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Masamune Oguri

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 105 1397 1323 32 31 472 36684

Masamune Oguri publications per year

The chart shows the history of publications by Masamune Oguri between 2001 and 2025, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Masamune Oguri published across 25 years, from 2001 to 2025, averaging 22.7 papers a year. Output peaked at 50 publications in 2018. 70 of the 567 publications appeared in the last two years.

No. of publications
10 20 30 40 50
Bar chart. Horizontal axis: year, 2001 to 2025. Vertical axis: number of publications, 0 to 50. Peak 50 publications in 2018. 2001: 2 publications 2002: 8 publications 2003: 8 publications 2004: 16 publications 2005: 15 publications 2006: 15 publications 2007: 16 publications 2008: 16 publications 2009: 15 publications 2010: 12 publications 2011: 11 publications 2012: 16 publications 2013: 10 publications 2014: 16 publications 2015: 20 publications 2016: 21 publications 2017: 32 publications 2018: 50 publications 2019: 30 publications 2020: 39 publications 2021: 41 publications 2022: 44 publications 2023: 44 publications 2024: 36 publications 2025: 34 publications
2001 2025

567 publications in total across all disciplines

View publications per year as a table
Masamune Oguri: publications per year, 2001 to 2025
Year Publications
2001 2
2002 8
2003 8
2004 16
2005 15
2006 15
2007 16
2008 16
2009 15
2010 12
2011 11
2012 16
2013 10
2014 16
2015 20
2016 21
2017 32
2018 50
2019 30
2020 39
2021 41
2022 44
2023 44
2024 36
2025 34
Total 567
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Masamune Oguri 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 Masamune Oguri sits on this spectrum.

No. of scientists
50 100 150
Bar chart with 70 bars. Horizontal axis: publications, 103–122 to 1,469+. Vertical axis: number of scientists, 0 to 162. Most scientists, 162, have 323–342 publications. The last bar groups every scientist with 1,469 publications or more. The highlighted bar, 463–482 publications, is where this scientist sits. 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
103–122 publications 1,469+

This scientist: 472 publications — 51st percentile

51% of scientists in this discipline score the same or lower.

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

View publications distribution as a table
Number of Physics scientists by publication count, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
Publications Scientists This scientist
103–122 7
123–142 10
143–162 31
163–182 35
183–202 53
203–222 81
223–242 85
243–262 112
263–282 114
283–302 126
303–322 136
323–342 162
343–362 155
363–382 156
383–402 134
403–422 145
423–442 147
443–462 131
463–482 131 472
483–502 116
503–522 106
523–542 103
543–562 87
563–582 84
583–602 94
603–622 70
623–642 76
643–662 60
663–682 54
683–702 60
703–722 48
723–742 64
743–762 48
763–782 37
783–802 43
803–822 34
823–842 36
843–862 32
863–882 32
883–902 31
903–922 25
923–942 15
943–962 24
963–982 13
983–1,002 21
1,003–1,022 21
1,023–1,042 16
1,043–1,062 9
1,063–1,082 19
1,083–1,102 11
1,103–1,122 17
1,123–1,142 11
1,143–1,162 7
1,163–1,182 4
1,183–1,202 10
1,203–1,222 8
1,223–1,242 16
1,243–1,262 4
1,263–1,282 10
1,283–1,302 5
1,303–1,322 7
1,323–1,342 4
1,343–1,362 8
1,363–1,382 6
1,383–1,402 7
1,403–1,422 3
1,423–1,442 4
1,443–1,462 4
1,463–1,468 3
1,469+ 100
Download as CSV

Masamune Oguri 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 Masamune Oguri sits on this spectrum.

No. of scientists
50 100 150
Bar chart with 59 bars. Horizontal axis: D-Index, 70–71 to 185+. Vertical axis: number of scientists, 0 to 167. Most scientists, 167, have 80–81 D-Index. The last bar groups every scientist with 185 D-Index or more. The highlighted bar, 104–105 D-Index, is where this scientist sits. 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
70–71 D-Index 185+

This scientist: 105 D-Index — 63rd percentile

63% of scientists in this discipline score the same or lower.

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

View D-Index distribution as a table
Number of Physics scientists by D-index, Research.com 2026 ranking edition. Based on 3,678 ranked scientists.
D-Index Scientists This scientist
70–71 76
72–73 110
74–75 143
76–77 153
78–79 144
80–81 167
82–83 167
84–85 166
86–87 132
88–89 155
90–91 134
92–93 137
94–95 102
96–97 112
98–99 110
100–101 116
102–103 97
104–105 103 105
106–107 87
108–109 90
110–111 67
112–113 78
114–115 75
116–117 67
118–119 69
120–121 60
122–123 59
124–125 53
126–127 42
128–129 41
130–131 33
132–133 32
134–135 45
136–137 19
138–139 24
140–141 28
142–143 31
144–145 22
146–147 20
148–149 12
150–151 16
152–153 24
154–155 23
156–157 15
158–159 15
160–161 11
162–163 17
164–165 12
166–167 11
168–169 9
170–171 9
172–173 11
174–175 4
176–177 8
178–179 5
180–181 3
182–183 4
184 4
185+ 99
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Overview

Masamune Oguri is affiliated with the Kavli Institute for the Physics and Mathematics of the Universe in Japan. Their research primarily focuses on the field of Physics and Astronomy, with a significant concentration in Astronomy and Astrophysics.

The main topics of their work cover a range of areas within astronomy and astrophysics, including:

  • Galaxies: Formation, Evolution, Phenomena
  • Astronomy and Astrophysical Research
  • Stellar, planetary, and galactic studies
  • Gamma-ray bursts and supernovae
  • Astrophysical Phenomena and Observations
  • Cosmology and Gravitation Theories
  • Adaptive optics and wavefront sensing

Their research spans multiple subfields, such as:

  • Astronomy and Astrophysics
  • Instrumentation
  • Atomic and Molecular Physics, and Optics
  • Nuclear and High Energy Physics
  • Electrical and Electronic Engineering

Masamune Oguri has a substantial record of publications, frequently publishing in the following venues:

  • arXiv (Cornell University)
  • The Astrophysical Journal
  • Monthly Notices of the Royal Astronomical Society
  • Astronomy and Astrophysics
  • Physical review. D/Physical review. D.

Regular collaborators include:

  • Adi Zitrin
  • J. M. Diego
  • Atsushi J. Nishizawa
  • Seiji Fujimoto
  • Gabriel Brammer

Recent papers authored or co-authored by Masamune Oguri include:

  • A Comprehensive Study of Galaxies at z ∼ 9-16 Found in the Early JWST Data: Ultraviolet Luminosity Functions and Cosmic Star Formation History at the Pre-reionization Epoch (2023), The Astrophysical Journal Supplement Series
  • Third data release of the Hyper Suprime-Cam Subaru Strategic Program (2021), Publications of the Astronomical Society of Japan
  • JWST Census for the Mass-Metallicity Star Formation Relations at z = 4-10 with Self-consistent Flux Calibration and Proper Metallicity Calibrators (2023), The Astrophysical Journal Supplement Series
  • Hyper Suprime-Cam Year 3 results: Cosmology from cosmic shear power spectra (2023), Physical review. D/Physical review. D.
  • The eROSITA Final Equatorial-Depth Survey (eFEDS) (2021), Astronomy and Astrophysics

Best Publications

  • LSST Science Book, Version 2.0

    Paul A. Abell;Julius Allison;Scott F. Anderson

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

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

  • Revising the Halofit Model for the Nonlinear Matter Power Spectrum

    Ryuichi Takahashi;Masanori Sato;Takahiro Nishimichi;Atsushi Taruya;Atsushi Taruya

  • Cosmology from cosmic shear power spectra with Subaru Hyper Suprime-Cam first-year data

    Chiaki Hikage;Masamune Oguri;Masamune Oguri;Takashi Hamana;Surhud More;Surhud More

  • Clustering of High Redshift ($z\ge 2.9$) Quasars from the Sloan Digital Sky Survey

    Yue Shen;Michael A. Strauss;Masamune Oguri;Joseph F. Hennawi

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

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

  • Gravitationally lensed quasars and supernovae in future wide-field optical imaging surveys

    Masamune Oguri;Philip J. Marshall;Philip J. Marshall

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

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

  • Clustering of High Redshift (Z >= 2.9) Quasars from the Sloan Digital Sky Survey

    Yue Shen;Michael Abram Strauss;Masamune Oguri;Masamune Oguri;Joseph F. Hennawi

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

    Hiroaki Aihara;Yusra AlSayyad;Makoto Ando;Robert Armstrong

  • Binary Quasars in the Sloan Digital Sky Survey: Evidence for Excess Clustering on Small Scales

    Joseph F. Hennawi;Michael A. Strauss;Masamune Oguri;Naohisa Inada

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

    Hiroaki Aihara;Robert Armstrong;Steven Bickerton;James Bosch

  • Hyper Suprime-Cam

    Satoshi Miyazaki;Yutaka Komiyama;Hidehiko Nakaya;Yukiko Kamata

  • Microlensing constraints on primordial black holes with the Subaru/HSC Andromeda observation

    Hiroko Niikura;Masahiro Takada;Naoki Yasuda;Robert H. Lupton

  • The Mass Distribution of SDSS J1004$+$4112 Revisited

    Masamune Oguri

  • Binary Quasars in the Sloan Digital Sky Survey: Evidence for Excess Clustering on Small Scales

    Joseph F. Hennawi;Joseph F. Hennawi;Michael Abram Strauss;Masamune Oguri;Masamune Oguri;Naohisa Inada

  • Microlensing constraints on primordial black holes with Subaru/HSC Andromeda observations

    Hiroko Niikura;Hiroko Niikura;Masahiro Takada;Naoki Yasuda;Robert H. Lupton

  • Hubble Frontier Fields First Complete Cluster Data: Faint Galaxies at $z\sim 5-10$ for UV Luminosity Functions and Cosmic Reionization

    Masafumi Ishigaki;Ryota Kawamata;Masami Ouchi;Masamune Oguri

  • Combined strong and weak lensing analysis of 28 clusters from the Sloan Giant Arcs Survey

    Masamune Oguri;Matthew B. Bayliss;Håkon Dahle;Keren Sharon

  • Discovery of a Giant Lya Emitter Near the Reionization Epoch

    Masami Ouchi;Yoshiaki Ono;Eiichi Egami;Tomoki Saito

Frequent Co-Authors

Masami Ouchi
Masami Ouchi University of Tokyo
Satoshi Miyazaki
Satoshi Miyazaki The Graduate University for Advanced Studies, SOKENDAI
Michael A. Strauss
Michael A. Strauss University of Oklahoma
Tom Broadhurst
Tom Broadhurst University of the Basque Country
Gordon T. Richards
Gordon T. Richards Drexel University
Donald P. Schneider
Donald P. Schneider Pennsylvania State University
Keiichi Umetsu
Keiichi Umetsu Institute of Astronomy and Astrophysics, Academia Sinica
Masahiro Takada
Masahiro Takada Kavli Institute for the Physics and Mathematics of the Universe
Robert H. Becker
Robert H. Becker University of California, Davis
Masayuki Tanaka
Masayuki Tanaka National Institutes of Natural Sciences

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