World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
92
Citations
32198
World Ranking
2106
National Ranking
45

H. K. C. Yee 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 H. K. C. Yee 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: 429 publications — 43rd percentile

43% of scientists in this discipline score the same or lower.

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

H. K. C. Yee 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 H. K. C. Yee 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: 92 D-Index — 44th percentile

44% 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

  • 2010 - Fellow of the Royal Society of Canada Academy of Science

Overview

H. K. C. Yee is affiliated with the University of Toronto in Canada and specializes in Physics and Astronomy, with a predominant focus on Astronomy and Astrophysics. Their research portfolio spans several subfields including Instrumentation, Nuclear and High Energy Physics, Electrical and Electronic Engineering, and Statistical and Nonlinear Physics.

The scientist's work encompasses a variety of main topics related to galactic and cosmic phenomena. These include:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Stellar, planetary, and galactic studies
  • Astrophysics and Star Formation Studies
  • Cosmology and Gravitation Theories
  • Astrophysics and Cosmic Phenomena
  • Gamma-ray bursts and supernovae

Yee has contributed to numerous publications, with a frequent presence in qualified scientific venues. The most common venues include:

  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal
  • arXiv (Cornell University)
  • OPAL (Open@LaTrobe) (La Trobe University)
  • Springer Link (Chiba Institute of Technology)

Collaborations with other researchers have been an integral part of their work. Frequent co-authors include:

  • Adam Muzzin
  • Gillian Wilson
  • Gregory Rudnick
  • R. Demarco
  • Allison Noble

The following is a selection of recent papers contributed to by H. K. C. Yee, reflecting the range and scope of their research interests:

  • The WiggleZ Dark Energy Survey: The growth rate of cosmic structure since redshift z=0.9, 2024, OPAL (Open@LaTrobe) (La Trobe University)
  • The WiggleZ Dark Energy Survey: Testing the cosmological model with baryon acoustic oscillations at z= 0.6, 2024, OPAL (Open@LaTrobe) (La Trobe University)
  • The WiggleZ Dark Energy Survey: the transition to large-scale cosmic homogeneity, 2024, OPAL (Open@LaTrobe) (La Trobe University)
  • The WiggleZ Dark Energy Survey: high-resolution kinematics of luminous star-forming galaxies, 2024, OPAL (Open@LaTrobe) (La Trobe University)
  • The GOGREEN survey: the environmental dependence of the star-forming galaxy main sequence at 1.0 < z < 1.5, 2020, Monthly Notices of the Royal Astronomical Society

Recognition for contributions in their field includes being named a Fellow of the Royal Society of Canada in 2010 within the Academy of Science.

Best Publications

  • The Hubble Space Telescope Cluster Supernova Survey. V. Improving the Dark-energy Constraints above z > 1 and Building an Early-type-hosted Supernova Sample

    N. Suzuki;N. Suzuki;D. Rubin;D. Rubin;C. Lidman;G. Aldering

  • 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

  • Differential Galaxy Evolution in Cluster and Field Galaxies at z ≈ 0.3

    Michael L. Balogh;Simon L. Morris;Simon L. Morris;H. K. C. Yee;H. K. C. Yee;R. G. Carlberg;R. G. Carlberg

  • The Average Mass and Light Profiles of Galaxy Clusters

    R. G. Carlberg;R. G. Carlberg;H. K. C. Yee;H. K. C. Yee;E. Ellingson;E. Ellingson

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

    Chris Blake;Sarah Brough;Matthew Colless;Carlos Contreras

  • The Average Mass-to-Light Profile of Galaxy Clusters

    R. G. Carlberg;H. K. C. Yee;E. Ellingson

  • Galaxy cluster virial masses and Omega

    R. G. Carlberg;H. K. C. Yee;E. Ellingson;R. Abraham

  • The Red-Sequence Cluster Survey. I. The Survey and Cluster Catalogs for Patches RCS 0926+37 and RCS 1327+29

    Michael D. Gladders;Michael D. Gladders;Michael D. Gladders;Howard K.C. Yee;Howard K.C. Yee

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

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

  • The Red-Sequence Cluster Survey I: The Survey and Cluster Catalogs for Patches RCS0926+37 and RCS1327+29

    Michael D. Gladders;Howard K.C. Yee

  • 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 Morphologies of Distant Galaxies. I. an Automated Classification System

    Roberto G. Abraham;Francisco Valdes;H. K. C. Yee;Sidney van den Bergh

  • 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

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

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

  • Evolution of the Galaxy Population Based on Photometric Redshifts in the Hubble Deep Field

    M. J. Sawicki;H. Lin;H. K. C. Yee

  • The Evolution of Population Gradients in Galaxy Clusters: The Butcher-Oemler Effect and Cluster Infall

    E. Ellingson;E. Ellingson;H. Lin;H. K. C. Yee;H. K. C. Yee;R. G. Carlberg;R. G. Carlberg

  • The average mass profile of galaxy clusters

    R. G. Carlberg;R. G. Carlberg;H. K. C. Yee;H. K. C. Yee;E. Ellingson;E. Ellingson;S. L. Morris;S. L. Morris

  • The CNOC2 Field Galaxy Luminosity Function. I. A Description of Luminosity Function Evolution

    Huan Lin;H. K. C. Yee;H. K. C. Yee;R. G. Carlberg;R. G. Carlberg;Simon L. Morris;Simon L. Morris

  • The Dependence of Cluster Galaxy Star Formation Rates on the Global Environment

    Mike L. Balogh;David Schade;David Schade;Simon L. Morris;Simon L. Morris;H. K. C. Yee;H. K. C. Yee

  • Star Formation in Cluster Galaxies at 0.2<z<0.55

    Mike L. Balogh;Simon L. Morris;Simon L. Morris;H. K. C. Yee;H. K. C. Yee;R. G. Carlberg;R. G. Carlberg

Frequent Co-Authors

Michael D. Gladders
Michael D. Gladders University of Chicago
Henk Hoekstra
Henk Hoekstra Leiden University
Rob Sharp
Rob Sharp Australian National University
Saul Perlmutter
Saul Perlmutter Lawrence Berkeley National Laboratory
Michael J. Drinkwater
Michael J. Drinkwater University of Queensland
Warrick J. Couch
Warrick J. Couch Swinburne University of Technology
Karl Glazebrook
Karl Glazebrook Swinburne University of Technology
Scott M. Croom
Scott M. Croom University of Sydney
Matthew Colless
Matthew Colless Australian National University
Barry F. Madore
Barry F. Madore Carnegie Institution for Science

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