381 publications appeared in the last two years.

No. of publications
10 20 30
Bar chart. Horizontal axis: year, 1996 to 2026. Vertical axis: number of publications, 0 to 34. Peak 34 publications in 2012. 1996: 2 publications 1997: 3 publications 1998: 3 publications 1999: 8 publications 2000: 6 publications 2001: 13 publications 2002: 16 publications 2003: 5 publications 2004: 16 publications 2005: 7 publications 2006: 19 publications 2007: 18 publications 2008: 10 publications 2009: 13 publications 2010: 14 publications 2011: 33 publications 2012: 34 publications 2013: 25 publications 2014: 11 publications 2015: 11 publications 2016: 10 publications 2017: 8 publications 2018: 9 publications 2019: 17 publications 2020: 13 publications 2021: 9 publications 2022: 8 publications 2023: 14 publications 2024: 7 publications 2025: 11 publications 2026: 8 publications
1996 2026

381 publications in total across all disciplines

View publications per year as a table
Martin Bureau: publications per year, 1996 to 2026
Year Publications
1996 2
1997 3
1998 3
1999 8
2000 6
2001 13
2002 16
2003 5
2004 16
2005 7
2006 19
2007 18
2008 10
2009 13
2010 14
2011 33
2012 34
2013 25
2014 11
2015 11
2016 10
2017 8
2018 9
2019 17
2020 13
2021 9
2022 8
2023 14
2024 7
2025 11
2026 8
Total 381
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Martin Bureau 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 Martin Bureau 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, 343–362 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: 345 publications — 27th percentile

27% 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
343–362 155 345
363–382 156
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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Martin Bureau 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 Martin Bureau 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, 84–85 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: 85 D-Index — 31st percentile

31% 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 85
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

Martin Bureau is affiliated with the University of Oxford in the United Kingdom. Their research primarily focuses on physics and astronomy, with a total of 155 publications in this broad field.

Their subfields of study include:

  • Astronomy and Astrophysics
  • Instrumentation
  • Atomic and Molecular Physics, and Optics
  • Nuclear and High Energy Physics
  • Mechanical Engineering

Martin Bureau's work covers main topics such as:

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

The scientist has published extensively in several venues, with a particular focus on:

  • Monthly Notices of the Royal Astronomical Society (34 publications)
  • arXiv (Cornell University) (14 publications)
  • The Astrophysical Journal (4 publications)
  • The Astrophysical Journal Supplement Series (3 publications)
  • Monthly Notices of the Royal Astronomical Society Letters (1 publication)

Some recent papers authored or co-authored by Martin Bureau include:

  • The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra, 2020, The Astrophysical Journal Supplement Series
  • The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data, 2022, Repository of the Academy's Library (Library of the Hungarian Academy of Sciences)
  • Revealing the intermediate-mass black hole at the heart of the dwarf galaxy NGC 404 with sub-parsec resolution ALMA observations, 2020, Monthly Notices of the Royal Astronomical Society
  • JINGLE - IV. Dust, H i gas, and metal scaling laws in the local Universe, 2020, Monthly Notices of the Royal Astronomical Society
  • WISDOM Project - X. The morphology of the molecular ISM in galaxy centres and its dependence on galaxy structure, 2022, Monthly Notices of the Royal Astronomical Society

Frequent co-authors collaborating with Martin Bureau include:

  • Timothy A. Davis
  • Michele Cappellari
  • Thomas G. Williams
  • Ilaria Ruffa
  • Fu-Heng Liang

Best Publications

  • The SAURON project - IV. The mass-to-light ratio, the virial mass estimator and the Fundamental Plane of elliptical and lenticular galaxies

    M Cappellari;R Bacon;M Bureau;MC Damen

  • The ATLAS3D project – I. A volume-limited sample of 260 nearby early-type galaxies: science goals and selection criteria

    Michele Cappellari;Eric Emsellem;Eric Emsellem;Eric Emsellem;Davor Krajnović;Richard M. Mcdermid

  • The ATLAS3D project – XX. Mass–size and mass–σ distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function

    Michele Cappellari;Richard M. McDermid;Katherine Alatalo;Leo Blitz

  • The SAURON project—V. Integral-field emission-line kinematics of 48 elliptical and lenticular galaxies

    Eric Emsellem;Michele Cappellari;Reynier F. Peletier;Reynier F. Peletier;Richard M. McDermid

  • The SAURON project – IX. A kinematic classification for early‐type galaxies

    Eric Emsellem;Michele Cappellari;Michele Cappellari;Davor Krajnović;Glenn Van De Ven;Glenn Van De Ven

  • Astronomical Society of the Pacific Conference Series

    P. Serra;Raffaella Morganti;Thomas Oosterloo;K. Alatalo

  • The ATLAS3D project – III. A census of the stellar angular momentum within the effective radius of early‐type galaxies: unveiling the distribution of fast and slow rotators

    Eric Emsellem;Eric Emsellem;Michele Cappellari;Davor Krajnović;Katherine Alatalo

  • The SAURON project – I. The panoramic integral-field spectrograph

    Roland Bacon;Yannick Copin;G. Monnet;Bryan W. Miller

  • The SAURON project. II. Sample and early results

    P.T. de Zeeuw;M. Bureau;E. Emsellem;R. Bacon

  • The SAURON project -- X. The orbital anisotropy of elliptical and lenticular galaxies: revisiting the (V/sigma,epsilon) diagram with integral-field stellar kinematics

    M. Cappellari;E. Emsellem;R. Bacon;M. Bureau

  • Systematic variation of the stellar initial mass function in early-type galaxies

    Michele Cappellari;Richard M. McDermid;Katherine Alatalo;Leo Blitz

  • The ATLAS3D project XV: benchmark for early-type galaxies scaling relations from 260 dynamical models: mass-to-light ratio, dark matter, fundamental plane and mass plane

    Michele Cappellari;Nicholas Scott;Nicholas Scott;Katherine Alatalo;Leo Blitz

  • The SAURON project — II. Sample and early results

    P. Tim de Zeeuw;M. Bureau;Eric Emsellem;R. Bacon

  • The 16th Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

    Romina Ahumada;Carlos Allende Prieto;Carlos Allende Prieto;Andrés Almeida;Friedrich Anders;Friedrich Anders

  • The SAURON project – X. The orbital anisotropy of elliptical and lenticular galaxies: revisiting the (V/σ, ɛ) diagram with integral‐field stellar kinematics

    Michele Cappellari;Michele Cappellari;Eric Emsellem;R. Bacon;M. Bureau

  • The SAURON project - III. Integral-field absorption-line kinematics of 48 elliptical and lenticular galaxies

    M. Sarzi;J. Falcon-Barroso;R. L. Davies;R. Bacon

  • The Sixteenth Data Release of the Sloan Digital Sky Surveys: First Release from the APOGEE-2 Southern Survey and Full Release of eBOSS Spectra

    Romina Ahumada;Carlos Allende Prieto;Andres Almeida;Friedrich Anders

  • The Atlas3D project -- XIII. Mass and morphology of HI in early-type galaxies as a function of environment

    Paolo Serra;Tom Oosterloo;Raffaella Morganti;Katherine Alatalo

  • The ATLAS3D project - II. Morphologies, kinemetric features and alignment between photometric and kinematic axes of early-type galaxies

    Davor Krajnović;Eric Emsellem;Eric Emsellem;Michele Cappellari;Katherine Alatalo

  • The ATLAS3D project - VII. A new look at the morphology of nearby galaxies: the kinematic morphology-density relation

    Michele Cappellari;Eric Emsellem;Eric Emsellem;Davor Krajnović;Richard M. McDermid

Frequent Co-Authors

Michele Cappellari
Michele Cappellari University of Oxford
Richard M. McDermid
Richard M. McDermid Macquarie University
Roger L. Davies
Roger L. Davies University of Oxford
Harald Kuntschner
Harald Kuntschner European Southern Observatory
Marc Sarzi
Marc Sarzi Armagh Observatory
Raffaella Morganti
Raffaella Morganti Netherlands Institute for Radio Astronomy
Tom Oosterloo
Tom Oosterloo Netherlands Institute for Radio Astronomy
P. T. de Zeeuw
P. T. de Zeeuw Leiden University
Sadegh Khochfar
Sadegh Khochfar University of Edinburgh
Leo Blitz
Leo Blitz University of California, Berkeley

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