World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
77
Citations
23953
World Ranking
3226
National Ranking
9

Tomotsugu Goto 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 Tomotsugu Goto 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: 330 publications — 23rd percentile

23% of scientists in this discipline score the same or lower.

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

Tomotsugu Goto 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 Tomotsugu Goto 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: 77 D-Index — 13th percentile

13% of scientists in this discipline score the same or lower.

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

Overview

Tomotsugu Goto is affiliated with the National Tsing Hua University in Taiwan. Their primary field of study is Physics and Astronomy, with a focus on Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Atomic and Molecular Physics and Optics, and Applied Mathematics.

The scientist's research topics broadly cover areas such as Galaxies: Formation, Evolution, Phenomena, Astronomy and Astrophysical Research, Gamma-ray bursts and supernovae, Pulsars and Gravitational Waves Research, Radio Astronomy Observations and Technology, Stellar, planetary, and galactic studies, and Astrophysical Phenomena and Observations.

Tomotsugu Goto has published extensively in numerous academic venues. Frequent publication venues include:

  • Monthly Notices of the Royal Astronomical Society
  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Astronomy and Astrophysics
  • Publications of the Astronomical Society of Australia

Selected recent papers include:

  • Energy functions of fast radio bursts derived from the first CHIME/FRB catalogue, 2022, Monthly Notices of the Royal Astronomical Society
  • BURSTT: Bustling Universe Radio Survey Telescope in Taiwan, 2022, Publications of the Astronomical Society of the Pacific
  • Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XVI. 69 New Quasars at 5.8 < z < 7.0, 2022, The Astrophysical Journal Supplement Series
  • No redshift evolution of non-repeating fast radio burst rates, 2020, Monthly Notices of the Royal Astronomical Society
  • Quasar Luminosity Function at z = 7, 2023, The Astrophysical Journal Letters

Frequent collaborators of Tomotsugu Goto include:

  • T. Hashimoto
  • Seong Jin Kim
  • Simon C-C Ho
  • Tiger Yu-Yang Hsiao
  • Ece Kilerci

Best Publications

  • The Infrared Astronomical Mission AKARI

    H. Murakami;H. Baba;P. Barthel;D.L. Clements

  • The infrared astronomical mission AKARI

    Hiroshi Murakami;Hajime Baba;Peter D. Barthel;David L. Clements

  • The Hyper Suprime-Cam SSP Survey: Overview and Survey Design

    H. Aihara;N. Arimoto;R. Armstrong;S. Arnouts

  • Galaxy Star Formation as a Function of Environment in the Early Data Release of the Sloan Digital Sky Survey

    Percy L. Gómez;Robert C. Nichol;Christopher J. Miller;Michael L. Balogh

  • The morphology–density relation in the Sloan Digital Sky Survey

    Tomotsugu Goto;Chisato Yamauchi;Yutaka Fujita;Sadanori Okamura

  • The Hyper Suprime-Cam SSP Survey: Overview and survey design

    Hiroaki Aihara;Nobuo Arimoto;Nobuo Arimoto;Robert Armstrong;Stéphane Arnouts

  • The Morphology - Density Relation in z ~ 1 Clusters

    M. Postman;M. Franx;N. Cross;B. Holden

  • Star formation rate indicators in the Sloan Digital Sky Survey

    A. M. Hopkins;C. J. Miller;R. C. Nichol;A. J. Connolly

  • The Morphology-Density Relation in z ~ 1 Clusters

    M. Postman;M. Franx;N.J.G. Cross;B. Holden

  • Star Formation Rate Indicators in the Sloan Digital Sky Survey

    A. M. Hopkins;C. J. Miller;R. C. Nichol;A. J. Connolly

  • First data release of the Hyper Suprime-Cam Subaru Strategic Program

    Hiroaki Aihara;Robert Armstrong;Steven Bickerton;James Bosch

  • STRONG-LENSING ANALYSIS OF A1689 FROM DEEP ADVANCED CAMERA IMAGES

    Tom Broadhurst;Narciso Benítez;Narciso Benítez;Dan Coe;Keren Sharon

  • The Far-Infrared Surveyor (FIS) for AKARI

    Mitsunobu Kawada;Hajime Baba;Peter D. Barthel;David Clements

  • The C4 clustering algorithm: clusters of galaxies in the Sloan Digital Sky Survey

    Christopher J. Miller;Robert C. Nichol;Robert C. Nichol;Daniel Reichart;Risa H. Wechsler

  • The Far-Infrared Surveyor (FIS) for AKARI

    Mitsunobu Kawada;Hajime Baba;Peter D. Barthel;David Clements

  • The Environmental Dependence of Galaxy Properties in the Local Universe: Dependences on Luminosity, Local Density, and System Richness

    Masayuki Tanaka;Tomotsugu Goto;Tomotsugu Goto;Sadanori Okamura;Kazuhiro Shimasaku

  • The Environmental Dependence of Galaxy Properties in the Local Universe: Dependence on Luminosity, Local Density, and System Richness

    Masayuki Tanaka;Tomotsugu Goto;Sadanori Okamura;Kazuhiro Shimasaku

  • The Cut-and-Enhance Method: Selecting Clusters of Galaxies from the Sloan Digital Sky Survey Commissioning Data

    Tomotsugu Goto;Tomotsugu Goto;Maki Sekiguchi;Robert C. Nichol;Neta A. Bahcall

  • The Cut & Enhance method : selecting clusters of galaxies from the SDSS commissioning data

    Tomotsugu Goto;Maki Sekiguchi;Robert C. Nichol;Neta A. Bahcall

  • Galaxy Star Formation as a function of Environment

    F. J. Castander;F. J. Castander;M. L. Balogh;M. Bernardi;M. Bernardi;R. G. Bower

Frequent Co-Authors

Glenn J. White
Glenn J. White The Open University
Takehiko Wada
Takehiko Wada Tohoku University
Stephen Serjeant
Stephen Serjeant The Open University
Myungshin Im
Myungshin Im Seoul National University
Marc Postman
Marc Postman Space Telescope Science Institute
Matthew A. Malkan
Matthew A. Malkan University of California, Los Angeles
Nobunari Kashikawa
Nobunari Kashikawa University of Tokyo
Masatoshi Imanishi
Masatoshi Imanishi The Graduate University for Advanced Studies, SOKENDAI
John P. Blakeslee
John P. Blakeslee National Optical-Infrared Astronomy Research Lab
Tohru Nagao
Tohru Nagao Ehime University

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