World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
82
Citations
17372
World Ranking
2885
National Ranking
251

Graham P. Smith 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 Graham P. Smith 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: 236 publications — 7th percentile

7% of scientists in this discipline score the same or lower.

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

Graham P. Smith 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 Graham P. Smith 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: 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.

Research.com Recognitions

  • 2012 - IEEE Fellow For contributions to the advancement of detectors for x-rays, charged particles and thermal neutrons

Overview

Graham P. Smith is affiliated with the University of Birmingham in the United Kingdom and works primarily in the fields of Physics and Astronomy. Their research covers a significant body of work with 86 publications, focusing mainly on Astronomy and Astrophysics as well as related subfields such as Instrumentation, Nuclear and High Energy Physics, Oceanography, and Computational Mechanics.

The scientist's research interests encompass several main topics, including:

  • Gamma-ray bursts and supernovae
  • Pulsars and Gravitational Waves Research
  • Galaxies: Formation, Evolution, Phenomena
  • Astrophysical Phenomena and Observations
  • Astronomy and Astrophysical Research
  • Astrophysics and Cosmic Phenomena
  • Stellar, planetary, and galactic studies

Graham P. Smith has contributed to various publication venues with varying frequencies, including:

  • arXiv (Cornell University) - 12 publications
  • Monthly Notices of the Royal Astronomical Society - 9 publications
  • Philosophical Transactions of the Royal Society A Mathematical Physical and Engineering Sciences - 6 publications
  • Nature Astronomy - 1 publication
  • The Astrophysical Journal Letters - 1 publication

Their recent papers feature collaborations with a range of co-authors and cover diverse astrophysical phenomena. Some notable papers include:

  • "Tight multimessenger constraints on the neutron star equation of state from GW170817 and a forward model for kilonova light-curve synthesis", published in 2021 in Monthly Notices of the Royal Astronomical Society
  • "What does strong gravitational lensing? The mass and redshift distribution of high-magnification lenses", published in 2020 in Monthly Notices of the Royal Astronomical Society
  • "The Birth of a Relativistic Jet Following the Disruption of a Star by a Cosmological Black Hole", published in 2022 in Nature Astronomy
  • "On building a cluster watchlist for identifying strongly lensed supernovae, gravitational waves and kilonovae", published in 2020 in Monthly Notices of the Royal Astronomical Society

Frequent collaborators include Dan Ryczanowski, M. Nicholl, Matteo Bianconi, B. P. Gompertz, and Andrew Robertson, reflecting ongoing research partnerships and contributions across related topics and studies.

Graham P. Smith was recognized as an IEEE Fellow in 2012 for contributions to the advancement of detectors for x-rays, charged particles, and thermal neutrons, indicating expertise in instrumentation and detector technology within their broader research framework.

Best Publications

  • Combining strong and weak gravitational lensing in abell 1689

    Marceau Limousin;Johan Richard;Johan Richard;Eric Jullo;Jean-Paul Kneib

  • LoCuSS: Subaru Weak Lensing Study of 30 Galaxy Clusters

    Nobuhiro Okabe;Nobuhiro Okabe;Masahiro Takada;Keiichi Umetsu;Keiichi Umetsu;Toshifumi Futamase

  • A Wide Field Hubble Space Telescope Study of the Cluster Cl0024+1654 at z=0.4 II: The Cluster Mass Distribution

    Jean-Paul Kneib;Patrick Hudelot;Richard S. Ellis;Tommaso Treu

  • The Dark Matter Distribution in the Central Regions of Galaxy Clusters: Implications for Cold Dark Matter

    David J. Sand;Tommaso Treu;Tommaso Treu;Graham P. Smith;Richard S. Ellis

  • A Hubble Space Telescope lensing survey of X-ray luminous galaxy clusters – IV. Mass, structure and thermodynamics of cluster cores at z = 0.2

    Graham P. Smith;Graham P. Smith;Jean-Paul Kneib;Ian Smail;Pasquale Mazzotta;Pasquale Mazzotta

  • Evolution since z = 1 of the Morphology-Density Relation for Galaxies

    Graham P. Smith;Tommaso Treu;Tommaso Treu;Richard S. Ellis;Sean M. Moran

  • The XXL Survey: I. Scientific motivations - XMM-Newton observing plan - Follow-up observations and simulation programme

    M. Pierre;F. Pacaud;C. Adami;S. Alis

  • A Wide-Field Hubble Space Telescope Study of the Cluster Cl 0024+1654 at z=0.4. II. The Cluster Mass Distribution

    Jean-Paul Kneib;Patrick Hudelot;Richard S. Ellis;Tommaso Treu;Tommaso Treu

  • Evolution Since z=1 of the Morphology-density Relation of Galaxies

    Graham P. Smith;Tommaso Treu;Richard S. Ellis;Sean M. Moran

  • The XXL Survey - I. Scientific motivations − XMM-Newton observing plan − Follow-up observations and simulation programme

    M. Pierre;F. Pacaud;C. Adami;S. Alis;S. Alis

  • LoCuSS: comparison of observed X-ray and lensing galaxy cluster scaling relations with simulations

    Y.-Y. Zhang;A. Finoguenov;H. Böhringer;J.-P. Kneib

  • A Keck Survey for Gravitationally Lensed Lyα Emitters in the Redshift Range 8.5 < z < 10.4: New Constraints on the Contribution of Low-Luminosity Sources to Cosmic Reionization

    Daniel P. Stark;Richard S. Ellis;Johan Richard;Johan Richard;Jean Paul Kneib

  • LoCuSS: Comparison of Observed X-ray and Lensing Galaxy Cluster Scaling Relations with Simulations

    Y.-Y. Zhang;A. Finoguenov;H. Boehringer;J.-P. Kneib

  • LoCuSS: THE SLOW QUENCHING OF STAR FORMATION IN CLUSTER GALAXIES AND THE NEED FOR PRE-PROCESSING

    C. P. Haines;C. P. Haines;C. P. Haines;M. J. Pereira;G. P. Smith;E. Egami

  • LoCuSS: the connection between brightest cluster galaxy activity, gas cooling and dynamical disturbance of X‐ray cluster cores

    Alastair J. R. Sanderson;Alastair C. Edge;Graham P. Smith

  • A Wide-Field Survey of Two z ~ 0.5 Galaxy Clusters: Identifying the Physical Processes Responsible for the Observed Transformation of Spirals into S0s

    Sean M. Moran;Richard S. Ellis;Tommaso Treu;Graham P. Smith

  • A Keck Survey for Gravitationally-Lensed Lyman-alpha Emitters in the Redshift Range 8.5 < z < 10.4: New Constraints on the Contribution of Low Luminosity Sources to Cosmic Reionization

    Daniel P. Stark;Richard S. Ellis;Johan Richard;Jean-Paul Kneib

  • LoCuSS: weak-lensing mass calibration of galaxy clusters

    Nobuhiro Okabe;Nobuhiro Okabe;Graham P. Smith

  • LoCuSS: A COMPARISON OF CLUSTER MASS MEASUREMENTS FROM XMM-NEWTON AND SUBARU—TESTING DEVIATION FROM HYDROSTATIC EQUILIBRIUM AND NON-THERMAL PRESSURE SUPPORT

    Yu Ying Zhang;Nobuhiro Okabe;Nobuhiro Okabe;Alexis Finoguenov;Graham P. Smith

  • The Dark Matter Distribution in the Central Regions of Galaxy Clusters

    David J. Sand;G.P. Smith;R.S. Ellis;T. Treu

Frequent Co-Authors

Jean-Paul Kneib
Jean-Paul Kneib École Polytechnique Fédérale de Lausanne
Ian Smail
Ian Smail Durham University
Eiichi Egami
Eiichi Egami University of Arizona
Richard S. Ellis
Richard S. Ellis University College London
Johan Richard
Johan Richard Lyon Observatory
Alexis Finoguenov
Alexis Finoguenov University of Helsinki
Tommaso Treu
Tommaso Treu University of California, Los Angeles
Harald Ebeling
Harald Ebeling University of Hawaii at Manoa
Alastair C. Edge
Alastair C. Edge Durham University
Rob Ivison
Rob Ivison European Southern Observatory

If you think any of the details on this page are incorrect, let us know.

Report an issue

We appreciate your kind effort to assist us to improve this page, it would be helpful providing us with as much detail as possible in the text box below:

Best Scientists Citing Graham P. Smith

Trending Scientists

Recently Published Articles