World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
95
Citations
30265
World Ranking
1943
National Ranking
52

Sarah Brough 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 Sarah Brough 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: 364 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.

Sarah Brough 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 Sarah Brough 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: 95 D-Index — 49th percentile

49% of scientists in this discipline score the same or lower.

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

Overview

Sarah Brough is affiliated with the University of New South Wales in Australia. Their research is situated predominantly within the domain of Physics and Astronomy, with a particular focus on Astronomy and Astrophysics, Instrumentation, Computational Mechanics, Atomic and Molecular Physics and Optics, and Nuclear and High Energy Physics.

Their work covers a range of scientific topics, including:

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

Brough has contributed extensively to the literature, with significant publications in major venues such as Monthly Notices of the Royal Astronomical Society, arXiv (Cornell University), The Astrophysical Journal, OPAL (Open@LaTrobe) (La Trobe University), and Astronomy and Astrophysics.

Recent papers authored or co-authored by Brough include:

  • "The WiggleZ Dark Energy Survey: The growth rate of cosmic structure since redshift z=0.9" (2024), published in OPAL (Open@LaTrobe) (La Trobe University)
  • "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
  • "The WiggleZ Dark Energy Survey: Testing the cosmological model with baryon acoustic oscillations at z= 0.6" (2024), published in OPAL (Open@LaTrobe) (La Trobe University)
  • "Measures of galaxy environment - I. What is 'environment'?" (2024), published in OPAL (Open@LaTrobe) (La Trobe University)
  • "The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity" (2024), published in OPAL (Open@LaTrobe) (La Trobe University)

Brough frequently collaborates with several co-authors, including:

  • S. M. Croom
  • Joss Bland-Hawthorn
  • Jesse van de Sande
  • Julia J. Bryant
  • M. S. Owers

Best Publications

  • 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 WiggleZ Dark Energy Survey: mapping the distance-redshift relation with baryon acoustic oscillations

    Chris Blake;Eyal A. Kazin;Florian Beutler;Tamara M. Davis;Tamara M. Davis

  • The WiggleZ Dark Energy Survey: joint measurements of the expansion and growth history at z < 1

    Chris Blake;Sarah Brough;Matthew Colless;Carlos Contreras

  • Galaxy And Mass Assembly: Stellar Mass Estimates

    Edward N Taylor;Andrew M Hopkins;Ivan K Baldry;Michael J I Brown

  • The Sydney-AAO Multi-object Integral field spectrograph

    Scott M. Croom;Jon S. Lawrence;Jon S. Lawrence;Joss Bland-Hawthorn;Julia J. Bryant

  • Galaxy And Mass Assembly (GAMA): stellar mass estimates

    Edward N Taylor;Edward N Taylor;Andrew M Hopkins;Ivan K Baldry;Michael J I Brown

  • 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

  • The WiggleZ Dark Energy Survey: survey design and first data release

    Michael J. Drinkwater;Russell J. Jurek;Chris Blake;David Woods;David Woods

  • Galaxy And Mass Assembly (GAMA): the galaxy stellar mass function at z < 0.06

    Ivan K Baldry;Simon P Driver;Simon P Driver;J Loveday;Edward Taylor;Edward Taylor

  • The WiggleZ Dark Energy Survey: the growth rate of cosmic structure since redshift z=0.9

    Chris Blake;Sarah Brough;Matthew Colless;Carlos Contreras

  • The SAMI Galaxy Survey: Instrument specification and target selection

    J. J. Bryant;J. J. Bryant;M. S. Owers;A. S. G. Robotham;S. M. Croom

  • GAMA: towards a physical understanding of galaxy formation

    Simon P. Driver;Peder Norberg;Ivan K. Baldry;Steven P. Bamford

  • Galaxy and Mass Assembly (GAMA): the GAMA galaxy group catalogue (G3Cv1)

    A Robotham;Peder Norberg;Simon Driver;Simon Driver;Ivan Baldry

  • The WiggleZ Dark Energy Survey: improved distance measurements to z = 1 with reconstruction of the baryonic acoustic feature

    Eyal A. Kazin;Jun Koda;Chris Blake;Nikhil Padmanabhan

  • Galaxy And Mass Assembly (GAMA): Structural Investigation of Galaxies via Model Analysis

    Lee S. Kelvin;Lee S. Kelvin;Simon P. Driver;Simon P. Driver;Aaron S. G. Robotham;Aaron S. G. Robotham;David T. Hill

  • Galaxy And Mass Assembly (GAMA): Structural Investigation of Galaxies via Model Analysis (SIGMA)

    Lee S. Kelvin;Simon P. Driver;Aaron S. G. Robotham;David T. Hill

  • The WiggleZ Dark Energy Survey: Final data release and cosmological results

    David Parkinson;Signe Riemer-Sørensen;Chris Blake;Gregory B. Poole

  • The Sydney-AAO Multi-object Integral field spectrograph (SAMI)

    Scott M. Croom;Jon S. Lawrence;Joss Bland-Hawthorn;Julia J. Bryant

  • GAMA: towards a physical understanding of galaxy formation

    Simon P Driver;Peder Norberg;Ivan K Baldry;Steven P Bamford

  • The WiggleZ Dark Energy Survey: testing the cosmological model with baryon acoustic oscillations at z= 0.6

    Chris Blake;Tamara Davis;Tamara Davis;Gregory B. Poole;David Parkinson

Frequent Co-Authors

Simon P. Driver
Simon P. Driver University of Western Australia
Scott M. Croom
Scott M. Croom University of Sydney
Joss Bland-Hawthorn
Joss Bland-Hawthorn University of Sydney
Andrew M. Hopkins
Andrew M. Hopkins Macquarie University
Rob Sharp
Rob Sharp Australian National University
Matthew Colless
Matthew Colless Australian National University
Kevin A. Pimbblet
Kevin A. Pimbblet University of Hull
Ivan K. Baldry
Ivan K. Baldry Liverpool John Moores University
Jochen Liske
Jochen Liske Universität Hamburg
Peder Norberg
Peder Norberg Durham University

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