World's Best Scientists 2026 revealed!

D-Index & Metrics

Physics

D-Index
82
Citations
22598
World Ranking
2864
National Ranking
86

Michitoshi Yoshida 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 Michitoshi Yoshida 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: 600 publications — 69th percentile

69% of scientists in this discipline score the same or lower.

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

Michitoshi Yoshida 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 Michitoshi Yoshida 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.

Overview

Michitoshi Yoshida is affiliated with the National Astronomical Observatory of Japan. Their research is situated primarily in the field of Physics and Astronomy, with a focus on Astronomy and Astrophysics, Instrumentation, and Atomic and Molecular Physics, and Optics.

The main topics covered in their work include stellar, planetary, and galactic studies, astrophysics and star formation studies, galaxies' formation, evolution, and phenomena, astro and planetary science, astronomy and astrophysical research, gamma-ray bursts and supernovae, and adaptive optics and wavefront sensing.

Yoshida has contributed to a number of scientific papers, notably:

  • The Seimei telescope project and technical developments (2020), Publications of the Astronomical Society of Japan
  • The ram pressure stripped radio tails of galaxies in the Coma cluster (2020), Monthly Notices of the Royal Astronomical Society
  • A universal correlation between warm and hot gas in the stripped tails of cluster galaxies (2021), Nature Astronomy
  • An H α/X-ray orphan cloud as a signpost of intracluster medium clumping (2021), Monthly Notices of the Royal Astronomical Society
  • What Are the Radial Distributions of Density, Outflow Rates, and Cloud Structures in the M82 Wind? (2023), The Astrophysical Journal

Their frequent coauthors include Hideyuki Izumiura, Yoichi Itoh, Huan-Yu Teng, Bun'ei Sato, and Takuya Takarada. These collaborations reflect repeated joint contributions, indicating a consistent research partnership across several projects.

Yoshida's work has been published in several key scientific venues, which include:

  • arXiv (Cornell University)
  • Publications of the Astronomical Society of Japan
  • Monthly Notices of the Royal Astronomical Society
  • The Astrophysical Journal
  • Ground-based and Airborne Instrumentation for Astronomy IX

The scientist's research covers instrumental development alongside observational and theoretical studies, as seen in their involvement with telescope projects and investigations into galactic phenomena and interstellar mediums.

Best Publications

  • 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

  • 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

  • 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

  • High Dispersion Spectrograph (HDS) for the Subaru Telescope

    Kunio Noguchi;Wako Aoki;Satoshi Kawanomoto;Hiroyasu Ando

  • FOCAS: The Faint Object Camera and Spectrograph for the Subaru Telescope

    Nobunari Kashikawa;Kentaro Aoki;Ryo Asai;Noboru Ebizuka

  • The Subaru/XMM-Newton Deep Survey (SXDS). II. Optical Imaging and Photometric Catalogs*

    Hisanori Furusawa;George Kosugi;Masayuki Akiyama;Tadafumi Takata

  • The Super-Kamiokande Collaboration

    T. Futagami;Y. Fukuda;T. Hayakawa;K. Inoue

  • The SUBARU Deep Field Project: Lymanα Emitters at a Redshift of 6.6

    Yoshiaki Taniguchi;Masaru Ajiki;Tohru Nagao;Tohru Nagao;Yasuhiro Shioya

  • Localization and broadband follow-up of the gravitational-wave transient GW150914

    B. P. Abbott;R. Abbott;T. D. Abbott;M. R. Abernathy

  • The Discovery of Primeval Large-Scale Structures with Forming Clusters at Redshift 6

    M. Ouchi;K. Shimasaku;M. Akiyama;K. Sekiguchi

  • The Discovery of Primeval Large-Scale Structures with Forming Clusters at Redshift 6*

    Masami Ouchi;Kazuhiro Shimasaku;Masayuki Akiyama;Kazuhiro Sekiguchi

  • The Discovery of Two Lyman α Emitters beyond Redshift 6 in the Subaru Deep Field

    Keiichi Kodaira;Yoshiaki Taniguchi;Nobunari Kashikawa;Norio Kaifu

  • Discovery of a Giant Lya Emitter Near the Reionization Epoch

    Masami Ouchi;Yoshiaki Ono;Eiichi Egami;Tomoki Saito

  • An Indirect Search for WIMPs in the Sun using 3109.6 days of upward-going muons in Super-Kamiokande

    T. Tanaka;K. Abe;Y. Hayato

  • Precise measurement of the solar neutrino day-night and seasonal variation in Super-Kamiokande-I

    M. B. Smy;Y. Ashie;S. Fukuda;Y. Fukuda

  • Down‐sizing in galaxy formation at z∼ 1 in the Subaru/XMM–Newton Deep Survey (SXDS)

    Tadayuki Kodama;Toru Yamada;Masayuki Akiyama;Kentaro Aoki

  • Rapid Variability of Blazar 3C 279 during Flaring States in 2013-2014 with Joint Fermi-LAT, NuSTAR, Swift, and Ground-Based Multi-wavelength Observations

    M. Hayashida;K. Nalewajko;G. M. Madejski;M. Sikora

  • A DOZEN NEW GALAXIES CAUGHT IN THE ACT : GAS STRIPPING AND EXTENDED EMISSION LINE REGIONS IN THE COMA CLUSTER

    Masafumi Yagi;Michitoshi Yoshida;Yutaka Komiyama;Nobunari Kashikawa

  • Early phase observations of extremely luminous Type Ia Supernova 2009dc

    M. Yamanaka;K. S. Kawabata;K. Kinugasa;M. Tanaka

Frequent Co-Authors

Kunihiro Ohta
Kunihiro Ohta University of Tokyo
Yasushi Fukazawa
Yasushi Fukazawa Hiroshima University
Nobunari Kashikawa
Nobunari Kashikawa University of Tokyo
Hisanori Furusawa
Hisanori Furusawa National Institutes of Natural Sciences
Nozomu Tominaga
Nozomu Tominaga Konan University
Sadanori Okamura
Sadanori Okamura University of Tokyo
Tomoki Morokuma
Tomoki Morokuma Chiba Institute of Technology
Masaomi Tanaka
Masaomi Tanaka Tohoku University
Masayuki Akiyama
Masayuki Akiyama Tohoku University
Mamoru Doi
Mamoru Doi University of Tokyo

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