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D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 71 3638 3455 150 147 163 17897

Raphael Gavazzi publications per year

The chart shows the history of publications by Raphael Gavazzi between 2002 and 2021, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Raphael Gavazzi published across 20 years, from 2002 to 2021, averaging 7.3 papers a year. Output peaked at 17 publications in 2015. 14 of the 145 publications appeared in the last two years.

No. of publications
5 10 15
Bar chart. Horizontal axis: year, 2002 to 2021. Vertical axis: number of publications, 0 to 17. Peak 17 publications in 2015. 2002: 2 publications 2003: 1 publication 2004: 3 publications 2005: 2 publications 2006: 3 publications 2007: 5 publications 2008: 9 publications 2009: 13 publications 2010: 11 publications 2011: 13 publications 2012: 7 publications 2013: 14 publications 2014: 8 publications 2015: 17 publications 2016: 5 publications 2017: 9 publications 2018: 3 publications 2019: 6 publications 2020: 6 publications 2021: 8 publications
2002 2021

145 publications in total across all disciplines

View publications per year as a table
Raphael Gavazzi: publications per year, 2002 to 2021
Year Publications
2002 2
2003 1
2004 3
2005 2
2006 3
2007 5
2008 9
2009 13
2010 11
2011 13
2012 7
2013 14
2014 8
2015 17
2016 5
2017 9
2018 3
2019 6
2020 6
2021 8
Total 145
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Raphael Gavazzi 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 Raphael Gavazzi 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, 163–182 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: 163 publications — 1st percentile

1% 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 35 163
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
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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Raphael Gavazzi 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 Raphael Gavazzi 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, 70–71 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: 71 D-Index — 2nd percentile

2% 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 71
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
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:

  • Galaxy
  • Astronomy
  • Milky Way

The scientist’s investigation covers issues in Astrophysics, Astronomy, Galaxy, Elliptical galaxy and Dark matter. His study involves Gravitational lens, Redshift, Einstein ring, Stellar mass and Fundamental plane, a branch of Astrophysics. He has included themes like Lens and Luminosity in his Gravitational lens study.

His work deals with themes such as Stellar population and Initial mass function, which intersect with Stellar mass. All of his Astronomy and Galactic halo and Weak gravitational lensing investigations are sub-components of the entire Astronomy study. The various areas that Raphael Gavazzi examines in his Dark matter study include Radius, Virial mass and Velocity dispersion.

His most cited work include:

  • A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34 (490 citations)
  • Dancing in the dark: galactic properties trace spin swings along the cosmic web (486 citations)
  • THE SLOAN LENS ACS SURVEY. X. STELLAR, DYNAMICAL, AND TOTAL MASS CORRELATIONS OF MASSIVE EARLY-TYPE GALAXIES (418 citations)

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

His main research concerns Astrophysics, Galaxy, Redshift, Astronomy and Dark matter. His work in Gravitational lens, Weak gravitational lensing, Stellar mass, Galaxy cluster and Elliptical galaxy are all subfields of Astrophysics research. His Stellar mass study combines topics from a wide range of disciplines, such as Stellar population and Initial mass function.

In his work, Telescope is strongly intertwined with Lens, which is a subfield of Galaxy. His Redshift research is multidisciplinary, relying on both Advanced Camera for Surveys, Submillimeter Array, Physical cosmology, Luminous infrared galaxy and Emission spectrum. His research integrates issues of Einstein radius, Halo, Dark matter halo, Radius and Mass distribution in his study of Dark matter.

He most often published in these fields:

  • Astrophysics (112.63%)
  • Galaxy (93.94%)
  • Redshift (50.51%)

What were the highlights of his more recent work (between 2015-2021)?

  • Astrophysics (112.63%)
  • Galaxy (93.94%)
  • Redshift (50.51%)

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

Raphael Gavazzi spends much of his time researching Astrophysics, Galaxy, Redshift, Gravitational lens and Astronomy. His work in Dark matter, Weak gravitational lensing, Line, Luminous infrared galaxy and Galaxy formation and evolution is related to Astrophysics. His Emission spectrum research extends to Galaxy, which is thematically connected.

The study incorporates disciplines such as Star formation, COSMIC cancer database, Luminosity and Baryon in addition to Redshift. Raphael Gavazzi focuses mostly in the field of Gravitational lens, narrowing it down to matters related to Lens and, in some cases, Convolutional neural network and Support vector machine. Particularly relevant to Interacting galaxy is his body of work in Astronomy.

Between 2015 and 2021, his most popular works were:

  • The Horizon-AGN Simulation: Morphological Diversity of Galaxies ,Promoted by AGN Feedback (205 citations)
  • Density profile of dark matter haloes and galaxies in the Horizon-AGN simulation : the impact of AGN feedback (86 citations)
  • The Strong Gravitational Lens Finding Challenge (47 citations)

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

  • Galaxy
  • Astronomy
  • Milky Way

Raphael Gavazzi mostly deals with Astrophysics, Galaxy, Redshift, Astronomy and Initial mass function. Gravitational lens, Dark matter, Star formation, Weak gravitational lensing and Luminosity are the subjects of his Astrophysics studies. His biological study spans a wide range of topics, including Lens and Support vector machine.

His Galaxy research is multidisciplinary, incorporating perspectives in Line and Star. Much of his study explores Astronomy relationship to Terahertz radiation. While the research belongs to areas of Initial mass function, Raphael Gavazzi spends his time largely on the problem of Stellar mass, intersecting his research to questions surrounding Fundamental plane, Einstein radius and Spitzer Space Telescope.

Best Publications

  • Dancing in the dark: galactic properties trace spin swings along the cosmic web

    Y. Dubois;C. Pichon;C. Welker;C. Welker;D. Le Borgne

  • A dust-obscured massive maximum-starburst galaxy at a redshift of 6.34

    Dominik A. Riechers;Dominik A. Riechers;C. M. Bradford;C. M. Bradford;D. L. Clements;C. D. Dowell;C. D. Dowell

  • THE SLOAN LENS ACS SURVEY. X. STELLAR, DYNAMICAL, AND TOTAL MASS CORRELATIONS OF MASSIVE EARLY-TYPE GALAXIES

    M. W. Auger;T. Treu;A. S. Bolton;R. Gavazzi;R. Gavazzi

  • The Sloan Lens ACS Survey. IV. The Mass Density Profile of Early-Type Galaxies out to 100 Effective Radii

    Raphaël Gavazzi;Tommaso Treu;Jason D. Rhodes;Léon V. E. Koopmans

  • CFHTLenS: the Canada–France–Hawaii Telescope Lensing Survey – imaging data and catalogue products

    T. Erben;H. Hildebrandt;H. Hildebrandt;L. Miller;L. van Waerbeke

  • The Sloan Lens ACS Survey. V. The Full ACS Strong-Lens Sample

    Adam S. Bolton;Scott Burles;Leon V. E. Koopmans;Tommaso Treu

  • The Initial Mass Function of Early-Type Galaxies

    Tommaso Treu;Tommaso Treu;Matthew W. Auger;Leon V. E. Koopmans;Raphael Gavazzi;Raphael Gavazzi

  • THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). I. INTRODUCTION TO THE SURVEY

    Laura Ferrarese;Patrick Côté;Jean-Charles Cuillandre;S. D. J. Gwyn

  • The Horizon-AGN Simulation: Morphological Diversity of Galaxies ,Promoted by AGN Feedback

    Yohan Dubois;Sébastien Peirani;Sébastien Peirani;Christophe Pichon;Julien Devriendt

  • THE STRUCTURE AND DYNAMICS OF MASSIVE EARLY-TYPE GALAXIES: ON HOMOLOGY, ISOTHERMALITY, AND ISOTROPY INSIDE ONE EFFECTIVE RADIUS

    L. V. E. Koopmans;Adam S. Bolton;T. Treu;O. Czoske

  • AGN-driven quenching of star formation: morphological and dynamical implications for early-type galaxies

    Yohan Dubois;Yohan Dubois;Raphaël Gavazzi;Sébastien Peirani;Joseph Silk;Joseph Silk;Joseph Silk

  • Detection of a dark substructure through gravitational imaging

    S. Vegetti;L. V. E. Koopmans;A. Bolton;T. Treu

  • THE SLOAN LENS ACS SURVEY. IX. COLORS, LENSING, AND STELLAR MASSES OF EARLY-TYPE GALAXIES

    M. W. Auger;T. Treu;A. S. Bolton;R. Gavazzi;R. Gavazzi

  • Multiple images of a highly magnified supernova formed by an early-type cluster galaxy lens

    Patrick L. Kelly;Steven A. Rodney;Tommaso Treu;Ryan J. Foley

  • Dark Matter Contraction and the Stellar Content of Massive Early-type Galaxies: Disfavoring 'Light' Initial Mass Functions

    M. W. Auger;T. Treu;R. Gavazzi;A. S. Bolton

  • Cosmology With Strong-lensing Systems

    Shuo Cao;Marek Biesiada;Marek Biesiada;Raphaël Gavazzi;Aleksandra Piórkowska

  • Gravitational Lens Models Based on Submillimeter Array Imaging of Herschel-selected Strongly Lensed Sub-millimeter Galaxies at z > 1.5

    R. S. Bussmann;I. Pérez-Fournon;I. Pérez-Fournon;S. Amber;J. Calanog

  • The Sloan Lens ACS Survey. VII. Elliptical Galaxy Scaling Laws from Direct Observational Mass Measurements

    Adam S. Bolton;Adam S. Bolton;Tommaso Treu;Leon V. E. Koopmans;Raphael Gavazzi;Raphael Gavazzi;Raphael Gavazzi

  • Evidence for dark matter contraction and a Salpeter IMF in a massive early-type galaxy

    Alessandro Sonnenfeld;Tommaso Treu;Raphael Gavazzi;Philip J. Marshall

  • Gas and Dust in a Submillimeter Galaxy at z = 4.24 from the Herschel Atlas

    P. Cox;M. Krips;R. Neri;A. Omont

Frequent Co-Authors

Tommaso Treu
Tommaso Treu University of California, Los Angeles
Rob Ivison
Rob Ivison European Southern Observatory
Ismael Perez-Fournon
Ismael Perez-Fournon University of La Laguna
Alain Omont
Alain Omont Institut d'Astrophysique de Paris
Asantha Cooray
Asantha Cooray University of California, Irvine
Isaac Roseboom
Isaac Roseboom University of Edinburgh
Leonidas A. Moustakas
Leonidas A. Moustakas California Institute of Technology
Joaquin Vieira
Joaquin Vieira University of Illinois at Urbana-Champaign
Duncan Farrah
Duncan Farrah University of Hawaii at Manoa
Léon V. E. Koopmans
Léon V. E. Koopmans University of Groningen

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