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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 94 1964 1864 52 50 574 42312

Fumio Abe publications per year

The chart shows the history of publications by Fumio Abe between 1983 and 2021, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Fumio Abe published across 39 years, from 1983 to 2021, averaging 14.8 papers a year. Output peaked at 45 publications in 2017. 39 of the 576 publications appeared in the last two years.

No. of publications
10 20 30 40
Bar chart. Horizontal axis: year, 1983 to 2021. Vertical axis: number of publications, 0 to 45. Peak 45 publications in 2017. 1983: 2 publications 1984: 2 publications 1985: 0 publications 1986: 2 publications 1987: 2 publications 1988: 3 publications 1989: 8 publications 1990: 10 publications 1991: 11 publications 1992: 15 publications 1993: 21 publications 1994: 15 publications 1995: 31 publications 1996: 22 publications 1997: 22 publications 1998: 41 publications 1999: 27 publications 2000: 8 publications 2001: 6 publications 2002: 6 publications 2003: 2 publications 2004: 8 publications 2005: 5 publications 2006: 2 publications 2007: 1 publication 2008: 10 publications 2009: 11 publications 2010: 14 publications 2011: 16 publications 2012: 23 publications 2013: 21 publications 2014: 18 publications 2015: 20 publications 2016: 29 publications 2017: 45 publications 2018: 30 publications 2019: 28 publications 2020: 17 publications 2021: 22 publications
1983 2021

576 publications in total across all disciplines

View publications per year as a table
Fumio Abe: publications per year, 1983 to 2021
Year Publications
1983 2
1984 2
1985 0
1986 2
1987 2
1988 3
1989 8
1990 10
1991 11
1992 15
1993 21
1994 15
1995 31
1996 22
1997 22
1998 41
1999 27
2000 8
2001 6
2002 6
2003 2
2004 8
2005 5
2006 2
2007 1
2008 10
2009 11
2010 14
2011 16
2012 23
2013 21
2014 18
2015 20
2016 29
2017 45
2018 30
2019 28
2020 17
2021 22
Total 576
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Fumio Abe 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 Fumio Abe 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, 563–582 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: 574 publications — 66th percentile

66% 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
483–502 116
503–522 106
523–542 103
543–562 87
563–582 84 574
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
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Fumio Abe 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 Fumio Abe 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, 94–95 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: 94 D-Index — 47th percentile

47% 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 94
96–97 112
98–99 110
100–101 116
102–103 97
104–105 103
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

What is he best known for?

The fields of study he is best known for:

  • Quantum mechanics
  • Astronomy
  • Particle physics

His primary areas of investigation include Astrophysics, Gravitational microlensing, Planet, Astronomy and Particle physics. His work in the fields of Astrophysics, such as Mass ratio, Bulge, Neptune and Orbital speed, intersects with other areas such as Einstein radius. His work carried out in the field of Gravitational microlensing brings together such families of science as Orbit, Gas giant and Primary.

His Planet research incorporates themes from Light curve and Stellar mass. Supersymmetry is closely connected to Nuclear physics in his research, which is encompassed under the umbrella topic of Particle physics. His studies deal with areas such as Top quark and Particle identification as well as Collider Detector at Fermilab.

His most cited work include:

  • Observation of top quark production in p̄p collisions with the collider detector at fermilab (899 citations)
  • Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing (526 citations)
  • Unbound or distant planetary mass population detected by gravitational microlensing (455 citations)

What are the main themes of his work throughout his whole career to date?

His main research concerns Astrophysics, Gravitational microlensing, Planet, Astronomy and Particle physics. The Light curve, Mass ratio, Brown dwarf and Planetary mass research Fumio Abe does as part of his general Astrophysics study is frequently linked to other disciplines of science, such as Einstein radius, therefore creating a link between diverse domains of science. The study incorporates disciplines such as Exoplanet, Parallax, Bulge and Proper motion in addition to Gravitational microlensing.

Planet and Low Mass are commonly linked in his work. His work on Galaxy and Rogue planet as part of general Astronomy research is often related to Microlensing Observations in Astrophysics, thus linking different fields of science. As a part of the same scientific family, Fumio Abe mostly works in the field of Particle physics, focusing on Nuclear physics and, on occasion, Production.

He most often published in these fields:

  • Astrophysics (49.82%)
  • Gravitational microlensing (48.23%)
  • Planet (32.98%)

What were the highlights of his more recent work (between 2017-2021)?

  • Gravitational microlensing (48.23%)
  • Astrophysics (49.82%)
  • Planet (32.98%)

In recent papers he was focusing on the following fields of study:

Fumio Abe spends much of his time researching Gravitational microlensing, Astrophysics, Planet, Light curve and Mass ratio. His work deals with themes such as Planetary system, Low Mass and Exoplanet, which intersect with Gravitational microlensing. Fumio Abe works mostly in the field of Astrophysics, limiting it down to topics relating to Parallax and, in certain cases, Lens, as a part of the same area of interest.

His work investigates the relationship between Planet and topics such as Subgiant that intersect with problems in Jovian. His Light curve research integrates issues from Anomaly and Event. His research in Mass ratio intersects with topics in Planetary mass, Gas giant and Circumbinary planet.

Between 2017 and 2021, his most popular works were:

  • Two new free-floating or wide-orbit planets from microlensing (35 citations)
  • Two new free-floating or wide-orbit planets from microlensing (35 citations)
  • A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray-luminous Classical Nova to Date (24 citations)

In his most recent research, the most cited papers focused on:

  • Quantum mechanics
  • Astronomy
  • Electron

Fumio Abe mainly investigates Gravitational microlensing, Astrophysics, Planet, Planetary system and Light curve. He combines subjects such as Low Mass, Brown dwarf and Bulge with his study of Gravitational microlensing. The Astrophysics study combines topics in areas such as Parallax and Orbit.

Fumio Abe has researched Planet in several fields, including Metallicity, Spectrometer, Binary star, Amplitude and Proper motion. His Planetary system research incorporates elements of Exoplanet, Magnification and Event. His Astronomy research is multidisciplinary, relying on both Gamma ray and Nuclear reaction.

Best Publications

  • Observation of top quark production in p̄p collisions with the collider detector at fermilab

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

  • The CDF Detector: An Overview

    F. Abe;D. Amidei;G. Apollinari;G. Ascoli

  • Discovery of a cool planet of 5.5 Earth masses through gravitational microlensing

    J.-P. Beaulieu;D. P. Bennett;P. Fouqué;A. Williams

  • Topology of three-jet events in p»p collisions at s=1.8 TeV

    F. Abe;D. Amidei;G. Apollinari;M. Atac

  • Observation of the Bc meson in pp¯ collisions at √s = 1.8 TeV

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

  • INCLUSIVE JET CROSS SECTION IN P P COLLISIONS AT S = 1.8 TEV

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

  • OGLE 2003-BLG-235/MOA 2003-BLG-53: A Planetary Microlensing Event

    I. A. Bond;A. Udalski;M. Jaroszyński;M. Jaroszyński;N. J. Rattenbury

  • Unbound or distant planetary mass population detected by gravitational microlensing

    T. Sumi;K. Kamiya;D. P. Bennett

  • Real-time difference imaging analysis of moa galactic bulge observations during 2000

    I.A. Bond;I.A. Bond;F. Abe;R.J. Dodd;R.J. Dodd;R.J. Dodd;J.B. Hearnshaw

  • Measurement of the antiproton-proton total cross section at s =546 and 1800 GeV

    F. Abe;M. Albrow;D. Amidei;C. Anway-Wiese

  • Discovery of a Jupiter/Saturn Analog with Gravitational Microlensing

    B. S. Gaudi;D. P. Bennett;A. Udalski;A. Gould

  • OGLE 2003-BLG-235/MOA 2003-BLG-53: A planetary microlensing event

    I. A. Bond;A. Udalski;M. Jaroszynski;N. J. Rattenbury

  • Measurement of the Top Quark Mass

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

  • FREQUENCY OF SOLAR-LIKE SYSTEMS AND OF ICE AND GAS GIANTS BEYOND THE SNOW LINE FROM HIGH-MAGNIFICATION MICROLENSING EVENTS IN 2005-2008

    A. Gould;Subo Dong;B. S. Gaudi;A. Udalski

  • Double parton scattering in [Formula presented] collisions at [Formula presented]

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

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

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

  • Evidence for top quark production in p̄p collisions at √s =1.8 TeV

    F. Abe;M. G. Albrow;S. R. Amendolia;D. Amidei

  • Search for new particles decaying to dijets at CDF

    F. Abe;H. Akimoto;A. Akopian;M. G. Albrow

  • A Cold Neptune-Mass Planet OGLE-2007-BLG-368Lb: Cold Neptunes Are Common

    T. Sumi;D.P. Bennett;I.A. Bond;A. Udalski

  • A Low-Mass Planet with a Possible Sub-Stellar-Mass Host in Microlensing Event MOA-2007-BLG-192

    D.P. Bennett;I.A. Bond;A. Udalski;T. Sumi

Frequent Co-Authors

David P. Bennett
David P. Bennett Goddard Space Flight Center
Yoshitaka Itow
Yoshitaka Itow Nagoya University
Yasushi Muraki
Yasushi Muraki Nagoya University
Igor Soszyński
Igor Soszyński University of Warsaw
Michał K. Szymański
Michał K. Szymański University of Warsaw
Andrew Gould
Andrew Gould The Ohio State University
Andrzej Udalski
Andrzej Udalski University of Warsaw
K. L. Byrum
K. L. Byrum Argonne National Laboratory
T. Devlin
T. Devlin Rutgers, The State University of New Jersey

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