World's Best Scientists 2026 revealed!
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Michiel Min

D-Index & Metrics

Discipline name D-Index World Ranking Current World Ranking National Ranking Current National Ranking Publications Citations
Physics 72 3600 3424 63 60 228 15070

Michiel Min publications per year

The chart shows the history of publications by Michiel Min between 2002 and 2021, highlighting the no. of papers published in each year and offering an overview of the publication velocity of this scholar. Michiel Min published across 20 years, from 2002 to 2021, averaging 11.9 papers a year. Output peaked at 23 publications in 2012. 23 of the 238 publications appeared in the last two years.

No. of publications
5 10 15 20
Bar chart. Horizontal axis: year, 2002 to 2021. Vertical axis: number of publications, 0 to 23. Peak 23 publications in 2012. 2002: 2 publications 2003: 4 publications 2004: 5 publications 2005: 13 publications 2006: 8 publications 2007: 7 publications 2008: 8 publications 2009: 9 publications 2010: 14 publications 2011: 15 publications 2012: 23 publications 2013: 16 publications 2014: 17 publications 2015: 15 publications 2016: 17 publications 2017: 19 publications 2018: 10 publications 2019: 13 publications 2020: 9 publications 2021: 14 publications
2002 2021

238 publications in total across all disciplines

View publications per year as a table
Michiel Min: publications per year, 2002 to 2021
Year Publications
2002 2
2003 4
2004 5
2005 13
2006 8
2007 7
2008 8
2009 9
2010 14
2011 15
2012 23
2013 16
2014 17
2015 15
2016 17
2017 19
2018 10
2019 13
2020 9
2021 14
Total 238
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Michiel Min 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 Michiel Min 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, 223–242 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: 228 publications — 7th percentile

7% 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 85 228
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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Michiel Min 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 Michiel Min 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, 72–73 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: 72 D-Index — 3rd percentile

3% 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 72
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:

  • Astronomy
  • Astrophysics
  • Optics

His main research concerns Astrophysics, Astronomy, Radiative transfer, Planet and Planetary system. His specific area of interest is Astrophysics, where Michiel Min studies Stars. His Radiative transfer research includes elements of Planetesimal and Photon.

The concepts of his Planet study are interwoven with issues in Astrobiology and Thick disk. In Planetary system, Michiel Min works on issues like Spectral energy distribution, which are connected to Solar analog, Starlight, Photoevaporation, Forward scatter and Surface brightness. His study in Exoplanet is interdisciplinary in nature, drawing from both Spectral line, James Webb Space Telescope and Atmospheric models.

His most cited work include:

  • The building blocks of planets within the ‘terrestrial’ region of protoplanetary disks (300 citations)
  • A 10 μm spectroscopic survey of Herbig Ae star disks: Grain growth and crystallization (287 citations)
  • A 10 micron spectroscopic survey of Herbig Ae star disks: grain growth and crystallization (284 citations)

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

Michiel Min mostly deals with Astrophysics, Astronomy, Radiative transfer, Stars and Planet. His study in the field of Circumstellar dust also crosses realms of Context. His Radiative transfer research incorporates elements of Astrochemistry, Opacity, T Tauri star, Planetesimal and Protoplanetary disk.

His work on Circumbinary planet, Planetary system and Young stellar object as part of general Stars research is frequently linked to Herbig Ae/Be star, bridging the gap between disciplines. His Planet study combines topics in areas such as Solar System and Light curve. His research in Spectral line intersects with topics in Extinction, Infrared and Silicate.

He most often published in these fields:

  • Astrophysics (107.47%)
  • Astronomy (41.67%)
  • Radiative transfer (44.83%)

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

  • Astrophysics (107.47%)
  • Exoplanet (17.24%)
  • Radiative transfer (44.83%)

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

His primary areas of study are Astrophysics, Exoplanet, Radiative transfer, Planet and Wavelength. His Astrophysics study frequently links to other fields, such as Spectral line. His Exoplanet study combines topics from a wide range of disciplines, such as Atmosphere, Brown dwarf and Opacity.

His research in Radiative transfer tackles topics such as Circumstellar dust which are related to areas like Red supergiant, Intensity, Supergiant and Sky. His Planet research incorporates themes from Protostar, Astrobiology, Solar System, Transit and Interstellar medium. His Stars study combines topics in areas such as Scattering and Interferometry.

Between 2017 and 2021, his most popular works were:

  • A chemical survey of exoplanets with ARIEL (145 citations)
  • Dust modeling of the combined ALMA and SPHERE datasets of HD 163296. Is HD 163296 really a Meeus group II disk (35 citations)
  • Dust modeling of the combined ALMA and SPHERE datasets of HD 163296. Is HD 163296 really a Meeus group II disk (35 citations)

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

  • Astronomy
  • Optics
  • Infrared

His primary areas of investigation include Astrophysics, Radiative transfer, Stars, Wavelength and Exoplanet. Michiel Min undertakes interdisciplinary study in the fields of Astrophysics and Sublimation through his works. The various areas that he examines in his Radiative transfer study include Astrochemistry and T Tauri star.

His work focuses on many connections between Stars and other disciplines, such as Scattering, that overlap with his field of interest in Polarimetry and SPHERES. As a part of the same scientific family, Michiel Min mostly works in the field of Wavelength, focusing on Millimeter and, on occasion, Grain growth, Young stellar object and Atmospheric radiative transfer codes. His research integrates issues of Astrobiology and Solar System in his study of Planet.

Best Publications

  • A 10 micron spectroscopic survey of Herbig Ae star disks: grain growth and crystallization

    R. van Boekel;M. Min;L.B.F.M. Waters;A. de Koter

  • A 10 μm spectroscopic survey of Herbig Ae star disks: Grain growth and crystallization

    R. van Boekel;R. van Boekel;M. Min;L.B.F.M. Waters;L.B.F.M. Waters;A. de Koter

  • The building blocks of planets within the ‘terrestrial’ region of protoplanetary disks

    R.J.H.M. van Boekel;R.J.H.M. van Boekel;M. Min;C. Leinert;L.B.F.M. Waters;L.B.F.M. Waters

  • A chemical survey of exoplanets with ARIEL

    Giovanna Tinetti;Pierre Drossart;Paul Eccleston;Paul Hartogh

  • Modeling optical properties of cosmic dust grains using a distribution of hollow spheres

    M. Min;J.W. Hovenier;A. de Koter

  • Three radial gaps in the disk of TW Hydrae imaged with SPHERE

    Roy van Boekel;Thomas Henning;Jonathan Menu;Jos de Boer

  • Benchmark problems for continuum radiative transfer - High optical depths, anisotropic scattering, and polarisation

    C. Pinte;T. J. Harries;M. Min;A. M. Watson

  • Radiative transfer in very optically thick circumstellar disks

    M. Min;C.P. Dullemond;C. Dominik;A. de Koter;A. de Koter

  • Dust coagulation and fragmentation in molecular clouds II. The opacity of the dust aggregate size distribution

    C.W. Ormel;M. Min;A.G.G.M. Tielens;C. Dominik

  • Coagulation and Fragmentation in molecular clouds. II. The opacity of the dust aggregate size distribution

    C. W. Ormel;M. Min;A. G. G. M. Tielens;C. Dominik

  • Consistent dust and gas models for protoplanetary disks I. Disk shape, dust settling, opacities, and PAHs

    Peter Woitke;M. Min;C. Pinte;C. Pinte;W. F. Thi

  • The thermal structure and the location of the snow line in the protosolar nebula: axisymmetric models with full 3-D radiative transfer

    M. Min;C.P. Dullemond;M. Kama;C. Dominik

  • The shape and composition of interstellar silicate grains

    M. Min;L. B. F. M. Waters;L. B. F. M. Waters;A. de Koter;J. W. Hovenier

  • Observing transiting planets with JWST. Prime targets and their synthetic spectral observations

    P. Mollière;R. van Boekel;J. Bouwman;Th. Henning

  • On the structure of the transition disk around TW Hya

    J. Menu;R. van Boekel;T. Henning;C. J. Chandler

  • Shape effects in scattering and absorption by randomly oriented particles small compared to the wavelength

    M. Min;J.W. Hovenier;A. de Koter

  • Observing transiting planets with JWST -- Prime targets and their synthetic spectral observations

    Paul Mollière;Roy van Boekel;Jeroen Bouwman;Thomas Henning

  • Three Radial Gaps in the Disk of TW Hydrae Imaged with SPHERE

    R. van Boekel;Th. Henning;J. Menu;J. Menu;J. de Boer;J. de Boer

  • Dust Evolution in Protoplanetary Disks Around Herbig Ae/Be Stars—the Spitzer View

    A Juhasz;J Bouwman;Th Henning;Bram Acke

  • Gas and dust structures in protoplanetary disks hosting multiple planets

    P. Pinilla;M. de Juan Ovelar;S. Ataiee;M. Benisty;M. Benisty

Frequent Co-Authors

Carsten Dominik
Carsten Dominik University of Amsterdam
A. de Koter
A. de Koter University of Amsterdam
Alexander G. G. M. Tielens
Alexander G. G. M. Tielens Leiden University
Francois Menard
Francois Menard Grenoble Alpes University
Jeroen Bouwman
Jeroen Bouwman Max Planck Society
Motohide Tamura
Motohide Tamura University of Tokyo
Th. Henning
Th. Henning Max Planck Society
Anthony Boccaletti
Anthony Boccaletti Paris Observatory
Sascha P. Quanz
Sascha P. Quanz ETH Zurich
Manuel Güdel
Manuel Güdel University of Vienna

External Links

Personal website of Michiel Min

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Best Scientists Citing Michiel Min

Francois Menard

Francois Menard

Grenoble Alpes University

Publications: 124

David J. Wilner

David J. Wilner

Harvard University

Publications: 119

Carsten Dominik

Carsten Dominik

University of Amsterdam

Publications: 114

Sean M. Andrews

Sean M. Andrews

Harvard University

Publications: 106

Cornelis P. Dullemond

Cornelis P. Dullemond

Heidelberg University

Publications: 105

Gaspard Duchêne

Gaspard Duchêne

Grenoble Alpes University

Publications: 105

Sebastian Wolf

Sebastian Wolf

Kiel University

Publications: 97

Motohide Tamura

Motohide Tamura

University of Tokyo

Publications: 94

Sascha P. Quanz

Sascha P. Quanz

ETH Zurich

Publications: 80

Andrea Isella

Andrea Isella

Rice University

Publications: 80

Jean-Charles Augereau

Jean-Charles Augereau

Grenoble Alpes University

Publications: 78

E. F. van Dishoeck

E. F. van Dishoeck

Leiden University

Publications: 67

Anthony Boccaletti

Anthony Boccaletti

Paris Observatory

Publications: 66

Th. Henning

Th. Henning

Max Planck Society

Publications: 61

Mickaël Bonnefoy

Mickaël Bonnefoy

Grenoble Alpes University

Publications: 59

Ilaria Pascucci

Ilaria Pascucci

University of Arizona

Publications: 57

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