World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
115
Citations
44267
World Ranking
998
National Ranking
95

Philip Best 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 Philip Best 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: 465 publications — 50th percentile

50% of scientists in this discipline score the same or lower.

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

Philip Best 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 Philip Best 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: 115 D-Index — 74th percentile

74% of scientists in this discipline score the same or lower.

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

Overview

Philip Best is affiliated with the University of Edinburgh in the United Kingdom and has contributed extensively to the field of Physics and Astronomy, with a particular focus on Astronomy and Astrophysics. Their work spans 235 publications within this broad area, including significant involvement in nuclear and high energy physics, instrumentation, computational mechanics, and oceanography as subfields.

The main topics explored in their research include:

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

Philip Best has published in a variety of academic venues, with recurrent appearances in:

  • Monthly Notices of the Royal Astronomical Society
  • arXiv (Cornell University)
  • Astronomy and Astrophysics
  • Springer Link (Chiba Institute of Technology)
  • University of Groningen research database (University of Groningen / Centre for Information Technology)

Some of the recent papers by Philip Best include:

  • The LOFAR Two-metre Sky Survey, 2022, Astronomy and Astrophysics
  • The LOFAR Two-metre Sky Survey: I. Survey description and preliminary data release, 2024, University of Groningen research database (University of Groningen / Centre for Information Technology)
  • The wide-field, multiplexed, spectroscopic facility WEAVE: Survey design, overview, and simulated implementation, 2023, Monthly Notices of the Royal Astronomical Society
  • Coherent radio emission from a quiescent red dwarf indicative of star-planet interaction, 2020, Nature Astronomy
  • The LOFAR Two-meter Sky Survey: Deep Fields Data Release 1, 2020, Astronomy and Astrophysics

Their frequent collaborators include:

  • H. J. A. Röttgering
  • R. Kondapally
  • M. J. Hardcastle
  • I. Prandoni
  • K. J. Duncan

Best Publications

  • LOFAR: The LOw-Frequency ARray

    M. P. van Haarlem;M. W. Wise;M. W. Wise;A. W. Gunst;George Heald

  • The Coevolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe

    Timothy M. Heckman;Philip N. Best

  • The Co-Evolution of Galaxies and Supermassive Black Holes: Insights from Surveys of the Contemporary Universe

    Timothy Heckman;Philip Best

  • The host galaxies of radio-loud AGN: mass dependencies, gas cooling and AGN feedback

    P. N. Best;G. Kauffmann;T. M. Heckman;J. Brinchmann

  • The host galaxies of radio-loud active galactic nuclei: mass dependences, gas cooling and active galactic nuclei feedback

    P. N. Best;G. Kauffmann;T. M. Heckman;J. Brinchmann

  • On the fundamental dichotomy in the local radio-AGN population: accretion, evolution and host galaxy properties

    Philip Best;T. M. Heckman

  • The SCUBA HAlf Degree Extragalactic Survey (SHADES) -- II. Submillimetre maps, catalogue and number counts

    K. Coppin;E.L. Chapin;A.M.J. Mortier;S.E. Scott

  • The SCUBA Half-Degree Extragalactic Survey – II. Submillimetre maps, catalogue and number counts

    K. Coppin;E. L. Chapin;E. L. Chapin;A. M. J. Mortier;S. E. Scott

  • The LOFAR Two-metre Sky Survey - II. First data release

    T. W. Shimwell;T. W. Shimwell;C. Tasse;C. Tasse;M. J. Hardcastle;A. P. Mechev

  • How special are Brightest Group and Cluster Galaxies

    Anja Von Der Linden;Philip N. Best;Guinevere Kauffmann;Simon D. M. White

  • On the prevalence of radio‐loud active galactic nuclei in brightest cluster galaxies: implications for AGN heating of cooling flows

    P. N. Best;A. von der Linden;G. Kauffmann;T. M. Heckman

  • Predicting dust extinction from the stellar mass of a galaxy

    Timothy Garn;Philip N. Best

  • A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS

    David Sobral;Ian Smail;Philip N. Best;James E. Geach

  • The role of black holes in galaxy formation and evolution

    A. Cattaneo;S. M. Faber;J. Binney;A. Dekel

  • A sample of radio-loud active galactic nuclei in the Sloan Digital Sky Survey

    Philip Best;G Kauffmann;T M Heckman;Z Ivezic

  • On the prevalence of radio-loud AGN in brightest cluster galaxies: implications for AGN heating of cooling flows

    P. N. Best;G. Kauffmann;T. M. Heckman;C. R. Kaiser

  • The evolution of the star formation activity in galaxies and its dependence on environment

    B. M. Poggianti;A. von der Linden;G. De Lucia;V. Desai

  • AGN-controlled cooling in elliptical galaxies

    Philip Best;C R Kaiser;T M Heckman;G Kauffmann

  • A deep ALMA image of the Hubble Ultra Deep Field

    James Dunlop;Ross McLure;A. D. Biggs;J. E. Geach

  • The evolution of the star formation activity in galaxies and its dependence on environment

    Bianca M. Poggianti;Anja von der Linden;Gabriella De Lucia;Vandana Desai

Frequent Co-Authors

Heino Falcke
Heino Falcke Radboud University
Matt J. Jarvis
Matt J. Jarvis University of Oxford
Marcus Brüggen
Marcus Brüggen Universität Hamburg
Ian Smail
Ian Smail Durham University
Michael W. Wise
Michael W. Wise Netherlands Institute for Space Research
Mark J. Bentum
Mark J. Bentum Eindhoven University of Technology
Huub Röttgering
Huub Röttgering Leiden University
Martin J. Hardcastle
Martin J. Hardcastle University of Hertfordshire
Annalisa Bonafede
Annalisa Bonafede National Institute for Astrophysics
Glenn J. White
Glenn J. White The Open University

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