World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
95
Citations
33432
World Ranking
1929
National Ranking
50

Hisanori Furusawa 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 Hisanori Furusawa 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: 247 publications — 9th percentile

9% of scientists in this discipline score the same or lower.

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

Hisanori Furusawa 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 Hisanori Furusawa 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

Hisanori Furusawa is affiliated with the National Institutes of Natural Sciences in Japan. Their research primarily spans the field of Physics and Astronomy, with a focus on several specific subfields including Astronomy and Astrophysics, Instrumentation, Nuclear and High Energy Physics, Control and Systems Engineering, and Atomic and Molecular Physics, and Optics.

Their main topics of study cover a range of astronomical phenomena and processes. These include:

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

Hisanori Furusawa has contributed to numerous recent publications in astronomy, some of which have attracted considerable citations. Selected papers include:

  • "Third data release of the Hyper Suprime-Cam Subaru Strategic Program," 2021, Publications of the Astronomical Society of Japan
  • "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
  • "Quasar Luminosity Function at z = 7," 2023, The Astrophysical Journal Letters
  • "Combining the CLAUDS and HSC-SSP surveys," 2022, Astronomy and Astrophysics
  • "MUSSES2020J: The Earliest Discovery of a Fast Blue Ultraluminous Transient at Redshift 1.063," 2022, The Astrophysical Journal Letters

The venues in which their work frequently appears include:

  • arXiv (Cornell University)
  • Publications of the Astronomical Society of Japan
  • The Astrophysical Journal Letters
  • The Astrophysical Journal Supplement Series
  • Astronomy and Astrophysics

Frequent collaborators in their publications are:

  • Satoshi Miyazaki
  • Masayuki Tanaka
  • Tadafumi Takata
  • Yoshiki Toba
  • Takuji Yamashita

Best Publications

  • Spectra and Light Curves of Six Type Ia Supernovae at 0.511 < z < 1.12 and the Union2 Compilation

    R. Amanullah;C. Lidman;D. Rubin;G. Aldering

  • SPECTRA AND HUBBLE SPACE TELESCOPE LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 <z< 1.12 AND THE UNION2 COMPILATION ∗

    Rahman Amanullah;Chris Lidman;D. Rubin;D. Rubin;G. Aldering

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

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

  • Statistics of 207 Lya Emitters at a Redshift Near 7: Constraints on Reionization and Galaxy Formation Models

    Masami Ouchi;Kazuhiro Shimasaku;Hisanori Furusawa;Tomoki Saito

  • The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lya Emitters from z=3.1 to 5.7 in the 1 deg^2 Field: Luminosity Functions and AGN

    Masami Ouchi;Kazuhiro Shimasaku;Masayuki Akiyama;Chris Simpson

  • Subaru Prime Focus Camera — Suprime-Cam

    Satoshi Miyazaki;Yutaka Komiyama;Maki Sekiguchi;Sadanori Okamura

  • STATISTICS OF 207 Lyα EMITTERS AT A REDSHIFT NEAR 7: CONSTRAINTS ON REIONIZATION AND GALAXY FORMATION MODELS*

    Masami Ouchi;Kazuhiro Shimasaku;Hisanori Furusawa;Tomoki Saito

  • Subaru Deep Survey V. A Census of Lyman Break Galaxies at z=4 and 5 in the Subaru Deep Fields: Photometric Properties

    M. Ouchi;K. Shimasaku;S. Okamura;H. Furusawa

  • The Subaru/XMM-Newton Deep Survey (SXDS). IV. Evolution of Lyα Emitters from z = 3.1 to 5.7 in the 1 deg2 Field: Luminosity Functions and AGN*

    Masami Ouchi;Kazuhiro Shimasaku;Masayuki Akiyama;Chris Simpson

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

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

  • The Hyper Suprime-Cam software pipeline

    James Bosch;Robert Armstrong;Steven Bickerton;Hisanori Furusawa

  • Subaru Deep Survey. VI. A Census of Lyman Break Galaxies at z ≃ 4 and 5 in the Subaru Deep Fields: Clustering Properties*

    Masami Ouchi;Kazuhiro Shimasaku;Kazuhiro Shimasaku;Sadanori Okamura;Sadanori Okamura;Hisanori Furusawa

  • Hyper Suprime-Cam: System design and verification of image quality

    Satoshi Miyazaki;Satoshi Miyazaki;Yutaka Komiyama;Yutaka Komiyama;Satoshi Kawanomoto;Yoshiyuki Doi

  • A galaxy at a redshift z = 6.96

    Masanori Iye;Masanori Iye;Kazuaki Ota;Nobunari Kashikawa;Hisanori Furusawa

  • Second Data Release of the Hyper Suprime-Cam Subaru Strategic Program

    Hiroaki Aihara;Yusra AlSayyad;Makoto Ando;Robert Armstrong

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

    Hiroaki Aihara;Robert Armstrong;Steven Bickerton;James Bosch

  • An optical spectrum of the afterglow of a γ-ray burst at a redshift of z = 6.295

    N. Kawai;G. Kosugi;K. Aoki;T. Yamada

  • Hyper Suprime-Cam

    Satoshi Miyazaki;Yutaka Komiyama;Hidehiko Nakaya;Yukiko Kamata

  • Subaru Deep Survey II. Luminosity Functions and Clustering Properties of Lya Emitters at z=4.86 in the Subaru Deep Field

    M. Ouchi;K. Shimasaku;H. Furusawa;M. Miyazaki

  • Completing the Census of Ly-alpha Emitters at the Reionization Epoch

    Nobunari Kashikawa;Kazuhiro Shimasaku;Yuichi Matsuda;Eiichi Egami

Frequent Co-Authors

Masami Ouchi
Masami Ouchi University of Tokyo
Kazuhiro Shimasaku
Kazuhiro Shimasaku University of Tokyo
Satoshi Miyazaki
Satoshi Miyazaki The Graduate University for Advanced Studies, SOKENDAI
Naoki Yasuda
Naoki Yasuda Kavli Institute for the Physics and Mathematics of the Universe
Nobunari Kashikawa
Nobunari Kashikawa University of Tokyo
Sadanori Okamura
Sadanori Okamura University of Tokyo
Mamoru Doi
Mamoru Doi University of Tokyo
Tomoki Morokuma
Tomoki Morokuma Chiba Institute of Technology
Masayuki Akiyama
Masayuki Akiyama Tohoku University
Tohru Nagao
Tohru Nagao Ehime University

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