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Nozomu Tominaga

Nozomu Tominaga

Konan University
Japan

D-Index & Metrics

Physics

D-Index
77
Citations
20030
World Ranking
3247
National Ranking
117

Nozomu Tominaga 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 Nozomu Tominaga 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: 357 publications — 29th percentile

29% of scientists in this discipline score the same or lower.

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

Nozomu Tominaga 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 Nozomu Tominaga 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

Nozomu Tominaga is affiliated with Konan University in Japan and has an extensive publication record primarily in the fields of Physics and Astronomy. Their research contributions notably span the subfields of Astronomy and Astrophysics, Nuclear and High Energy Physics, Instrumentation, Atomic and Molecular Physics, and Optics, as well as Statistical and Nonlinear Physics.

The scientist's work covers several main topics, including studies on gamma-ray bursts and supernovae, stellar, planetary, and galactic research, astrophysical phenomena and observations, and pulsars and gravitational waves research. Additional focus areas include astrophysics and cosmic phenomena, as well as galaxy formation, evolution, and phenomena.

Tominaga's publications appear frequently in major venues such as arXiv (Cornell University), The Astrophysical Journal, Monthly Notices of the Royal Astronomical Society, The Astrophysical Journal Letters, and Publications of the Astronomical Society of Japan.

Notable recent papers by Tominaga and collaborators include:

  • Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. II. Elemental Abundances (2022, The Astrophysical Journal)
  • JWST Identification of Extremely Low C/N Galaxies with [N/O] ≳ 0.5 at z ∼ 6-10 Evidencing the Early CNO-cycle Enrichment and a Connection with Globular Cluster Formation (2023, The Astrophysical Journal)
  • Discovery of the Fastest Early Optical Emission from Overluminous SN Ia 2020hvf: A Thermonuclear Explosion within a Dense Circumstellar Environment (2021, The Astrophysical Journal Letters)
  • EMPRESS. XIII. Chemical Enrichment of Young Galaxies Near and Far at z ∼ 0 and 4-10: Fe/O, Ar/O, S/O, and N/O Measurements with a Comparison of Chemical Evolution Models (2024, The Astrophysical Journal)
  • Unravelling the Asphericities in the Explosion and Multifaceted Circumstellar Matter of SN 2023ixf (2024, The Astrophysical Journal)

Frequent coauthors of Tominaga include:

  • Masaomi Tanaka (27 joint publications)
  • Takashi J. Moriya (19 joint publications)
  • Shigeyuki Sako (16 joint publications)
  • Tomoki Morokuma (16 joint publications)
  • Ryou Ohsawa (15 joint publications)

Best Publications

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

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

  • Nucleosynthesis in Stars and the Chemical Enrichment of Galaxies

    Ken'ichi Nomoto;Chiaki Kobayashi;Nozomu Tominaga

  • Galactic Chemical Evolution: Carbon through Zinc

    Chiaki Kobayashi;Hideyuki Umeda;Ken ichi Nomoto;Nozomu Tominaga

  • Nucleosynthesis yields of core-collapse supernovae and hypernovae, and galactic chemical evolution

    Ken'ichi Nomoto;Nozomu Tominaga;Hideyuki Umeda;Chiaki Kobayashi

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

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

  • Supernova Nucleosynthesis in Population III 13-50 M☉ Stars and Abundance Patterns of Extremely Metal-poor Stars

    Nozomu Tominaga;Hideyuki Umeda;Ken ichi Nomoto

  • The first chemical enrichment in the universe and the formation of hyper metal-poor stars

    Nobuyuki Iwamoto;Hideyuki Umeda;Nozomu Tominaga;Ken'ichi Nomoto

  • A neutron-star-driven X-ray flash associated with supernova SN 2006aj.

    Paolo A. Mazzali;Jinsong Deng;Ken'ichi Nomoto;Ken'ichi Nomoto;Daniel N. Sauer

  • Supernova Nucleosynthesis in Population III 13 -- 50 $M_{\odot}$ Stars and Abundance Patterns of Extremely Metal-Poor Stars

    Nozomu Tominaga;Hideyuki Umeda;Ken'ichi Nomoto

  • THE MASS SPECTRUM OF THE FIRST STARS

    Hajime Susa;Kenji Hasegawa;Nozomu Tominaga;Nozomu Tominaga

  • The host galaxy of a fast radio burst

    E. F. Keane;E. F. Keane;S. Johnston;S. Bhandari;S. Bhandari;E. Barr

  • Evolution of Dust in Primordial Supernova Remnants: Can Dust Grains Formed in the Ejecta Survive and Be Injected into the Early Interstellar Medium?

    Takaya Nozawa;Takashi Kozasa;Asao Habe;Eli Dwek

  • The metamorphosis of supernova SN 2008D/XRF 080109: a link between supernovae and GRBs/hypernovae.

    Paolo A. Mazzali;Stefano Valenti;Stefano Valenti;Massimo Della Valle;Guido Chincarini;Guido Chincarini

  • An asymmetric energetic type Ic supernova viewed off-axis, and a link to gamma ray bursts.

    Paolo A. Mazzali;Koji S. Kawabata;Keiichi Maeda;Ken'ichi Nomoto

  • The Type Ic Hypernova SN 2003dh/GRB 030329

    Paolo A. Mazzali;Paolo A. Mazzali;Jinsong Deng;Nozomu Tominaga;Keiichi Maeda

  • The SUrvey for Pulsars and Extragalactic Radio Bursts – II. New FRB discoveries and their follow-up.

    S. Bhandari;S. Bhandari;S. Bhandari;E.F. Keane;E.F. Keane;E.D. Barr;E.D. Barr;E.D. Barr;A. Jameson;A. Jameson

  • J-GEM observations of an electromagnetic counterpart to the neutron star merger GW170817

    Yousuke Utsumi;Masaomi Tanaka;Nozomu Tominaga;Nozomu Tominaga;Michitoshi Yoshida

  • The unique type ib supernova 2005bf at nebular phases : A possible birth event of a strongly magnetized neutron star

    K. Maeda;M. Tanaka;K. Nomoto;N. Tominaga

  • Kilonova from post-merger ejecta as an optical and near-Infrared counterpart of GW170817

    Masaomi Tanaka;Yousuke Utsumi;Paolo A. Mazzali;Nozomu Tominaga;Nozomu Tominaga

  • Light-curve modelling of superluminous supernova 2006gy: collision between supernova ejecta and a dense circumstellar medium

    Takashi J. Moriya;Takashi J. Moriya;Sergei I. Blinnikov;Sergei I. Blinnikov;Nozomu Tominaga;Nozomu Tominaga;Naoki Yoshida;Naoki Yoshida

Frequent Co-Authors

Ken'ichi Nomoto
Ken'ichi Nomoto University of Tokyo
Masaomi Tanaka
Masaomi Tanaka Tohoku University
Tomoki Morokuma
Tomoki Morokuma Chiba Institute of Technology
Paolo A. Mazzali
Paolo A. Mazzali Liverpool John Moores University
Mamoru Doi
Mamoru Doi University of Tokyo
Naoki Yasuda
Naoki Yasuda Kavli Institute for the Physics and Mathematics of the Universe
Michitoshi Yoshida
Michitoshi Yoshida National Astronomical Observatory of Japan
Elena Pian
Elena Pian National Institute for Astrophysics
Hisanori Furusawa
Hisanori Furusawa National Institutes of Natural Sciences
Naoki Yoshida
Naoki Yoshida University of Tokyo

External Links

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